ASCL Code Record
[ascl:1402.020]
XNS: Axisymmetric equilibrium configuration of neutron stars
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.
- Code site:
- http://www.arcetri.inaf.it/science/ahead/XNS/index.html
- Used in:
- 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
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