2015
DOI: 10.1515/awutp-2015-0211
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Relativistic Rotating Boltzmann Gas Using the Tetrad Formalism

Abstract: We consider an application of the tetrad formalism introduced by Cardall et al. [Phys. Rev. D 88 (2013) 023011] to the problem of a rigidly rotating relativistic gas in thermal equilibrium and discuss the possible applications of this formalism to relativistic lattice Boltzmann simulations. We present in detail the transformation to the comoving frame, the choice of tetrad, as well as the explicit calculation and analysis of the components of the equilibrium particle flow four-vector and of the equilibrium st… Show more

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Cited by 10 publications
(29 citation statements)
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“…The kinetic theory formulation gives the macroscopic SET Tαρ as the second order moment of the distribution function f : 5) where the integration measure d 3 p/p0 is Lorentz-invariant. The SET corresponding to the distribution (7.2) can be found by first performing a series expansion of the equilibrium distribution function (7.2) in powers of ǫ [18,19,20]:…”
Section: Kinetic Theory Resultsmentioning
confidence: 99%
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“…The kinetic theory formulation gives the macroscopic SET Tαρ as the second order moment of the distribution function f : 5) where the integration measure d 3 p/p0 is Lorentz-invariant. The SET corresponding to the distribution (7.2) can be found by first performing a series expansion of the equilibrium distribution function (7.2) in powers of ǫ [18,19,20]:…”
Section: Kinetic Theory Resultsmentioning
confidence: 99%
“…The energy density and pressure arising from the Maxwell-Jüttner distribution function (7.7) can be found in closed form [18,19,29]:…”
Section: Kinetic Theory Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…For comparison with our later work on adS, it is instructive to compare the above QFT results on Minkowski space-time with the classical energy density and pressure for a thermal gas of particles, computed in the framework of RKT. For particles with mass m, momentum pα, at inverse temperature β, the Bose-Einstein and Fermi-Dirac thermal distribution functions are, respectively [12][13][14]…”
Section: Qft and Rkt On Minkowski Space-timementioning
confidence: 99%
“…Remarkably, on Minkowski space-time, for both scalars and fermions the classical thermal SET is identical to the quantum t.e.v. (2.8) [12,13,15]:…”
Section: B)mentioning
confidence: 99%