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IR divergences and kinetic equation in de Sitter space. (Poincare patch; principal series)
A bstract We explicitly show that the one loop IR correction to the two-point function in de Sitter space scalar QFT does not reduce just to the mass renormalization. The proper interpretation of the loop corrections is via particle creation revealing itself through the generation of the quantum ave...
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Published in: | The journal of high energy physics 2012-01, Vol.2012 (1), Article 66 |
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container_title | The journal of high energy physics |
container_volume | 2012 |
creator | Akhmedov, E. T. |
description | A
bstract
We explicitly show that the one loop IR correction to the two-point function in de Sitter space scalar QFT does not reduce just to the mass renormalization. The proper interpretation of the loop corrections is via particle creation revealing itself through the generation of the quantum averages
and
, which slowly change in time. We show that this observation in particular means that loop corrections to correlation functions in de Sitter space can not be obtained via analytical continuation of those calculated on the sphere.
We find harmonics for which the particle number
dominates over the anomalous expectation values
and
. For these harmonics the Dyson-Schwinger equation reduces in the IR limit to the kinetic equation. We solve the latter equation, which allows us to sum up all loop leading IR contributions to the Whiteman function. We perform the calculation for the principle series real scalar fields both in expanding and contracting Poincare patches. |
doi_str_mv | 10.1007/JHEP01(2012)066 |
format | article |
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bstract
We explicitly show that the one loop IR correction to the two-point function in de Sitter space scalar QFT does not reduce just to the mass renormalization. The proper interpretation of the loop corrections is via particle creation revealing itself through the generation of the quantum averages
and
, which slowly change in time. We show that this observation in particular means that loop corrections to correlation functions in de Sitter space can not be obtained via analytical continuation of those calculated on the sphere.
We find harmonics for which the particle number
dominates over the anomalous expectation values
and
. For these harmonics the Dyson-Schwinger equation reduces in the IR limit to the kinetic equation. We solve the latter equation, which allows us to sum up all loop leading IR contributions to the Whiteman function. We perform the calculation for the principle series real scalar fields both in expanding and contracting Poincare patches.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP01(2012)066</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer-Verlag</publisher><subject>Classical and Quantum Gravitation ; Elementary Particles ; Harmonics ; High energy physics ; Kinetic equations ; Mathematical analysis ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Relativity Theory ; Scalars ; String Theory</subject><ispartof>The journal of high energy physics, 2012-01, Vol.2012 (1), Article 66</ispartof><rights>SISSA, Trieste, Italy 2012</rights><rights>SISSA, Trieste, Italy 2012.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c376t-ba107f2b12cc17facad05696595644ab490240110d279d615c63e7faac43d69e3</citedby><cites>FETCH-LOGICAL-c376t-ba107f2b12cc17facad05696595644ab490240110d279d615c63e7faac43d69e3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/2398240079/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/2398240079?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25752,27923,27924,37011,44589,74997</link.rule.ids></links><search><creatorcontrib>Akhmedov, E. T.</creatorcontrib><title>IR divergences and kinetic equation in de Sitter space. (Poincare patch; principal series)</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>A
bstract
We explicitly show that the one loop IR correction to the two-point function in de Sitter space scalar QFT does not reduce just to the mass renormalization. The proper interpretation of the loop corrections is via particle creation revealing itself through the generation of the quantum averages
and
, which slowly change in time. We show that this observation in particular means that loop corrections to correlation functions in de Sitter space can not be obtained via analytical continuation of those calculated on the sphere.
We find harmonics for which the particle number
dominates over the anomalous expectation values
and
. For these harmonics the Dyson-Schwinger equation reduces in the IR limit to the kinetic equation. We solve the latter equation, which allows us to sum up all loop leading IR contributions to the Whiteman function. We perform the calculation for the principle series real scalar fields both in expanding and contracting Poincare patches.</description><subject>Classical and Quantum Gravitation</subject><subject>Elementary Particles</subject><subject>Harmonics</subject><subject>High energy physics</subject><subject>Kinetic equations</subject><subject>Mathematical analysis</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Relativity Theory</subject><subject>Scalars</subject><subject>String Theory</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNp1kL1PwzAQxS0EEqUws1piaYe0ZydxajGhqtCiSlR8LCyW61yKS0lSO0Hiv8dVkGBhujvp_d7dPUIuGYwYQDa-n89WwAYcGB-CEEekx4DLaJJk8vhPf0rOvN8CsJRJ6JHXxSPN7Se6DZYGPdVlTt9tiY01FPetbmxVUlvSHOmTbRp01Nfa4IgOVpUtjXZIa92Yt2tauzDbWu-oR2fRD8_JSaF3Hi9-ap-83M6ep_No-XC3mN4sIxNnoonWmkFW8DXjxrCs0EbnkAopUpmKJNHrRAJPgDHIeSZzwVIjYgw6bZI4FxLjPrnqfGtX7Vv0jdpWrSvDSsVjOQkwZDKoxp3KuMp7h4UKB39o96UYqEOAqgtQHQJUIcBAQEf4w2sbdL--_yHfjc1xXg</recordid><startdate>20120101</startdate><enddate>20120101</enddate><creator>Akhmedov, E. T.</creator><general>Springer-Verlag</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope></search><sort><creationdate>20120101</creationdate><title>IR divergences and kinetic equation in de Sitter space. (Poincare patch; principal series)</title><author>Akhmedov, E. T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c376t-ba107f2b12cc17facad05696595644ab490240110d279d615c63e7faac43d69e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Classical and Quantum Gravitation</topic><topic>Elementary Particles</topic><topic>Harmonics</topic><topic>High energy physics</topic><topic>Kinetic equations</topic><topic>Mathematical analysis</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Relativity Theory</topic><topic>Scalars</topic><topic>String Theory</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Akhmedov, E. T.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><jtitle>The journal of high energy physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Akhmedov, E. T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>IR divergences and kinetic equation in de Sitter space. (Poincare patch; principal series)</atitle><jtitle>The journal of high energy physics</jtitle><stitle>J. High Energ. Phys</stitle><date>2012-01-01</date><risdate>2012</risdate><volume>2012</volume><issue>1</issue><artnum>66</artnum><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>A
bstract
We explicitly show that the one loop IR correction to the two-point function in de Sitter space scalar QFT does not reduce just to the mass renormalization. The proper interpretation of the loop corrections is via particle creation revealing itself through the generation of the quantum averages
and
, which slowly change in time. We show that this observation in particular means that loop corrections to correlation functions in de Sitter space can not be obtained via analytical continuation of those calculated on the sphere.
We find harmonics for which the particle number
dominates over the anomalous expectation values
and
. For these harmonics the Dyson-Schwinger equation reduces in the IR limit to the kinetic equation. We solve the latter equation, which allows us to sum up all loop leading IR contributions to the Whiteman function. We perform the calculation for the principle series real scalar fields both in expanding and contracting Poincare patches.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer-Verlag</pub><doi>10.1007/JHEP01(2012)066</doi><oa>free_for_read</oa></addata></record> |
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subjects | Classical and Quantum Gravitation Elementary Particles Harmonics High energy physics Kinetic equations Mathematical analysis Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Relativity Theory Scalars String Theory |
title | IR divergences and kinetic equation in de Sitter space. (Poincare patch; principal series) |
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