1995/12/06 by S. Samurović, Srdjan Samurovic, Samurovic, Srdjan +3
Computer Science · Physics and Astronomy · #Astrophysics (astro-ph) #Computational Physics and Python Applications #Cosmology and Gravitation Theories #FOS: Physical sciences #Scientific Research and Discoveries #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9512029
5 pages, plain TeX, also available on the Web as gzipped PostScript file at http://www.interware.it/users/rastko/decneutr.html published in "Proceedings of the First Yugoslav Conference on Spectral Line Shapes" (Publ. Obs. Astron. Belgrade No. 50 (1995), 121-125)
arxiv created 1995/12/06 · openalex publication_date 1995/12/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Using simple physical reasoning we have estimated the wavelengths and line-widths of spectral lines arising from the decays of massive neutrinos. We have, also, to some extent, discussed the possible consequences of these decays in observable astrophysical settings. We have compared our conclusions with the predictions of the decaying dark matter (DDM) model and cold + hot dark matter (\rm Cν2DM) model.