Book contents
- Frontmatter
- Contents
- Contributors
- Introduction
- Preface
- PART A THEORETICAL APPROACHES
- PART B PRACTICAL APPROACHES
- Numerical asymptotics
- Instabilities in rapidly rotating polytropes
- Gravitational radiation from coalescing binary neutron stars
- “Critical” behaviour in massless scalar field collapse
- Godunov-type methods applied to general relativistic stellar collapse
- Astrophysical sources of gravitational waves and neutrinos
- Gravitational radiation from 3D gravitational stellar core collapse
- A vacuum fully relativistic 3D numerical code
- Solution of elliptic equations in numerical relativity using multiquadrics
- Self-gravitating thin discs around rotating black holes
- An ADI scheme for a black hole problem
- Time-symmetric ADI and causal reconnection
- The numerical study of topological defects
- Computations of bubble growth during the cosmological quark-hadron transition
- Initial data of axisymmetric gravitational waves with a cosmological constant
- PANEL DISCUSSION
A vacuum fully relativistic 3D numerical code
Published online by Cambridge University Press: 15 December 2009
- Frontmatter
- Contents
- Contributors
- Introduction
- Preface
- PART A THEORETICAL APPROACHES
- PART B PRACTICAL APPROACHES
- Numerical asymptotics
- Instabilities in rapidly rotating polytropes
- Gravitational radiation from coalescing binary neutron stars
- “Critical” behaviour in massless scalar field collapse
- Godunov-type methods applied to general relativistic stellar collapse
- Astrophysical sources of gravitational waves and neutrinos
- Gravitational radiation from 3D gravitational stellar core collapse
- A vacuum fully relativistic 3D numerical code
- Solution of elliptic equations in numerical relativity using multiquadrics
- Self-gravitating thin discs around rotating black holes
- An ADI scheme for a black hole problem
- Time-symmetric ADI and causal reconnection
- The numerical study of topological defects
- Computations of bubble growth during the cosmological quark-hadron transition
- Initial data of axisymmetric gravitational waves with a cosmological constant
- PANEL DISCUSSION
Summary
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- Approaches to Numerical Relativity , pp. 258 - 264Publisher: Cambridge University PressPrint publication year: 1992