EoS BPS-BPP + Pure Neutron Matter/ Baryonic Matter

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SUMMARY

The discussion focuses on integrating the equations of state (EoS) for high-density BPS-BBP with pure neutron matter and baryonic matter plus an electron gas. The user has data for the BPS-BBP EoS, which includes neutron drip and anticipates nuclei disintegration at approximately 1014 g/cm3. The challenge lies in ensuring that the graphs of these EoS intersect at the correct densities, as the current graphs do not align as expected.

PREREQUISITES
  • Understanding of BPS-BBP equations of state
  • Knowledge of neutron gas dynamics
  • Familiarity with baryonic matter and electron gas interactions
  • Proficiency in graphing and interpreting high-density matter equations
NEXT STEPS
  • Research methods for integrating BPS-BBP EoS with neutron gas models
  • Explore the effects of baryonic matter on neutron gas behavior
  • Study the implications of electron gas in high-density environments
  • Learn about graphical representation techniques for complex EoS
USEFUL FOR

This discussion is beneficial for astrophysicists, nuclear physicists, and researchers working on high-density matter equations of state, particularly those focusing on neutron stars and baryonic matter interactions.

Leonardo Machado
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Hello everyone,
Today I'm asking you for help to put together these two equations of state for high densities BPS-BBP with a eos of a pure neutron gas or a non interacting n + p + e gas.

I have already the data of BPS-BBP equation of state, with includes neutron drip and let a open space to nuclei disintegration at its end ( ~1014 g/cm3), so i must attach any of theses types of matter, only a baryonic matter plus a electron gas.

Anyone here has experience with that so can help me? My graph of these eos are not touching, or touching in a density bellow the expected.
 
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Here is the graph with these eos ( bbp-bps, pure neutron gas and non-interactive baryonic matter + electron gas)

It is allowed to introduce this kind of link on the forum ??
 

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