Gravitational waves from primordial black holes and new weak scale phenomena

Article, Preprint English OPEN
Davoudiasl, Hooman ; Giardino, Pier Paolo (2017)
  • Publisher: Elsevier
  • Journal: Physics letters B, volume 768, pages 198-202 (issn: 0370-2693, eissn: 1873-2445)
  • Related identifiers: doi: 10.1016/j.physletb.2017.02.054
  • Subject: High Energy Physics - Phenomenology | Primordial black holes | Physics | Advanced LIGO/VIRGO | Gravitational waves | Phase transition | QC1-999 | Nuclear and High Energy Physics | Astrophysics - Cosmology and Nongalactic Astrophysics
    arxiv: General Relativity and Quantum Cosmology | Astrophysics::High Energy Astrophysical Phenomena | Astrophysics::Cosmology and Extragalactic Astrophysics

We entertain the possibility that primordialblack holes of mass $\sim (10^{26}$--$10^{29})$~g, with Schwarzschild radii of $\mathcal{O}{\text{cm}}$, constitute $\sim 10\%$ or more of cosmic dark matter, as allowed by various constraints. These black holes would typicall... View more
  • References (35)
    35 references, page 1 of 4

    [1] K.A. Olive, et al., Particle Data Group Collaboration, Chin. Phys. C 38 (2014) 090001, http://dx.doi.org/10.1088/1674-1137/38/9/090001.

    [2] B.J. Carr, S.W. Hawking, Mon. Not. R. Astron. Soc. 168 (1974) 399.

    [3] P. Meszaros, Astron. Astrophys. 37 (1974) 225.

    [4] B.J. Carr, Astrophys. J. 201 (1975) 1, http://dx.doi.org/10.1086/153853.

    [5] For a review on the subject see for example M.Y. Khlopov, Res. Astron. Astrophys. 10 (2010) 495, http://dx.doi.org/10.1088/1674-4527/10/6/001, arXiv: 0801.0116 [astro-ph].

    [6] F. Capela, M. Pshirkov, P. Tinyakov, Phys. Rev. D 87 (2) (2013) 023507, http:// dx.doi.org/10.1103/PhysRevD.87.023507, arXiv:1209.6021 [astro-ph.CO]; F. Capela, M. Pshirkov, P. Tinyakov, Phys. Rev. D 87 (12) (2013) 123524, http:// dx.doi.org/10.1103/PhysRevD.87.123524, arXiv:1301.4984 [astro-ph.CO]; F. Capela, M. Pshirkov, P. Tinyakov, Phys. Rev. D 90 (8) (2014) 083507, http:// dx.doi.org/10.1103/PhysRevD.90.083507, arXiv:1403.7098 [astro-ph.CO].

    [7] K. Griest, A.M. Cieplak, M.J. Lehner, Phys. Rev. Lett. 111 (18) (2013) 181302, http://dx.doi.org/10.1103/PhysRevLett.111.181302.

    [8] B. Carr, F. Kuhnel, M. Sandstad, arXiv:1607.06077 [astro-ph.CO].

    [9] H. Niikura, et al., arXiv:1701.02151 [astro-ph.CO].

    [10] K. Jedamzik, Phys. Rev. D 55 (1997) 5871, http://dx.doi.org/10.1103/PhysRevD. 55.5871, arXiv:astro-ph/9605152; K. Jedamzik, J.C. Niemeyer, Phys. Rev. D 59 (1999) 124014, http://dx.doi.org/ 10.1103/PhysRevD.59.124014, arXiv:astro-ph/9901293.

  • Metrics
    No metrics available
Share - Bookmark