Hi, I would like to know more physics about the single stable neutron star solved using the toolkit as part of my master's project. Would you be able to throw some light on this? And I have a question about the time scales used in this particular problem, they are of order 10^-6, usually, neutron stars are highly compact objects, In this problem, the density was of the order 10^-3 why are these scales chosen, and this paper said (https://arxiv.org/abs/1111.3344.) the spikes in the graphs are due to the interaction with the artificial atmosphere I would like to know more about it. I am attaching my results. Warm regards
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