The interior space-time metric for a rotating spherical star

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Discussion Overview

The discussion revolves around the search for a space-time metric that describes the interior of spherically symmetric rotating stars. Participants express interest in finding solutions that differ from the exterior metrics typically available, such as those related to slowly rotating stars and frame dragging effects.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested

Main Points Raised

  • One participant seeks a metric for the interior of a rotating star, noting that existing resources primarily focus on exterior metrics.
  • Another participant mentions that finding an interior solution approximating a Kerr Metric is an open problem, suggesting uncertainty in the current state of research.
  • Several references to academic papers are provided, indicating ongoing research and various approaches to the problem of interior metrics for rotating stars.
  • A participant points out a potential typo in one of the referenced papers, indicating that there may be issues in the literature that need clarification.

Areas of Agreement / Disagreement

Participants do not appear to reach a consensus on the existence of a suitable interior metric for rotating stars, and multiple competing views and references are presented without resolution.

Contextual Notes

The discussion highlights limitations in existing literature, including potential errors in published papers and the ongoing nature of research in this area.

Gravitino
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I was looking for a space time metric that describes the INTERIOR of spherically symmetric rotating stars. However, wherever I look it is always the metric for an exterior of "slowly rotating star" (frame dragging effect) or something similar to it but always the metric AROUND the object (exterior). Is there any solution for interior of the star? I know already the interior Schwarzschild solution but is there the same for a rotating star? Thanks in advance.
 
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Finding the interior solution for something approximating a Kerr Metric is an open problem, as I recall.

Good luck, and keep us informed?
 
These references have been passed on to me -

http://arxiv.org/abs/gr-qc/9910001
Michael Bradley, Gyula Fodor, Mattias Marklund, Zoltán Perjés
The Wahlquist metric cannot describe an isolated rotating body

http://arxiv.org/abs/gr-qc/0202065
R. J. Wiltshire
Slowly, rotating non-stationary, fluid solutions of Einstein's equations and their match to Kerr empty space-time

http://arxiv.org/abs/gr-qc/0207099
Gyula Fodor, Zolt{á}n Perj{é}s, Michael Bradley
Slowly rotating charged fluid balls and their matching to an exterior domain

http://arxiv.org/abs/gr-qc/0304097
Ron Wiltshire
Slowly rotating, compact fluid sources embedded in Kerr empty space-time

http://arxiv.org/abs/gr-qc/0601024
Ron Wiltshire
Isotropy, shear, symmetry and exact solutions for relativistic fluid spheres

http://arxiv.org/abs/gr-qc/0612046
Michael Bradley, Daniel Eriksson, Gyula Fodor, Istvan Racz
Slowly rotating fluid balls of Petrov type D
 

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