Pith. sign in

REVIEW 1 cited by

Numerical hydrodynamics in special relativity

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/9906333 v1 pith:RBPTPADW submitted 1999-06-21 astro-ph

Jose M. Marti (1) , Ewald Mueller (2) ((1) Departamento de Astronomia y Astrofisica , Universidad de Valencia , Spain (2) MPI fuer Astrophysik , Garching , Germany) This is my paper · ORCID
classification astro-ph
keywords methodsnumericalsrhdhydrodynamicsreviewspecialanalyzedapplication
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

This review is concerned with a discussion of numerical methods for the solution of the equations of special relativistic hydrodynamics (SRHD). Particular emphasis is put on a comprehensive review of the application of high-resolution shock-capturing methods in SRHD. Results obtained with different numerical SRHD methods are compared, and two astrophysical applications of SRHD flows are discussed. An evaluation of the various numerical methods is given and future developments are analyzed.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A "Neural" Riemann solver for Relativistic Hydrodynamics

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Small neural networks trained on exact solutions can replace the iterative root-finding in a relativistic Riemann solver, giving exact-like accuracy about 14 times faster in 1D tests.

Pith tools