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Sterile Neutrino Dark Matter in the Galaxy


Bilić, Neven; Tupper, G. B.; Viollier, R. D.
Sterile Neutrino Dark Matter in the Galaxy // Particle Physics and the Universe : Proceedings of the 9th Adriatic meeting, Sept. 2003, Dubrovnik / Trampetić, Josip ; Wess, Julius (ur.).
Heidelberg: Springer, 2005. str. 39-45 doi:10.1007/3-540-26798-0_4 (predavanje, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)


Naslov
Sterile Neutrino Dark Matter in the Galaxy

Autori
Bilić, Neven ; Tupper, G. B. ; Viollier, R. D.

Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni

Izvornik
Particle Physics and the Universe : Proceedings of the 9th Adriatic meeting, Sept. 2003, Dubrovnik / Trampetić, Josip ; Wess, Julius - Heidelberg : Springer, 2005, 39-45

ISBN
978-3-540-22803-5

Skup
9th Adriatic Meeting "Particle Physics and the Universe"

Mjesto i datum
Dubrovnik, Hrvatska, 04-14.09.2003

Vrsta sudjelovanja
Predavanje

Vrsta recenzije
Međunarodna recenzija

Ključne riječi
Sterile neutrino ; dark matter

Sažetak
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.

Izvorni jezik
Engleski

Znanstvena područja
Fizika

Napomena
Springer Proceedings in Physics, Volume 98



POVEZANOST RADA


Projekt / tema
0098002

Ustanove
Institut "Ruđer Bošković", Zagreb

Autor s matičnim brojem:
Nevenko Bilić, (3635)

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