Thermal emission from bare quark matter surfaces of hot strange stars

Mar, 2001
10 pages
Published in:
  • Astrophys.J.Lett. 550 (2001) L179
e-Print:

Citations per year

2001200720132019202502468
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