We study different stages of the neutron star cooling by computing neutron star properties at various temperatures and entropies using an effective chiral model including hadronic and quark degrees of freedom. Macroscopic properties of the star such as mass and radius are calculated and compared wit
✦ LIBER ✦
Jet quenching as a probe of dense matter
✍ Scribed by Miklos Gyulassy; Michael Plümer
- Publisher
- Elsevier Science
- Year
- 1991
- Tongue
- English
- Weight
- 236 KB
- Volume
- 527
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
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