Lattimer-Swesty Equation of State code

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Lattimer-Swesty Equation of State Code

Post by owlice » Tue Feb 21, 2012 10:30 am

[c]Lattimer-Swesty Equation of State Code[/c][/b]
Abstract: The Lattimer-Swesty Equation of State code is rapid enough to use directly in hydrodynamical simulations such as stellar collapse calculations. It contains an adjustable nuclear force that accurately models both potential and mean-field interactions and allows for the input of various nuclear parameters, including the bulk incompressibility parameter, the bulk and surface symmetry energies, the symmetric matter surface tension, and the nucleon effective masses. This permits parametric studies of the equation of state in astrophysical situations. The equation of state is modeled after the Lattimer, Lamb, Pethick, and Ravenhall (LLPR) compressible liquid drop model for nuclei, and includes the effects of interactions and degeneracy of the nucleon outside nuclei.

Credit: Lattimer, James M.; Swesty, F. Douglas

Site: http://www.astro.sunysb.edu/dswesty/lseos.html
http://adsabs.harvard.edu/abs/1991NuPhA.535..331L

Bibcode: 2012ascl.soft02011L

ID: ascl:1202.011
Last edited by Ada Coda on Sun Dec 23, 2018 8:24 pm, edited 1 time in total.
Reason: Updated code entry.
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