Sterile Neutrino Dark Matter in the Galaxy (CROSBI ID 498821)
Prilog sa skupa u časopisu | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Bilić, Neven ; Tupper, G. B. ; Viollier, R. D.
engleski
Sterile Neutrino Dark Matter in the Galaxy
The accurate WMAP data [1] have recently provided us with compelling evidence that the Universe is approximately critical on the largest scale. About 73% of its total energy resides is in unclustered dark energy (perhaps in the form of a cosmological constant) and approximately 27% is in nonrelativistic dark matter which clusters gravitationally. Included in this dark matter component is between 4 and 5% of the total energy in baryonic matter, mostly in the form of dark gas and dust. About 0.5% of the total energy accounts for baryonic matter contained in stars. The total energy of the microwave background and relativistic or nonrelativistic active neutrinos is less than about 0.1% of the critical energy of the Universe today.
sterile neutrino ; dark matter
Springer Proceedings in Physics, Volume 98
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Podaci o prilogu
39-45.
2005.
nije evidentirano
objavljeno
10.1007/3-540-26798-0_4
Podaci o matičnoj publikaciji
Springer proceedings in physics
Trampetić, Josip ; Wess, Julius
Heidelberg: Springer
978-3-540-22803-5
0930-8989
Podaci o skupu
Nepoznat skup
predavanje
29.02.1904-29.02.2096