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PBH dark matter from axion inflation

Valerie Domcke
(
- APC, Paris
)
,
Francesco Muia
(
- Oxford U., Theor. Phys.
)
,
Mauro Pieroni
(
- APC, Paris
)
,
Lukas T. Witkowski
(
- APC, Paris
)

Apr 11, 2017

42 pages

Published in:

JCAP 07 (2017) 048

Published: Jul 27, 2017

e-Print:

1704.03464 [astro-ph.CO]

DOI:

10.1088/1475-7516/2017/07/048

View in:

reference search104 citations

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Abstract: (arXiv)

Protected by an approximate shift symmetry, axions are well motivated candidates for driving cosmic inflation. Their generic coupling to the Chern-Simons term of any gauge theory gives rise to a wide range of potentially observable signatures, including equilateral non-Gaussianites in the CMB, chiral gravitational waves in the range of direct gravitational wave detectors and primordial black holes (PBHs). In this paper we revisit these predictions for axion inflation models non-minimally coupled to gravity. Contrary to the case of minimally coupled models which typically predict scale-invariant mass distributions for the generated PBHs at small scales, we demonstrate how broadly peaked PBH spectra naturally arises in this setup. For specific parameter values, all of dark matter can be accounted for by PBHs.

Note:

33 pages plus appendices, 9 figures

inflation: model
black hole: primordial
coupling: minimal
axion
dark matter
gravitational radiation detector
cosmic background radiation
gravitational radiation
gravitational radiation: emission
gauge field theory

References(153)

Figures(13)

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