Global asymptotic dynamics of cosmological Einsteinian cubic gravity - INSPIRE

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Global asymptotic dynamics of cosmological Einsteinian cubic gravity

Israel Quiros
(
- Guanajuato U.
)
,
Ricardo García-Salcedo
(
- CICATA-Legaria, IPN
)
,
Tame Gonzalez
(
- Guanajuato U.
)
,
Jorge Luis Morales Martínez
(
- Guanajuato U.
)
,
Ulises Nucamendi
(
- IFM-UMSNH, Michoacan and
- CINVESTAV, IPN
)

Mar 25, 2020

9 pages

Published in:

Phys.Rev.D 102 (2020) 4, 044018

Published: Aug 8, 2020

e-Print:

2003.10516 [gr-qc]

DOI:

10.1103/PhysRevD.102.044018

View in:

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Abstract: (APS)

We investigate the cosmological dynamics of an up to cubic curvature correction to general relativity (GR) known as cosmological Einsteinian cubic gravity, whose vacuum spectrum consists of the graviton exclusively. Its cosmology is well posed as an initial value problem. We are able to uncover the global asymptotic structure of the phase space of this theory. It is revealed that an inflationary, matter-dominated big bang is the global past attractor, which means that inflation is the starting point of any physically meaningful cosmic history. Given that higher-order curvature corrections to GR are assumed to influence the cosmological dynamics at early times—the high energy/large curvature limit—late-time inflation is possible only if one considers a nonvanishing cosmological constant term.

Note:

9 pages, 3 figures. A figure and several bibliographic references added. Acknowledgments modified

General relativity, alternative theories of gravity
curvature: correction
curvature: higher-order
expansion: acceleration
energy: high
inflation
cosmological constant
boundary condition
cosmological model
general relativity

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