Tachyon constant-roll inflation
arXiv:1801.03487 · doi:10.1103/PhysRevD.97.083006
Abstract
The constant-roll inflation is studied where the inflaton is taken as a tachyon field. Since in this approach the second slow-roll parameter is assumed to be of order one instead of being small, then the perturbation parameters will be considered again. The results are compared with observational data, and it is confirmed that the model could stand as a proper candidate for inflation.
16 pages, 8 figures, Typos corrected, references added
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- Tsallis holographic dark energy for inflation
- Warm Tachyon Inflation and Swampland Criteria
- Holographic realization of constant roll inflation and dark energy: An unified scenario
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- Observational constraints on DBI constant-roll inflation
- Brane inflation and Trans-Planckian censorship conjecture
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- Natural Inflation with non minimal coupling to gravity in gravity under the Palatini formalism
- Generalizing the Constant-roll Condition in Scalar Inflation
- Holographic warm inflation
- Tsallis holographic inflation in gravity: CMB constraints, reheating, and swampland implications
- Analytical Insights into Constant-Roll Condition: Extending the Paradigm to Non-Canonical Models
- Constant-roll inflation with tachyon field in the holographic braneworld
- Tachyon constant-roll inflation in Randall-Sundrum II cosmology
- Constant Roll Inflationary Dynamics with Generalized Potentials in Gravity
- Can Gibbons-Hawking Radiation and Inflation Arise Due to Spacetime Quanta?