Comprehensive asymmetric dark matter model

Article, Preprint English OPEN
Lonsdale, Stephen J. ; Volkas, Raymond R. (2018)
  • Publisher: APS
  • Journal: Physical Review D (issn: 2470-0029)
  • Related identifiers: doi: 10.1103/PhysRevD.97.103510
  • Subject: High Energy Physics - Phenomenology
    arxiv: High Energy Physics::Phenomenology | Astrophysics::Cosmology and Extragalactic Astrophysics

Asymmetric dark matter (ADM) is motivated by the similar cosmological mass densities measured for ordinary and dark matter. We present a comprehensive theory for ADM that addresses the mass density similarity, going beyond the usual ADM explanations of similar number de... View more
  • References (110)
    110 references, page 1 of 11

    [1] P. A. R. Ade et al. (Planck), Astron. Astrophys. 594, A13 (2016).

    [2] H. Davoudiasl and R. N. Mohapatra, New J. Phys. 14, 095011 (2012).

    [3] K. Petraki and R. R. Volkas, Int. J. Mod. Phys. A 28, 1330028 (2013).

    [4] K. M. Zurek, Phys. Rep. 537, 91 (2014).

    [5] T. Lee and C.-N. Yang, Phys. Rev. 104, 254 (1956).

    [6] I. Kobzarev, L. Okun, and I. Pomeranchuk, Sov. J. Nucl. Phys. 3, 837 (1966).

    [7] M. Pavsic, Int. J. Theor. Phys. 9, 229 (1974).

    [8] S. Blinnikov and M. Y. Khlopov, Sov. J. Nucl. Phys. 36, 472 (1982).

    [9] S. Blinnikov and M. Khlopov, Sov. Astron. Lett. 27, 371 (1983).

    [10] R. Foot, H. Lew, and R. Volkas, Phys. Lett. B 272, 67 (1991).

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