Signatures of primordial black hole dark matter

被引：165

作者：

Belotsky, K. M. ^{[1
]}

Dmitriev, A. E. ^{[1
]}

Esipova, E. A. ^{[1
]}

Gani, V. A. ^{[1
,2
]}

Grobov, A. V. ^{[1
]}

Khlopov, M. Yu ^{[1
,3
]}

Kirillov, A. A. ^{[1
]}

Rubin, S. G. ^{[1
]}

Svadkovsky, I. V. ^{[1
]}

机构：

[1] Natl Res Nucl Univ, MEPHI Moscow Engn Phys Inst, Moscow 115409, Russia

[2] Inst Theoret & Expt Phys, Natl Res Ctr Kurchatov Inst, Moscow 117218, Russia

[3] APC Lab, F-75205 Paris 13, France

来源：

MODERN PHYSICS LETTERS A | 2014年 / 29卷 / 37期

关键词：

Elementary particles; early Universe; primordial black holes; dark matter; primordial black hole clusters; reionization of the Universe; cosmic electromagnetic radiation; indirect effects of the dark matter; LARGE-AREA TELESCOPE; SYMMETRY-BREAKING; COSMOLOGICAL TEST; CLUSTERS;

D O I：

10.1142/S0217732314400057

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 (BHs) 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. PBHs in this range of mass can give solution of the problem of reionization in the Universe at the redshift z similar to 5-10. Clusters of massive PBHs can serve as a nonlinear seeds for galaxy formation, while PBHs evaporating in such clusters can provide an interesting interpretation for the observations of point-like gamma-ray sources. Analysis of possible PBH signatures represents a universal probe for super-high energy physics in the early Universe in studies of indirect effects of the dark matter.

引用

页数：15

共 35 条

[1] FERMI LARGE AREA TELESCOPE FIRST SOURCE CATALOG [J].

Abdo, A. A. ;

Ackermann, M. ;

Ajello, M. ;

Allafort, A. ;

Antolini, E. ;

Atwood, W. B. ;

Axelsson, M. ;

Baldini, L. ;

Ballet, J. ;

Barbiellini, G. ;

Bastieri, D. ;

Baughman, B. M. ;

Bechtol, K. ;

Bellazzini, R. ;

Belli, F. ;

Berenji, B. ;

Bisello, D. ;

Blandford, R. D. ;

Bloom, E. D. ;

Bonamente, E. ;

Bonnell, J. ;

Borgland, A. W. ;

Bouvier, A. ;

Bregeon, J. ;

Brez, A. ;

Brigida, M. ;

Bruel, P. ;

Burnett, T. H. ;

Busetto, G. ;

Buson, S. ;

Caliandro, G. A. ;

Cameron, R. A. ;

Campana, R. ;

Canadas, B. ;

Caraveo, P. A. ;

Carrigan, S. ;

Casandjian, J. M. ;

Cavazzuti, E. ;

Ceccanti, M. ;

Cecchi, C. ;

Celik, Oe. ;

Charles, E. ;

Chekhtman, A. ;

Cheung, C. C. ;

Chiang, J. ;

Cillis, A. N. ;

Ciprini, S. ;

Claus, R. ;

Cohen-Tanugi, J. ;

Conrad, J. .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2010, 188 (02) :405-436

[2] Z′ at the LHC: interference and finite width effects in Drell-Yan [J].

Accomando, Elena ;

Becciolini, Diego ;

Belyaev, Alexander ;

Moretti, Stefano ;

Shepherd-Themistocleous, Claire .

JOURNAL OF HIGH ENERGY PHYSICS, 2013, (10)

[3]

[Anonymous], 2003, JHEP

[4] THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION [J].

Atwood, W. B. ;

Abdo, A. A. ;

Ackermann, M. ;

Althouse, W. ;

Anderson, B. ;

Axelsson, M. ;

Baldini, L. ;

Ballet, J. ;

Band, D. L. ;

Barbiellini, G. ;

Bartelt, J. ;

Bastieri, D. ;

Baughman, B. M. ;

Bechtol, K. ;

Bederede, D. ;

Bellardi, F. ;

Bellazzini, R. ;

Berenji, B. ;

Bignami, G. F. ;

Bisello, D. ;

Bissaldi, E. ;

Blandford, R. D. ;

Bloom, E. D. ;

Bogart, J. R. ;

Bonamente, E. ;

Bonnell, J. ;

Borgland, A. W. ;

Bouvier, A. ;

Bregeon, J. ;

Brez, A. ;

Brigida, M. ;

Bruel, P. ;

Burnett, T. H. ;

Busetto, G. ;

Caliandro, G. A. ;

Cameron, R. A. ;

Caraveo, P. A. ;

Carius, S. ;

Carlson, P. ;

Casandjian, J. M. ;

Cavazzuti, E. ;

Ceccanti, M. ;

Cecchi, C. ;

Charles, E. ;

Chekhtman, A. ;

Cheung, C. C. ;

Chiang, J. ;

Chipaux, R. ;

Cillis, A. N. ;

Ciprini, S. .

ASTROPHYSICAL JOURNAL, 2009, 697 (02) :1071-1102

[5] Primordial black holes and the observed Galactic 511 keV line [J].

Bambia, Cosimo ;

Dolgov, Alexander D. ;

Petrov, Alexey A. .

PHYSICS LETTERS B, 2008, 670 (03) :174-178

[6]

Belotsky K., ARXIV14098601

[7] Clusters of black holes as point-like gamma-ray sources [J].

Belotsky, K. M. ;

Berkov, A. V. ;

Kirillov, A. A. ;

Rubin, S. G. .

ASTROPARTICLE PHYSICS, 2011, 35 (01) :28-32

[8] Black Hole Clusters in Our Galaxy [J].

Belotsky, K. M. ;

Berkov, A. V. ;

Kirillov, A. A. ;

Rubin, S. G. .

GRAVITATION & COSMOLOGY, 2011, 17 (01) :27-30

[9]

Berezinsky V., 1990, Astrophysics of cosmic rays

[10] Multidimensional world, inflation, and modern acceleration [J].

Bronnikov, K. A. ;

Rubin, S. G. ;

Svadkovsky, I. V. .

PHYSICAL REVIEW D, 2010, 81 (08)

← 1 2 3 4 →