Large blue isocurvature spectral index signals time-dependent mass

Daniel J. H. Chung
Phys. Rev. D 94, 043524 – Published 23 August 2016

Abstract

We show that if a spectator linear isocurvature dark matter field degree of freedom has a constant mass through its entire evolution history, the maximum measurable isocurvature spectral index that is consistent with the current tensor-to-scalar ratio bound of about r0.1 is about nI2.4, even if experiments can be sensitive to a 106 contamination of the predominantly adiabatic power spectrum with an isocurvature power spectrum at the shortest observable length scales. Hence, any foreseeable future measurement of a blue isocurvature spectral index larger than 2.4 may provide nontrivial evidence for dynamical degrees of freedom with time-dependent masses during inflation. The bound is not sensitive to the details of the reheating scenario and can be made mildly smaller if r is better constrained in the future.

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  • Received 2 October 2015

DOI:https://doi.org/10.1103/PhysRevD.94.043524

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Daniel J. H. Chung1,2,*

  • 1Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA
  • 2Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA

  • *danielchung@wisc.edu

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Issue

Vol. 94, Iss. 4 — 15 August 2016

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