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Sterile Neutrino Dark Matter in the Galaxy (CROSBI ID 498821)

Prilog sa skupa u časopisu | izvorni znanstveni rad | međunarodna recenzija

Bilić, Neven ; Tupper, G. B. ; Viollier, R. D. Sterile Neutrino Dark Matter in the Galaxy // Springer proceedings in physics / Trampetić, Josip ; Wess, Julius (ur.). 2005. str. 39-45 doi: 10.1007/3-540-26798-0_4

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

Povezanost rada

Fizika

Poveznice