Nucleonic Direct Urca Processes and Cooling of the Massive Neutron Star by Antikaon Condensations

Table 1

Values of NS masses M and the corresponding radii R calculated for the center densities of and optical potential of antikaons  = 0, −80, −90, −100, −110, −120, and −130 MeV. The critical temperature of the protonic superfluids is also listed for  = 0 to −130 MeV and .

	0	−80	−90	−100	−110	−120	−130
Case no.	1	2	3	4	5	6	7
	2.051	2.051	2.051	2.051	2.039	1.972	1.887
	2.235	2.233	2.203	2.161	2.105	2.032	1.940
	2.325	2.279	2.245	2.199	2.140	2.064	1.966
	13.050	13.050	13.050	13.050	13.065	13.126	13.178
	12.715	12.720	12.793	12.864	12.926	12.974	12.997
	12.347	12.526	12.593	12.647	12.684	12.692	12.714
	24.924	31.078	30.656	30.274	22.394	0.708	0.459