2011
DOI: 10.1016/j.jmaa.2011.04.017
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Riemann problem for the relativistic Chaplygin Euler equations

Abstract: The relativistic Euler equations for a Chaplygin gas are studied. The Riemann problem is solved constructively. There are five kinds of Riemann solutions, in which four only contain different contact discontinuities and the other involves delta shock waves. Under suitable generalized Rankine-Hugoniot relation and entropy condition, the existence and uniqueness of delta-shock solutions are established.

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Cited by 45 publications
(23 citation statements)
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“…In this section, we briefly review the Riemann solutions of and with initial data (v(xMathClass-punc,0)MathClass-punc,ρ(xMathClass-punc,0)) MathClass-rel= (vMathClass-bin±MathClass-punc,ρMathClass-bin±)MathClass-punc,MathClass-bin±x MathClass-rel> 0MathClass-punc, where ρ ± > 0, the detailed study of which can be found in . For more details about the Riemann problem for hyperbolic conservation laws, please see .…”
Section: Preliminariesmentioning
confidence: 99%
See 1 more Smart Citation
“…In this section, we briefly review the Riemann solutions of and with initial data (v(xMathClass-punc,0)MathClass-punc,ρ(xMathClass-punc,0)) MathClass-rel= (vMathClass-bin±MathClass-punc,ρMathClass-bin±)MathClass-punc,MathClass-bin±x MathClass-rel> 0MathClass-punc, where ρ ± > 0, the detailed study of which can be found in . For more details about the Riemann problem for hyperbolic conservation laws, please see .…”
Section: Preliminariesmentioning
confidence: 99%
“…For system (1.1) and (1.7), Cheng et al [26] solved the Riemann problem and established the existence and uniqueness of delta shock solutions. In this model, the formation of delta shock exhibits some phenomena during the evolution of the universe, such as the formation and development of the black hole, the boom and inflation of the universe and so on.…”
Section: Introductionmentioning
confidence: 99%
“…The Euler system of conservation laws of energy and momentum for a Chaplygin gas in special relativity reads (cf. ): {falsenonefalsearrayarrayaxistMathClass-open(p+ρc2MathClass-close)v2c2MathClass-open(c2v2MathClass-close)+ρ+xMathClass-open(p+ρc2MathClass-close)vc2v2=0,arrayaxistMathClass-open(p+ρc2MathClass-close)vc2v2+xMathClass-open(p+ρc2MathClass-close)v2c2v2+p=0, where ρ , p and v represent the proper energy density, the pressure and the particle speed, respectively. The equations of state is p(ρ)MathClass-rel=MathClass-bin−1ρMathClass-punc,2emqquadforρMathClass-rel>0MathClass-punc. System models the dynamics of plane waves in special relativistic fluids in a two‐dimensional Minkowski time‐space ( x 0 , x 1 ): divTM...…”
Section: Applicationsmentioning
confidence: 99%
“…The Euler system of conservation laws of energy and momentum for a Chaplygin gas in special relativity reads (cf. [34][35][36]…”
Section: The Relativistic Euler Equations For Chaplygin Gasesmentioning
confidence: 99%
“…Y. Brenier [1] studied the one dimensional Riemann problems and obtained the solutions with concentration. Cheng and Yang [9] studied the Riemann problem for the relativistic Chaplygin Euler equations. In addition, D. Serre [40] studied the interaction of pressure waves for the 2-D isentropic irrotational Chaplygin gas.…”
Section: Introductionmentioning
confidence: 99%