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Title: Primordial extremal black holes as dark matter

Abstract

We show that primordial (nearly) extremal black holes with a wide range of masses from the Planck scale to around 109 g could be cosmologically stable and provide a viable explanation for dark matter, given a dark electromagnetism and a heavy dark electron. Hawking radiation and Schwinger discharge processes are suppressed by near extremality and the heaviness of the dark electron, respectively. The merger events of binary systems with opposite charges generate nonextremal black holes, whose subsequent Hawking evaporation produces transient neutrino and gamma ray signals to be observed at telescopes like IceCube and HAWC. The relationship between the near-extremal black hole and dark electron masses could also shed light on the weak gravity conjecture.

Authors:
; ORCiD logo
Publication Date:
Research Org.:
Univ. of Wisconsin, Madison, WI (United States)
Sponsoring Org.:
USDOE Office of Science (SC); National Science Foundation (NSF)
OSTI Identifier:
1603200
Alternate Identifier(s):
OSTI ID: 1803133
Grant/Contract Number:  
SC0017647; PHY-1066293
Resource Type:
Published Article
Journal Name:
Physical Review D
Additional Journal Information:
Journal Name: Physical Review D Journal Volume: 101 Journal Issue: 5; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; Physics

Citation Formats

Bai, Yang, and Orlofsky, Nicholas. Primordial extremal black holes as dark matter. United States: N. p., 2020. Web. doi:10.1103/PhysRevD.101.055006.
Bai, Yang, & Orlofsky, Nicholas. Primordial extremal black holes as dark matter. United States. https://doi.org/10.1103/PhysRevD.101.055006
Bai, Yang, and Orlofsky, Nicholas. Wed . "Primordial extremal black holes as dark matter". United States. https://doi.org/10.1103/PhysRevD.101.055006.
@article{osti_1603200,
title = {Primordial extremal black holes as dark matter},
author = {Bai, Yang and Orlofsky, Nicholas},
abstractNote = {We show that primordial (nearly) extremal black holes with a wide range of masses from the Planck scale to around 109 g could be cosmologically stable and provide a viable explanation for dark matter, given a dark electromagnetism and a heavy dark electron. Hawking radiation and Schwinger discharge processes are suppressed by near extremality and the heaviness of the dark electron, respectively. The merger events of binary systems with opposite charges generate nonextremal black holes, whose subsequent Hawking evaporation produces transient neutrino and gamma ray signals to be observed at telescopes like IceCube and HAWC. The relationship between the near-extremal black hole and dark electron masses could also shed light on the weak gravity conjecture.},
doi = {10.1103/PhysRevD.101.055006},
journal = {Physical Review D},
number = 5,
volume = 101,
place = {United States},
year = {Wed Mar 04 00:00:00 EST 2020},
month = {Wed Mar 04 00:00:00 EST 2020}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1103/PhysRevD.101.055006

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Cited by: 29 works
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