Cosmological aspects of cubic Galileon massive gravity

@article{Aslmarand2021CosmologicalAO,
  title={Cosmological aspects of cubic Galileon massive gravity},
  author={Shahabeddin Mostafanazhad Aslmarand and Amin Rezaei Akbarieh and Yousef Izadi and Sobhan Kazempour and Lijing Shao},
  journal={Physical Review D},
  year={2021}
}
Shahabeddin M. Aslmarand, ∗ Amin Rezaei Akbarieh, † Yousef Izadi, ‡ Sobhan Kazempour, § and Lijing Shao ¶ Department of Physics, Florida Atlantic University, Boca Raton, FL 33431, USA Faculty of Physics, University of Tabriz, Tabriz 51666-16471, Iran Department of Physics and Applied Physics, University of Massachusetts, Lowell, MA 01854, USA Faculty of Physics, University of Tabriz, Tabriz 51666-16471, Iran Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871… Expand

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References

SHOWING 1-10 OF 65 REFERENCES
A new quasidilaton theory of massive gravity
We present a new quasidilaton theory of Poincare invariant massive gravity, based on the recently proposed framework of matter coupling that makes it possible for the kinetic energy of theExpand
Nonlinear stability of cosmological solutions in massive gravity
We investigate nonlinear stability of two classes of cosmological solutions in massive gravity: isotropic Friedmann-Lemaitre-Robertson-Walker (FLRW) solutions and anisotropic FLRW solutions. For thisExpand
Galileon inflation
Galileon inflation is a radiatively stable higher derivative model of inflation. The model is determined by a finite number of relevant operators which are protected by a covariant generalization ofExpand
The Confrontation between General Relativity and Experiment
  • C. Will
  • Physics, Medicine
  • Living reviews in relativity
  • 2001
TLDR
Tests of general relativity at the post-Newtonian level have reached high precision, including the light defl ection the Shapiro time delay, the perihelion advance of Mercury, and the Nordtvedt effect in lunar motion. Expand
Initial conditions for the Galileon dark energy
Galileon models are among the most appealing candidates for Dark Energy. The reason is twofold: classically, they provide a tracking solution leading to an almost DeSitter space starting from veryExpand
Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive gravity
Abstract Motivated by the recent no-go result of homogeneous and isotropic solutions in the nonlinear massive gravity, we study fixed points of evolution equations for a Bianchi type-I universe. WeExpand
Testing general relativity with present and future astrophysical observations
One century after its formulation, Einstein's general relativity (GR) has made remarkable predictions and turned out to be compatible with all experimental tests. Most of these tests probe the theoryExpand
Future supernovae data and quintessence models
The possibility of unambiguously determining the equation of state of the cosmic dark energy with existing and future supernovae data is investigated. We consider four evolution laws for thisExpand
Dark Energy and the Accelerating Universe
Ten years ago, the discovery that the expansion of the universe is accelerating put in place the last major building block of the present cosmological model, in which the universe is composed of 4%Expand
Strong Interactions and Stability in the DGP Model
The model of Dvali, Gabadadze, and Porrati (DGP) gives a simple geometrical setup in which gravity becomes 5-dimensional at distances larger than a length scale lambda(DGP). We show that this theoryExpand
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