There is a newer version of the record available.

Published April 22, 2022 | Version v1

hydro-bulk-1D

Authors/Creators

  • 1. CAMK-PAN

Description

1-dimensional general relativistic hydrodynamic code with bulk viscosity.

`hydro-bulk-1D` tests the correspondence between the bulk viscous formulation
of the multi-component fluid and that of the Israel-Stewart theories
(see Gavassino, Antonelli, and Haskell, 2021, CQG 38:075001)
in the context of neutron stars.

The theory and the code are described in the following papers:

* [1] Camelio, Gavassino, Antonelli, Bernuzzi, and Haskell, "Simulating bulk viscosity in neutron stars. I. Formalism", PRD 107:103031 (2023).
* [2] Camelio, Gavassino, Antonelli, Bernuzzi, and Haskell, "Simulating bulk viscosity in neutron stars. II. Evolution in spherical symmetry", PRD 107:103032 (2023).

`hydro-bulk-1D` is released under the MIT License.

If you use `hydro-bulk-1D` in your research, please cite Refs. [1] and [2].

EDIT 2023-05-19: for the version of the code updated during peer-review of Refs. [1] and [2], see new code version.

Notes

This work was supported by the Polish National Science Centre (NCN) grant number OPUS 2019/33/B/ST9/00942.

Files

LICENSE.txt

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Additional details

Related works

References

  • Camelio, Gavassino, Antonelli, Bernuzzi, and Haskell, "Simulating bulk viscosity in neutron stars. I. Formalism", PRD 107:103031 (2023).
  • Camelio, Gavassino, Antonelli, Bernuzzi, and Haskell, "Simulating bulk viscosity in neutron stars. II. Evolution in spherical symmetry", PRD 107:103032 (2023).