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$\mathcal O(10) M_\odot$ primordial black holes and string axion dark matter
Keisuke Inomata, Masahiro Kawasaki, Kyohei Mukaida, Yuichiro Tada, Tsutomu T. Yanagida

$\mathcal O(10) M_\odot$ primordial black holes and string axion dark matter

Science & Mathematics Published 2017 Verification Pending

Overview & Synopsis

LIGO-Virgo collaboration has found black holes as heavy as M∼30M⊙ 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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Document Information

Document Title $\mathcal O(10) M_\odot$ primordial black holes and string axion dark matter
Author / Organization Keisuke Inomata, Masahiro Kawasaki, Kyohei Mukaida, Yuichiro Tada, Tsutomu T. Yanagida
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2017
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-45559
Original Source Link Visit Source Page on hal.science »