Abstract
It is investigated whether or not the direct URCA process proceeds in neutron-star matter with kaon condensation, in connection with potential contribution of the nuclear symmetry energy. We find a region in density-symmetry-energy plane in a model-independent way, where the direct URCA process occurs as a unique rapid cooling process in the kaon condensed phase. Symmetry energies with moderate density dependence pass through this region.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
