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• W3100754934 abstract "We show that the direct Urca process of neutrino emission is allowed in two possible phases of nonspherical nuclei (inverse cylinders and inverse spheres) in the mantle of a neutron star near the crust-core interface. The process is open because neutrons and protons move in a periodic potential created by inhomogeneous nuclear structures. In this way the nucleons acquire large quasimomenta needed to satisfy momentum-conservation in the neutrino reaction. The appropriate neutrino emissivity in a nonsuperfluid matter is about 2–3 orders of magnitude higher than the emissivity of the modified Urca process in the stellar core. The process may noticeably accelerate the cooling of low-mass neutron stars." @default.
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• W3100754934 date "2004-06-29" @default.
• W3100754934 modified "2023-10-18" @default.
• W3100754934 title "Direct Urca process in a neutron star mantle" @default.
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• W3100754934 doi "https://doi.org/10.1051/0004-6361:20040288" @default.
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