Symbolic computation and perfect fluids in general relativity
DOI10.1017/S0004972700022139zbMath0940.83002OpenAlexW2161579415MaRDI QIDQ4953133
Publication date: 26 July 2000
Published in: Bulletin of the Australian Mathematical Society (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1017/s0004972700022139
Einstein's field equationstetrad formalismmaplerelativistic perfect fluidssymbolic implementation of Newman-Penrose formalism
Symbolic computation and algebraic computation (68W30) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Equations of motion in general relativity and gravitational theory (83C10) Computational methods for problems pertaining to relativity and gravitational theory (83-08)
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Uses Software
Cites Work
- Theorems on shear-free perfect fluids with their Newtonian analogues
- The Maple package NPTOOLS; a symbolic algebra package for tetrad formalisms in general relativity
- Shear-free perfect fluids with zero magnetic Weyl tensor
- Shear-free perfect fluids in general relativity. I. Petrov type N Weyl tensor
- An Approach to Gravitational Radiation by a Method of Spin Coefficients
- Shear-free perfect fluids in general relativity: IV. Petrov type III spacetimes
- Shear-free perfect fluids in general relativity: III. Petrov type III spacetimes
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