中子星大气中的氢原子：束缚能的解析近似
原子物理
2008-02-03 v1 天体物理学
摘要
针对在磁中子星典型的 G 至 G 磁场中任意运动的氢原子，构造了其束缚能的解析近似。
引用
@article{arxiv.physics/9708024,
title = {Hydrogen atoms in neutron star atmospheres: Analytical approximations for binding energies},
author = {A. Y. Potekhin},
journal= {arXiv preprint arXiv:physics/9708024},
year = {2008}
}
备注
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