Cooling of Akmal-Pandharipande-Ravenhall neutron stars with a rotochemical heating source

[1]
Haensel P,Potekhin A Y,Yakovlev D G.Neutron Stars.1.Equation of State and Structure.New York:Springer,2007[2] Lattimer J M,Prakash M.Phys.Rep.,2007,442:109-165[3] Lattimer J M,Pethick C J,Prakash M,Haensel P.Phys.Rev.Lett.,1991,66:2701-2704[4] Lombardo U,Schulze H-J.Superfluidity in Neutron Star matter,in Physics of Neutron Star Interiors.Edited by Blaschke D,Glendenning N,Sedrakian A.Springer,Berlin,2001,30-53[5] Page D,Lattimer J M,Prakash M,Steiner A W.ApJSS,2004,155:623[6] Reisenegger A.ApJ,1995,442:749[7] Gusakov M E,Kaminker A D,Yakovlev D G,Gnedin O Y.MNRAS,2005,363:555[8] Yakovlev D G,Pethick C J.Ann.Rev.Astron.Astrophys.,2004,42:169[9] Kaminker A D,Haensel P,Yakovlev D G.AA,2001,373:L17[10] Flowers E G,Ruderman M,Sutherland P G.ApJ,1979,205:541[11] Haensel P.A A,1992,262:131[12] Yakovlev D G,Kaminker A D,Gnedin O Y,Haensel P.Phys.Rep.,2001,354:1[13] Fern(a)dez F,Reisenegger A.ApJ,2005,625:291[14] Akmal A,Pandharipande V R,Ravenhall D G.Phys.Rev.C,1998,58:1804[15] Heiselberg H,Hjorth-Jensen M.ApJ,1999,525:L45[16] Potekhin A Y,Yakovlev D G,Chabrier G,Gnedin O Y.ApJ,2003,594:404[17] Yakovlev D G,Gnedin O Y,Kaminker A D,Potekhin A Y.AIP Conf.Proc,2008,983:379