Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
aswns [2022/08/16 07:12]
theoastro
aswns [2022/08/16 20:55] (current)
theoastro [Further documentation:]
Line 1: Line 1:
  ====== ASWNS  ======  ====== ASWNS  ======
 +
 +==== Summary ==== 
  
 ASWNS  stands for "Arcetri-Stockholm-Warsaw Neutron Stars". The code was mainly developed by G. Camelio, is an extension of the [[https://arxiv.org/abs/1401.4308|XNS-v2 code]] , and computes rotating neutron star configurations using the extended Conformal Flatness approximation and is written in FORTRAN 90. ASWNS  stands for "Arcetri-Stockholm-Warsaw Neutron Stars". The code was mainly developed by G. Camelio, is an extension of the [[https://arxiv.org/abs/1401.4308|XNS-v2 code]] , and computes rotating neutron star configurations using the extended Conformal Flatness approximation and is written in FORTRAN 90.
Line 8: Line 10:
   * [[https://arxiv.org/abs/1908.11258|to study baroclinic neutron star configurations]]    * [[https://arxiv.org/abs/1908.11258|to study baroclinic neutron star configurations]] 
   * [[https://arxiv.org/abs/2011.10557|to model hot, nonbarotropic, differentially rotating neutron star merger remnants]]   * [[https://arxiv.org/abs/2011.10557|to model hot, nonbarotropic, differentially rotating neutron star merger remnants]]
 +
 +==== Further documentation: ====
 +   * [[Installation_ASWNS|Installation]]
 +   * [[Examples_ASWNS|Examples (non-barotropic stars and configurations at the Kepler limit)]]
 +   * [[general_aswns|General settings]]
Last modified: le 2022/08/16 07:12