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It generally consists of two different metals immersed in electrolytes, or of individual half-cells with different metals and their ions in solution connected by a [[salt bridge]] or separated by a porous membrane. Volta was the inventor of the [[voltaic pile]], the first [[battery (electricity)|electrical battery]]. In common usage, the word "battery" has come to include a single galvanic cell, but a battery properly consists of multiple cells.<ref>[http://www.merriam-webster.com/dictionary/battery "battery" (def. 4b)], ''Merriam-Webster Online Dictionary'' (2008). Retrieved 6 August 2008.</ref>}} {{term|term=[[Gamma rays]]|content='''[[Gamma rays]]'''}}{{defn|defn=A gamma ray, or gamma radiation (symbol γ or <math>\gamma</math>), is a penetrating form of [[electromagnetic radiation]] arising from the [[radioactive decay]] of [[atomic nucleus|atomic nuclei]]. It consists of the shortest wavelength electromagnetic waves and so imparts the highest [[photon energy]].}} {{term|term=[[Gas]]|content='''[[Gas]]'''}}{{defn|defn=Is one of the [[state of matter|four fundamental states of matter]] (the others being [[solid]], [[liquid]], and [[plasma (physics)|plasma]]). A pure gas may be made up of individual [[atoms]] (e.g. a [[noble gas]] like [[neon]]), [[chemical element|elemental]] molecules made from one type of atom (e.g. [[oxygen]]), or [[chemical compound|compound]] molecules made from a variety of atoms (e.g. [[carbon dioxide]]). A gas [[mixture]], such as [[Earth's atmosphere|air]], contains a variety of pure gases. What distinguishes a gas from liquids and solids is the vast separation of the individual gas particles.}} {{term|term=[[Pressure measurement#Absolute, gauge and differential pressures — zero reference|Gauge pressure]]|content='''[[Pressure measurement#Absolute, gauge and differential pressures — zero reference|Gauge pressure]]'''}}{{defn|defn=Is zero-referenced against ambient air pressure, so it is equal to absolute pressure minus atmospheric pressure.}} {{term|term=[[Geiger counter]]|content='''[[Geiger counter]]'''}}{{defn|defn=Is an instrument used for detecting and measuring [[ionizing radiation]]. Also known as a ''Geiger–Muller counter'' (or ''Geiger–Müller counter''), it is widely used in applications such as radiation [[dosimetry]], [[radiological protection]], [[experimental physics]], and the [[nuclear industry]].}} {{term|term=[[General relativity]]|content='''[[General relativity]]'''}}{{defn|defn=General relativity, also known as the ''general theory of relativity'', is the [[differential geometry|geometric]] [[scientific theory|theory]] of [[gravitation]] published by [[Albert Einstein]] in 1915 and is the current description of gravitation in [[modern physics]]. General [[theory of relativity|relativity]] generalizes [[special relativity]] and refines [[Newton's law of universal gravitation]], providing a unified description of gravity as a geometric property of [[space]] and [[time in physics|time]] or [[four-dimensional]] [[spacetime]]. In particular, the ''{{vanchor|[[curvature]] of spacetime|Spacetime curvature|curvature of spacetime}}'' is directly related to the [[energy]] and [[momentum]] of whatever [[matter]] and [[radiation]] are present. The relation is specified by the [[Einstein field equations]], a system of [[partial differential equation]]s.}} {{term|term=[[Geometric mean]]|content='''[[Geometric mean]]'''}}{{defn|defn=In mathematics, the geometric mean is a [[mean]] or [[average]], which indicates the [[central tendency]] or typical value of a set of numbers by using the product of their values (as opposed to the [[arithmetic mean]] which uses their sum). The geometric mean is defined as the [[Nth root|{{math|''n''}}th root]] of the [[product (mathematics)|product]] of {{mvar|n}} numbers, i.e., for a set of numbers {{math|''x''<sub>1</sub>, ''x''<sub>2</sub>, ..., ''x<sub>n</sub>''}}, the geometric mean is defined as :<math>\left(\prod_{i=1}^n x_i\right)^\frac{1}{n}=\sqrt[n]{x_1 x_2 \cdots x_n}</math>}} {{term|term=[[Geometry]]|content='''[[Geometry]]'''}}{{defn|defn=Is, with [[arithmetic]], one of the oldest branches of [[mathematics]]. It is concerned with properties of space that are related with distance, shape, size, and relative position of figures.<ref name="Risi2015">{{cite book |author=Vincenzo De Risi |title=Mathematizing Space: The Objects of Geometry from Antiquity to the Early Modern Age |url=https://books.google.com/books?id=1m11BgAAQBAJ&pg=PA1 |date=31 January 2015 |publisher=Birkhäuser |isbn=978-3-319-12102-4 |pages=1–}}</ref> A mathematician who works in the field of geometry is called a [[list of geometers|geometer]].}} {{term|term=[[Geophysics]]|content='''[[Geophysics]]'''}}{{defn|defn=Is a subject of [[natural science]] concerned with the physical processes and [[physical property|physical properties]] of the [[Earth]] and its surrounding space environment, and the use of quantitative methods for their analysis. The term ''geophysics'' sometimes refers only to geological applications: Earth's [[figure of the Earth|shape]]; its [[gravitational]] and [[Earth's magnetic field|magnetic fields]]; its [[structure of the Earth|internal structure]] and [[Earth#Chemical composition|composition]]; its [[geodynamics|dynamics]] and their surface expression in [[plate tectonics]], the generation of [[magma]]s, [[volcanism]] and rock formation.<ref name=Sheriff1991>{{harvnb|Sheriff|1991}}</ref> However, modern geophysics organizations and pure scientists use a broader definition that includes the [[water cycle]] including snow and ice; [[geophysical fluid dynamics|fluid dynamics]] of the oceans and the [[atmosphere]]; [[atmospheric electricity|electricity]] and [[magnetism]] in the [[ionosphere]] and [[magnetosphere]] and solar–terrestrial relations; and analogous problems associated with the [[Moon]] and other planets.<ref name=Sheriff1991/><ref name=IUGG>{{harvnb|IUGG|2011}}</ref><ref name=AGUscience>{{harvnb|AGU|2011}}</ref><ref name="Gutenberg (1929)">Gutenberg, B., 1929, Lehrbuch der Geophysik. Leipzig. Berlin (Gebruder Borntraeger).</ref><ref name="Runcorn">Runcorn, S.K, (editor-in-chief), 1967, International dictionary of geophysics:. Pergamon, Oxford, 2 volumes, 1,728 pp., 730 fig</ref>}} {{term|term=[[Geotechnical engineering]]|content='''[[Geotechnical engineering]]'''}}{{defn|defn=Also known as ''geotechnics'', is the branch of [[civil engineering]] concerned with the engineering behavior of [[earth materials]]. It uses the principles and methods of [[soil mechanics]] and [[rock mechanics]] for the solution of [[engineering]] problems and the design of engineering works. It also relies on knowledge of [[geology]], [[hydrology]], [[geophysics]], and other related sciences.}} {{term|term=[[Gluon]]|content='''[[Gluon]]'''}}{{defn|defn=Is an [[elementary particle]] that acts as the exchange particle (or [[gauge boson]]) for the [[strong interaction|strong force]] between [[quark]]s. It is analogous to the exchange of [[photon]]s in the [[electromagnetic force]] between two [[charged particle]]s.<ref name=HyperPhysics>{{cite web |author=C.R. Nave |title=The Color Force |url=http://hyperphysics.phy-astr.gsu.edu/hbase/forces/color.html |work=[[HyperPhysics]] |publisher=[[Georgia State University]], Department of Physics |access-date=2012-04-02 }}</ref> In layman's terms, they "glue" quarks together, forming [[hadron]]s such as [[proton]]s and [[neutron]]s. In technical terms, gluons are [[vector boson|vector]] [[gauge boson]]s that mediate [[strong interaction]]s of [[quark]]s in [[quantum chromodynamics]] (QCD). Gluons themselves carry the [[color charge]] of the strong interaction. This is unlike the [[photon]], which mediates the [[electromagnetic force|electromagnetic interaction]] but lacks an electric charge. Gluons therefore participate in the strong interaction in addition to mediating it, making QCD significantly harder to analyze than [[quantum electrodynamics]] (QED).}} {{term|term=[[Graham's law]]|content='''[[Graham's law]]'''}}{{defn|defn=''Graham's law of effusion'' (also called ''Graham's law of [[diffusion]]'') was formulated by Scottish physical chemist [[Thomas Graham (chemist)|Thomas Graham]] in 1848.<ref name="LM">[[Keith J. Laidler]] and John M. Meiser, ''Physical Chemistry'' (Benjamin/Cummings 1982), pp.&nbsp;18–19</ref> Graham found experimentally that the rate of [[effusion]] of a gas is inversely proportional to the square root of the mass of its particles.<ref name="LM"/> This formula can be written as: :<math>{\mbox{Rate}_1 \over \mbox{Rate}_2}=\sqrt{M_2 \over M_1}</math>, where: :Rate<sub>1</sub> is the rate of effusion for the first gas. (volume or number of moles per unit time). :Rate<sub>2</sub> is the rate of effusion for the second gas. :''M<sub>1</sub>'' is the [[molar mass]] of gas 1 :''M<sub>2</sub>'' is the molar mass of gas 2.}} {{term|term=[[Gravitational constant]]|content='''[[Gravitational constant]]'''}}{{defn|defn=The gravitational constant (also known as the ''universal gravitational constant'', the ''Newtonian constant of gravitation'', or the ''Cavendish gravitational constant''),{{efn|"Newtonian constant of gravitation" is the name introduced for ''G'' by Boys (1894). Use of the term by T.E. Stern (1928) was misquoted as "Newton's constant of gravitation" in ''Pure Science Reviewed for Profound and Unsophisticated Students'' (1930), in what is apparently the first use of that term. Use of "Newton's constant" (without specifying "gravitation" or "gravity") is more recent, as "Newton's constant" was also used for the [[heat transfer coefficient]] in [[Newton's law of cooling]], but has by now become quite common, e.g. Calmet et al, ''Quantum Black Holes'' (2013), p. 93; P. de Aquino, ''Beyond Standard Model Phenomenology at the LHC'' (2013), p. 3. The name "Cavendish gravitational constant", sometimes "Newton–Cavendish gravitational constant", appears to have been common in the 1970s to 1980s, especially in (translations from) Soviet-era Russian literature, e.g. Sagitov (1970 [1969]), ''Soviet Physics: Uspekhi'' 30 (1987), Issues 1–6, p. 342 [etc.]. "Cavendish constant" and "Cavendish gravitational constant" is also used in Charles W. Misner, Kip S. Thorne, John Archibald Wheeler, "Gravitation", (1973), 1126f. Colloquial use of "Big G", as opposed to "[[little g]]" for gravitational acceleration dates to the 1960s (R.W. Fairbridge, ''The encyclopedia of atmospheric sciences and astrogeology'', 1967, p. 436; note use of "Big G's" vs. "little g's" as early as the 1940s of the [[Einstein tensor]] ''G''<sub>''μν''</sub> vs. the [[metric tensor]] ''g''<sub>''μν''</sub>, ''Scientific, medical, and technical books published in the United States of America: a selected list of titles in print with annotations: supplement of books published 1945–1948'', Committee on American Scientific and Technical Bibliography National Research Council, 1950, p. 26).|name=|group=}} denoted by the letter {{math|''G''}}, is an [[empirical]] [[physical constant]] involved in the calculation of [[gravitational]] effects in [[Sir Isaac Newton]]'s [[Newton's law of universal gravitation|law of universal gravitation]] and in [[Albert Einstein]]'s [[general relativity|general theory of relativity]].}} {{term|term=[[Gravitational energy]]|content='''[[Gravitational energy]]'''}}{{defn|defn=Gravitational energy or ''gravitational potential energy'' is the [[potential energy]] a [[mass]]ive object has in relation to another massive object due to [[gravity]]. It is the potential energy associated with the [[gravitational field]], which is released (converted into [[kinetic energy]]) when the objects [[free fall|fall]] towards each other. Gravitational potential energy increases when two objects are brought further apart. For two pairwise interacting point particles, the gravitational potential energy <math>U</math> is given by :<math>U=-\frac{GMm}{R},</math> where <math>M</math> and <math>m</math> are the masses of the two particles, <math>R</math> is the distance between them, and <math>G</math> is the [[gravitational constant]].<ref name=gpe>{{cite web |title=Gravitational Potential Energy |url=http://hyperphysics.phy-astr.gsu.edu/hbase/gpot.html |website=hyperphysics.phy-astr.gsu.edu |access-date=10 January 2017}}</ref> Close to the Earth's surface, the gravitational field is approximately constant, and the gravitational potential energy of an object reduces to :<math>U=mgh</math> where <math>m</math> is the object's mass, <math>g=GM_E/R_E^2</math> is the [[gravity of Earth]], and <math>h</math> is the height of the object's [[center of mass]] above a chosen reference level.<ref name=gpe/>}} {{term|term=[[Gravitational field]]|content='''[[Gravitational field]]'''}}{{defn|defn=In [[physics]], a gravitational field is a [[scientific model|model]] used to explain the influences that a massive body extends into the space around itself, producing a force on another massive body.<ref>{{cite book |author-link=Richard Feynman |first=Richard |last=Feynman |title=The Feynman Lectures on Physics |volume=I |publisher=Addison Wesley Longman |year=1970 |isbn=978-0-201-02115-8 |url=https://feynmanlectures.caltech.edu/I_07.html}}</ref> Thus, a gravitational [[field (physics)|field]] is used to explain [[gravity|gravitational]] phenomena, and is measured in [[newton (unit)|newtons]] per [[kilogram]] (N/kg). In its original concept, [[gravity]] was a [[force]] between point [[mass]]es. Following [[Isaac Newton]], [[Pierre-Simon Laplace]] attempted to model gravity as some kind of [[radiation]] field or [[fluid]], and since the 19th century, explanations for gravity have usually been taught in terms of a field model, rather than a point attraction. In a field model, rather than two particles attracting each other, the particles distort [[spacetime]] via their mass, and this distortion is what is perceived and measured as a "force".{{citation needed|date=August 2020}} In such a model one states that matter moves in certain ways in response to the curvature of spacetime,<ref>{{cite book |title=General Relativity from A to B |first1=Robert |last1=Geroch |publisher=[[University of Chicago Press]] |date=1981 |isbn=978-0-226-28864-2 |page=181 |url=https://books.google.com/books?id=UkxPpqHs0RkC&pg=PA181}} </ref> and that there is either ''no gravitational force'',<ref>{{cite book |title=Einstein's General Theory of Relativity: with Modern Applications in Cosmology |first1=Øyvind |last1=Grøn |first2=Sigbjørn |last2=Hervik |publisher=Springer Japan |date=2007 |isbn=978-0-387-69199-2 |page=256 |url=https://books.google.com/books?id=IyJhCHAryuUC&pg=PA256}} </ref> or that gravity is a [[fictitious force]].<ref>{{cite book |title=A Short Course in General Relativity |edition=3 |first1=J. |last1=Foster |first2=J. D. |last2=Nightingale |publisher=Springer Science & Business |date=2006 |isbn=978-0-387-26078-5 |page=55 |url=https://books.google.com/books?id=wtoKZODmoVsC&pg=PA55}} </ref> Gravity is distinguished from other forces by its obedience to the [[equivalence principle]].}} {{term|term=[[Gravitational potential]]|content='''[[Gravitational potential]]'''}}{{defn|defn=In [[classical mechanics]], the gravitational potential at a location is equal to the [[work (physics)|work]] ([[energy]] transferred) per unit mass that would be needed to move an object to that location from a fixed reference location. It is [[analogous]] to the [[electric potential]] with [[mass]] playing the role of [[charge (physics)|charge]]. The reference location, where the potential is zero, is by convention [[infinitely]] far away from any mass, resulting in a negative potential at any [[wikt:finite|finite]] distance. In mathematics, the gravitational potential is also known as the [[Newtonian potential]] and is fundamental in the study of [[potential theory]]. It may also be used for solving the electrostatic and magnetostatic fields generated by uniformly charged or polarized ellipsoidal bodies.<ref>{{cite book |title=Electrostatics and magnetostatics of polarized ellipsoidal bodies: the depolarization tensor method |first1=C.E. |last1=Solivérez |edition=1st English |year=2016 |publisher=Free Scientific Information |isbn=978-987-28304-0-3}}</ref>}} {{term|term=[[Gravitational wave]]|content='''[[Gravitational wave]]'''}}{{defn|defn=Gravitational waves are disturbances in the curvature of [[spacetime]], generated by accelerated masses, that [[wave propagation|propagate as waves]] outward from their source at the [[speed of light]]. They were proposed by [[Henri Poincaré]] in 1905<ref>{{cite web |title=Sur la dynamique de l'électron - Note de Henri Poincaré publiée dans les Comptes rendus de l'Académie des sciences de la séance du 5 juin 1905 - Membres de l'Académie des sciences depuis sa création |trans-title=On the dynamics of the electron - Note by Henri Poincaré published in the Reports of the Academy of Sciences of the session of June 5, 1905 - Members of the Academy of Sciences since its creation |url=https://www.academie-sciences.fr/pdf/dossiers/Poincare/Poincare_pdf/Poincare_CR1905.pdf |access-date=3 November 2023 |website=academie-sciences.fr |language=fr}}</ref> and subsequently [[#History|predicted in 1916]]<ref>{{cite journal |author=Einstein, A |title=Näherungsweise Integration der Feldgleichungen der Gravitation |date=June 1916 |url=http://einstein-annalen.mpiwg-berlin.mpg.de/related_texts/sitzungsberichte |journal=[[Prussian Academy of Sciences |Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften Berlin]] |volume=part 1 |pages=688–696 |bibcode=1916SPAW.......688E |access-date=2014-11-15 |archive-url=https://web.archive.org/web/20160115224321/http://einstein-annalen.mpiwg-berlin.mpg.de/related_texts/sitzungsberichte |archive-date=2016-01-15}}</ref><ref name="Gravitationswellen">{{cite journal |author=Einstein, A |title=Über Gravitationswellen |date=1918 |url=http://einstein-annalen.mpiwg-berlin.mpg.de/related_texts/sitzungsberichte |journal=Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften Berlin |volume=part 1 |pages=154–167 |bibcode=1918SPAW.......154E |access-date=2014-11-15 |archive-url=https://web.archive.org/web/20160115224321/http://einstein-annalen.mpiwg-berlin.mpg.de/related_texts/sitzungsberichte |archive-date=2016-01-15}}</ref> by [[Albert Einstein]] on the basis of his [[general relativity|general theory of relativity]].<ref>{{cite web |last=Finley |first=Dave |title=Einstein's gravity theory passes toughest test yet: Bizarre binary star system pushes study of relativity to new limits |url=http://phys.org/news/2013-04-einstein-gravity-theory-toughest-bizarre.html |publisher=Phys.Org}}</ref><ref>[http://www.dpf99.library.ucla.edu/session14/barish1412.pdf The Detection of Gravitational Waves using LIGO, B. Barish] {{webarchive|url=https://web.archive.org/web/20160303205650/http://www.dpf99.library.ucla.edu/session14/barish1412.pdf |date=2016-03-03}}</ref> Gravitational waves transport energy as ''gravitational radiation'', a form of [[radiant energy]] similar to [[electromagnetic radiation]].<ref>{{cite journal |title=On gravitational waves |journal=Journal of the Franklin Institute |date=January 1937 |last1=Einstein |first1=Albert |last2=Rosen |first2=Nathan |author2-link=Nathan Rosen |volume=223 |issue=1 |pages=43–54 |doi=10.1016/S0016-0032(37)90583-0 |bibcode=1937FrInJ.223...43E}}</ref> [[Newton's law of universal gravitation]], part of [[classical mechanics]], does not provide for their existence, since that law is predicated on the assumption that physical interactions propagate instantaneously (at infinite speed){{snd}}showing one of the ways the methods of classical physics are unable to explain phenomena associated with relativity.}} {{term|term=[[Gravity]]|content='''[[Gravity]]'''}}{{defn|defn=Or ''gravitation'', is a [[list of natural phenomena|natural phenomenon]] by which all things with [[mass]] or [[energy]]—including [[planet]]s, [[star]]s, [[galaxy|galaxies]], and even [[light]]<ref name="Comins">{{cite book |last1=Comins |first1=Neil F. |last2=Kaufmann |first2=William J. |title=Discovering the Universe: From the Stars to the Planets |publisher=MacMillan |date=2008 |page=347 |url=https://books.google.com/books?id=J1d9HJHlISkC&pg=PA347 |isbn=978-1-4292-3042-1 |bibcode=2009dufs.book.....C }}</ref>—are brought toward (or ''gravitate'' toward) one another. On [[Earth]], gravity gives [[weight]] to [[physical body|physical objects]], and the [[Moon]]'s [[gravitation of the Moon|gravity]] causes the ocean [[tide]]s. The gravitational attraction of the original gaseous matter present in the [[Universe]] caused it to begin [[coalescence (physics)|coalescing]] and [[star formation|forming stars]] and caused the stars to group together into galaxies, so gravity is responsible for many of the large-scale structures in the Universe. Gravity has an infinite range, although its effects become increasingly weaker as objects get further away.}} {{term|term=[[Ground state]]|content='''[[Ground state]]'''}}{{defn|defn=The ground state of a [[quantum mechanics|quantum-mechanical]] system is its lowest-[[energy]] [[stationary state|state]]; the energy of the ground state is known as the [[zero-point energy]] of the system. An [[excited state]] is any state with energy greater than the ground state. In [[quantum field theory]], the ground state is usually called the [[vacuum state]] or the [[vacuum#The quantum-mechanical vacuum|vacuum]].}} {{Glossary of engineering ToC}} {{Glossary end}} </textarea><div class="templatesUsed"></div><p id="mw-returnto">Return to <a href="/wiki/Glossary_of_engineering:_A%E2%80%93L" title="Glossary of engineering: A–L">Glossary of engineering: A–L</a>.</p> <noscript><img src="https://login.wikimedia.org/wiki/Special:CentralAutoLogin/start?type=1x1" alt="" width="1" height="1" style="border: none; position: absolute;"></noscript> <div class="printfooter" data-nosnippet="">Retrieved from "<a dir="ltr" href="https://en.wikipedia.org/wiki/Glossary_of_engineering:_A–L">https://en.wikipedia.org/wiki/Glossary_of_engineering:_A–L</a>"</div></div> <div id="catlinks" class="catlinks catlinks-allhidden" data-mw="interface"></div> </div> </main> </div> <div class="mw-footer-container"> <footer id="footer" class="mw-footer" > <ul id="footer-info"> </ul> <ul id="footer-places"> <li id="footer-places-privacy"><a href="https://foundation.wikimedia.org/wiki/Special:MyLanguage/Policy:Privacy_policy">Privacy policy</a></li> <li id="footer-places-about"><a href="/wiki/Wikipedia:About">About Wikipedia</a></li> <li id="footer-places-disclaimers"><a href="/wiki/Wikipedia:General_disclaimer">Disclaimers</a></li> <li id="footer-places-contact"><a href="//en.wikipedia.org/wiki/Wikipedia:Contact_us">Contact Wikipedia</a></li> <li id="footer-places-wm-codeofconduct"><a href="https://foundation.wikimedia.org/wiki/Special:MyLanguage/Policy:Universal_Code_of_Conduct">Code of Conduct</a></li> <li id="footer-places-developers"><a href="https://developer.wikimedia.org">Developers</a></li> <li id="footer-places-statslink"><a href="https://stats.wikimedia.org/#/en.wikipedia.org">Statistics</a></li> <li id="footer-places-cookiestatement"><a href="https://foundation.wikimedia.org/wiki/Special:MyLanguage/Policy:Cookie_statement">Cookie statement</a></li> <li id="footer-places-mobileview"><a href="//en.m.wikipedia.org/w/index.php?title=Glossary_of_engineering:_A%E2%80%93L&action=edit&section=7&mobileaction=toggle_view_mobile" class="noprint stopMobileRedirectToggle">Mobile view</a></li> </ul> <ul id="footer-icons" class="noprint"> <li id="footer-copyrightico"><a href="https://wikimediafoundation.org/" class="cdx-button cdx-button--fake-button cdx-button--size-large cdx-button--fake-button--enabled"><img src="/static/images/footer/wikimedia-button.svg" width="84" height="29" alt="Wikimedia Foundation" loading="lazy"></a></li> <li id="footer-poweredbyico"><a href="https://www.mediawiki.org/" class="cdx-button cdx-button--fake-button cdx-button--size-large cdx-button--fake-button--enabled"><img src="/w/resources/assets/poweredby_mediawiki.svg" alt="Powered by MediaWiki" width="88" height="31" loading="lazy"></a></li> </ul> </footer> </div> </div> </div> <div class="vector-settings" id="p-dock-bottom"> <ul></ul> </div><script>(RLQ=window.RLQ||[]).push(function(){mw.config.set({"wgHostname":"mw-web.codfw.main-5cd4cd96d5-4j8tq","wgBackendResponseTime":357,"wgPageParseReport":{"limitreport":{"cputime":"0.078","walltime":"0.108","ppvisitednodes":{"value":418,"limit":1000000},"postexpandincludesize":{"value":17740,"limit":2097152},"templateargumentsize":{"value":6556,"limit":2097152},"expansiondepth":{"value":9,"limit":100},"expensivefunctioncount":{"value":0,"limit":500},"unstrip-depth":{"value":0,"limit":20},"unstrip-size":{"value":469,"limit":5000000},"entityaccesscount":{"value":0,"limit":400},"timingprofile":["100.00% 79.134 1 -total"," 99.85% 79.019 2 Template:Blocked_text"," 43.41% 34.353 2 Template:Replace"," 39.84% 31.527 1 Template:Colocationwebhost"," 36.39% 28.796 1 Template:Hidden"," 15.45% 12.230 1 Template:Hidden_begin"," 14.57% 11.528 1 Template:Tlx"," 2.38% 1.883 1 Template:Hidden_end"," 2.03% 1.603 1 MediaWiki:Wikimedia-globalblocking-blockedtext-mistake"," 1.57% 1.239 1 MediaWiki:Wikimedia-globalblocking-blockedtext-mistake-email-steward"]},"scribunto":{"limitreport-timeusage":{"value":"0.015","limit":"10.000"},"limitreport-memusage":{"value":1043358,"limit":52428800}},"cachereport":{"origin":"mw-web.codfw.main-5cd4cd96d5-4j8tq","timestamp":"20241127010143","ttl":2592000,"transientcontent":false}}});});</script> </body> </html>