TACHYONIC UNIVERSES IN PATCH COSMOLOGIES WITH Ω > 1
DOI10.1142/S0217732309030849zbMath1181.83262arXiv0808.2830OpenAlexW2004955499MaRDI QIDQ3401051
Ramón Herrera, Joel Saavedra, Pedro Labraña, Sergio del Campo, Carlos Leiva
Publication date: 28 January 2010
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0808.2830
Relativistic cosmology (83F05) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Radiative transfer in astronomy and astrophysics (85A25)
Cites Work
- On the cosmological relevance of the tachyon
- Inflation from a tachyon fluid?
- Closed inflationary universe with tachyonic field
- Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects
- Non-conventional cosmology from a brane universe
- Cosmological evolution of the rolling tachyon
- Israel conditions for the Gauss-Bonnet theory and the Friedmann equation on the brane universe
- Extended open inflationary universes
- An Alternative to Compactification
- Finite Temperature Systems of Brane-Antibrane Pairs and Non-BPS D-Branes
- General Gauss Bonnet brane cosmology
- Inflationary attractor in Gauss–Bonnet brane cosmology
- CLOSED INFLATIONARY UNIVERSE MODELS IN BRANE WORLD COSMOLOGY
- Extended closed inflationary universes
- Inflationary universe: A possible solution to the horizon and flatness problems
- A NOTE ON THE STRUCTURAL STABILITY OF TACHYONIC INFLATION
This page was built for publication: TACHYONIC UNIVERSES IN PATCH COSMOLOGIES WITH Ω > 1
