Dynamics of ultrarelativistic jets
Küçük Resim Yok
Tarih
2007
Yazarlar
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
AMER INST PHYSICS
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
We investigate the dynamics and morphology of jets propagating into the interstellar medium using 2D special relativistic hydrodynamics code. The calculations are performed assuming axisymmetric geometry and trace a long propagation of jets. The jets are assumed to be higher density than the ambient gas. The relativistic astrophysical jet is modeled for ultrarelativistic flow case. The dynamics of jet flowing is then determined by the ambient parameters such as densities, and velocities of the jets and the momentum impulse applied to the computational surface. We obtain solutions for the jet structure, propagation of jet during the time evolution, and variation in the Mach number, pressure and Lorentz factor on the computational domain at a fixed time.
Açıklama
6th International Conference of the Balkan-Physical-Union -- AUG 22-26, 2006 -- Istanbul, TURKEY
Anahtar Kelimeler
relativistic hydrodynamics, jets, numerical relativity, shock wave
Kaynak
SIX INTERNATIONAL CONFERENCE OF THE BALKAN PHYSICAL UNION
WoS Q Değeri
N/A
Scopus Q Değeri
N/A
Cilt
899
