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</div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1603.02907">arXiv:1603.02907</a> <span> [<a href="https://arxiv.org/pdf/1603.02907">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="General Physics">physics.gen-ph</span> </div> </div> <p class="title is-5 mathjax"> Heuristic arguments in favor of the view that the forces which form the bound systems of elementary particles propagate instantaneously </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Anicin%2C+I">Ivan Anicin</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1603.02907v1-abstract-short" style="display: inline;"> We make use of the well-known properties of spontaneous decays of stationary states of bound systems of elementary particles to support the view that the forces which form these systems propagate instantaneously at the moment of their decay. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1603.02907v1-abstract-full" style="display: none;"> We make use of the well-known properties of spontaneous decays of stationary states of bound systems of elementary particles to support the view that the forces which form these systems propagate instantaneously at the moment of their decay. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1603.02907v1-abstract-full').style.display = 'none'; document.getElementById('1603.02907v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 March, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, no figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1305.2572">arXiv:1305.2572</a> <span> [<a href="https://arxiv.org/pdf/1305.2572">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2014.01.065">10.1016/j.nima.2014.01.065 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> On the omnipresent background gamma radiation of the continuous spectrum </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Banjanac%2C+R">R. Banjanac</a>, <a href="/search/physics?searchtype=author&query=Maleti%C4%87%2C+D">D. Maleti膰</a>, <a href="/search/physics?searchtype=author&query=Jokovi%C4%87%2C+D">D. Jokovi膰</a>, <a href="/search/physics?searchtype=author&query=Veselinovi%C4%87%2C+N">N. Veselinovi膰</a>, <a href="/search/physics?searchtype=author&query=Dragi%C4%87%2C+A">A. Dragi膰</a>, <a href="/search/physics?searchtype=author&query=Udovi%C4%8Di%C4%87%2C+V">V. Udovi膷i膰</a>, <a href="/search/physics?searchtype=author&query=Ani%C4%8Din%2C+I">I. Ani膷in</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1305.2572v2-abstract-short" style="display: inline;"> The background spectrum of a germanium detector, shielded from the radiations arriving from the lower and open for the radiations arriving from the upper hemisphere is studied, both in a ground level and in an underground laboratory. It is established that the continuous portion of this background spectrum is mostly due to the radiations that arrive from the upper hemisphere of the continuous spec… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1305.2572v2-abstract-full').style.display = 'inline'; document.getElementById('1305.2572v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1305.2572v2-abstract-full" style="display: none;"> The background spectrum of a germanium detector, shielded from the radiations arriving from the lower and open for the radiations arriving from the upper hemisphere is studied, both in a ground level and in an underground laboratory. It is established that the continuous portion of this background spectrum is mostly due to the radiations that arrive from the upper hemisphere of the continuous spectrum similar to the instrumental one. The intensity of this radiation of an average energy of about 120 keV is estimated to about 8000 photons/m2s 2蟺srad in a ground level laboratory, and to about 5000 photons/m2s 2蟺srad at the depth of 25 m.w.e. Rough estimates of the dose that it contributes to the skin are about 1.5 nSv/h and 1 nSv/h respectively. Simulations by GEANT4 and CORSIKA demonstrate that this radiation is both of cosmic and terrestrial origin, mixed in proportion that still has to be determined. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1305.2572v2-abstract-full').style.display = 'none'; document.getElementById('1305.2572v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 May, 2013; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 12 May, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 5 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1304.7879">arXiv:1304.7879</a> <span> [<a href="https://arxiv.org/pdf/1304.7879">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Atmospheric and Oceanic Physics">physics.ao-ph</span> </div> </div> <p class="title is-5 mathjax"> Further investigations into the connection between cosmic rays and climate </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Dragi%C4%87%2C+A">A. Dragi膰</a>, <a href="/search/physics?searchtype=author&query=Veselinovi%C4%87%2C+N">N. Veselinovi膰</a>, <a href="/search/physics?searchtype=author&query=Maleti%C4%87%2C+D">D. Maleti膰</a>, <a href="/search/physics?searchtype=author&query=Jokovi%C4%87%2C+D">D. Jokovi膰</a>, <a href="/search/physics?searchtype=author&query=Banjanac%2C+R">R Banjanac</a>, <a href="/search/physics?searchtype=author&query=Udovi%C4%8Di%C4%87%2C+V">V. Udovi膷i膰</a>, <a href="/search/physics?searchtype=author&query=Ani%C4%8Din%2C+I">I. Ani膷in</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1304.7879v1-abstract-short" style="display: inline;"> Our previous results on the connection between the Forbush decreases (FD) of cosmic-ray intensity and the deviations from the expected values of the diurnal temperature range (DTR) are briefly revisited. The same type of analysis is then extended to the cases of sudden increases of cosmic-ray intensity (GLE), as well as to the search for lattitude effects in the observed correlations. We find that… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1304.7879v1-abstract-full').style.display = 'inline'; document.getElementById('1304.7879v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1304.7879v1-abstract-full" style="display: none;"> Our previous results on the connection between the Forbush decreases (FD) of cosmic-ray intensity and the deviations from the expected values of the diurnal temperature range (DTR) are briefly revisited. The same type of analysis is then extended to the cases of sudden increases of cosmic-ray intensity (GLE), as well as to the search for lattitude effects in the observed correlations. We find that all the investigated correlations appear to manifest both the expected signs and the plausible phase relations, though each one only at the modest confidence level. Moreover, it appears that there is some proportionality between the magnitude of a cosmic-ray intensity change and a corresponding DTR deviation, both in the case of FD and GLE events. Eventual increase of the confidence levels at which these correlations are established would have to wait for the significant increase of the number of well defined and sufficiently intense recorded departures of cosmic-ray intensity from its stationary mean value. On the other hand, the probability of such an accidental multiple coincidence of independent pieces of evidence is certainly very low. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1304.7879v1-abstract-full').style.display = 'none'; document.getElementById('1304.7879v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 April, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">9 pages, 3 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1203.4607">arXiv:1203.4607</a> <span> [<a href="https://arxiv.org/pdf/1203.4607">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.2298/NTRP1101064N">10.2298/NTRP1101064N <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The New Setup in the Belgrade Low-Level and Cosmic-Ray Laboratory </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Dragi%C4%87%2C+A">Aleksandar Dragi膰</a>, <a href="/search/physics?searchtype=author&query=Udovi%C4%8Di%C4%87%2C+V">Vladimir Udovi膷i膰</a>, <a href="/search/physics?searchtype=author&query=Banjanac%2C+R">Radomir Banjanac</a>, <a href="/search/physics?searchtype=author&query=Jokovi%C4%87%2C+D">Dejan Jokovi膰</a>, <a href="/search/physics?searchtype=author&query=Maleti%C4%87%2C+D">Dimitrije Maleti膰</a>, <a href="/search/physics?searchtype=author&query=Veselinovi%C4%87%2C+N">Nikola Veselinovi膰</a>, <a href="/search/physics?searchtype=author&query=Savi%C4%87%2C+M">Mihailo Savi膰</a>, <a href="/search/physics?searchtype=author&query=Puzovi%C4%87%2C+J">Jovan Puzovi膰</a>, <a href="/search/physics?searchtype=author&query=Ani%C4%8Din%2C+I+V">Ivan V. Ani膷in</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1203.4607v1-abstract-short" style="display: inline;"> The Belgrade underground laboratory consists of two interconnected spaces, a ground level laboratory and a shallow underground one, at 25 m.w.e.. The laboratory hosts a low-background gamma spectroscopy system and cosmic-ray muon detectors. With recently adopted digital data acquisition system it is possible to study simultaneously independent operation of two detector systems, as well as processe… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1203.4607v1-abstract-full').style.display = 'inline'; document.getElementById('1203.4607v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1203.4607v1-abstract-full" style="display: none;"> The Belgrade underground laboratory consists of two interconnected spaces, a ground level laboratory and a shallow underground one, at 25 m.w.e.. The laboratory hosts a low-background gamma spectroscopy system and cosmic-ray muon detectors. With recently adopted digital data acquisition system it is possible to study simultaneously independent operation of two detector systems, as well as processes induced by cosmic-ray muons in germanium spectrometers. Characteristics and potentials of present experimental setup, together with some preliminary results for the flux of fast neutrons and stopped muons are reported. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1203.4607v1-abstract-full').style.display = 'none'; document.getElementById('1203.4607v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 March, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">12 pages, 16 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nuclear Technology & Radiation Protection: Year 2011, Vol. 26, No. 3, pp.181-192 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0912.4300">arXiv:0912.4300</a> <span> [<a href="https://arxiv.org/pdf/0912.4300">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/5/03/P03010">10.1088/1748-0221/5/03/P03010 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Radiation hardness qualification of PbWO4 scintillation crystals for the CMS Electromagnetic Calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=The+CMS+Electromagnetic+Calorimeter+Group"> The CMS Electromagnetic Calorimeter Group</a>, <a href="/search/physics?searchtype=author&query=Adzic%2C+P">P. Adzic</a>, <a href="/search/physics?searchtype=author&query=Almeida%2C+N">N. Almeida</a>, <a href="/search/physics?searchtype=author&query=Andelin%2C+D">D. Andelin</a>, <a href="/search/physics?searchtype=author&query=Anicin%2C+I">I. Anicin</a>, <a href="/search/physics?searchtype=author&query=Antunovic%2C+Z">Z. Antunovic</a>, <a href="/search/physics?searchtype=author&query=Arcidiacono%2C+R">R. Arcidiacono</a>, <a href="/search/physics?searchtype=author&query=Arenton%2C+M+W">M. W. Arenton</a>, <a href="/search/physics?searchtype=author&query=Auffray%2C+E">E. Auffray</a>, <a href="/search/physics?searchtype=author&query=Argiro%2C+S">S. Argiro</a>, <a href="/search/physics?searchtype=author&query=Askew%2C+A">A. Askew</a>, <a href="/search/physics?searchtype=author&query=Baccaro%2C+S">S. Baccaro</a>, <a href="/search/physics?searchtype=author&query=Baffioni%2C+S">S. Baffioni</a>, <a href="/search/physics?searchtype=author&query=Balazs%2C+M">M. Balazs</a>, <a href="/search/physics?searchtype=author&query=Bandurin%2C+D">D. Bandurin</a>, <a href="/search/physics?searchtype=author&query=Barney%2C+D">D. Barney</a>, <a href="/search/physics?searchtype=author&query=Barone%2C+L+M">L. M. Barone</a>, <a href="/search/physics?searchtype=author&query=Bartoloni%2C+A">A. Bartoloni</a>, <a href="/search/physics?searchtype=author&query=Baty%2C+C">C. Baty</a>, <a href="/search/physics?searchtype=author&query=Beauceron%2C+S">S. Beauceron</a>, <a href="/search/physics?searchtype=author&query=Bell%2C+K+W">K. W. Bell</a>, <a href="/search/physics?searchtype=author&query=Bernet%2C+C">C. Bernet</a>, <a href="/search/physics?searchtype=author&query=Besancon%2C+M">M. Besancon</a>, <a href="/search/physics?searchtype=author&query=Betev%2C+B">B. Betev</a>, <a href="/search/physics?searchtype=author&query=Beuselinck%2C+R">R. Beuselinck</a> , et al. (245 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0912.4300v1-abstract-short" style="display: inline;"> Ensuring the radiation hardness of PbWO4 crystals was one of the main priorities during the construction of the electromagnetic calorimeter of the CMS experiment at CERN. The production on an industrial scale of radiation hard crystals and their certification over a period of several years represented a difficult challenge both for CMS and for the crystal suppliers. The present article reviews t… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0912.4300v1-abstract-full').style.display = 'inline'; document.getElementById('0912.4300v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0912.4300v1-abstract-full" style="display: none;"> Ensuring the radiation hardness of PbWO4 crystals was one of the main priorities during the construction of the electromagnetic calorimeter of the CMS experiment at CERN. The production on an industrial scale of radiation hard crystals and their certification over a period of several years represented a difficult challenge both for CMS and for the crystal suppliers. The present article reviews the related scientific and technological problems encountered. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0912.4300v1-abstract-full').style.display = 'none'; document.getElementById('0912.4300v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 December, 2009; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2009. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">24 pages, 19 figures, available on CMS information server at http://cms.cern.ch/iCMS/</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> CMS Note 2009/016 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 5:P03010,2010 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0503172">arXiv:physics/0503172</a> <span> [<a href="https://arxiv.org/pdf/physics/0503172">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="History and Philosophy of Physics">physics.hist-ph</span> </div> </div> <p class="title is-5 mathjax"> The Neutrino - Its Past, Present and Future </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Anicin%2C+I+V">Ivan V. Anicin</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="physics/0503172v1-abstract-short" style="display: inline;"> The review consists of two parts. In the first part the critical points in the past, present and future of neutrino physics (nuclear, particle and astroparticle) are reviewed. In the second part the contributions of Yugoslav physics to the physics of the neutrino are commented upon. The review is meant as a first reading for the newcomers to the field of neutrino physics. </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0503172v1-abstract-full" style="display: none;"> The review consists of two parts. In the first part the critical points in the past, present and future of neutrino physics (nuclear, particle and astroparticle) are reviewed. In the second part the contributions of Yugoslav physics to the physics of the neutrino are commented upon. The review is meant as a first reading for the newcomers to the field of neutrino physics. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0503172v1-abstract-full').style.display = 'none'; document.getElementById('physics/0503172v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 22 March, 2005; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2005. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">60 pages, 9 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> SFIN (Institute of Physics, Belgrade) year XV, Series A: Conferences, No. A2 (2002) 3-59 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0501108">arXiv:physics/0501108</a> <span> [<a href="https://arxiv.org/pdf/physics/0501108">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</span> </div> </div> <p class="title is-5 mathjax"> Late-Night Thoughts About the Significance of a Small Count of Nuclear or Particle Events </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Anicin%2C+I+V">Ivan V. Anicin</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="physics/0501108v3-abstract-short" style="display: inline;"> Reconciliation of frequentist and Bayesian approaches to elementary treatment of data in nuclear and particle physics is attempted. Unique procedure to express the significance of a small count in presence of background is henceforth proposed and discussed in some detail. </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0501108v3-abstract-full" style="display: none;"> Reconciliation of frequentist and Bayesian approaches to elementary treatment of data in nuclear and particle physics is attempted. Unique procedure to express the significance of a small count in presence of background is henceforth proposed and discussed in some detail. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0501108v3-abstract-full').style.display = 'none'; document.getElementById('physics/0501108v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 25 February, 2005; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 20 January, 2005; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2005. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">18 pages, 9 figures, titles to subsections added, typos corrected</span> </p> </li> </ol> <div class="is-hidden-tablet">  <span class="help" 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