Hydrogen atoms in neutron star atmospheres: Analytical approximations for binding energies
Abstract
Description
Analytical approximations are constructed for binding energies of hydrogen atoms arbitrarily moving in magnetic fields 7\times10^{11} G to 2\times10^{13} G, typical of magnetic neutron stars.
6 pages, 1 figure, LaTeX using plenum.sty and epsf.sty (included). To appear in Proc. of 172 WE-Heraeus-Seminar on Atoms and Molecules in Strong External Fields, Bad Honnef, 7-11 April 1997, ed. P. Schmelcher & W. Schweizer (New York: Plenum). Postscript version also available at http://www.ioffe.rssi.ru/dtastrop.html
6 pages, 1 figure, LaTeX using plenum.sty and epsf.sty (included). To appear in Proc. of 172 WE-Heraeus-Seminar on Atoms and Molecules in Strong External Fields, Bad Honnef, 7-11 April 1997, ed. P. Schmelcher & W. Schweizer (New York: Plenum). Postscript version also available at http://www.ioffe.rssi.ru/dtastrop.html