Pregled bibliografske jedinice broj: 215112
Acoustic horizons in axially symmetric relativistic accretion
Acoustic horizons in axially symmetric relativistic accretion // Classical and Quantum Gravity, 23 (2006), 2371-2393 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 215112 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Acoustic horizons in axially symmetric relativistic accretion
Autori
Abraham, Hrvoje ; Bilić, Neven ; Das, T.K.
Izvornik
Classical and Quantum Gravity (0264-9381) 23
(2006);
2371-2393
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
accoustic horizon; accretion
Sažetak
Transonic accretion onto astrophysical objects is a unique example of analogue black hole realized in nature. In the framework of acoustic geometry we study axially symmetric accretion and wind of a rotating astrophysical black hole or of a neutron star assuming isentropic flow of a fluid described by a polytropic equation of state. In particular we analyze the causal structure of multitransonic configurations with two sonic points and a shock. Retarded and advanced null curves clearly demonstrate the presence of the acoustic black hole at regular sonic points and of the white hole at the shock. We calculate the analogue surface gravity and the Hawking temperature for the inner and the outer acoustic horizons.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
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