Primordial black holes from inflaton fragmentation into oscillons

Eric Cotner, Alexander Kusenko, and Volodymyr Takhistov
Phys. Rev. D 98, 083513 – Published 9 October 2018

Abstract

We show that fragmentation of the inflaton into long-lived spatially localized oscillon configurations can lead to copious production of black holes. In simple inflation models primordial black holes of sublunar mass can form, and they can account for all of the dark matter. We also explore the possibility that solar-mass primordial black holes, particularly relevant for gravitational wave astronomy, are produced from the same mechanism.

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  • Received 15 January 2018
  • Revised 5 May 2018

DOI:https://doi.org/10.1103/PhysRevD.98.083513

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Eric Cotner1,*, Alexander Kusenko1,2,†, and Volodymyr Takhistov1,‡

  • 1Department of Physics and Astronomy, University of California, Los Angeles, California 90095-1547, USA
  • 2Kavli Institute for the Physics and Mathematics of the Universe (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan

  • *ecotner@physics.ucla.edu
  • kusenko@ucla.edu
  • vtakhist@physics.ucla.edu

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Issue

Vol. 98, Iss. 8 — 15 October 2018

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