Dissipative relativistic hydrodynamics

Details Dissipative relativistic hydrodynamics Dissipative relativistic hydrodynamics

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..953i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Sept.-Oct. 1989, p. 953-964. In Russian.

Statistics

Computation

1

Computational Astrophysics, Hydrodynamics, Relativity, Entropy, Navier-Stokes Equation, Shock Wave Propagation, Supernovae, Tensors

Scientific paper

Using the comoving reference frame in the general noninertial case, the relativistic hydrodynamics equations are derived, taking account of dissipative effects in matter. An exact form for the dissipative tensor components is obtained from the entropy production equation. A closed system of equations of dissipative relativistic hydrodynamics in the comoving reference frame is thus obtained as a relativistic generalization of the standard Navier-Stokes equations for Lagrangian coordinates. This approach can be used to study shock-wave propagation in supernova envelopes.

Affiliated with

Also associated with

No associations

Rating

Dissipative relativistic hydrodynamics does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dissipative relativistic hydrodynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dissipative relativistic hydrodynamics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1528442