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  Distortion of neutron stars with a toroidal magnetic field

Frieben, J., & Rezzolla, L. (2015). Distortion of neutron stars with a toroidal magnetic field. In Proceedings of the MG13 Meeting on General Relativity (pp. 2387-2389). World Scientific.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0024-DCC1-7 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0024-DCC2-5
Genre: Conference Paper

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1402.3258v2.pdf (Preprint), 371KB
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 Creators:
Frieben, Joachim1, Author
Rezzolla, Luciano1, Author              
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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 Abstract: Models of rotating relativistic stars with a toroidal magnetic field have been computed for a sample of eight equations of state of cold dense matter. Non-rotating models admit important levels of magnetization and quadrupole distortion accompanied by a seemingly unlimited growth in size. Rotating models reach the mass-shedding limit at smaller angular velocities than in the non-magnetized case according to the larger circumferential equatorial radius induced by the magnetic field. Moreover, they can be classified as prolate-prolate, oblate-prolate, or oblate-oblate with respect to surface deformation and quadrupole distortion. Simple expressions for surface and quadrupole deformation are provided that are valid up to magnetar field strengths and rapid rotation.

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 Dates: 2015
 Publication Status: Published in print
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 Rev. Method: -
 Identifiers: DOI: 10.1142/9789814623995_0447
arXiv: 1402.3258
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Title: The Thirteenth Marcel Grossmann Meeting
Place of Event: Stockholm University, Sweden
Start-/End Date: 2012-07-01 - 2012-07-07

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Title: Proceedings of the MG13 Meeting on General Relativity
Source Genre: Proceedings
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Publ. Info: World Scientific
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 2387 - 2389 Identifier: -