Thermal emission from bare quark matter surfaces of hot strange stars
Mar, 200110 pages
Published in:
- Astrophys.J.Lett. 550 (2001) L179
e-Print:
- astro-ph/0103361 [astro-ph]
DOI:
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Abstract: (arXiv)
We consider the thermal emission of photons and electron-positron pairs from the bare quark surface of a hot strange star. The radiation of high-energy (> 20 MeV) equilibrium photons prevails at the surface temperature T_S > 5 x 10^{10} K, while below this temperature, 8 x 10^8 < T_S < 5 x 10^{10} K, emission of electron-positron pairs created by the Coulomb barrier at the quark surface dominates. The thermal luminosity of a hot strange star in both photons and pairs is estimated.- matter: strangeness
- quark: matter
- star: surface
- energy: flux
- photon: emission
- electron: pair production
- luminosity
- temperature
- numerical calculations
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