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