Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
12011488 | Nuclear Physics A | 2018 | 37 Pages |
Abstract
We demonstrate that the existing neutron-star cooling data can be appropriately described within “the nuclear medium cooling scenario” including hyperons under the assumption that different compact-star sources have different masses. We use a stiff equation of state of the relativistic mean-field model MKVORHÏ with hadron effective couplings and masses dependent on the scalar field. It fulfills a large number of experimental constraints on the equation of state of the nuclear matter including the 2Mâ lower bound for the maximum compact-star mass and the constraint for the pressure from the heavy-ion particle flow. We select appropriate S01 proton and Î hyperon pairing gap profiles from those exploited in the literature and allow for a variation of the effective pion gap controlling the efficiency of the medium modified Urca process. The P23 neutron pairing gap is assumed to be negligibly small in our scenario. The possibility of the pion, kaon and charged Ï-meson condensations is for simplicity suppressed. The resulting cooling curves prove to be sensitive to the value and the density dependence of the pp pairing gap and rather insensitive to the values of the S01 neutron pairing gaps.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
H. Grigorian, D.N. Voskresensky, K.A. Maslov,