pith. sign in

arxiv: astro-ph/9605187 · v1 · submitted 1996-05-30 · 🌌 astro-ph · gr-qc

Gravitational waves from neutron stars

classification 🌌 astro-ph gr-qc
keywords generalgravitationalresultsbreakingnewtonianrelativityspontaneousstars
0
0 comments X
read the original abstract

Contents: 1. Introduction 2. Spontaneous symmetry breaking 2.1 Review of classical results about Maclaurin/Jacobi ellipsoids 2.2 Spontaneous breaking of symmetry: a general phenomenom 2.3 Previous results for compressible Newtonian stars 2.4 Generation of gravitational waves 2.5 Finding the equilibrium configurations of a rotating star in the Newtonian regime 2.6 Extension to general relativity 2.7 First integral of fluid motion in general relativity 2.8 Gravitational field equations 2.9 Numerical results 3. CW emission from pulsars 4. Discussion and conclusion Appendix: Relativistic hydrodynamics in an accelerated frame

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

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

  1. The First Model-Independent Upper Bound on Micro-lensing Signature of the Highest Mass Binary Black Hole Event GW231123

    gr-qc 2025-12 conditional novelty 7.0

    No definitive lensing is detected in GW231123, though a potential microlensing feature with modulation amplitude up to 0.8 at 95% confidence is noted, limited by large waveform systematics in short signals.