Cosmological models with Yang-Mills fields

E. Elizalde; A. J. López-Revelles; S. D. Odintsov; S. Yu Vernov

doi:10.1134/S1063778813080097

Cosmological models with Yang-Mills fields

E. Elizalde, A. J. López-Revelles, S. D. Odintsov, S. Yu Vernov

Research output: Contribution to journal › Article › Research › peer-review

12 Citations (Scopus)

Abstract

Cosmological models with an SU(2) Yang-Mills field are studied. For a specific model with a minimally coupled Yang-Mills Lagrangian, which includes an arbitrary function of the second-order term and a fourth-order term, a corresponding reconstruction program is proposed. It is shown that the model with minimal coupling has no de Sitter solutions, for any nontrivial function of the second-order term. To get de Sitter solutions, a gravitational model with nonminimally coupled Yang-Mills fields is then investigated. It is shown that the model with non-minimal coupling has in fact a de Sitter solution, even in absence of the cosmological constant term. © 2013 Pleiades Publishing, Ltd.

Original language	English
Pages (from-to)	996-1003
Journal	Physics of Atomic Nuclei
Volume	76
Issue number	8
DOIs	https://doi.org/10.1134/S1063778813080097
Publication status	Published - 1 Aug 2013

Access to Document

10.1134/S1063778813080097

Fingerprint Dive into the research topics of 'Cosmological models with Yang-Mills fields'. Together they form a unique fingerprint.

Cite this

@article{2523c8fb85834c4095c9b24bd970f110,

title = "Cosmological models with Yang-Mills fields",

abstract = "Cosmological models with an SU(2) Yang-Mills field are studied. For a specific model with a minimally coupled Yang-Mills Lagrangian, which includes an arbitrary function of the second-order term and a fourth-order term, a corresponding reconstruction program is proposed. It is shown that the model with minimal coupling has no de Sitter solutions, for any nontrivial function of the second-order term. To get de Sitter solutions, a gravitational model with nonminimally coupled Yang-Mills fields is then investigated. It is shown that the model with non-minimal coupling has in fact a de Sitter solution, even in absence of the cosmological constant term. {\textcopyright} 2013 Pleiades Publishing, Ltd.",

author = "E. Elizalde and L{\'o}pez-Revelles, {A. J.} and Odintsov, {S. D.} and Vernov, {S. Yu}",

year = "2013",

month = aug,

day = "1",

doi = "10.1134/S1063778813080097",

language = "English",

volume = "76",

pages = "996--1003",

journal = "Physics of Atomic Nuclei",

issn = "1063-7788",

publisher = "Maik Nauka-Interperiodica Publishing",

number = "8",

}

TY - JOUR

T1 - Cosmological models with Yang-Mills fields

AU - Elizalde, E.

AU - López-Revelles, A. J.

AU - Odintsov, S. D.

AU - Vernov, S. Yu

PY - 2013/8/1

Y1 - 2013/8/1

N2 - Cosmological models with an SU(2) Yang-Mills field are studied. For a specific model with a minimally coupled Yang-Mills Lagrangian, which includes an arbitrary function of the second-order term and a fourth-order term, a corresponding reconstruction program is proposed. It is shown that the model with minimal coupling has no de Sitter solutions, for any nontrivial function of the second-order term. To get de Sitter solutions, a gravitational model with nonminimally coupled Yang-Mills fields is then investigated. It is shown that the model with non-minimal coupling has in fact a de Sitter solution, even in absence of the cosmological constant term. © 2013 Pleiades Publishing, Ltd.

AB - Cosmological models with an SU(2) Yang-Mills field are studied. For a specific model with a minimally coupled Yang-Mills Lagrangian, which includes an arbitrary function of the second-order term and a fourth-order term, a corresponding reconstruction program is proposed. It is shown that the model with minimal coupling has no de Sitter solutions, for any nontrivial function of the second-order term. To get de Sitter solutions, a gravitational model with nonminimally coupled Yang-Mills fields is then investigated. It is shown that the model with non-minimal coupling has in fact a de Sitter solution, even in absence of the cosmological constant term. © 2013 Pleiades Publishing, Ltd.

U2 - 10.1134/S1063778813080097

DO - 10.1134/S1063778813080097

M3 - Article

VL - 76

SP - 996

EP - 1003

JO - Physics of Atomic Nuclei

JF - Physics of Atomic Nuclei

SN - 1063-7788

IS - 8

ER -