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

Inomata, Keisuke; Kawasaki, Masahiro; Mukaida, Kyohei; Tada, Yuichiro; Yanagida, Tsutomu T.

doi:10.1103/PhysRevD.96.123527

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

Keisuke Inomata
(
- Tokyo U., ICRR and
- Tokyo U., IPMU
)
,
Masahiro Kawasaki
(
- Tokyo U., ICRR and
- Tokyo U., IPMU
)
,
Kyohei Mukaida
(
- Tokyo U., IPMU
)
,
Yuichiro Tada
(
- Tokyo U., ICRR and
- Tokyo U., IPMU and
- Paris, Inst. Astrophys. and
- ILP, Paris
)
,
Tsutomu T. Yanagida
(
- Tokyo U., IPMU
)

Sep 22, 2017

13 pages

Published in:

Phys.Rev.D 96 (2017) 12, 123527

Published: Dec 26, 2017

e-Print:

1709.07865 [astro-ph.CO]

DOI:

10.1103/PhysRevD.96.123527

Report number:

IPMU-17-0133

View in:

pdf

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Abstract: (APS)

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.

Note:

12 pages, 8 figures; v2: published version

axion: string
axion
dark matter
black hole: primordial
gravitational radiation: emission
strong interaction: CP
inflation
WIMP
O(10)
LIGO

References(108)

Figures(8)

[1]

The QCD axion and moduli stabilisation

Joseph P. Conlon
(
- Cambridge U., DAMTP
)

- JHEP 05 (2006) 078
•
e-Print:
- hep-th/0602233
•
DOI:
- 10.1088/1126-6708/2006/05/078

[2]

Axions In String Theory

Peter Svrcek
(
- Stanford U., Phys. Dept. and
- SLAC
)
,
Edward Witten
(
- Princeton, Inst. Advanced Study
)

- JHEP 06 (2006) 051
•
e-Print:
- hep-th/0605206
•
DOI:
- 10.1088/1126-6708/2006/06/051

[3]

String theoretic QCD axion with stabilized saxion and the pattern of supersymmetry breaking

Kiwoon Choi
(
- KAIST, Taejon
)
,
Kwang Sik Jeong
(
- KAIST, Taejon
)

- JHEP 01 (2007) 103
•
e-Print:
- hep-th/0611279
•
DOI:
- 10.1088/1126-6708/2007/01/103

[4]

Can decaying particles raise the upper bound on the Peccei-Quinn scale?

- Phys.Lett.B 383 (1996) 313-316
•
e-Print:
- hep-ph/9510461
•
DOI:
- 10.1016/0370-2693(96)00743-5

[5]

Cosmological problems of the string axion alleviated by high scale SUSY of $m_{3/2}$ $\simeq$ 10–100TeV

Masahiro Kawasaki
(
- Tokyo U., ICRR and
- Tokyo U., IPMU
)
,
Tsutomu T. Yanagida
(
- Tokyo U., IPMU
)
,
Norimi Yokozaki
(
- INFN, Rome
)

- Phys.Lett.B 753 (2016) 389-394
•
e-Print:
- 1510.04171
•
DOI:
- 10.1016/j.physletb.2015.12.043

[6]

Are isocurvature fluctuations of the M theory axion observable?

M. Kawasaki
(
- Tokyo U., ICRR
)
,
T. Yanagida
(
- Tokyo U.
)

- Prog.Theor.Phys. 97 (1997) 809-812
•
e-Print:
- hep-ph/9703261
•
DOI:
- 10.1143/PTP.97.809

[7]

Initial conditions for inflation — A short review

Robert Brandenberger
(
- McGill U. and
- Zurich, ETH
)

- Int.J.Mod.Phys.D 26 (2016) 01, 1740002
•
e-Print:
- 1601.01918
•
DOI:
- 10.1142/S0218271817400028

[8]

De Sitter vacua in string theory

Shamit Kachru
(
- Stanford U., Phys. Dept. and
- SLAC
)
,
Renata Kallosh
(
- Stanford U., Phys. Dept.
)
,
Andrei D. Linde
(
- Stanford U., Phys. Dept.
)
,
Sandip P. Trivedi
(
- Tata Inst.
)

- Phys.Rev.D 68 (2003) 046005
•
e-Print:
- hep-th/0301240
•
DOI:
- 10.1103/PhysRevD.68.046005

[9]

A Framework for the landscape

- Phys.Rev.D 70 (2004) 126007
•
e-Print:
- hep-th/0408133
•
DOI:
- 10.1103/PhysRevD.70.126007

[10]

The Anthropic landscape of string theory

Leonard Susskind
(
- Stanford U., Phys. Dept.
)

•
e-Print:
- hep-th/0302219

[11]

Quantization of four form fluxes and dynamical neutralization of the cosmological constant

- JHEP 06 (2000) 006
•
e-Print:
- hep-th/0004134
•
DOI:
- 10.1088/1126-6708/2000/06/006

[12]

Dynamical tuning of the initial condition for new inflation in supergravity

- Phys.Lett.B 411 (1997) 249-255
•
e-Print:
- hep-ph/9707201
•
DOI:
- 10.1016/S0370-2693(97)01040-X

[13]

Observation of Gravitational Waves from a Binary Black Hole Merger

LIGO Scientific and
Virgo

Collaborations

•

B.P. Abbott
(
- Caltech
)

et al.

- Phys.Rev.Lett. 116 (2016) 6, 061102
•
e-Print:
- 1602.03837
•
DOI:
- 10.1103/PhysRevLett.116.061102

[14]

GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

LIGO Scientific and
Virgo

Collaborations

•

B. P. Abbott
(
- LIGO Lab., Caltech
)

et al.

- Phys.Rev.Lett. 116 (2016) 24, 241103
•
e-Print:
- 1606.04855
•
DOI:
- 10.1103/PhysRevLett.116.241103

[15]

GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

LIGO Scientific and
VIRGO

Collaborations

•

Benjamin P. Abbott
(
- LIGO Lab., Caltech
)

et al.

- Phys.Rev.Lett. 118 (2017) 22, 221101,
- Phys.Rev.Lett. 121 (2018) 12, 129901 (erratum)
•
e-Print:
- 1706.01812
•
DOI:
- 10.1103/PhysRevLett.118.221101

[16]

Astrophysical Implications of the Binary Black-Hole Merger GW150914

LIGO Scientific and
Virgo

Collaborations

•

B.P. Abbott
(
- Caltech
)

et al.

- Astrophys.J.Lett. 818 (2016) 2, L22
•
e-Print:
- 1602.03846
•
DOI:
- 10.3847/2041-8205/818/2/L22

[17]

On The Maximum Mass of Stellar Black Holes

et al.

- Astrophys.J. 714 (2010) 1217-1226
•
e-Print:
- 0904.2784
•
DOI:
- 10.1088/0004-637X/714/2/1217

[18]

The mass spectrum of compact remnants from the PARSEC stellar evolution tracks

Mario Spera
(
- Padua Observ.
)
,
Michela Mapelli
(
- Padua Observ. and
- INFN, Milan Bicocca
)
,
Alessandro Bressan
(
- SISSA, Trieste and
- Padua Observ.
)

- Mon.Not.Roy.Astron.Soc. 451 (2015) 4, 4086-4103
•
e-Print:
- 1505.05201
•
DOI:
- 10.1093/mnras/stv1161

[19]

Did LIGO detect dark matter?

Simeon Bird
(
- Johns Hopkins U.
)
,
Ilias Cholis
(
- Johns Hopkins U.
)
,
Julian B. Muñoz
(
- Johns Hopkins U.
)
,
Yacine Ali-Haïmoud
(
- Johns Hopkins U.
)
,
Marc Kamionkowski
(
- Johns Hopkins U.
)

et al.

- Phys.Rev.Lett. 116 (2016) 20, 201301
•
e-Print:
- 1603.00464
•
DOI:
- 10.1103/PhysRevLett.116.201301

[20]

The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO

Sebastien Clesse
(
- RWTH Aachen U.
)
,
Juan García-Bellido
(
- Madrid, IFT
)

- Phys.Dark Univ. 15 (2017) 142-147
•
e-Print:
- 1603.05234
•
DOI:
- 10.1016/j.dark.2016.10.002

[21]

Primordial Black Hole Scenario for the Gravitational-Wave Event GW150914

Misao Sasaki
(
- Kyoto U., Yukawa Inst., Kyoto
)
,
Teruaki Suyama
(
- Tokyo U., RESCEU
)
,
Takahiro Tanaka
(
- Kyoto U.
)
,
Shuichiro Yokoyama
(
- Rikkyo U.
)

- Phys.Rev.Lett. 117 (2016) 6, 061101,
- Phys.Rev.Lett. 121 (2018) 5, 059901 (erratum)
•
e-Print:
- 1603.08338
•
DOI:
- 10.1103/PhysRevLett.117.061101