Differences
This shows you the differences between two versions of the page.
| Both sides previous revision
Previous revision
Next revision
|
Previous revision
|
aswns [2022/08/16 07:14]
theoastro |
aswns [2022/08/16 20:55] (current)
theoastro [Further documentation:] |
| ====== ASWNS ====== | ====== ASWNS ====== |
| |
| == Summary == | ==== 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. |
| * [[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:== | ==== Further documentation: ==== |
| * [[Installation_ASWNS|Installation]] | * [[Installation_ASWNS|Installation]] |
| *[[Examples_ASWNS|Examples]] | * [[Examples_ASWNS|Examples (non-barotropic stars and configurations at the Kepler limit)]] |
| *[[Analysis_ASWNS|Analysis]] | * [[general_aswns|General settings]] |
