Thermal inflation with a thermal waterfall scalar field coupled to a light spectator scalar field

Konstantinos Dimopoulos, David H. Lyth, and Arron Rumsey
Phys. Rev. D 95, 103503 – Published 11 May 2017

Abstract

A new model of thermal inflation is introduced, in which the mass of the thermal waterfall field is dependent on a light spectator scalar field. Using the δN formalism, the “end of inflation” scenario is investigated in order to ascertain whether this model is able to produce the dominant contribution to the primordial curvature perturbation. A multitude of constraints are considered so as to explore the parameter space, with particular emphasis on key observational signatures. For natural values of the parameters, the model is found to yield a sharp prediction for the scalar spectral index and its running, well within the current observational bounds.

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  • Received 14 March 2017

DOI:https://doi.org/10.1103/PhysRevD.95.103503

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Konstantinos Dimopoulos*, David H. Lyth, and Arron Rumsey

  • Consortium for Fundamental Physics, Physics Department, Lancaster University, Lancaster LA1 4YB, United Kingdom

  • *konst.dimopoulos@lancaster.ac.uk
  • d.lyth@lancaster.ac.uk
  • a.rumsey@lancaster.ac.uk

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Issue

Vol. 95, Iss. 10 — 15 May 2017

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