I spent the morning writing in Tsalmantza and my HMF paper. This is my top priority for October. In the afternoon, Feryal Ozel (Arizona) gave a great talk about getting precise neutron-star mass and radius information to constrain the nuclear equation of state at high densities. She is doing very nice data analysis with very nice data and can rule out huge classes of equation-of-state models. She also showed some nice results on neutron-star masses from other areas, and (after the talk) showed me some hierarchical inferences about neutron-star mass distribution functions as a function of binary companion type.
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