The interior space-time metric for a rotating spherical star

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SUMMARY

The discussion centers on the search for an interior space-time metric for spherically symmetric rotating stars, specifically seeking a solution analogous to the interior Schwarzschild solution for rotating stars. Participants highlight that existing metrics primarily describe the exterior, such as the Kerr Metric and its associated frame-dragging effects. Key references provided include works by Michael Bradley, Gyula Fodor, and Ron Wiltshire, which explore slowly rotating non-stationary fluid solutions and their relationship to Kerr empty space-time.

PREREQUISITES
  • Understanding of general relativity and Einstein's equations
  • Familiarity with the Schwarzschild and Kerr metrics
  • Knowledge of fluid dynamics in relativistic contexts
  • Ability to interpret academic papers in theoretical physics
NEXT STEPS
  • Research the interior Schwarzschild solution and its implications
  • Study the slowly rotating non-stationary fluid solutions of Einstein's equations
  • Examine the Wahlquist metric and its limitations in describing isolated rotating bodies
  • Explore the concept of trapped null geodesics in rotating interior metrics
USEFUL FOR

The discussion is beneficial for theoretical physicists, astrophysicists, and researchers focused on general relativity, particularly those investigating the interior metrics of rotating stars and their implications in astrophysical models.

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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