Producing massive sterile neutrinos as warm Dark Matter

dc.creatorDolgov, A. D.
dc.creatorHansen, S. H.
dc.date2001-03-12
dc.date2001-06-27
dc.date.accessioned2026-07-07T03:44:11Z
dc.date.available2026-07-07T03:44:11Z
dc.descriptionThis paper has been withdrawn by the authors. This paper started with a wrong term describing elastic scattering. The correct form of the kinetic equations for the density matrix are derived e.g. in A. Dolgov, Yad. Fiz. 33 (1981) 1309; K. Enqvist, K. Kainulainen and J. Maalampi, Nucl. Phys. B 349 (1991) 754; G. Sigl and G. Raffelt, Nucl. Phys. B 406 (1993) 423. When using the correct form of the kinetic equations, the result is in good agreement with old results, A. Dolgov and S. Hansen, hep-ph/0009083.
dc.descriptionThis paper has been withdrawn by the authors. This paper started with a wrong term describing elastic scattering. The correct form of the kinetic equations for the density matrix are derived e.g. in A. Dolgov, Yad. Fiz. 33 (1981) 1309; K. Enqvist, K. Kainulainen and J. Maalampi, Nucl. Phys. B 349 (1991) 754; G. Sigl and G. Raffelt, Nucl. Phys. B 406 (1993) 423. When using the correct form of the kinetic equations, the result is in good agreement with old results, A. Dolgov and S. Hansen, hep-ph/0009083
dc.identifierhttps://arxiv.org/abs/hep-ph/0103118
dc.identifierhttp://arxiv.org/abs/hep-ph/0103118
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40460
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleProducing massive sterile neutrinos as warm Dark Matter
dc.typetext

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