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Titlebook: Atoms in Strong Magnetic Fields; Quantum Mechanical T Hanns Ruder,Günter Wunner,Florian Geyer Book 1994 Springer-Verlag Berlin Heidelberg 1

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期刊全称Atoms in Strong Magnetic Fields
期刊简称Quantum Mechanical T
影响因子2023Hanns Ruder,Günter Wunner,Florian Geyer
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学科分类Astronomy and Astrophysics Library
图书封面Titlebook: Atoms in Strong Magnetic Fields; Quantum Mechanical T Hanns Ruder,Günter Wunner,Florian Geyer Book 1994 Springer-Verlag Berlin Heidelberg 1
影响因子In this book we summarize the essential results of our efforts over the years to calculate energies, wave functions, and electromagnetic transitions of atoms as functions of the magnetic field strength from laboratory fields up to neutron star magnetic fields. Motivated by the observational evidence of huge magnetic 5 fields with strengths up to 10 T in the vicinity of white dwarf stars and of up 9 to 10 T in the vicinity of neutron stars the authors, together with coworkers and candidates for doctor and diploma degrees, have investigated this ,fasci­ nating quantum mechanical problem more or less continuously since 1978. The extensive tables and figures in the appendices represent the most complete data set to date in this field of research. For practical use all numbers are available by "anonymous ftp" over Internet. The first direct measurement of a neutron star magnetic field by Trum­ per and his group, who observed a cyclotron feature at about 50 ke V in the spectrum of the X-ray pulsar Hercules X-I corresponding to a field strength of 8 several 10 T, stimulated investigations of atoms within the framework of the adiabatic approximation, which is well justified for such field
Pindex Book 1994
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Die Tatkraft der vier Basisemotionen,ltonian of an electron in a static Coulomb potential and in a uniform magnetic field then reads for spin-down states . where the magnetic field is assumed to point in the .-direction and .. = ..+... The energies of the corresponding spin-up states are obtained by simply adding .. The eigenstates of
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,Führung, Verbundenheit und Vertrauen,) are given for the 38 lowest-lying states of the static Coulomb problem — corresponding to the H atom with infinite proton mass — and for magnetic field strengths in the range 10. ≤ . ≤ 10.. The tables are ordered according to the azimuthal quantum number . and the .-parity .. The states are labell
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,Führung, Verbundenheit und Vertrauen,sary to cover arbitrary .. does not, in general, justify the effort. However, in the limit of intense magnetic fields, where the adiabatic approximation is applicable — that is, the factorization of the wave function in a single product of a Landau wave function and a longitudinal part —, an asympto
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optical spectra of magnetized white dwarf stars, which had defied interpretation for almost 50 years, in terms of . components of hydrogen lines in magnetic fields of several 10. T (Angel et al. 1985; Greenstein et al. 1985; Wunner et al. 1985b; Schmidt et al., 1986a,b). By . components we mean thos
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he justification for this approach was furnished by Lindgren and Virtamo (1979), who, by numerically solving Dirac’s equation, showed that relativistic effects on the Coulomb binding energies remain negligible even for magnetic field strengths of up to 4.7 × 10. T. From this it is obvious that the i
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