Search: onr:"swepub:oai:DiVA.org:kth-337414" > Carroll stories
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000 | 04315naa a2200457 4500 | |
001 | oai:DiVA.org:kth-337414 | |
003 | SwePub | |
008 | 231003s2023 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-223939 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3374142 URI |
024 | 7 | a https://doi.org/10.1007/JHEP09(2023)1482 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2239392 URI |
040 | a (SwePub)kthd (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a de Boer, Janu Institute for Theoretical Physics and Delta Institute for Theoretical Physics, University of Amsterdam, P.O. Box 94485, 1090 GL, Amsterdam, The Netherlands4 aut |
245 | 1 0 | a Carroll stories |
264 | 1 | b Springer Nature,c 2023 |
338 | a print2 rdacarrier | |
500 | a QC 20231031 | |
520 | a We study various aspects of the Carroll limit in which the speed of light is sent to zero. A large part of this paper is devoted to the quantization of Carroll field theories. We show that these exhibit infinite degeneracies in the spectrum and may suffer from non-normalizable ground states. As a consequence, partition functions of Carroll systems are ill-defined and do not lead to sensible thermodynamics. These seemingly pathological properties might actually be a virtue in the context of flat space holography. Better defined is the Carroll regime, in which we consider the leading order term in an expansion around vanishing speed of light without taking the strict Carroll limit. Such an expansion may lead to sensible notions of Carroll thermodynamics. An interesting example is a gas of massless particles with an imaginary chemical potential conjugate to the momentum. In the Carroll regime we show that the partition function of such a gas leads to an equation of state with w = −1. As a separate story, we study aspects of Carroll gravity and couplings to Carrollian energy-momentum tensors. We discuss many examples of solutions to Carroll gravity, including wormholes, Maxwell fields, solutions with a cosmological constant, and discuss the structure of geodesics in a Carroll geometry. The coupling of matter to Carroll gravity also allows us to derive energy-momentum tensors for hypothetical Carroll fluids from expanding relativistic fluids as well as directly from hydrostatic partition functions. | |
650 | 7 | a NATURVETENSKAPx Fysikx Annan fysik0 (SwePub)103992 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Other Physics Topics0 (SwePub)103992 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng |
653 | a Black Holes | |
653 | a Field Theories in Lower Dimensions | |
653 | a Field Theory Hydrodynamics | |
653 | a Space-Time Symmetries | |
700 | 1 | a Hartong, Jelleu School of Mathematics and Maxwell Institute for Mathematical Sciences, University of Edinburgh, Peter Guthrie Tait Road, Edinburgh, EH9 3FD, UK4 aut |
700 | 1 | a Obers, Niels A.u Stockholms universitet,Nordiska institutet för teoretisk fysik (Nordita),Nordita SU; The Niels Bohr Institute, Copenhagen University, Blegdamsvej 17, DK-2100, Copenhagen Ø, Denmark4 aut0 (Swepub:su)niob8745 |
700 | 1 | a Sybesma, Watseu Science Institute, University of Iceland, Dunhaga 3, 107, Reykjavík, Iceland4 aut |
700 | 1 | a Vandoren, Stefanu Institute for Theoretical Physics, Utrecht University, Princetonplein 5, 3584 CE, Utrecht, The Netherlands4 aut |
710 | 2 | a Institute for Theoretical Physics and Delta Institute for Theoretical Physics, University of Amsterdam, P.O. Box 94485, 1090 GL, Amsterdam, The Netherlandsb School of Mathematics and Maxwell Institute for Mathematical Sciences, University of Edinburgh, Peter Guthrie Tait Road, Edinburgh, EH9 3FD, UK4 org |
773 | 0 | t Journal of High Energy Physics (JHEP)d : Springer Natureg 2023:9q 2023:9x 1126-6708x 1029-8479 |
856 | 4 | u https://doi.org/10.1007/JHEP09(2023)148y Fulltext |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-337414 |
856 | 4 8 | u https://doi.org/10.1007/JHEP09(2023)148 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-223939 |
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