• Open Access

Neutron stars at the dark matter direct detection frontier

Nirmal Raj, Philip Tanedo, and Hai-Bo Yu
Phys. Rev. D 97, 043006 – Published 9 February 2018

Abstract

Neutron stars capture dark matter efficiently. The kinetic energy transferred during capture heats old neutron stars in the local galactic halo to temperatures detectable by upcoming infrared telescopes. We derive the sensitivity of this probe in the framework of effective operators. For dark matter heavier than a GeV, we find that neutron star heating can set limits on the effective operator cutoff that are orders of magnitude stronger than possible from terrestrial direct detection experiments in the case of spin-dependent and velocity-suppressed scattering.

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  • Received 6 August 2017

DOI:https://doi.org/10.1103/PhysRevD.97.043006

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsInterdisciplinary PhysicsParticles & Fields

Authors & Affiliations

Nirmal Raj1,*, Philip Tanedo2,†, and Hai-Bo Yu2,‡

  • 1Department of Physics, University of Notre Dame, 225 Nieuwland Hall, Notre Dame, Indiana 46556, USA
  • 2Department of Physics and Astronomy, University of California, Riverside, California 92521, USA

  • *nraj@nd.edu
  • flip.tanedo@ucr.edu
  • haiboyu@ucr.edu

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Issue

Vol. 97, Iss. 4 — 15 February 2018

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