Universality in the run-up of shock waves to the surface of a star
We investigate the run-up of a shock wave from inside to the surface of a perfect fluid star in equilibrium and bounded by vacuum. Near the surface we approximate the fluid motion as plane-symmetric and the gravitational field as constant. We consider the 'hot' equation of state P = (? ? 1...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
2011-04-09.
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| Subjects: | |
| Online Access: | Get fulltext |