Exact solution of one-dimensional relativistic jet with relativistic equation of state

被引:7
作者
Joshi, Raj Kishor [1 ,2 ]
Chattopadhyay, Indranil [1 ]
Ryu, Dongsu [3 ]
Yadav, Lallan [2 ]
机构
[1] Aryabhatta Res Inst Observat Sci ARIES, Naini Tal 263002, India
[2] Deen Dayal Upadhyaya Gorakhpur Univ, Dept Phys, Gorakhpur 273009, Uttar Pradesh, India
[3] UNIST, Dept Phys, Sch Nat Sci, Ulsan 44919, South Korea
基金
新加坡国家研究基金会;
关键词
hydrodynamics; relativistic processes; shock waves; galaxies: jets; stars: jets; PIECEWISE PARABOLIC METHOD; ACCRETION FLOWS; HYDRODYNAMICS; MODELS; CODE;
D O I
10.1093/mnras/stab364
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the evolution of one-dimensional relativistic jets, using the exact solution of the Riemann problem for relativistic flows. For this purpose, we solve equations for the ideal special relativistic fluid composed of dissimilar particles in flat space-time and the thermodynamics of fluid is governed by a relativistic equation of state. We obtain the exact solution of jets impinging on denser ambient media. The time variation of the cross-section of the jet-head is modelled and incorporated. We present the initial condition that gives rise to a reverse shock. If the jet-head cross-section increases in time, the jet propagation speed slows down significantly and the reverse-shock may recede opposite to the propagation direction of the jet. We show that the composition of jet and ambient medium can affect the jet solution significantly. For instance, the propagation speed depends on the composition and is maximum for a pair-dominated jet, rather than a pure electron-positron or electron-proton jet. The propagation direction of the reverse-shock may also strongly depend on the composition of the jet.
引用
收藏
页码:5227 / 5244
页数:18
相关论文
共 62 条
[1]   Three-dimensional simulations of relativistic precessing jets probing the structure of superluminal sources [J].
Aloy, MA ;
Martí, JM ;
Gómez, JL ;
Agudo, N ;
Müller, E ;
Ibáñez, JM .
ASTROPHYSICAL JOURNAL, 2003, 585 (02) :L109-L112
[2]   INSTABILITIES AND NONRADIAL MOTION IN SN-1987A [J].
ARNETT, D ;
FRYXELL, B ;
MULLER, E .
ASTROPHYSICAL JOURNAL, 1989, 341 (02) :L63-L66
[3]   RIEMANN SOLVER FOR RELATIVISTIC HYDRODYNAMICS [J].
BALSARA, DS .
JOURNAL OF COMPUTATIONAL PHYSICS, 1994, 114 (02) :284-297
[4]   OVERPRESSURED COCOONS IN EXTRAGALACTIC RADIO-SOURCES [J].
BEGELMAN, MC ;
CIOFFI, DF .
ASTROPHYSICAL JOURNAL, 1989, 345 (01) :L21-L24
[5]   TWIN-EXHAUST MODEL FOR DOUBLE RADIO-SOURCES [J].
BLANDFORD, RD ;
REES, MF .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1974, 169 (03) :395-415
[6]  
Chandrasekhar S., 1938, INTRO STUDY STELLAR
[7]  
Chattopadhya I., 2013, ASTRONOMICAL SOC IND, V9, P13
[8]   Estimation of mass outflow rates from viscous relativistic accretion discs around black holes [J].
Chattopadhyay, Indranil ;
Kumar, Rajiv .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 459 (04) :3792-3811
[9]   EFFECTS OF THE COMPOSITION ON TRANSONIC PROPERTIES OF ACCRETION FLOWS AROUND BLACK HOLES [J].
Chattopadhyay, Indranil ;
Chakrabarti, Sandip K. .
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2011, 20 (09) :1597-1615
[10]   EFFECTS OF FLUID COMPOSITION ON SPHERICAL FLOWS AROUND BLACK HOLES [J].
Chattopadhyay, Indranil ;
Ryu, Dongsu .
ASTROPHYSICAL JOURNAL, 2009, 694 (01) :492-501