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About The Physics of Stellar Collapse (And GR Hydrodynamics)
The document outlines the physics of stellar collapse and core-collapse supernovae. It discusses how massive stars evolve and eventually collapse once they exhaust their nuclear fuel. The collapse is initiated by the reduction of electron degeneracy pressure in the iron core as electrons are captured onto protons. General relativistic effects and the stiffening of the nuclear equation of state above nuclear density halt the collapse and cause a rebound, launching a shock wave, but additional heating is required to power a successful supernova explosion.
Detailed Information
| Author: | ['Sovan Chakraborty'] |
|---|---|
| Publication Year: | 2020 |
| Pages: | 66 |
| Language: | English |
| Format: | |
| Price: | FREE |
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