Abstract
1. The equation of state and nuclear composition are calculated for cold matter below neutron-drip density (∼4×1011 g/cm3) using recent nuclear data. 2. Nuclear transmutations of hot and dense matter taking care of the freezing of nuclear reactions are discussed for three types of temperature and density changes.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
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
