Fetching the paper…

Reading the bibliography…

Signatures of primordial black hole dark matter · Around

2014

Signatures of primordial black hole dark matter

Belotsky, K. M., Dmitriev, A. D., Esipova, E. A. et al.

Original
PDF
Post on X

Understand

The nonbaryonic dark matter of the Universe is assumed to consist of new stable forms of matter.

Their stability reflects symmetry of micro world and mechanisms of its symmetry breaking.
In the early Universe heavy metastable particles can dominate, leaving primordial black holes (PBHs) after their decay, as well as the structure of particle symmetry breaking gives rise to cosmological phase transitions, from which massive black holes and/or their clusters can originate.
PBHs can be formed in such transitions within a narrow interval of masses about $10^{17}$g and, avoiding severe observational constraints on PBHs, can be a candidate for the dominant form of dark matter.

Built on

S. W. Hawking, Comm. Math. Phys
1975
Earlier work this paper cites.
D. N. Page and S. W. Hawking, Astrophys. J
1976
Earlier work this paper cites.
M. Y. Khlopov and A. G. Polnarev, Phys. Lett. B
1980
Earlier work this paper cites.
L. A. Kofman and A. D. Linde, Nucl. Phys
1987
Earlier work this paper cites.
V. S. Berezinsky and V. L. Ginzburg, Astrophysics of cosmic rays
1990
Earlier work this paper cites.
R. A. Cameron et al
1992
Earlier work this paper cites.
A. S. Sakharov and M. Y. Khlopov, Phys. of Atom. Nucl
1993
Earlier work this paper cites.
R. V. Konoplich, et al
1999
Earlier work this paper cites.
S. G. Rubin, M. Y. Khlopov, and A. S. Sakharov, Grav. Cosmol
2000
Earlier work this paper cites.
S. G. Rubin, A. S. Sakharov, and M. Y. Khlopov, Sov. Phys. JETP
2001
Earlier work this paper cites.
H.-C. Cheng, et al
2002
Earlier work this paper cites.

Similar

M. R. Douglas, JHEP
2003
Cited alongside, same era.
S. G. Rubin, Grav. Cosmol
2003
Cited alongside, same era.
V. I. Dokuchaev and Y. N. Eroshenko, AApTr
2003
Cited alongside, same era.
C. Winkler et al
2003
Cited alongside, same era.
V. I. Dokuchaev, Y. N. Eroshenko, and S. G. Rubin, Grav. Cosmol
2005
Cited alongside, same era.
G. Weidenspointner et al
2006
Cited alongside, same era.
L. Titarchuk, P. Chardonnet, Astrophys. J
2006
Cited alongside, same era.

Then

B. J. Carr, et al
2010
Later among the works it cites.
K. A. Bronnikov, S. G. Rubin, I. V. Svadkovsky, Phys. Rev. D
2010
Later among the works it cites.
A. A. Abdo et al
2010
Later among the works it cites.
A. V. Grobov et al
2011
Later among the works it cites.
K. M. Belotsky et al
2011
Later among the works it cites.
K. M. Belotsky et al
2011
Later among the works it cites.
M. Y. Khlopov, Int. J. Mod. Phys. A
2013
Later among the works it cites.
A. Belyaev, et al

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

C. Bambi, A. D. Dolgov, A. A. Petrov, Phys. Lett. B

2008

Cited alongside, same era.

V. I. Dokuchaev, Y. N. Eroshenko, and S. G. Rubin, Astronomy Reports

2008

Cited alongside, same era.

W. B. Atwood et al

2009

Cited alongside, same era.

M. Y. Khlopov, RAA

2010

Cited alongside, same era.

V. A. Gani, A. E. Dmitriev, and S. G. Rubin, in preparation

Cited in the paper.

2013

Later among the works it cites.

P. Pani and A. Loeb, JCAP

2014

Closest in time.

S. G. Rubin, arXiv: 1403.2062 [gr-qc]

2062

Closest in time.