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  Highly accurate calculation of rotating neutron stars

Ansorg, M., Kleinwächter, A., & Meinel, R. (2002). Highly accurate calculation of rotating neutron stars. Astronomy & Astrophysics, 381(3), L49-L52. doi:10.1051/0004-6361:20011643.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-540F-1 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-5410-C
Genre: Journal Article

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L49-L52.pdf (Publisher version), 163KB
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 Creators:
Ansorg, Marcus1, Author
Kleinwächter, Andreas, Author
Meinel, Reinhard, Author
Affiliations:
1Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24012              

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 Abstract: A new spectral code for constructing general-relativistic models of rapidly rotating stars with an unprecedented accuracy is presented. As a first application, we reexamine uniformly rotating homogeneous stars and compare our results with those obtained by several previous codes. Moreover, representative relativistic examples corresponding to highly flattened rotating bodies are given.

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 Dates: 2002-01
 Publication Status: Issued
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 Identifiers: eDoc: 367494
DOI: 10.1051/0004-6361:20011643
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Title: Astronomy & Astrophysics
  Alternative Title : Astron. Astrophys.
Source Genre: Journal
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Pages: - Volume / Issue: 381 (3) Sequence Number: - Start / End Page: L49 - L52 Identifier: -