Abstract
The strong electric field near the surface of a strange star is discussed, and its supporting interaction to the normal nuclear crust is calculated by using a self-consistent method. It is proved that the crust would begin not to be supported by this electric field at a quite low density at the crust base, much lower than the previously assumed neutron drip density.
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
