TY - GEN
T1 - Cooling of compact stars with Quark-Hadron Mixed Phase in the colour superconductive state
AU - Noda, Tsuneo
AU - Hashimoto, Masaaki
AU - Yasutake, Nobutoshi
AU - Maruyama, Toshiki
AU - Tatsumi, Toshitaka
AU - Fujimoto, Masayuki
PY - 2010
Y1 - 2010
N2 - Recently, the central source of Cassiopeia A (Cas A) has been observed, which indicates that the star has large mass and high effective temperature. We suspect that the compact object cools by the standard neutrino emission. We assume that the compact object contains quark matter with colour superconductivity and calculate cooling curves. Considering the Quark-Hadron Mixed Phase, we obtain cooling curves which are found to be consistent with the observations.
AB - Recently, the central source of Cassiopeia A (Cas A) has been observed, which indicates that the star has large mass and high effective temperature. We suspect that the compact object cools by the standard neutrino emission. We assume that the compact object contains quark matter with colour superconductivity and calculate cooling curves. Considering the Quark-Hadron Mixed Phase, we obtain cooling curves which are found to be consistent with the observations.
UR - https://www.scopus.com/pages/publications/77956637427
UR - https://www.scopus.com/pages/publications/77956637427#tab=citedBy
U2 - 10.1063/1.3485174
DO - 10.1063/1.3485174
M3 - Conference contribution
AN - SCOPUS:77956637427
SN - 9780735408197
T3 - AIP Conference Proceedings
SP - 384
EP - 386
BT - 10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10
T2 - 10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10
Y2 - 8 March 2010 through 10 March 2010
ER -