Pregled bibliografske jedinice broj: 48586
On the Formation of Degenerate Heavy Neutrino Stars
On the Formation of Degenerate Heavy Neutrino Stars // Physics Letters B, 515 (2001), 105-110 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 48586 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
On the Formation of Degenerate Heavy Neutrino Stars
Autori
Bilić, Neven ; Lindebaum, R.J. ; Tupper, G.B. ; Viollier, R.D.
Izvornik
Physics Letters B (0370-2693) 515
(2001);
105-110
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
self-gravitating; Fermi gas; Bose condensate; neutrino stars
Sažetak
The dynamics of a self-gravitating cold Fermi gas is described using the analogy with an interacting self-gravitating Bose condensate having the same Thomas-Fermi limit. The dissipationless formation of a heavy neutrino star through gravitational collapse and ejection of matter is demonstrated numerically. Such neutrino stars offer an alternative to black holes for the supermassive compact dark objects at the centers of galaxies.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus
