Stability of a noncanonical scalar field model during cosmological date
From MaRDI portal
Publication:1682330
DOI10.1155/2016/3047461zbMath1375.83068arXiv1512.05571OpenAlexW2220165915WikidataQ59121811 ScholiaQ59121811MaRDI QIDQ1682330
T. Golanbari, Khaled Saaidi, Haidar Sheikhahmadi, Z. Ossoulian
Publication date: 30 November 2017
Published in: Advances in High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1512.05571
Cites Work
- Chameleon mechanism with a new potential
- Strong and weak gravitational field in \(R+\mu ^{4}/R\) gravity
- The generalized second law for the interacting new agegraphic dark energy in a non-flat FRW universe enclosed by the dynamical apparent horizon
- Spherical symmetric solution in \(f(R)\) model around charged black hole
- Cosmological constant -- the weight of the vacuum
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Non-commutative and commutative vacua effects in a scalar torsion scenario
- The cosmological constant and dark energy
- Mach's Principle and a Relativistic Theory of Gravitation
- SPACE–TIME IN LIGHT OF KÁROLYHÁZY UNCERTAINTY RELATION
- Effective Field Theory, Black Holes, and the Cosmological Constant
- Cosmological parameters from SDSS and WMAP
- The world as a hologram
- Modified gravity as an alternative for ΛCDM cosmology
- FIELD THEORY OF TACHYON MATTER
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Inflationary universe: A possible solution to the horizon and flatness problems
- QCD phase transition with a power law chameleon scalar field in the bulk
- The cosmological constant problem
- Mach's Principle and a Relativistic Theory of Gravitation. II