Cosmological Perturbations via Quantum Corrections in M-Theory
In the early universe, it is important to take into account the quantum effect of gravity to explain the feature of inflation. In this paper, we consider the M-theory effective action which consists of 11-dimensional supergravity and (Weyl)<inline-formula><math xmlns="http://www.w3.org...
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oai:doaj.org-article:77e596c7150c483693a045e45deae01a2021-11-25T19:09:40ZCosmological Perturbations via Quantum Corrections in M-Theory10.3390/universe71104252218-1997https://doaj.org/article/77e596c7150c483693a045e45deae01a2021-11-01T00:00:00Zhttps://www.mdpi.com/2218-1997/7/11/425https://doaj.org/toc/2218-1997In the early universe, it is important to take into account the quantum effect of gravity to explain the feature of inflation. In this paper, we consider the M-theory effective action which consists of 11-dimensional supergravity and (Weyl)<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>4</mn></msup></semantics></math></inline-formula> terms. The equations of motion are solved perturbatively, and the solution describes the inflation-like expansion in 4-dimensional spacetime. Equations of motion for tensor perturbations around this background are derived perturbatively. We also check that the equations of motion are obtained from the effective action up to the second order of the perturbations. Finally, we solve the equations of motion for the tensor perturbations perturbatively and obtain analytic expressions for them.Kazuho HiragaYoshifumi HyakutakeMDPI AGarticleinflationM-theoryquantum gravityElementary particle physicsQC793-793.5ENUniverse, Vol 7, Iss 425, p 425 (2021) |
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inflation M-theory quantum gravity Elementary particle physics QC793-793.5 |
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inflation M-theory quantum gravity Elementary particle physics QC793-793.5 Kazuho Hiraga Yoshifumi Hyakutake Cosmological Perturbations via Quantum Corrections in M-Theory |
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In the early universe, it is important to take into account the quantum effect of gravity to explain the feature of inflation. In this paper, we consider the M-theory effective action which consists of 11-dimensional supergravity and (Weyl)<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>4</mn></msup></semantics></math></inline-formula> terms. The equations of motion are solved perturbatively, and the solution describes the inflation-like expansion in 4-dimensional spacetime. Equations of motion for tensor perturbations around this background are derived perturbatively. We also check that the equations of motion are obtained from the effective action up to the second order of the perturbations. Finally, we solve the equations of motion for the tensor perturbations perturbatively and obtain analytic expressions for them. |
format |
article |
author |
Kazuho Hiraga Yoshifumi Hyakutake |
author_facet |
Kazuho Hiraga Yoshifumi Hyakutake |
author_sort |
Kazuho Hiraga |
title |
Cosmological Perturbations via Quantum Corrections in M-Theory |
title_short |
Cosmological Perturbations via Quantum Corrections in M-Theory |
title_full |
Cosmological Perturbations via Quantum Corrections in M-Theory |
title_fullStr |
Cosmological Perturbations via Quantum Corrections in M-Theory |
title_full_unstemmed |
Cosmological Perturbations via Quantum Corrections in M-Theory |
title_sort |
cosmological perturbations via quantum corrections in m-theory |
publisher |
MDPI AG |
publishDate |
2021 |
url |
https://doaj.org/article/77e596c7150c483693a045e45deae01a |
work_keys_str_mv |
AT kazuhohiraga cosmologicalperturbationsviaquantumcorrectionsinmtheory AT yoshifumihyakutake cosmologicalperturbationsviaquantumcorrectionsinmtheory |
_version_ |
1718410224593797120 |