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XNS: Axisymmetric equilibrium configuration of neutron stars

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XNS: Axisymmetric equilibrium configuration of neutron stars

Postby owlice » Fri Feb 14, 2014 2:58 pm

XNS: Axisymmetric equilibrium configuration of neutron stars

Abstract: XNS solves for the axisymmetric equilibrium configuration of neutron stars in general relativity. It can model differentially rotating and magnetic fields that are either purely toroidal, purely poloidal or in the mixed twisted torus configuration. Einsten's equations are solved using the XCFC approximation for the metric in spherical coordinates.

Credit: Bucciantini, N.; Pili, A. G.; Del Zanna, L.

Site: http://www.arcetri.astro.it/science/ahe ... index.html
http://adsabs.harvard.edu/abs/2014ASPC..488..211B

Bibcode: 2014ascl.soft02020B

Preferred citation method: http://adsabs.harvard.edu/abs/2011A&A...528A.101B and http://adsabs.harvard.edu/abs/2014MNRAS.439.3541P

ID: ascl:1402.020
Last edited by Ada Coda on Tue Feb 06, 2018 6:34 am, edited 1 time in total.
Reason: Updated code entry.
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