Visual-Field
发表于 2025-3-25 03:36:44
Electromagnetic Transition Probabilities, are involved, whereas in strong magnetic fields the .-degeneracy is completely destroyed. Let us, therefore, begin by briefly reviewing the considerations, and the formulae, which are valid also for strong magnetic fields.
肌肉
发表于 2025-3-25 10:50:04
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配偶
发表于 2025-3-25 12:31:12
Relativistic Effects, Nuclear Mass Effects, and Landau-Excited States,d. The purpose of this section is to demonstrate that, in spite of its smallness, the spin-orbit interaction can produce drastic effects because it reduces the invariance group of the Hamiltonian (see also Wunner et al. 1985a).
Vertical
发表于 2025-3-25 19:41:04
,Führung in dynamischen Zeiten, against its own gravitational forces. The catastrophic collapse to a neutron star is usually accompanied by a supernova explosion, in which the star becomes almost as bright as a whole galaxy consisting of a hundred billion suns. Typical values of relevant physical parameters are listed in Table 1.1 in comparison with our sun.
transdermal
发表于 2025-3-25 20:21:43
,Die eigenen Ressourcen zutage fördern,erefore, an additional gauge transformation is necessary to preserve the translational invariance of . Thus we arrive at the following form of the generalized momentum operator: . (. = 1, 2, 3 denotes the Cartesian components).
institute
发表于 2025-3-26 03:03:03
white dwarf spectra is obvious when one considers that the magnetic field strength varies (in a dipolar geometry) by a factor of two across the white dwarf and thus all fast moving wavelengths are smeared out.
加入
发表于 2025-3-26 08:18:25
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atopic
发表于 2025-3-26 10:59:32
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乐意
发表于 2025-3-26 13:33:14
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小卷发
发表于 2025-3-26 19:05:06
Stationary Lines and White Dwarf Spectra,white dwarf spectra is obvious when one considers that the magnetic field strength varies (in a dipolar geometry) by a factor of two across the white dwarf and thus all fast moving wavelengths are smeared out.