Nonrelativistic effective field theory for axions

Eric Braaten, Abhishek Mohapatra, and Hong Zhang
Phys. Rev. D 94, 076004 – Published 13 October 2016

Abstract

Axions can be described by a relativistic field theory with a real scalar field ϕ whose self-interaction potential is a periodic function of ϕ. Low-energy axions, such as those produced in the early Universe by the vacuum misalignment mechanism, can be described more simply by a nonrelativistic effective field theory with a complex scalar field ψ whose effective potential is a function of ψ*ψ. We determine the coefficients in the expansion of the effective potential to fifth order in ψ*ψ by matching low-energy axion scattering amplitudes. In order to describe a Bose-Einstein condensate of axions that is too dense to truncate the expansion of the effective potential in powers of ψ*ψ, we develop a sequence of systematically improvable approximations to the effective potential that resum terms of all orders in ψ*ψ.

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  • Received 5 April 2016

DOI:https://doi.org/10.1103/PhysRevD.94.076004

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Eric Braaten*, Abhishek Mohapatra, and Hong Zhang

  • Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA

  • *braaten@mps.ohio-state.edu
  • mohapatra.16@buckeyemail.osu.edu
  • zhang.5676@osu.edu

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Issue

Vol. 94, Iss. 7 — 1 October 2016

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