2010/05/25 by Chun-Mei Pi, Pi, Chun-Mei
Earth and Planetary Sciences · Physics and Astronomy · #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High-pressure geophysics and materials #Pulsars and Gravitational Waves Research #Quantum, superfluid, helium dynamics #astro-ph.HE
paper · pdf · doi:10.48550/arxiv.1005.4473
7 pages, 2 figures. To appear in Proceedings for "Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, KIAA at Peking University, Beijing - P. R. China [http://vega.bac.pku.edu.cn/rxxu/csqcd.htm]
arxiv created 2010/05/25 · openalex publication_date 2010/05/25 · arxiv updated 2010/05/26 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The authors take the rotochemical heating effect into account, which may make the cooling scenario different. Their model is consistent with the observation data.