O(10)M primordial black holes and string axion dark matter

Keisuke Inomata, Masahiro Kawasaki, Kyohei Mukaida, Yuichiro Tada, and Tsutomu T. Yanagida
Phys. Rev. D 96, 123527 – Published 26 December 2017

Abstract

LIGO-Virgo collaboration has found black holes as heavy as M30M through the detections of the gravitational waves emitted during their mergers. Primordial black holes (PBHs) produced by inflation could be an origin of such BHs. While it is tempting to presume that these PBHs constitute all dark matter (DM), there exist a number of constraints for PBHs with O(10)M which contradict with the idea of PBHs as all DM. Also, it is known that weakly interacting massive particle (WIMP) that is a common DM candidate is almost impossible to coexist with PBHs. These observations motivate us to pursue another candidate of DM. In this paper, we assume that the string axion solving the strong CP problem makes up all DM, and discuss the coexistence of string axion DM and inflationary PBHs for LIGO events.

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  • Received 10 October 2017

DOI:https://doi.org/10.1103/PhysRevD.96.123527

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Keisuke Inomata1,2, Masahiro Kawasaki1,2, Kyohei Mukaida2, Yuichiro Tada1,2,3,4, and Tsutomu T. Yanagida2

  • 1ICRR, University of Tokyo, Kashiwa 277-8582, Japan
  • 2Kavli IPMU (WPI), UTIAS, University of Tokyo, Kashiwa 277-8583, Japan
  • 3IInstitut d’Astrophysique de Paris, UMR-7095 du CNRS, Université Pierre et Marie Curie, 98 bis bd Arago, 75014 Paris, France
  • 4Sorbonne Universités, Institut Lagrange de Paris, 98 bis bd Arago, 75014 Paris, France

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Issue

Vol. 96, Iss. 12 — 15 December 2017

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