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Combined Analysis

NMMA is capable of performing combined analyses to constrain:

  • the neutron star equation of state (EOS), and
  • the Hubble Constant.

In the following, we will take as an example the EOS analysis.

EOS analysis

Generate a simulation set First of all, you need to create an output directory, this output will host all the data that will be used to constrain the EOS. 

mkdir -p ./output
Last modified: le 2022/02/22 10:31

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