An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars
For densities beyond nuclear saturation, there is still a large uncertainty in the equations of state (EoSs) of dense matter that translate into uncertainties in the internal structure of neutron stars. The MUSES Calculation Engine provides a free and open-source composable workflow management syste...
Furkejuvvon:
| Váldodahkkit: | , , |
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| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
MDPI AG
2025-06-01
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| Ráidu: | Universe |
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| Liŋkkat: | https://www.mdpi.com/2218-1997/11/7/200 |
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