Neuhauser, D. and Koonin, S. E. and Langanke, K. (1987) Structure of matter in strong magnetic fields. Physical Review A, 36 (9). pp. 4163-4175. ISSN 1050-2947 http://resolver.caltech.edu/CaltechAUTHORS:NEUpra87
See Usage Policy.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:NEUpra87
We give a detailed presentation of Hartree-Fock calculations of atoms and molecular chains in 10^12 G magnetic fields, as are supposed to exist on the surface of neutron stars. These calculations are the first self-consistent ones treating exchange properly for atoms heavier than helium in high fields. We find that the isolated atom is energetically favored over molecular chains for Z>2 at fields greater than 1×10^12G and for Z>4 at fields greater than 5×10^12 G. These results indicate that matter on the surface of neutron stars is bound very weakly, if at all.
|Additional Information:||©1987 The American Physical Society. Received 13 April 1987.|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||09 Oct 2007|
|Last Modified:||26 Dec 2012 09:44|
Repository Staff Only: item control page