Summary
The homogeneous nucleation at constant temperature of a one-component plasma is studied and possible consequences for the structure of neutron star crusts are examined.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Tanaka S. andIchimaru S.,Phys. Rev. A,35 (1987) 4743.
Ichimaru S., Iyetomi H., Mitake S. andItoh N.,Astrophys. J.,265 (1983) L83.
Baym G., Bethe H. andPethick C.,Nucl. Phys. A,175 (1971) 225;Baym G., Pethick C. andSutherland P.,Astrophys. J.,170 (1971) 299.
Burrows A. andLattimer J. M.,Astrophys. J.,307 (1986) 178.
Shapiro S. L. andTeukolsky S. A.,Black Holes, White Dwarfs and Neutron Stars (Wiley, New York, N.Y.) 1983.
Kelton K. F.,Solid State Phys.,45 (1991) 75.
Gutzow I., Kashchiev D. andAvramov I.,J. Non-Cryst. Solids,73 (1985) 477.
Avrami M.,J. Chem. Phys.,8 (1940) 212.
Cohen M. M. andTurnbull D.,J. Chem. Phys.,31 (1959) 1164.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
De Blasio, F.V. Nucleation of a one-component plasma and structure of neutron star crusts. Nuov Cim A 108, 431–436 (1995). https://doi.org/10.1007/BF02813600
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/BF02813600