Superbounce and loop quantum cosmology ekpyrosis from modified gravity
As is known, in modified cosmological theories of gravity many of the cosmologies which could not be generated by standard Einstein gravity, can be consistently described by F ( R ) theories. Using known reconstruction techniques, we investigate which F ( R ) theories can lead to a Hubble parameter...
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Published in: | Astrophysics and space science Vol. 359; no. 1; pp. 1 - 11 |
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Main Author: | |
Format: | Journal Article |
Language: | English |
Published: |
Dordrecht
Springer Netherlands
01-09-2015
Springer Nature B.V |
Subjects: | |
Online Access: | Get full text |
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Summary: | As is known, in modified cosmological theories of gravity many of the cosmologies which could not be generated by standard Einstein gravity, can be consistently described by
F
(
R
)
theories. Using known reconstruction techniques, we investigate which
F
(
R
)
theories can lead to a Hubble parameter describing two types of cosmological bounces, the superbounce model, related to supergravity and non-supersymmetric models of contracting ekpyrosis and also the Loop Quantum Cosmology modified ekpyrotic model. Since our method is an approximate method, we investigate the problem at large and small curvatures. As we evince, both models yield power law reconstructed
F
(
R
)
gravities, with the most interesting new feature being that both lead to accelerating cosmologies, in the large curvature approximation. The mathematical properties of the some Friedmann-Robertson-Walker spacetimes
M
, that describe superbounce-like cosmologies are also pointed out, with regards to the group of curvature collineations
C
C
(
M
)
. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0004-640X 1572-946X |
DOI: | 10.1007/s10509-015-2478-1 |