Transient Phenomena from Gas Erupting Neutron Stars

Starquakes probably occur in rapidly spinning or ultra high field neutron stars. In this article, we argue that highly compressed gas containing electron-positron pairs could evaporate and erupt from inside the star when a crack forms then heals during starquake. Under influence of existing oscillation modes star, may have sufficiently large size long lifetime. An appropriate amount can into magnetosphere with relativistic nearly uniform velocity, producing various transient bursting phenomena.