Dark Matter in the Halo of the Galaxy (CROSBI ID 483844)
Prilog sa skupa u zborniku | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Bilić, Neven ; Tupper, Gary B. ; Viollier, Raoul D.
engleski
Dark Matter in the Halo of the Galaxy
We consider a self-gravitating noninteracting fermion gas at nonzero temperature as a model for the dark matter halo of the Galaxy. This fermion gas model is then shown to imply the existence of a supermassive compact dark object at the Galactic center.
dark matter; selfgravitating gas; Galactic center; Galactic halo
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Podaci o prilogu
164-172-x.
2002.
objavljeno
Podaci o matičnoj publikaciji
Proceedings of the 4th International Heidelberg Conference on Dark Matter in Astro and Particle Physics (DARK 2002)
Klapdor-Kleingrothaus, H. V. ; Viollier, R. D.
Berlin : Heidelberg: Springer
Podaci o skupu
DARK 2002: 4th International Heidelberg Conference on Dark Matter in Astro and Particle Physics
predavanje
04.02.2002-09.02.2002
Cape Town, Južnoafrička Republika
