On the tachyon inflation
Xin-zhou Li, Dao-jun Liu, Jian-gang Hao

TL;DR
This paper analyzes tachyon inflation, highlighting differences from ordinary scalar field inflation, and demonstrates through exact solutions and perturbation calculations that tachyon fields can produce sufficient inflation.
Contribution
It provides a detailed calculation of scalar and tensor perturbations in tachyon inflation and introduces an exact solution with inverse squared potential.
Findings
Tachyon inflation can produce enough inflation via the Hamilton-Jacobi approach.
An exact solution with inverse squared potential is proposed and analyzed.
Power spectra of the tachyon inflation model are computed.
Abstract
Although the formulas of tachyon inflation correspond to those of the inflation driven by the ordinary scalar field, there is obvious difference between them, which can not be neglected. We calculate the scalar and tensor perturbation of the string theory inspired tachyon inflation, which has been widely studied recently. We also show, through the Hamilton-Jacobi approach, that the the rolling tachyon can essentially produce enough inflation. An exact solution with the inverse squared potential of tachyon field has been proposed and its power spectra has been analyzed.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Computational Physics and Python Applications · Solar and Space Plasma Dynamics
