High-temperature expansion of the free energy of a massive scalar field in a curved space
The high-temperature expansion of the free energy of a free, massive scalar field propagating in a static space-time is derived in terms of the Minakshisundaram coefficients. The method is an extension of a conformal transformation technique using zeta functions.
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Veröffentlicht in: | Phys. Rev. D; (United States) 1988-11, Vol.38 (10), p.3327-3329 |
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container_title | Phys. Rev. D; (United States) |
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creator | DOWKER, J. S SCHOFIELD, J. P |
description | The high-temperature expansion of the free energy of a free, massive scalar field propagating in a static space-time is derived in terms of the Minakshisundaram coefficients. The method is an extension of a conformal transformation technique using zeta functions. |
doi_str_mv | 10.1103/PhysRevD.38.3327 |
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S</creatorcontrib><creatorcontrib>SCHOFIELD, J. P</creatorcontrib><creatorcontrib>Department of Theoretical Physics, The University of Manchester, Manchester, England</creatorcontrib><collection>Pascal-Francis</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Phys. Rev. D; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>DOWKER, J. S</au><au>SCHOFIELD, J. P</au><aucorp>Department of Theoretical Physics, The University of Manchester, Manchester, England</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>High-temperature expansion of the free energy of a massive scalar field in a curved space</atitle><jtitle>Phys. Rev. D; (United States)</jtitle><addtitle>Phys Rev D Part Fields</addtitle><date>1988-11-15</date><risdate>1988</risdate><volume>38</volume><issue>10</issue><spage>3327</spage><epage>3329</epage><pages>3327-3329</pages><issn>0556-2821</issn><eissn>1089-4918</eissn><coden>PRVDAQ</coden><abstract>The high-temperature expansion of the free energy of a free, massive scalar field propagating in a static space-time is derived in terms of the Minakshisundaram coefficients. The method is an extension of a conformal transformation technique using zeta functions.</abstract><cop>Ridge, NY</cop><pub>American Physical Society</pub><pmid>9959086</pmid><doi>10.1103/PhysRevD.38.3327</doi><tpages>3</tpages></addata></record> |
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subjects | ASTROPHYSICS COSMOLOGY DIFFERENTIAL EQUATIONS ENERGY ENERGY-MOMENTUM TENSOR EQUATIONS EQUATIONS OF MOTION Exact sciences and technology FREE ENERGY FUNCTIONS General relativity and gravitation GREEN FUNCTION INTEGRAL TRANSFORMATIONS MASS MELLIN TRANSFORM METRICS PARTIAL DIFFERENTIAL EQUATIONS PHYSICAL PROPERTIES Physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS PROPAGATOR Quantum gravity SCALAR FIELDS SCHROEDINGER EQUATION SPACE-TIME TEMPERATURE DEPENDENCE TENSORS THERMODYNAMIC PROPERTIES TRANSFORMATIONS WAVE EQUATIONS 645400 -- High Energy Physics-- Field Theory |
title | High-temperature expansion of the free energy of a massive scalar field in a curved space |
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