Hydrogen atoms in neutron star atmospheres: Analytical approximations for binding energies

Simple item page
dc.creatorPotekhin, A. Y.
dc.date1997-08-21
dc.date.accessioned2026-07-07T09:16:21Z
dc.date.available2026-07-07T09:16:21Z
dc.descriptionAnalytical 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.
dc.description6 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
dc.identifierhttps://arxiv.org/abs/physics/9708024
dc.identifierhttp://arxiv.org/abs/physics/9708024
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/153326
dc.subjectAtomic Physics
dc.subjectAstrophysics
dc.titleHydrogen atoms in neutron star atmospheres: Analytical approximations for binding energies
dc.typetext

Files

Collections

arXiv