Lessons from T-mu(mu) on inflation models: Two-scalar theory and Yukawa theory
DC Field | Value | Language |
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dc.contributor.author | Ayuki Kamada | - |
dc.contributor.author | Takumi Kuwahara | - |
dc.date.accessioned | 2020-12-22T03:02:40Z | - |
dc.date.accessioned | 2020-12-22T03:02:40Z | - |
dc.date.available | 2020-12-22T03:02:40Z | - |
dc.date.available | 2020-12-22T03:02:40Z | - |
dc.date.created | 2020-06-29 | - |
dc.date.issued | 2020-05 | - |
dc.identifier.issn | 2470-0010 | - |
dc.identifier.uri | https://pr.ibs.re.kr/handle/8788114/7857 | - |
dc.description.abstract | © 2020 authors. Published by the American Physical Society. We demonstrate two properties of the trace of the energy-momentum tensor T-mu(mu) in the flat spacetime. One is the decoupling of heavy degrees of freedom; i.e., heavy degrees of freedom leave no effect for low-energy T-mu(mu)-inserted amplitudes. This is intuitively apparent from the effective field theory point of view, but one has to take into account the so-called trace anomaly to explicitly demonstrate the decoupling. As a result, for example, in the R-2 inflation model, scalaron decay is insensitive to heavy degrees of freedom when a matter sector minimally couples to gravity (up to a nonminimal coupling of a matter scalar field other than the scalaron). The other property is a quantum contribution to a nonminimal coupling of a scalar field. The nonminimal coupling disappears from the action in the flat spacetime, but leaves the so-called improvement term in T-mu(mu). We study the renormalization group equation of the nonminimal coupling to discuss its quantum-induced value and implications for inflation dynamics. We work it out in the two-scalar theory and Yukawa theory | - |
dc.language | 영어 | - |
dc.publisher | AMER PHYSICAL SOC | - |
dc.title | Lessons from T-mu(mu) on inflation models: Two-scalar theory and Yukawa theory | - |
dc.type | Article | - |
dc.type.rims | ART | - |
dc.identifier.wosid | 000533498700006 | - |
dc.identifier.scopusid | 2-s2.0-85091189607 | - |
dc.identifier.rimsid | 72526 | - |
dc.contributor.affiliatedAuthor | Ayuki Kamada | - |
dc.contributor.affiliatedAuthor | Takumi Kuwahara | - |
dc.identifier.doi | 10.1103/PhysRevD.101.096012 | - |
dc.identifier.bibliographicCitation | Physical Review d, v.101, no.9, pp.096012-1 | - |
dc.relation.isPartOf | Physical Review d | - |
dc.citation.title | Physical Review d | - |
dc.citation.volume | 101 | - |
dc.citation.number | 9 | - |
dc.citation.startPage | 096012-1 | - |
dc.description.journalClass | 1 | - |
dc.description.journalClass | 1 | - |
dc.description.isOpenAccess | N | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.relation.journalWebOfScienceCategory | Physics, Particles & Fields | - |
dc.subject.keywordPlus | ENERGY-MOMENTUM-TENSOR | - |
dc.subject.keywordPlus | DIMENSIONAL RENORMALIZATION | - |
dc.subject.keywordPlus | TRACE ANOMALIES | - |
dc.subject.keywordPlus | SCALAR | - |
dc.subject.keywordPlus | GRAVITY | - |
dc.subject.keywordPlus | REGULARIZATION | - |
dc.subject.keywordPlus | COSMOLOGY | - |