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Numerical hydrodynamics of relativis...

Choi, Eunwoo.

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Numerical hydrodynamics of relativistic extragalactic jets.

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Numerical hydrodynamics of relativistic extragalactic jets./
作者:	Choi, Eunwoo.
面頁冊數:	139 p.
附註:	Adviser: Paul J. Wiita.
Contained By:	Dissertation Abstracts International68-04B.
標題:	Physics, Theory. -
電子資源:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3260554

Numerical hydrodynamics of relativistic extragalactic jets.
Choi, Eunwoo.

Numerical hydrodynamics of relativistic extragalactic jets. - 139 p.

Adviser: Paul J. Wiita.

Thesis (Ph.D.)--Georgia State University, 2007.

Index words. Extragalactic jets, Hydrodynamics, Numerical methods, Special relativitySubjects--Topical Terms:

1019422
Physics, Theory.

Numerical hydrodynamics of relativistic extragalactic jets.
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035 $a (UMI)AAI3260554
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100 1 $a Choi, Eunwoo. $3 1266203
245 1 0 $a Numerical hydrodynamics of relativistic extragalactic jets.
300 $a 139 p.
500 $a Adviser: Paul J. Wiita.
500 $a Source: Dissertation Abstracts International, Volume: 68-04, Section: B, page: 2427.
502 $a Thesis (Ph.D.)--Georgia State University, 2007.
520 $a Index words. Extragalactic jets, Hydrodynamics, Numerical methods, Special relativity
520 $a This dissertation describes a multidimensional relativistic hydrodynamic code which solves the special relativistic hydrodynamic equations as a hyperbolic system of conservation laws based on the total variation diminishing (TVD) scheme. Several standard tests and test simulations are presented to demonstrate the accuracy, robustness and flexibility of the code. Using this code we have studied three-dimensional hydrodynamic interactions of relativistic extragalactic jets with two-phase ambient media. The deflection angle of the jet is influenced more by the density contrast of the cloud than by the beam Mach number of the jet, and a relativistic jet with low relativistic beam Mach number can eventually be slightly bent after it crosses the dense cloud. Relativistic jet impacts on dense clouds do not necessarily destroy the clouds completely, and much of the cloud body can survive as a coherent blob due to the combination of the geometric influence of off-axis collisions and the lower rate of cloud fragmentation through the Kelvin-Helmholtz instability for relativistic flows. We find that relativistic jets interacting with clouds can produce synchrotron emission knots similar to structures observed in many VLBI-scale radio sources and the synchrotron emission peaks right before the jet passes through the cloud.
590 $a School code: 0079.
650 4 $a Physics, Theory. $3 1019422
690 $a 0753
710 2 $a Georgia State University. $3 1018518
773 0 $t Dissertation Abstracts International $g 68-04B.
790 $a 0079
790 1 0 $a Wiita, Paul J., $e advisor
791 $a Ph.D.
792 $a 2007
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3260554