Abstract
The linear stability of a plane relativistic shock has been investigated. Restrictions are found on the equation of state in order for the shock to be stable. A comparison is made with the results obtained in the framework of (nonlinear) corrugation stability.
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
