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Two recent tests of loop quantum gravity theory
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<span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7074315/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #1 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" > <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353">kodama</span></span> <!--<h5 class="userTitle message-userTitle" dir="auto">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7074315" data-lb-caption-desc="kodama · Apr 2, 2024 at 8:19 PM"> <div class="message-fields message-fields--before"> <dl class="pairs pairs--columns pairs--fixedSmall pairs--customField" data-field="summary"> <dt>TL;DR Summary</dt> <dd>on electromagnetic properties of charged leptons and via the Lensing Effect</dd> </dl> </div> <article class="message-body js-selectToQuote"> <div > <div class="bbWrapper">2 recent gains on loop quantum gravity theory<br /> <br /> arXiv:2403.18606 (gr-qc)<br /> [Submitted on 27 Mar 2024]<br /> Test the Loop Quantum Gravity Theory via the Lensing Effect<br /> Lai Zhao, Meirong Tang, Zhaoyi Xu<br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> Recently, scholars such as Lewandowski, Ma, and Yang have successfully derived a quantum-corrected black hole model in loop quantum gravity (Phys.Rev.Lett.130.101501 (2023)), which is a modification of the Schwarzschild black hole. In this paper, we calculate the strong/weak gravitational lensing effects under the quantum-corrected black hole model, taking the supermassive black holes M87* and SgrA* as the subjects of study to explore the impact of the quantum correction parameter α on the positions of images and the Einstein ring. Our calculations show that in the case of strong gravitational lensing, the lensing coefficient a¯ increases with an increase in the quantum correction parameter, while the deflection angle and the lensing coefficient b¯ decrease with an increase in the quantum correction parameter. The quantum correction parameter α has a significant impact in the context of supermassive black holes. In weak gravitational lensing, the quantum correction parameter α plays a suppressive role. Our theoretical analysis suggests that with advancements in future astrophysical observation techniques, it might be possible to test loop quantum gravity theory using the gravitational lensing effect.<br /> <br /> Subjects: General Relativity and Quantum Cosmology (gr-qc)<br /> Cite as: arXiv:2403.18606 [gr-qc]<br /> (or arXiv:2403.18606v1 [gr-qc] for this version) </div> </div> </blockquote><br /> <a href="https://doi.org/10.48550/arXiv.2403.18606" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.48550/arXiv.2403.18606</a><br /> <br /> and<br /> <br /> [Submitted on 7 Dec 2023 (v1), last revised 28 Dec 2023 (this version, v2)]<br /> Shadows of Loop Quantum Black Holes: Semi-analytical Simulations of Loop Quantum Gravity Effects on Sagittarius A* and M 87*<br /> Hong-Xuan Jiang, Cheng Liu, Indu K. Dihingia, Yosuke Mizuno, Haiguang Xu, Tao Zhu, Qiang Wu<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> In this study, we delve into the observational implications of rotating Loop Quantum Black Holes (LQBHs) within an astrophysical framework. We employ semi-analytical General Relativistic Radiative Transfer (GRRT) computations to study the emission from the accretion flow around LQBHs. Our findings indicate that the increase of Loop Quantum Gravity (LQG) effects results in an enlargement of the rings from LQBHs, thereby causing a more circular polarization pattern in the shadow images. We make comparisons with the Event Horizon Telescope (EHT) observations of Sgr\,A∗ and M\,87∗, which enable us to determine an upper limit for the polymetric function P in LQG. The upper limit for Sgr\,A∗ is 0.2, while for M\,87∗ it is 0.07. Both black holes exhibit a preference for a relatively high spin (a≳0.5 for Sgr\,A∗ and 0.5≲a≲0.7 for M\,87∗). The constraints for Sgr\,A∗ are based on black hole spin and ring diameter, whereas for M\,87∗, the constraints are further tightened by the polarimetric pattern. In essence, our simulations provide observational constraints on the effect of LQG in supermassive black holes (SMBH), providing the most consistent comparison with observation.<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Astrophysical Phenomena (astro-ph.HE)<br /> Cite as: arXiv:2312.04288 [gr-qc]<br /> (or arXiv:2312.04288v2 [gr-qc] for this version) </div> </div> </blockquote><br /> <a href="https://doi.org/10.48550/arXiv.2312.04288" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.48550/arXiv.2312.04288</a><br /> <br /> and<br /> <br /> arXiv:2305.04336 (gr-qc)<br /> [Submitted on 7 May 2023 (v1), last revised 30 Oct 2023 (this version, v2)]<br /> Strong Gravitational Lensing by Loop Quantum Gravity Motivated Rotating Black Holes and EHT Observations<br /> Jitendra Kumar, Shafqat Ul Islam, Sushant G. Ghosh<br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> We investigate gravitational lensing in the strong deflection regime by loop quantum gravity (LQG)-motivated rotating black hole (LMRBH) metrics with an additional parameter l besides mass M and rotation a. The LMRBH spacetimes are regular everywhere, asymptotically encompassing the Kerr black hole as a particular case and, depending on the parameters, describe black holes with one horizon only (BH-I), black holes with an event horizon and a Cauchy horizon (BH-II), black holes with three horizons (BH-III), or black holes with no horizons (NH) spacetime. It turns out that as the LQG parameter l increases, the unstable photon orbit radius xps, the critical impact parameter ups, the deflection angle αD(θ) and angular position θ∞ also increases. Meanwhile, the angular separation s decreases, and relative magnitude rmag increases with increasing l for prograde motion but they show opposite behaviour for the retrograde motion. For Sgr A*, the angular position θ∞ is ∈ (16.4, 39.8) μas, while for M87* ∈ (12.33, 29.9) μas. The angular separation s, for SMBHs Sgr A* and M87*, differs significantly, with values ranging ∈ (0.008-0.376) μas for Sgr A* and ∈ (0.006-0.282) μas for M87*. We estimate the time delay between the first and second relativistic images using twenty supermassive galactic centre black holes as lenses. Our analysis concludes that, within the 1σ region, a significant portion of the BH-I and BH-II and for a small portion of BH-III parameter space agrees with the EHT results of M87* and Sgr A* whereas NH is completely ruled out. We discover that the EHT results of Sgr A* place more stringent limits on the parameter space of LMRBH black holes than those established by the EHT results of M87*. <br /> <br /> Comments: 16 Pages, 11 Figures, 3 Tables, Accepted for publication in EPJC<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc); Astrophysics of Galaxies (astro-ph.GA)<br /> Cite as: arXiv:2305.04336 [gr-qc]<br /> (or arXiv:2305.04336v2 [gr-qc] for this version) </div> </div> </blockquote><br /> and <br /> <br /> arXiv:2302.10482 (gr-qc)<br /> [Submitted on 21 Feb 2023 (v1), last revised 29 Apr 2023 (this version, v2)]<br /> Observational tests of quantum extension of Schwarzschild spacetime in loop quantum gravity with stars in the galactic center<br /> Jian-Ming Yan, Cheng Liu, Tao Zhu, Qiang Wu, Anzhong Wang<br /> <br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> In this paper, we use the publicly available observational data of 17 stellar stars orbiting Sgr A* to test the quantum extension of Schwarzschild spacetime in loop quantum gravity (LQG). For our purpose, we transform the geodesical evolution of a massive particle in the quantum-extended Schwarzschild black hole to the perturbed Kepler problem and calculate the effects of LQG on the pericentre advance of the stellar stars. With these effects, one is able to compare them with the publicly available astrometric and spectroscopic data of stellar stars in the galactic center. We perform Monte Carlo Markov Chain (MCMC) simulations to probe the possible LQG effects on the orbit of S-stars. No significant evidence of the quantum-extended Schwarzschild black hole from LQG is found. Among the posterior analyses of 17 S-stars, the result of S2 gives the strongest bound on the LQG parameter Aλ, which places an upper bound at 95\% confidence level on Aλ to be Aλ<0.302. <br /> <br /> Comments: 12 pages, 6 figures<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th)<br /> Cite as: arXiv:2302.10482 [gr-qc]<br /> (or arXiv:2302.10482v2 [gr-qc] for this version)<br /> <br /> <a href="https://doi.org/10.48550/arXiv.2302.10482" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.48550/arXiv.2302.10482</a><br /> Journal reference: Phys. Rev. D 107, 084043 (2023)<br /> Related DOI: <br /> <a href="https://doi.org/10.1103/PhysRevD.107.084043" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.1103/PhysRevD.107.084043</a> </div> </div> </blockquote><br /> <br /> arXiv:2403.17197 (hep-th)<br /> [Submitted on 25 Mar 2024]<br /> Loop Quantum Gravity effects on electromagnetic properties of charged leptons<br /> João Paulo S. Melo, Mario J. Neves, Jefferson M. A. Paixão, José A. Helayël-Neto<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> The efforts in this contribution consist in reassessing a modified Dirac equation that incorporates a γ0γ5-Lorentz-symmetry violating (LSV) term induced as a Loop Quantum Gravity (LQG) effect. Originally, this equation has been applied and considered as a good scenario for describing a number of investigations on the flight time of cosmic photons and neutrinos, which suggests that the speed of light in vacuum, in connection with the geometry that describes a granular space-time, takes an energy-dependent form, e.g., v(E)=1±E/ELSV, with ELSV≈6,5×1017 GeV for neutrinos. Once LQG provides a viable way to consistently understand this picture, we pursue an analysis of this effective Dirac equation to inspect some of its properties. These include: the derivation of the modified fermionic propagator, attainment of the Gordon decomposition of the vector current with minimal electromagnetic coupling to obtain information on the form factors, examination of the non-relativistic limit of the equation, evaluation of the spin- and velocity-dependent corrections to the Coulomb potential due to LQG effects, and the modified Hamiltonian in the low-relativistic regime. The study of the form factors may open up paths to set up bounds on the LQG parameters from the precision measurements of electromagnetic attributes of the charged leptons, such as their respective electric and magnetic dipole moments.<br /> <br /> Comments: 11 pages, 2 figures<br /> Subjects: High Energy Physics - Theory (hep-th); High Energy Physics - Phenomenology (hep-ph)<br /> Cite as: arXiv:2403.17197 [hep-th]<br /> (or arXiv:2403.17197v1 [hep-th] for this version)) </div> </div> </blockquote><br /> <a href="https://doi.org/10.48550/arXiv.2403.17197" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.48550/arXiv.2403.17197</a><br /> <br /> any comment on test loop quantum gravity theory on electromagnetic properties of charged leptons and via the Lensing Effect<br /> <br /> are those predictions the strong/weak gravitational lensing effects under the quantum-corrected black hole model, taking the supermassive black holes M87* and SgrA* as the subjects of study on unique to loop quantum gravity theory<br /> or<br /> could string theory, SUGRA, semiclassical gravity also make predictions strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA* via the Lensing Effect<br /> <br /> what if observations of strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA* confirm loop quantum gravity theory<br /> <br /> attributes of the charged leptons, such as their respective electric and magnetic dipole moments is something useful for connecting to experiment by electron EDM<br /> <br /> if loop quantum gravity theory on electromagnetic properties of charged leptons and via the Lensing Effect confirm by future experiment should Nobel Prize be awarded and loop quantum gravity theorywins over string theory ?</div> </div> <div class="js-selectToQuoteEnd"> </div> <div class="googleads_fixed"> <script async 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href="https://phys.org/physics-news/" target="_blank">Physics news</a> on Phys.org <ul class="phys_items"> <li><a href="https://phys.org/news/2025-02-unexpected-nucleus-prompts-reevaluation-atomic.html" target="_blank">Unexpected shape of lead-208 nucleus prompts reevaluation of atomic nuclei models</a></li> <li><a href="https://phys.org/news/2025-02-scientists-elusive-liquid-transition-deep.html" target="_blank">Scientists map elusive liquid-liquid transition point using deep neural network</a></li> <li><a href="https://phys.org/news/2025-02-links-disparate-pion-reactions-nuclear.html" target="_blank">New calculation links disparate pion reactions in nuclear physics</a></li> </ul> </div> <article class="message message--post js-post js-inlineModContainer " data-author="kodama" data-content="post-7078031" id="js-post-7078031" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7078031/"> <meta itemprop="parentItem" itemscope 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class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7078031" data-lb-caption-desc="kodama · Apr 14, 2024 at 2:15 PM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper">"Our theoretical analysis suggests that with advancements in future astrophysical observation techniques, it might be possible to test loop quantum gravity theory using the gravitational lensing effect."<br /> <br /> <br /> LQG makes specific predictions on strong gravitational lensing for the supermassive black holes M87* and SgrA* that can be observed, in principle, by Event Horizon Telescope (EHT) observations or future telescopes.<br /> <br /> what if these LQG predictions of gravitational lensing for the supermassive black holes M87* and SgrA* are verified?<br /> <br /> there was a recent solar eclipse in the USA.<br /> <br /> isn't this like the original test of GR vs Newton during the 1919 solar eclipse, here GR vs LQG using gravitational lensing</div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList "> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="ohwilleke" data-content="post-7078406" id="js-post-7078406" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7078406/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7078406"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-04-15T16:33:14-0500" data-time="1713216794" data-date-string="Apr 15, 2024" data-time-string="4:33 PM" title="Apr 15, 2024 at 4:33 PM" itemprop="datePublished">Apr 15, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7078406/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #3 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/ohwilleke.19562/"> <meta itemprop="url" content="https://www.physicsforums.com/members/ohwilleke.19562/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="19562"><span itemprop="name">ohwilleke</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Ocean</h5>--> <!----> <!-- Start Member Achievements --> <div class="post-badges"> <div class="post-badge badge-star" data-xf-init="tooltip" title="Click to Support PF"> <i class="fa--xf fal fa-star" aria-hidden="true"></i><span> Gold Member</span> </div> </div> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs 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Scientists have proposed ways to test if reality is closer to the LQG or the classical GR prediction. But, nobody has actually done those tests at the level of precision necessary to actually distinguish between the two theories with any meaningful statistical significance.</div> </div> <div class="js-selectToQuoteEnd"> </div> <div class="googleads_fixed"> <script async src="https://pagead2.googlesyndication.com/pagead/js/adsbygoogle.js?client=ca-pub-6580726045122001" crossorigin="anonymous"></script> <!-- PF 2ndPost 300x250 --> <ins class="adsbygoogle" style="display:block" data-ad-client="ca-pub-6580726045122001" data-ad-slot="5961342082" data-ad-format="auto" data-full-width-responsive="true"></ins> <script> (adsbygoogle = window.adsbygoogle || []).push({}); </script> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="4" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList is-active"> <ul class="reactionSummary"> <li><span class="reaction reaction--small reaction--1" data-reaction-id="1"><i aria-hidden="true"></i><img src="data:image/gif;base64,R0lGODlhAQABAIAAAAAAAP///yH5BAEAAAAALAAAAAABAAEAAAIBRAA7" class="reaction-sprite js-reaction" alt="Like" title="Like" /></span></li> </ul> <span class="u-srOnly">Likes</span> <bdi>Crispybacon</bdi>, <bdi>pines-demon</bdi>, <bdi>weirdoguy</bdi> and 1 other person </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="kodama" data-content="post-7078515" id="js-post-7078515" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7078515/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7078515"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-04-16T00:19:55-0500" data-time="1713244795" data-date-string="Apr 16, 2024" data-time-string="12:19 AM" title="Apr 16, 2024 at 12:19 AM" itemprop="datePublished">Apr 16, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7078515/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #4 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7078515" data-lb-caption-desc="kodama · Apr 16, 2024 at 12:19 AM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper"><blockquote data-attributes="member: 19562" data-quote="ohwilleke" data-source="post: 7078406" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> ohwilleke said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> The headline of the OP is a bit misleading. Scientists have proposed ways to test if reality is closer to the LQG or the classical GR prediction. But, nobody has actually done those tests at the level of precision necessary to actually distinguish between the two theories with any meaningful statistical significance. </div> </div> </blockquote><br /> what do you think of strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA*as a way to test quantum gravity effects ?<br /> <br /> does string theory make any predictions of strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA*?<br /> <br /> could quantum gravity effects show up as strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA*</div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList "> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="weirdoguy" data-content="post-7078531" id="js-post-7078531" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7078531/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7078531"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-04-16T02:56:20-0500" data-time="1713254180" data-date-string="Apr 16, 2024" data-time-string="2:56 AM" title="Apr 16, 2024 at 2:56 AM" itemprop="datePublished">Apr 16, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7078531/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #5 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/weirdoguy.464738/"> <meta itemprop="url" content="https://www.physicsforums.com/members/weirdoguy.464738/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="464738"><span itemprop="name">weirdoguy</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Mountain</h5>--> <!----> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,167</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>1,123</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7078531" data-lb-caption-desc="weirdoguy · Apr 16, 2024 at 2:56 AM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper"><blockquote data-attributes="member: 551353" data-quote="kodama" data-source="post: 7078515" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> kodama said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> what do you think </div> </div> </blockquote><br /> What do <b>you</b> think?</div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="3" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList is-active"> <ul class="reactionSummary"> <li><span class="reaction reaction--small reaction--1" data-reaction-id="1"><i aria-hidden="true"></i><img src="data:image/gif;base64,R0lGODlhAQABAIAAAAAAAP///yH5BAEAAAAALAAAAAABAAEAAAIBRAA7" class="reaction-sprite js-reaction" alt="Like" title="Like" /></span></li> </ul> <span class="u-srOnly">Likes</span> <bdi>ohwilleke</bdi>, <bdi>berkeman</bdi> and <bdi>pines-demon</bdi> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="ohwilleke" data-content="post-7078727" id="js-post-7078727" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7078727/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7078727"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-04-16T14:50:56-0500" data-time="1713297056" data-date-string="Apr 16, 2024" data-time-string="2:50 PM" title="Apr 16, 2024 at 2:50 PM" itemprop="datePublished">Apr 16, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7078727/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #6 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/ohwilleke.19562/"> <meta itemprop="url" content="https://www.physicsforums.com/members/ohwilleke.19562/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="19562"><span itemprop="name">ohwilleke</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Ocean</h5>--> <!----> <!-- Start Member Achievements --> <div class="post-badges"> <div class="post-badge badge-star" data-xf-init="tooltip" title="Click to Support PF"> <i class="fa--xf fal fa-star" aria-hidden="true"></i><span> Gold Member</span> </div> </div> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>2,578</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>1,530</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7078727" data-lb-caption-desc="ohwilleke · Apr 16, 2024 at 2:50 PM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper"><blockquote data-attributes="member: 551353" data-quote="kodama" data-source="post: 7078515" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> kodama said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> what do you think of strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA*as a way to test quantum gravity effects ? </div> </div> </blockquote>It is a great and obvious way to test quantum gravity effects, once you have the telescopes (defined broadly to include anything that makes an astronomy observation) to do it. Since they are, by definition, at the heart of these galaxies, however, sifting through the foregrounds to observe what you really want to see is challenging.<br /> <blockquote data-attributes="member: 551353" data-quote="kodama" data-source="post: 7078515" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> kodama said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> does string theory make any predictions of strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA*? </div> </div> </blockquote>String theory makes no predictions and has no observational support. It isn't really even really a theory so much as an approach to come up with a theory that no one has managed to set forth yet.<br /> <blockquote data-attributes="member: 551353" data-quote="kodama" data-source="post: 7078515" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> kodama said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> could quantum gravity effects show up as strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA* </div> </div> </blockquote>Yes.</div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> <div class="message-lastEdit"> Last edited: <time class="u-dt" dir="auto" datetime="2024-04-16T16:28:37-0500" data-time="1713302917" data-date-string="Apr 16, 2024" data-time-string="4:28 PM" title="Apr 16, 2024 at 4:28 PM" itemprop="dateModified">Apr 16, 2024</time> </div> </div> <footer class="message-footer"> <div 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itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7078790/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7078790"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-04-16T20:45:31-0500" data-time="1713318331" data-date-string="Apr 16, 2024" data-time-string="8:45 PM" title="Apr 16, 2024 at 8:45 PM" itemprop="datePublished">Apr 16, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7078790/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #7 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7078790" data-lb-caption-desc="kodama · Apr 16, 2024 at 8:45 PM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper"><blockquote data-attributes="member: 19562" data-quote="ohwilleke" data-source="post: 7078727" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> ohwilleke said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> It is a great and obvious way to test quantum gravity effects, once you have the telescopes (defined broadly to include anything that makes an astronomy observation) to do it. Since they are, by definition, at the heart of these galaxies, however, sifting through the foregrounds to observe what you really want to see is challenging.<br /> <br /> String theory makes no predictions and has no observational support. It isn't really even really a theory so much as an approach to come up with a theory that no one has managed to set forth yet.<br /> <br /> Yes. </div> </div> </blockquote><br /> this<br /> arXiv:2305.04336 (gr-qc)<br /> [Submitted on 7 May 2023 (v1), last revised 30 Oct 2023 (this version, v2)]<br /> Strong Gravitational Lensing by Loop Quantum Gravity Motivated Rotating Black Holes and EHT Observations<br /> Jitendra Kumar, Shafqat Ul Islam, Sushant G. Ghosh<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> We estimate the time delay between the first and second relativistic images using twenty supermassive galactic centre black holes as lenses. Our analysis concludes that, within the 1σ region, a significant portion of the BH-I and BH-II and for a small portion of BH-III parameter space agrees with the EHT results of M87* and Sgr A* whereas NH is completely ruled out. We discover that the EHT results of Sgr A* place more stringent limits on the parameter space of LMRBH black holes than those established by the EHT results of M87*. </div> </div> </blockquote><br /> . Our analysis concludes that, within the 1σ region, perhaps 5σ might be measured in more advanced degree with better quality telescopes<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> String theory makes no predictions and has no observational support. It isn't really even really a theory so much as an approach to come up with a theory that no one has managed to set forth yet. </div> </div> </blockquote><br /> String theory predicts massless spin 2, identify with the gravitons<br /> <br /> gravitons in qft is a type of quantum gravity<br /> <br /> does gravitons spin 2 in qft or super gravity quantum gravity effects show up as strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA*?<br /> <br /> <br /> if successful loop quantum gravity theory 5σ quantum gravity effects show up as strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA* could other quantum gravity theory reproduce the same results</div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> <div class="message-lastEdit"> Last edited: <time class="u-dt" dir="auto" datetime="2024-04-16T20:55:10-0500" data-time="1713318910" data-date-string="Apr 16, 2024" data-time-string="8:55 PM" title="Apr 16, 2024 at 8:55 PM" itemprop="dateModified">Apr 16, 2024</time> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList is-active"> <ul class="reactionSummary"> <li><span class="reaction reaction--small reaction--5" data-reaction-id="5"><i aria-hidden="true"></i><img src="data:image/gif;base64,R0lGODlhAQABAIAAAAAAAP///yH5BAEAAAAALAAAAAABAAEAAAIBRAA7" class="reaction-sprite js-reaction" alt="Sad" title="Sad" /></span></li> </ul> <span class="u-srOnly">Likes</span> <bdi>weirdoguy</bdi> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="kodama" data-content="post-7080508" id="js-post-7080508" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7080508/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7080508"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-04-22T09:01:45-0500" data-time="1713794505" data-date-string="Apr 22, 2024" data-time-string="9:01 AM" title="Apr 22, 2024 at 9:01 AM" itemprop="datePublished">Apr 22, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7080508/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #8 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7080508" data-lb-caption-desc="kodama · Apr 22, 2024 at 9:01 AM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper">arXiv:2404.12811 (gr-qc)<br /> [Submitted on 19 Apr 2024]<br /> Black Hole shadows of α′-corrected black holes<br /> F. Agurto-Sepúlveda, J. Oliva, M. Oyarzo, D.R.G Schleicher<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> In this paper we study the qualitative features induces by corrections to GR coming from String Theory, on the shadows of rotating black holes. We deal with the slowly rotating black hole solutions up to order O(a3), to first order in α′, including also the dilaton. We provide a detailed characterization of the geometry, as well as the ISCO and photon ring, and then we proceed to obtain the black hole images within the relativistic thin-disk model. We characterize the images by computing the diameter, displacement and asymmetry. A comparison with the Kerr case, indicates that all these quantities grow due to the α′ correction, and that the departure from GR for different observable is enhanced depending on the angle of view, namely for the diameter the maximum departure is obtained when the system is face-on, while for the displacement and asymmetry the departure from GR is maximized for edge-on point of view.<br /> <br /> Comments: 14 pages, 8 figures<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics - Theory (hep-th)<br /> Cite as: arXiv:2404.12811 [gr-qc]<br /> (or arXiv:2404.12811v1 [gr-qc] for this version) </div> </div> </blockquote><br /> "corrections to GR coming from String Theory, on the shadows of rotating black holes" vs "gravitational lensing in the strong deflection regime by loop quantum gravity (LQG)-motivated rotating black hole"<br /> <br /> "In this paper, we calculate the strong/weak gravitational lensing effects under the quantum-corrected black hole model, taking the supermassive black holes M87* and SgrA* as the subjects of study to explore the impact of the quantum correction parameter α on the positions of images and the Einstein ring."<br /> <br /> vs<br /> "In this paper we study the qualitative features induces by corrections to GR coming from String Theory, on the shadows of rotating black holes. We deal with the slowly rotating black hole solutions up to order O(a3), to first order in α′, including also the dilaton. We provide a detailed characterization of the geometry, as well as the ISCO and photon ring,"<br /> <br /> similar to lqg<br /> both papers on quantum corrections to GR , on the shadows of rotating black holes<br /> <br /> would be interested to compare quantum corrections to GR coming from String Theory, on the shadows of rotating black holes with loop quantum gravity (LQG)-motivated rotating black hole strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA* with real world observations</div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> <div class="message-lastEdit"> Last edited: <time class="u-dt" dir="auto" datetime="2024-04-22T13:33:57-0500" data-time="1713810837" data-date-string="Apr 22, 2024" data-time-string="1:33 PM" title="Apr 22, 2024 at 1:33 PM" itemprop="dateModified">Apr 22, 2024</time> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" 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class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-04-22T09:41:37-0500" data-time="1713796897" data-date-string="Apr 22, 2024" data-time-string="9:41 AM" title="Apr 22, 2024 at 9:41 AM" itemprop="datePublished">Apr 22, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7080525/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #9 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/vanadium-50.110252/"> <meta itemprop="url" content="https://www.physicsforums.com/members/vanadium-50.110252/" /> <div class="message-userDetails"> <span class="message-name"><a href="/members/vanadium-50.110252/" class="username " dir="auto" data-user-id="110252" data-xf-init="member-tooltip"><span itemprop="name">Vanadium 50</span></a></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Universe</h5>--> <!----> <!-- Start Member Achievements --> <div class="post-badges"> <div class="post-badge badge-shield" data-xf-init="tooltip" title="Retired Mentor"> <i class="fa--xf fal fa-shield" aria-hidden="true" style="font-size:12px;color:#990033;"></i><span> Staff Emeritus</span> </div> <div class="post-badge badge-university" data-xf-init="tooltip" title="Verified Expert in Science and Math"> <i class="fa--xf fal fa-university" aria-hidden="true"></i><span> Science Advisor</span> </div> <div class="post-badge badge-book" data-xf-init="tooltip" title="Verified Expert in Academia"> <i class="fa--xf fal fa-book" aria-hidden="true"></i><span> Education Advisor</span> </div> </div> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>35,001</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>21,677</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7080525" data-lb-caption-desc="Vanadium 50 · Apr 22, 2024 at 9:41 AM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper"><blockquote data-attributes="member: 551353" data-quote="kodama" data-source="post: 7080508" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> kodama said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> similar to lqg </div> </div> </blockquote>In that both can be printed on A4 paper, yes.<br /> <br /> You keep pointing us to papers that do not say what you say they do. You did it with the X17 and you're doing it now. It is more than a little annoying.</div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="1" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList is-active"> <ul class="reactionSummary"> <li><span class="reaction reaction--small reaction--1" data-reaction-id="1"><i aria-hidden="true"></i><img src="data:image/gif;base64,R0lGODlhAQABAIAAAAAAAP///yH5BAEAAAAALAAAAAABAAEAAAIBRAA7" class="reaction-sprite js-reaction" alt="Like" title="Like" /></span></li> </ul> <span class="u-srOnly">Likes</span> <bdi>ShadowKraz</bdi> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="kodama" data-content="post-7080728" id="js-post-7080728" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7080728/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7080728"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-04-22T21:29:16-0500" data-time="1713839356" data-date-string="Apr 22, 2024" data-time-string="9:29 PM" title="Apr 22, 2024 at 9:29 PM" itemprop="datePublished">Apr 22, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7080728/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #10 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7080728" data-lb-caption-desc="kodama · Apr 22, 2024 at 9:29 PM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper">of interest <br /> <br /> arXiv:2403.09756 (gr-qc)<br /> [Submitted on 14 Mar 2024 (v1), last revised 21 Apr 2024 (this version, v2)]<br /> Signatures of the accelerating black holes with a cosmological constant from the Sgr~A⋆ and M87⋆ shadow prospects<br /> L. Chakhchi, H. El Moumni, K. Masmar<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> Recently, the Event Horizon Telescope (EHT) achieved the realization of an image of the supermassive black hole Sgr~A⋆ showing an angular shadow diameter D=48.7±7μas and the fractional deviation δ=−0.08+0.09−0.09 (VLTI),−0.04+0.09−0.10 (Keck), alongside the earlier image of M87⋆ with angular diameter D=42±3μas, deviation δ=−0.01+0.17−0.17 and deviations from circularity estimated to be ΔC≲10%. In addition, the shadow radii are assessed within the ranges 3.38≤rsM≤6.91 for M87⋆ and 3.85≤rsM≤5.72 as well as 3.95≤rsM≤5.92 for Sgr~A⋆ using the Very Large Telescope Interferometer (VLTI) and Keck observatories, respectively. These values are provided with 1-σ and 2-σ measurements. Such realizations can unveil a better comprehension of gravitational physics at the horizon scale. In this paper, we use the EHT observational results for M87⋆ and Sgr~A⋆ to elaborate the constraints on parameters of accelerating black holes with a cosmological constant. Concretely, we utilize the mass and distance of both black holes to derive the observables associated with the accelerating black hole shadow. First, we compare our findings with observed quantities such as angular diameter, circularity, shadow radius, and the fractional deviation from the M87⋆ data. This comparison reveals constraints within the acceleration parameter and the cosmological constant...<br /> Lastly, one cannot rule out the possibility of the negative values for the cosmological constant on the emergence of accelerated black hole solutions within the context of minimal gauged supergravity... <br /> <br /> Comments: 37 pages, 10 figures, references updated<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics - Theory (hep-th)<br /> Cite as: arXiv:2403.09756 [gr-qc]<br /> (or arXiv:2403.09756v2 [gr-qc] for this version)<br /> <br /> <a href="https://doi.org/10.48550/arXiv.2403.09756" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.48550/arXiv.2403.09756</a><br /> Journal reference: Physics of the Dark Universe 44 (2024) 101501<br /> Related DOI: <br /> <a href="https://doi.org/10.1016/j.dark.2024.101501" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.1016/j.dark.2024.101501</a> </div> </div> </blockquote></div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList "> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="ShadowKraz" data-content="post-7094406" id="js-post-7094406" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7094406/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7094406"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-06-07T11:35:04-0500" data-time="1717778104" data-date-string="Jun 7, 2024" data-time-string="11:35 AM" title="Jun 7, 2024 at 11:35 AM" itemprop="datePublished">Jun 7, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7094406/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #11 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/shadowkraz.747904/"> <meta itemprop="url" content="https://www.physicsforums.com/members/shadowkraz.747904/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="747904"><span itemprop="name">ShadowKraz</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Quark</h5>--> <!----> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>54</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>32</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7094406" data-lb-caption-desc="ShadowKraz · Jun 7, 2024 at 11:35 AM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper"><blockquote data-attributes="member: 110252" data-quote="Vanadium 50" data-source="post: 7080525" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> Vanadium 50 said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> In that both can be printed on A4 paper, yes.<br /> <br /> You keep pointing us to papers that do not say what you say they do. You did it with the X17 and you're doing it now. It is more than a little annoying. </div> </div> </blockquote>It seems the OP is more confused, possibly on a higher level, about these things than I am.</div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList "> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="kodama" data-content="post-7114440" id="js-post-7114440" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7114440/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7114440"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-08-21T22:00:56-0500" data-time="1724295656" data-date-string="Aug 21, 2024" data-time-string="10:00 PM" title="Aug 21, 2024 at 10:00 PM" itemprop="datePublished">Aug 21, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7114440/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #12 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7114440" data-lb-caption-desc="kodama · Aug 21, 2024 at 10:00 PM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper">arXiv:2408.11603 [pdf, html, other]<br /> Gravitational lensing effect of black holes in effective quantum gravity<br /> Hao Liu, Meng-Yun Lai, Xiao-Yin Pan, Hyat Huang, De-Cheng Zou<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc) <br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> In the present work, we investigate the gravitational lensing effects of two quantum-modified black hole models recently proposed in effective quantum gravity. The light deflection angles in both the weak field limit and the strong field limit are calculated. Furthermore, we use the data of the supermassive black holes SgrA* and M87* and calculate the lensing observables in the strong field limit. We find that the quantum parameter plays a role analogous to the electric charge in the weak gravitational lensing, whereas in the strong field limit, the effect of the quantum parameter on the deflection angle, the angular separation and the relative magnification is opposite to that of the electric charge, the scalar charge and the quantum parameters in some gravity theories. The results indicate the discrepancies between the classical black holes and the two quantum-modified black hole models that depend on the quantum correction, making them a valuable tool for differentiating between these black hole models. </div> </div> </blockquote></div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList "> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="kodama" data-content="post-7118520" id="js-post-7118520" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7118520/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7118520"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-09-09T23:33:28-0500" data-time="1725942808" data-date-string="Sep 9, 2024" data-time-string="11:33 PM" title="Sep 9, 2024 at 11:33 PM" itemprop="datePublished">Sep 9, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7118520/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #13 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7118520" data-lb-caption-desc="kodama · Sep 9, 2024 at 11:33 PM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper">Submitted on 9 Sep 2024]<br /> Gravitational lensing and shadows from thin-disks in Loop Quantum Gravity self-dual black holes<br /> David J. Patiño Pomares, Diego Rubiera-Garcia<br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> We analyze gravitational lensing and their cast images from thin-disks in shadow observations of a family of spherically symmetric black hole solutions previously derived within the framework of Loop Quantum Gravity. Such black holes depend on two parameters (besides the mass of the black hole itself), P and a0, the latter imbuing the configurations with an interior wormhole structure. Using the bounds from the Event Horizon Telescope regarding the shadow's radius of Sgr A∗ that constrain the parameter P≲0.08(2σ) (at a0=0), we study the modifications to weak and strong gravitational lensing induced by these geometries as compared to the Schwarzschild black hole within this range. In particular, we discuss several observables in the strong field regime related to the luminosity decay, the angular separation, and the flux ratio between multiples images of the source. Furthermore, we consider the cast images of these black holes when illuminated by a geometrically and optically thin accretion disk according to several semi-analytic profiles for the disk's emission. <br /> <br /> Comments: 12 pages, 6 figures<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc)<br /> Cite as: arXiv:2409.05371 [gr-qc]<br /> (or arXiv:2409.05371v1 [gr-qc] for this version)<br /> <br /> <a href="https://doi.org/10.48550/arXiv.2409.05371" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.48550/arXiv.2409.05371</a> </div> </div> </blockquote></div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList "> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="kodama" data-content="post-7118789" id="js-post-7118789" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7118789/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7118789"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-09-11T14:09:02-0500" data-time="1726081742" data-date-string="Sep 11, 2024" data-time-string="2:09 PM" title="Sep 11, 2024 at 2:09 PM" itemprop="datePublished">Sep 11, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7118789/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #14 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7118789" data-lb-caption-desc="kodama · Sep 11, 2024 at 2:09 PM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper">arXiv:2409.05897 (gr-qc)<br /> [Submitted on 5 Sep 2024]<br /> Gravitational lensing in holonomy corrected spherically symmetric black holes with phantom global monopoles<br /> Faizuddin Ahmed<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> In this paper, we address a theoretical investigation of the gravitational lensing phenomenon within the space-time framework of a holonomy-corrected spherically symmetric black hole (BH), incorporating both ordinary and phantom global monopoles. Our focus lies on the analysis of null geodesics within this black hole background, examining the influence of ordinary and phantom global monopoles on the effective potential of null geodesics of the system. Afterwards, we derive analytical expressions for the deflection angle of photon light, considering weak field limit. The obtain expressions are presented up to the second order of the Loop Quantum Gravity parameter, enabling a thorough examination of the impact of ordinary and phantom global monopoles on the deflection angle. <br /> <br /> Comments: 12 pages, 3 figures, accepted in IJGMMP (this https URL)<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc)<br /> Cite as: arXiv:2409.05897 [gr-qc]<br /> (or arXiv:2409.05897v1 [gr-qc] for this version)<br /> <br /> <a href="https://doi.org/10.48550/arXiv.2409.05897" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.48550/arXiv.2409.05897</a> </div> </div> </blockquote></div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" content="https://schema.org/LikeAction" /> </div> <div class="reactionsBar js-reactionsList "> </div> <div class="js-historyTarget message-historyTarget toggleTarget" data-href="trigger-href"></div> </footer> </div> </div> </div> </article> <!-- RSS here --> <article class="message message--post js-post js-inlineModContainer " data-author="kodama" data-content="post-7119049" id="js-post-7119049" itemscope itemtype="https://schema.org/Comment" itemid="https://www.physicsforums.com/posts/7119049/"> <meta itemprop="parentItem" itemscope itemid="https://www.physicsforums.com/threads/two-recent-tests-of-loop-quantum-gravity-theory.1061460/" /> <span class="u-anchorTarget" id="post-7119049"></span> <div class="message-header"> <header class="message-attribution message-attribution--split"> <ul class="message-attribution-main listInline "> <li class="u-concealed"> <time class="u-dt" dir="auto" datetime="2024-09-12T22:22:52-0500" data-time="1726197772" data-date-string="Sep 12, 2024" data-time-string="10:22 PM" title="Sep 12, 2024 at 10:22 PM" itemprop="datePublished">Sep 12, 2024</time> </li> </ul> <ul class="message-attribution-opposite message-attribution-opposite--list "> <li> <span style="cursor:pointer;" data-xf-init="share-tooltip" data-href="/posts/7119049/share" aria-label="Share" role="button" rel="nofollow"> <i class="fa--xf fal fa-share-alt" aria-hidden="true"></i> </span> </li> <li> #15 </li> </ul> </header> </div> <div class="message-inner"> <div class="message-cell message-cell--user"> <section class="message-user" itemprop="author" itemscope itemtype="https://schema.org/Person" itemid="https://www.physicsforums.com/members/kodama.551353/"> <meta itemprop="url" content="https://www.physicsforums.com/members/kodama.551353/" /> <div class="message-userDetails"> <span class="message-name"><span class="username " dir="auto" data-user-id="551353"><span itemprop="name">kodama</span></span></span> <!--<h5 class="userTitle message-userTitle" dir="auto" itemprop="jobTitle">A PF Cell</h5>--> <!----> <span class="threadstarter" data-xf-init="tooltip" title="Thread Starter"><i class="fal fa-user-edit"></i></span> <!-- Start Member Achievements --> <!-- End Member Achievements --> </div> <div class="message-userExtras"> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-comments fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Messages"></i></dt> <dd>1,026</dd> </dl> <dl class="pairs pairs--justified"> <dt><i class="fa--xf fal fa-thumbs-up fa-fw" aria-hidden="true" data-xf-init="tooltip" title="Reaction score"></i></dt> <dd>139</dd> </dl> </div> <span class="message-userArrow"></span> </section> </div> <div class="message-cell message-cell--main"> <div class="message-main js-quickEditTarget"> <div class="message-content js-messageContent"> <div class="message-userContent lbContainer js-lbContainer " data-lb-id="post-7119049" data-lb-caption-desc="kodama · Sep 12, 2024 at 10:22 PM"> <article class="message-body js-selectToQuote"> <div itemprop="text"> <div class="bbWrapper">Submitted on 12 Sep 2024]<br /> Probing Quantum Gravity Effects with Eccentric Extreme Mass-Ratio Inspirals<br /> Guoyang Fu, Yunqi Liu, Bin Wang, Jian-Pin Wu, Chao Zhang<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> In this paper, we investigate the impact of loop quantum gravity (LQG) on extreme mass-ratio inspirals (EMRIs), and the results indicate that LQG effects cause the orbital decay to occur faster compared to the Schwarzschild case. Furthermore, we use the augmented analytic kludge approach to generate EMRI waveforms and study the LISA's capability to detect the LQG effect with faithfulness. Additionally, employing the Fisher information matrix method for parameter estimation, we estimate that after one year of observation, the uncertainty in r0 reduces to approximately 6.59×10−4 with a signal-to-noise ratio of 49. <br /> <br /> Comments: 22 pages,7 figures<br /> Subjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th)<br /> Cite as: arXiv:2409.08138 [gr-qc]<br /> (or arXiv:2409.08138v1 [gr-qc] for this version)<br /> <br /> <a href="https://doi.org/10.48550/arXiv.2409.08138" target="_blank" class="link link--external" rel="nofollow ugc noopener">https://doi.org/10.48550/arXiv.2409.08138</a> </div> </div> </blockquote></div> </div> <div class="js-selectToQuoteEnd"> </div> </article> </div> </div> <footer class="message-footer"> <div class="message-microdata" itemprop="interactionStatistic" itemtype="https://schema.org/InteractionCounter" itemscope> <meta itemprop="userInteractionCount" content="0" /> <meta itemprop="interactionType" 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In this paper, we calculate the strong/weak gravitational lensing effects under the quantum-corrected black hole model, taking the supermassive black holes M87* and SgrA* as the subjects of study to explore the impact of the quantum correction parameter \u03b1 on the positions of images and the Einstein ring. Our calculations show that in the case of strong gravitational lensing, the lensing coefficient a\u00af increases with an increase in the quantum correction parameter, while the deflection angle and the lensing coefficient b\u00af decrease with an increase in the quantum correction parameter. The quantum correction parameter \u03b1 has a significant impact in the context of supermassive black holes. In weak gravitational lensing, the quantum correction parameter \u03b1 plays a suppressive role. Our theoretical analysis suggests that with advancements in future astrophysical observation techniques, it might be possible to test loop quantum gravity theory using the gravitational lensing effect.\n\nSubjects: General Relativity and Quantum Cosmology (gr-qc)\nCite as: arXiv:2403.18606 [gr-qc]\n (or arXiv:2403.18606v1 [gr-qc] for this version)\n\n\nhttps://doi.org/10.48550/arXiv.2403.18606\n\nand\n\n [Submitted on 7 Dec 2023 (v1), last revised 28 Dec 2023 (this version, v2)]\nShadows of Loop Quantum Black Holes: Semi-analytical Simulations of Loop Quantum Gravity Effects on Sagittarius A* and M 87*\nHong-Xuan Jiang, Cheng Liu, Indu K. Dihingia, Yosuke Mizuno, Haiguang Xu, Tao Zhu, Qiang Wu\n\n\nIn this study, we delve into the observational implications of rotating Loop Quantum Black Holes (LQBHs) within an astrophysical framework. We employ semi-analytical General Relativistic Radiative Transfer (GRRT) computations to study the emission from the accretion flow around LQBHs. Our findings indicate that the increase of Loop Quantum Gravity (LQG) effects results in an enlargement of the rings from LQBHs, thereby causing a more circular polarization pattern in the shadow images. We make comparisons with the Event Horizon Telescope (EHT) observations of Sgr\\,A\u2217 and M\\,87\u2217, which enable us to determine an upper limit for the polymetric function P in LQG. The upper limit for Sgr\\,A\u2217 is 0.2, while for M\\,87\u2217 it is 0.07. Both black holes exhibit a preference for a relatively high spin (a\u22730.5 for Sgr\\,A\u2217 and 0.5\u2272a\u22720.7 for M\\,87\u2217). The constraints for Sgr\\,A\u2217 are based on black hole spin and ring diameter, whereas for M\\,87\u2217, the constraints are further tightened by the polarimetric pattern. In essence, our simulations provide observational constraints on the effect of LQG in supermassive black holes (SMBH), providing the most consistent comparison with observation.\nSubjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Astrophysical Phenomena (astro-ph.HE)\nCite as: arXiv:2312.04288 [gr-qc]\n (or arXiv:2312.04288v2 [gr-qc] for this version)\n\n\nhttps://doi.org/10.48550/arXiv.2312.04288\n\nand\n\n arXiv:2305.04336 (gr-qc)\n[Submitted on 7 May 2023 (v1), last revised 30 Oct 2023 (this version, v2)]\nStrong Gravitational Lensing by Loop Quantum Gravity Motivated Rotating Black Holes and EHT Observations\nJitendra Kumar, Shafqat Ul Islam, Sushant G. Ghosh\n We investigate gravitational lensing in the strong deflection regime by loop quantum gravity (LQG)-motivated rotating black hole (LMRBH) metrics with an additional parameter l besides mass M and rotation a. The LMRBH spacetimes are regular everywhere, asymptotically encompassing the Kerr black hole as a particular case and, depending on the parameters, describe black holes with one horizon only (BH-I), black holes with an event horizon and a Cauchy horizon (BH-II), black holes with three horizons (BH-III), or black holes with no horizons (NH) spacetime. It turns out that as the LQG parameter l increases, the unstable photon orbit radius xps, the critical impact parameter ups, the deflection angle \u03b1D(\u03b8) and angular position \u03b8\u221e also increases. Meanwhile, the angular separation s decreases, and relative magnitude rmag increases with increasing l for prograde motion but they show opposite behaviour for the retrograde motion. For Sgr A*, the angular position \u03b8\u221e is \u2208 (16.4, 39.8) \u03bcas, while for M87* \u2208 (12.33, 29.9) \u03bcas. The angular separation s, for SMBHs Sgr A* and M87*, differs significantly, with values ranging \u2208 (0.008-0.376) \u03bcas for Sgr A* and \u2208 (0.006-0.282) \u03bcas for M87*. We estimate the time delay between the first and second relativistic images using twenty supermassive galactic centre black holes as lenses. Our analysis concludes that, within the 1\u03c3 region, a significant portion of the BH-I and BH-II and for a small portion of BH-III parameter space agrees with the EHT results of M87* and Sgr A* whereas NH is completely ruled out. We discover that the EHT results of Sgr A* place more stringent limits on the parameter space of LMRBH black holes than those established by the EHT results of M87*. \n\nComments: 16 Pages, 11 Figures, 3 Tables, Accepted for publication in EPJC\nSubjects: General Relativity and Quantum Cosmology (gr-qc); Astrophysics of Galaxies (astro-ph.GA)\nCite as: arXiv:2305.04336 [gr-qc]\n (or arXiv:2305.04336v2 [gr-qc] for this version) \n\nand \n\n arXiv:2302.10482 (gr-qc)\n[Submitted on 21 Feb 2023 (v1), last revised 29 Apr 2023 (this version, v2)]\nObservational tests of quantum extension of Schwarzschild spacetime in loop quantum gravity with stars in the galactic center\nJian-Ming Yan, Cheng Liu, Tao Zhu, Qiang Wu, Anzhong Wang\n \n\n In this paper, we use the publicly available observational data of 17 stellar stars orbiting Sgr A* to test the quantum extension of Schwarzschild spacetime in loop quantum gravity (LQG). For our purpose, we transform the geodesical evolution of a massive particle in the quantum-extended Schwarzschild black hole to the perturbed Kepler problem and calculate the effects of LQG on the pericentre advance of the stellar stars. With these effects, one is able to compare them with the publicly available astrometric and spectroscopic data of stellar stars in the galactic center. We perform Monte Carlo Markov Chain (MCMC) simulations to probe the possible LQG effects on the orbit of S-stars. No significant evidence of the quantum-extended Schwarzschild black hole from LQG is found. Among the posterior analyses of 17 S-stars, the result of S2 gives the strongest bound on the LQG parameter A\u03bb, which places an upper bound at 95\\% confidence level on A\u03bb to be A\u03bb<0.302. \n\nComments: 12 pages, 6 figures\nSubjects: General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th)\nCite as: arXiv:2302.10482 [gr-qc]\n (or arXiv:2302.10482v2 [gr-qc] for this version)\n \nhttps://doi.org/10.48550/arXiv.2302.10482\nJournal reference: Phys. Rev. D 107, 084043 (2023)\nRelated DOI: \nhttps://doi.org/10.1103/PhysRevD.107.084043\n\n\n\n arXiv:2403.17197 (hep-th)\n[Submitted on 25 Mar 2024]\nLoop Quantum Gravity effects on electromagnetic properties of charged leptons\nJo\u00e3o Paulo S. Melo, Mario J. Neves, Jefferson M. A. Paix\u00e3o, Jos\u00e9 A. Helay\u00ebl-Neto\n\n\nThe efforts in this contribution consist in reassessing a modified Dirac equation that incorporates a \u03b30\u03b35-Lorentz-symmetry violating (LSV) term induced as a Loop Quantum Gravity (LQG) effect. Originally, this equation has been applied and considered as a good scenario for describing a number of investigations on the flight time of cosmic photons and neutrinos, which suggests that the speed of light in vacuum, in connection with the geometry that describes a granular space-time, takes an energy-dependent form, e.g., v(E)=1\u00b1E/ELSV, with ELSV\u22486,5\u00d71017 GeV for neutrinos. Once LQG provides a viable way to consistently understand this picture, we pursue an analysis of this effective Dirac equation to inspect some of its properties. These include: the derivation of the modified fermionic propagator, attainment of the Gordon decomposition of the vector current with minimal electromagnetic coupling to obtain information on the form factors, examination of the non-relativistic limit of the equation, evaluation of the spin- and velocity-dependent corrections to the Coulomb potential due to LQG effects, and the modified Hamiltonian in the low-relativistic regime. The study of the form factors may open up paths to set up bounds on the LQG parameters from the precision measurements of electromagnetic attributes of the charged leptons, such as their respective electric and magnetic dipole moments.\n\nComments: 11 pages, 2 figures\nSubjects: High Energy Physics - Theory (hep-th); High Energy Physics - Phenomenology (hep-ph)\nCite as: arXiv:2403.17197 [hep-th]\n (or arXiv:2403.17197v1 [hep-th] for this version))\n\n\nhttps://doi.org/10.48550/arXiv.2403.17197\n\nany comment on test loop quantum gravity theory on electromagnetic properties of charged leptons and via the Lensing Effect\n\nare those predictions the strong/weak gravitational lensing effects under the quantum-corrected black hole model, taking the supermassive black holes M87* and SgrA* as the subjects of study on unique to loop quantum gravity theory\nor\ncould string theory, SUGRA, semiclassical gravity also make predictions strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA* via the Lensing Effect\n\nwhat if observations of strong gravitational lensing, the lensing of supermassive black holes M87* and SgrA* confirm loop quantum gravity theory\n\nattributes of the charged leptons, such as their respective electric and magnetic dipole moments is something useful for connecting to experiment by electron EDM\n\nif loop quantum gravity theory on electromagnetic properties of charged leptons and via the Lensing Effect confirm by future experiment should Nobel Prize be awarded and loop quantum gravity theorywins over string theory ?" }, "publisher": { "@type": "Organization", "name": "Physics Forums: Science Discussion, Homework Help, Articles", "alternateName": "Physics Forums", "description": "Join Physics Forums, where students, scientists, and enthusiasts come together to explore and discuss the current understanding and practice of various scientific fields.", "url": "https://www.physicsforums.com", "logo": "https://www.physicsforums.com/styles/physicsforums/images/physics-forums-logo-og.png" } } </script> <script type="text/javascript" src="https://www.physicsforums.com/copyright.js" defer></script> <script> function parseNewPost(postid) { var newpost = document.getElementById("js-post-" + postid), npa = [newpost]; MathJax.typeset(npa); } function parsePreview() { var preview = document.getElementsByClassName("xfPreview"); MathJax.typeset(preview); } function parseNewConversationPost(postid) { var newpost = document.getElementsByClassName("convMessage-" + postid); MathJax.typeset(newpost); } function parseNewProfilePost(postid) { var newpost = document.getElementById("js-profilePost-" + postid), npa = [newpost]; MathJax.typeset(npa); } function parseTooltip() { MathJax.typeset(); } </script> </body> </html>