New relativistic dissipative fluid dynamics from kinetic theory
2013; Elsevier BV; Volume: 720; Issue: 4-5 Linguagem: Inglês
10.1016/j.physletb.2013.02.025
ISSN1873-2445
AutoresAmaresh Jaiswal, Rajeev S. Bhalerao, Subrata Pal,
Tópico(s)Cosmology and Gravitation Theories
ResumoStarting with the relativistic Boltzmann equation where the collision term is generalized to include nonlocal effects via gradients of the phase-space distribution function, and using Grad's 14-moment approximation for the distribution function, we derive equations for the relativistic dissipative fluid dynamics. We compare them with the corresponding equations obtained in the standard Israel-Stewart and related approaches. Our method generates all the second-order terms that are allowed by symmetry, some of which have been missed by the traditional approaches based on the 14-moment approximation, and the coefficients of other terms are altered. The first-order or Navier-Stokes equations too get modified. Significance of these findings is demonstrated in the framework of one-dimensional scaling expansion of the matter formed in relativistic heavy-ion collisions.
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