Abstract
We calculate the specific heat of superfluid neutrons in the inner crust of neutron stars, taking into account the role played by the nuclei in the lattice. We have found a strong increase in the calculated specific heat respect to that associated with a uniform neutron superfluid.
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References
G. Baym, H. A. Bethe and C. J. Pethick, Nucl. Phys.A175 (1971) 225.
J. Negele and D. Vautherin, Nucl. Phys.A207 (1973) 298.
H. Kucharek, P. Ring and P. Schuck, Z. Phys.A334, 119 (1989).
J. Dechargè and D. Gogny, Phys. Rev.C21 (1980) 1568.
F. De Blasio, G. Lazzari, Nuovo Cim.A, in press.
T. Takatsuka, Prog. Theor. Phys.71 (1984) 1432.