Relativistic perfect fluids in local thermal equilibrium

被引:12
|
作者
Coll, Bartolome [1 ]
Josep Ferrando, Joan [1 ,2 ]
Antonio Saez, Juan [3 ]
机构
[1] Univ Valencia, Dept Astron & Astrofis, E-46100 Valencia, Spain
[2] Univ Valencia, Observ Astron, Valencia 46980, Spain
[3] Univ Valencia, Dept Matemat Econ & Empresa, Valencia 46022, Spain
关键词
Thermodynamics; Energy tensors; Relativistic perfect fluids; Ideal gases;
D O I
10.1007/s10714-017-2225-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Every evolution of a fluid is uniquely described by an energy tensor. But the converse is not true: an energy tensor may describe the evolution of different fluids. The problem of determining them is called here the inverse problem. This problem may admit unphysical or non-deterministic solutions. This paper is devoted to solve the inverse problem for perfect energy tensors in the class of perfect fluids evolving in local thermal equilibrium (l.t.e.). The starting point is a previous result (Coll and Ferrando in J Math Phys 30: 2918-2922, 1989) showing that thermodynamic fluids evolving in l.t.e. admit a purely hydrodynamic characterization. This characterization allows solving this inverse problem in a very compact form. The paradigmatic case of perfect energy tensors representing the evolution of ideal gases is studied in detail and some applications and examples are outlined.
引用
收藏
页数:23
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