The Milne spacetime and the hadronic Rindler horizon

Abstract

A direct relation between the time dependent Milne geometry and the Rindler spacetime is shown. Milne's metric corresponds to that one beyond Rindler's event horizon (in the region $t\succ |x|)$). It was found that the shear tensor from the dissipative term of the RHIC expanding fireball has the same structure as that corresponding to the anisotropic fluid from the black hole interior, even though the latter geometry is curved.

7 pages, references added, no figures, version published in Int. J. Mod. Phys. D19, (8 - 10), 1379 - 1384 (2010)

References in corpus (6)

• Conformal Relativistic Viscous Hydrodynamics: Applications to RHIC results at sqrt(s_NN) = 200 GeV
• Thermal Hadronization and Hawking-Unruh Radiation in QCD
• Gravity dual of 1+1 dimensional Bjorken expansion
• The Exact String Black-Hole behind the hadronic Rindler horizon?
• Is the Rindler horizon energy nonvanishing ?
• Casimir energy in the gauge/gravity description of Bjorken flow?

Cited by in corpus (3)

• High-order quadrature-based lattice Boltzmann models for the flow of ultrarelativistic rarefied gases
• Rindler horizon entropy from nonstationarity
• Role of the remnant symmetries in gravitational theories based on absolute parallelism: a 2D standpoint