Dark radiation

Dark radiation (also dark electromagnetism)^[1] is a postulated type of radiation that mediates interactions of dark matter.

By analogy to the way photons mediate electromagnetic interactions between particles in the Standard Model (called baryonic matter in cosmology), dark radiation is proposed to mediate interactions between dark matter particles.^[1] Similar to dark matter particles, the hypothetical dark radiation does not interact with Standard Model particles.

There has been no notable evidence for the existence of such radiation; baryonic matter contains multiple interacting particle types, but it is not known if dark matter does. Cosmic microwave background data may indicate that the number of effective neutrino degrees of freedom is more than 3.046, which is slightly more than the standard case for 3 types of neutrino.^[2] This extra degree of freedom could arise from having a non-trivial amount of dark radiation in the universe. One possible candidate for dark radiation is the sterile neutrino.^{[citation needed]}

References

^ ^a ^b Ackerman, Lotty; et al. (2008). "Dark Matter and Dark Radiation". Physical Review D. 79 (2): 023519. arXiv:0810.5126. Bibcode:2009PhRvD..79b3519A. doi:10.1103/PhysRevD.79.023519. S2CID 10056950.
^ Archidiacono, Maria; Calabrese, Erminia; Melchiorri, Alessandro (2011). "The Case for Dark Radiation". arXiv:1109.2767v1 [astro-ph.CO].

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[Ackerman2008-1] Ackerman, Lotty; et al. (2008). "Dark Matter and Dark Radiation". Physical Review D. 79 (2): 023519. arXiv:0810.5126. Bibcode:2009PhRvD..79b3519A. doi:10.1103/PhysRevD.79.023519. S2CID 10056950.

[Archidiacono2012-2] Archidiacono, Maria; Calabrese, Erminia; Melchiorri, Alessandro (2011). "The Case for Dark Radiation". arXiv:1109.2767v1 [astro-ph.CO].

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See also

References