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Volumn 94, Issue 10, 2005, Pages

511 keV photons from color superconducting dark matter

Author keywords

[No Author keywords available]

Indexed keywords

DARK MATTER (DM); ELECTRON POSITRON ANNHILATION PROCESSES; ENERGY DENSITIES; NUCLEOSYNTHESIS;

EID: 18044370851     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.94.101301     Document Type: Review
Times cited : (97)

References (30)
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    • R. E. Lingenfelter and R. Ramaty, in Positron-Electron Pairs in Astrophysics, edited by M. L. Burns, A. K. Harding, and R. Ramaty, AIP Conf. Proc. No. 101 (AIP, New York, 1983), p. 267.
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    • A.R. Zhitnitsky, J. Cosmol. Astropart. Phys. 10 (2003) 010; Nucl. Phys. B (Proc. Suppl.) 124, 99 (2003); J. Phys. G 30, S513 (2004).
    • (2003) Nucl. Phys. B (Proc. Suppl.) , vol.124 , pp. 99
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    • 84860809649 scopus 로고    scopus 로고
    • A.R. Zhitnitsky, J. Cosmol. Astropart. Phys. 10 (2003) 010; Nucl. Phys. B (Proc. Suppl.) 124, 99 (2003); J. Phys. G 30, S513 (2004).
    • (2004) J. Phys. G , vol.30
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    • (1998) Phys. Lett. B , vol.422 , pp. 247
    • Alford, M.1    Rajagopal, K.2    Wilczek, F.3
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    • K. Rajagopal and F. Wilczek, hep-ph/0011333
    • K. Rajagopal and F. Wilczek, hep-ph/0011333.
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    • (2002) Theoretical Astrophysics , vol.3
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    • note
    • In such a rough estimate we assume that the transmission coefficient for a proton hitting the ball is the order of 1. As we argued in [13] the transmission can actually be strongly suppressed for the small energies due to the large reflection from the superconducting region of the bulk of the QCD ball.
  • 29
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    • W. de Boer et al., astro-ph/0408272
    • W. de Boer et al., astro-ph/0408272.


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