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Phase space of modified Gauss-Bonnet gravity
Sante Carloni1, José P Mimoso2
1Centro Multidisciplinar de Astrofísica-CENTRA, Instituto Superior Tecnico-IST, Universidade de Lisboa-UL, Avenida Rovisco Pais 1, 1049-001 Lisbon, Portugal.
We explore Gauss-Bonnet gravity models for the universe's evolution. Our findings reveal conditions for cosmic acceleration and identify finite-time singularities, similar to f(R) gravity, due to higher-order equations.
Area of Science:
- Cosmology and Gravitational Physics
- Theoretical Physics
Background:
- Friedmann-Lemaître-Robertson-Walker (FLRW) spacetimes are fundamental to modern cosmology.
- Gauss-Bonnet gravity offers an extension to Einstein's general relativity, incorporating higher-order curvature terms.
Purpose of the Study:
- To investigate the dynamical evolution of non-vacuum FLRW spacetimes within Gauss-Bonnet gravity.
- To identify conditions leading to cosmic acceleration and analyze the phase space of these theories.
Main Methods:
- Development and application of a novel method to explore the phase space of Gauss-Bonnet gravity models.
- Analysis of dynamical equations to derive general conditions for specific cosmological behaviors.
Main Results:
- Demonstrated the transition from decelerating to accelerating expansion in various Gauss-Bonnet gravity models.
- Identified general conditions on the gravitational action that ensure accelerated expansion.
- Revealed the existence of finite-time singularities as attractors for specific initial conditions, analogous to f(R) gravity.
Conclusions:
- The presence of finite-time singularities in Gauss-Bonnet gravity is attributed to the fourth-order derivative terms in the field equations.
- Gauss-Bonnet gravity provides a framework for exploring diverse cosmological evolutions, including accelerated expansion.
- The study highlights the importance of higher-order gravity theories in understanding cosmic dynamics and potential instabilities.
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