Numerical simulation of the disk dynamics around the black hole: Bondi-Hoyle accretion

Küçük Resim Yok

Tarih

2014

Dergi Başlığı

Dergi ISSN

Cilt Başlığı

Yayıncı

WORLD SCIENTIFIC PUBL CO PTE LTD

Erişim Hakkı

info:eu-repo/semantics/closedAccess

Özet

We have solved the General Relativistic Hydrodynamic (GRH) equations using the high resolution shock capturing scheme (HRSCS) to find out the dependency of the disk dynamics to the Mach number, adiabatic index, the black hole rotation parameter and the outer boundary of the computational domain around the non-rotating and rotating black holes. We inject the gas to computational domain at upstream and downstream regions at the same time with different initial conditions. It is found that variety of the mass accretion rates and shock cone structures strongly depend on Mach number and adiabatic index of the gas. The shock cones on the accretion disk are important physical mechanisms to trap existing oscillation modes, thereupon these trapped modes may generate strong X-rays observed by different X-ray satellites. Besides, our numerical approach also show that the shock cones produces the flip-flop oscillation around the black holes. The flip-flop instabilities which are monitored in our simulations may explain the erratic spin behavior of the compact objects (the black holes and neutron stars) seen from observed data.

Açıklama

Anahtar Kelimeler

Black hole, Bondi-Hoyle accretion, shock cone, instability

Kaynak

MODERN PHYSICS LETTERS A

WoS Q Değeri

Q3

Scopus Q Değeri

Q2

Cilt

29

Sayı

21

Künye