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Additional resources for Methods of Experimental Physics. Neutron scattering B (AP, 1986-1987)
1996). At these extremely high field strengths the Lorentz force acting on an atomic electron equals or exceeds the Coulomb binding force even for low-lying states, and a recalculation of the atomic structure becomes necessary. , 1989), there are still many open questions associated with the general case of magnetic and electric fields. It is the purpose of this work, to examine the influence of the additional electric field on the hydrogen atom in the atmosphere of magnetic white dwarf stars.
Rep. 199:231. , 1996a, Hydrogen atom in very strong magnetic and electric fields, Phys. Rev. A 53:2135. , 1996b, Stationary hydrogen lines in magnetic and electric fields of white dwarf stars, Astron. Astrophys. 314:700. , 1997, Numerical simulation of electronic wavepacket evolution, SFB 382 Report Nr. 78, Phys. Rev. A submitted. , 1994, Line broadening in the presence of strong magnetic fields, Astron. Astrophys. 282:179. , 1996, Observation of flux and polarization spectra of white dwarfs with low magnetic fields, Astron.
Bignami, G. , Caraveo, P. , 1996, Multiwavelength data suggest a cyclotron feature on the hot thermal continuum of Geminga, Astrophys. J. 456:L111. , and Pavlov, G. , 1996, Polarization modes in a strongly magnetized hydrogen gas, Astrophys. J. 469:373. Burkova, L. , Dzialoshinskii, I. , Drukarev, G. , and Monozon, B. , 1976, Hydrogen-like systems in crossed electric and magnetic fields, Zh. Exp. Teor. Fiz. (Sov. Phys. JETP) 71:526. Caraveo, P. , 1997, Neutron star astronomy, Adv. , in press. Caraveo, P.
Methods of Experimental Physics. Neutron scattering B (AP, 1986-1987) by Author Unknown