Inflation from (R+γRn−2Λ) gravity in higher dimensions; Physical Review D; Vol. 95, iss. 10
| Parent link: | Physical Review D: particles, fields, gravitation, and cosmology.— , 1970- Vol. 95, iss. 10.— 2017.— [103507, 7 p.] |
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| 要約: | Title screen We propose a derivation of the inflaton scalar potential from the higher (D) dimensional (R+γRn−2Λ) gravity, with the new coupling constant γ and the cosmological constant Λ. We assume that a compactification of extra dimensions happened before inflation, so that the inflaton scalar potential in four spacetime dimensions appears to be dependent upon the parameters (γ,Λ,D,n). We find that phenomenology and consistency require n=D/2, while the dimension Dhas to be a multiple of four. We calculate the potential for any D, and determine the values of γ and Λfrom observations. The cases of D=8 and D=12 are considered in more detail. Our approach results in the viable models of chaotic large-field inflation, and leads to the sharp predictions of an observable value of the tensor-to-scalar ratio r of the cosmic microwave background radiation. Режим доступа: по договору с организацией-держателем ресурса |
| 言語: | 英語 |
| 出版事項: |
2017
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| 主題: | |
| オンライン･アクセス: | https://doi.org/10.1103/PhysRevD.95.103507 |
| フォーマット: | 電子媒体 図書の章 |
| KOHA link: | https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=655326 |
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| 200 | 1 | |a Inflation from (R+γRn−2Λ) gravity in higher dimensions |f S. V. Ketov, Nakada Hiroshi | |
| 203 | |a Text |c electronic | ||
| 300 | |a Title screen | ||
| 320 | |a [References: 27 tit.] | ||
| 330 | |a We propose a derivation of the inflaton scalar potential from the higher (D) dimensional (R+γRn−2Λ) gravity, with the new coupling constant γ and the cosmological constant Λ. We assume that a compactification of extra dimensions happened before inflation, so that the inflaton scalar potential in four spacetime dimensions appears to be dependent upon the parameters (γ,Λ,D,n). We find that phenomenology and consistency require n=D/2, while the dimension Dhas to be a multiple of four. We calculate the potential for any D, and determine the values of γ and Λfrom observations. The cases of D=8 and D=12 are considered in more detail. Our approach results in the viable models of chaotic large-field inflation, and leads to the sharp predictions of an observable value of the tensor-to-scalar ratio r of the cosmic microwave background radiation. | ||
| 333 | |a Режим доступа: по договору с организацией-держателем ресурса | ||
| 461 | |t Physical Review D |o particles, fields, gravitation, and cosmology |d 1970- | ||
| 463 | |t Vol. 95, iss. 10 |v [103507, 7 p.] |d 2017 | ||
| 610 | 1 | |a электронный ресурс | |
| 610 | 1 | |a труды учёных ТПУ | |
| 700 | 1 | |a Ketov |b S. V. |c physicist |c Professor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences |f 1960- |g Sergey Vladimirovich |3 (RuTPU)RU\TPU\pers\36631 |9 19672 | |
| 701 | 0 | |a Nakada Hiroshi | |
| 712 | 0 | 2 | |a Национальный исследовательский Томский политехнический университет (ТПУ) |b Физико-технический институт (ФТИ) |b Кафедра прикладной физики (№ 12) (ПФ) |3 (RuTPU)RU\TPU\col\18729 |
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