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  Highly accurate calculation of rotating neutron stars - Detailed description of the numerical methods

Ansorg, M., Kleinwächter, A., & Meinel, R. (2003). Highly accurate calculation of rotating neutron stars - Detailed description of the numerical methods. Astronomy & Astrophysics, 405(2), 711-721. doi:10.1051/0004-6361:20030618.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-5219-A Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-521A-8
Genre: Journal Article

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711-721.pdf (Publisher version), 247KB
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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: We give a detailed description of the recently developed multi-domain spectral method for constructing highly accurate general-relativistic models of rapidly rotating stars. For both "ordinary" and "critical" configurations, we show using representative examples, how the accuracy improves as the order of the approximation increases. As well as homogeneous fluid bodies, we also discuss models of polytropic and strange stars.

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 Dates: 2003-07
 Publication Status: Issued
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 Identifiers: eDoc: 367495
DOI: 10.1051/0004-6361:20030618
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Title: Astronomy & Astrophysics
  Alternative Title : Astron. Astrophys.
Source Genre: Journal
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Pages: - Volume / Issue: 405 (2) Sequence Number: - Start / End Page: 711 - 721 Identifier: -