Pregled bibliografske jedinice broj: 83494
On the Formation of Degenerate Heavy Fermion Stars
On the Formation of Degenerate Heavy Fermion Stars // Proceedings of the 4th International Heidelberg Conference on Dark Matter in Astro and Particle Physics (DARK 2002) / Klapdor-Kleingrothaus, H. V. ; Viollier, R. D. (ur.).
Berlin : Heidelberg: Springer, 2002. str. 149-156 (predavanje, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
CROSBI ID: 83494 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
On the Formation of Degenerate Heavy Fermion Stars
Autori
Lindebaum, Robert ; Bilić, Neven ; Tupper, Gary B. ; Viollier, Raoul D.
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
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, 2002, 149-156
Skup
DARK 2002: 4th International Heidelberg Conference on Dark Matter in Astro and Particle Physics
Mjesto i datum
Cape Town, Južnoafrička Republika, 04.02.2002. - 09.02.2002
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
dark matter; selfgravitating gas; Galactic center; fermion stars
Sažetak
The dynamical formation of a compact fermion star from a cold self-gravitating Fermi gas is described using an analogy with the interacting self-gravitating Bose condensate which has the same Thomas-Fermi limit. The dissipationless formation of the compact object by ejection of matter is demonstrated numerically. These fermion stars offer an alternative for the supermassive compact dark objects at the centers of galaxies.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA