Ultraviolet sensitivity in Higgs-Starobinsky inflation
The general scalar-tensor theory that includes all the dimension-four terms has parameter regions that can produce successful inflation consistent with cosmological observations. This theory is in fact the same as the Higgs-Starobinsky inflation, when the scalar is identified with the Standard Model...
Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
August 2023
|
| In: |
Journal of cosmology and astroparticle physics
Year: 2023, Issue: 8, Pages: 1-24 |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2023/08/045 |
| Online Access: | Verlag, kostenfrei, Volltext: https://doi.org/10.1088/1475-7516/2023/08/045 Verlag, kostenfrei, Volltext: https://dx.doi.org/10.1088/1475-7516/2023/08/045 
|
| Author Notes: | Sung Mook Lee, Tanmoy Modak, Kin-ya Oda and Tomo Takahashi |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1868616266 | ||
| 003 | DE-627 | ||
| 005 | 20240730082318.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 231027s2023 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1088/1475-7516/2023/08/045 |2 doi | |
| 035 | |a (DE-627)1868616266 | ||
| 035 | |a (DE-599)KXP1868616266 | ||
| 035 | |a (OCoLC)1425210003 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Lee, Sung Mook |e VerfasserIn |0 (DE-588)1269739042 |0 (DE-627)1818244055 |4 aut | |
| 245 | 1 | 0 | |a Ultraviolet sensitivity in Higgs-Starobinsky inflation |c Sung Mook Lee, Tanmoy Modak, Kin-ya Oda and Tomo Takahashi |
| 264 | 1 | |c August 2023 | |
| 300 | |b Illustrationen | ||
| 300 | |a 24 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Veröffentlicht: 18. August 2023 | ||
| 500 | |a Gesehen am 27.10.2023 | ||
| 520 | |a The general scalar-tensor theory that includes all the dimension-four terms has parameter regions that can produce successful inflation consistent with cosmological observations. This theory is in fact the same as the Higgs-Starobinsky inflation, when the scalar is identified with the Standard Model Higgs boson. We consider possible dimension-six operators constructed from non-derivative terms of the scalar field and the Ricci scalar as perturbations. We investigate how much suppression is required for these operators to avoid disrupting the successful inflationary predictions. To ensure viable cosmological predictions, the suppression scale for the sixth power of the scalar should be as high as the Planck scale. For the other terms, much smaller scales are sufficient. | ||
| 700 | 1 | |a Modak, Tanmoy |e VerfasserIn |0 (DE-588)123853239X |0 (DE-627)1765936446 |4 aut | |
| 700 | 1 | |a Oda, Kin-ya |e VerfasserIn |4 aut | |
| 700 | 1 | |a Takahashi, Tomo |e VerfasserIn |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Journal of cosmology and astroparticle physics |d London : IOP, 2003 |g (2023), 8 vom: Aug., Artikel-ID 045, Seite 1-24 |h Online-Ressource |w (DE-627)361339771 |w (DE-600)2104147-7 |w (DE-576)106869809 |x 1475-7516 |7 nnas |a Ultraviolet sensitivity in Higgs-Starobinsky inflation |
| 773 | 1 | 8 | |g year:2023 |g number:8 |g month:08 |g elocationid:045 |g pages:1-24 |g extent:24 |a Ultraviolet sensitivity in Higgs-Starobinsky inflation |
| 856 | 4 | 0 | |u https://doi.org/10.1088/1475-7516/2023/08/045 |x Verlag |x Resolving-System |z kostenfrei |3 Volltext |
| 856 | 4 | 0 | |u https://dx.doi.org/10.1088/1475-7516/2023/08/045 |x Verlag |z kostenfrei |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20231027 | ||
| 993 | |a Article | ||
| 994 | |a 2023 | ||
| 998 | |g 123853239X |a Modak, Tanmoy |m 123853239X:Modak, Tanmoy |d 130000 |d 130300 |e 130000PM123853239X |e 130300PM123853239X |k 0/130000/ |k 1/130000/130300/ |p 2 | ||
| 999 | |a KXP-PPN1868616266 |e 439924450X | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"language":["eng"],"recId":"1868616266","type":{"media":"Online-Ressource","bibl":"article-journal"},"note":["Veröffentlicht: 18. August 2023","Gesehen am 27.10.2023"],"title":[{"title":"Ultraviolet sensitivity in Higgs-Starobinsky inflation","title_sort":"Ultraviolet sensitivity in Higgs-Starobinsky inflation"}],"person":[{"role":"aut","roleDisplay":"VerfasserIn","display":"Lee, Sung Mook","given":"Sung Mook","family":"Lee"},{"given":"Tanmoy","family":"Modak","role":"aut","roleDisplay":"VerfasserIn","display":"Modak, Tanmoy"},{"given":"Kin-ya","family":"Oda","role":"aut","display":"Oda, Kin-ya","roleDisplay":"VerfasserIn"},{"given":"Tomo","family":"Takahashi","role":"aut","roleDisplay":"VerfasserIn","display":"Takahashi, Tomo"}],"relHost":[{"origin":[{"publisherPlace":"London","dateIssuedDisp":"2003-","publisher":"IOP","dateIssuedKey":"2003"}],"id":{"issn":["1475-7516"],"zdb":["2104147-7"],"eki":["361339771"]},"physDesc":[{"extent":"Online-Ressource"}],"title":[{"title":"Journal of cosmology and astroparticle physics","subtitle":"JCAP ; an IOP and SISSA journal","title_sort":"Journal of cosmology and astroparticle physics"}],"type":{"media":"Online-Ressource","bibl":"periodical"},"disp":"Ultraviolet sensitivity in Higgs-Starobinsky inflationJournal of cosmology and astroparticle physics","note":["Gesehen am 14.07.2021"],"recId":"361339771","corporate":[{"role":"isb","roleDisplay":"Herausgebendes Organ","display":"Institute of Physics"},{"role":"isb","roleDisplay":"Herausgebendes Organ","display":"Scuola Internazionale Superiore di Studi Avanzati"}],"language":["eng"],"pubHistory":["Nachgewiesen 2003 -"],"part":{"text":"(2023), 8 vom: Aug., Artikel-ID 045, Seite 1-24","extent":"24","year":"2023","pages":"1-24","issue":"8"},"titleAlt":[{"title":"JCAP"}]}],"physDesc":[{"noteIll":"Illustrationen","extent":"24 S."}],"id":{"doi":["10.1088/1475-7516/2023/08/045"],"eki":["1868616266"]},"origin":[{"dateIssuedDisp":"August 2023","dateIssuedKey":"2023"}],"name":{"displayForm":["Sung Mook Lee, Tanmoy Modak, Kin-ya Oda and Tomo Takahashi"]}} | ||
| SRT | |a LEESUNGMOOULTRAVIOLE2023 | ||