Reduction of the Mass of the Proto-Quark Star during Cooling
The integral parameters (mass, radius) of hot proto-quark stars that are formed in supernova explosion are studied. We use the MIT bag model to determine the pressure of up-down and strage quark matter at finite temperature and in the regime where neutrinos are trapped. It is shown that such stars a...
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| Format: | Article |
| Language: | English |
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MDPI AG
2021-01-01
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| Series: | Particles |
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| Online Access: | https://www.mdpi.com/2571-712X/4/1/4 |