NeutronStarOscillations.jl
Abstract
Julia code for solving the equations of motion governing linearized radial perturbations of spherically symmetric neutron stars in the frequency and time domains. Methods are provided for inviscid perfect fluid stars and viscous stars within the frameworks of Eckart and Bemfica-Disconzi-Noronha-Kovtun (BDNK) hydrodynamics.
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 24 March 2026