Work

Self-gravitating Bjorken flow

Year: 2012

Type: article

Abstract: I present a solution to the full Einstein-fluid equations representing a self-gravitating Bjorken flow. The motion and the geometry become inhomogeneous in the plane transversal to the flow and the energy density profile acquires, due to gravity, corrections in terms of proper time as compared to the original test hydrodynamics. The transverse distribution of energy density, for example, becomes $ϵ(\ensuremath{\tau},r)/ϵ(\ensuremath{\tau},0)={cosh}^{\ensuremath{-}4}(3ar)$.

Source: Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields

DOI: 10.1103/physrevd.85.124006

Author: Alexander Feinstein

Institution: University of the Basque Country

Language: English

Topic: High-Energy Particle Collisions Research

Subfield: Nuclear and High Energy Physics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

OpenAlex ID: W1965479093

FWCI:

Cites: 16

Cited by:

Related to: 10