標(biāo)題: Titlebook: Atoms in Strong Magnetic Fields; Quantum Mechanical T Hanns Ruder,Günter Wunner,Florian Geyer Book 1994 Springer-Verlag Berlin Heidelberg 1 [打印本頁(yè)] 作者: incompatible 時(shí)間: 2025-3-21 18:20
書(shū)目名稱(chēng)Atoms in Strong Magnetic Fields影響因子(影響力)
書(shū)目名稱(chēng)Atoms in Strong Magnetic Fields影響因子(影響力)學(xué)科排名
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書(shū)目名稱(chēng)Atoms in Strong Magnetic Fields讀者反饋
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作者: fibroblast 時(shí)間: 2025-3-21 23:48 作者: 非秘密 時(shí)間: 2025-3-22 03:00
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 作者: Neonatal 時(shí)間: 2025-3-22 05:24
,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作者: Angiogenesis 時(shí)間: 2025-3-22 10:00
,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作者: 孵卵器 時(shí)間: 2025-3-22 13:46 作者: EXCEL 時(shí)間: 2025-3-22 18:45
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作者: beta-carotene 時(shí)間: 2025-3-22 22:23
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作者: Encumber 時(shí)間: 2025-3-23 02:19 作者: DENT 時(shí)間: 2025-3-23 07:24 作者: amplitude 時(shí)間: 2025-3-23 11:34 作者: Gudgeon 時(shí)間: 2025-3-23 16:15 作者: Champion 時(shí)間: 2025-3-23 20:22
Astronomy and Astrophysics Libraryhttp://image.papertrans.cn/b/image/164836.jpg作者: 反復(fù)無(wú)常 時(shí)間: 2025-3-24 00:47 作者: Retrieval 時(shí)間: 2025-3-24 06:02 作者: projectile 時(shí)間: 2025-3-24 08:31
0941-7834 nsitions 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 sta作者: notification 時(shí)間: 2025-3-24 12:43 作者: myalgia 時(shí)間: 2025-3-24 18:44 作者: allude 時(shí)間: 2025-3-24 21:51 作者: 泥沼 時(shí)間: 2025-3-25 02:33 作者: Visual-Field 時(shí)間: 2025-3-25 03:36
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.作者: 肌肉 時(shí)間: 2025-3-25 10:50 作者: 配偶 時(shí)間: 2025-3-25 12:31
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).作者: Vertical 時(shí)間: 2025-3-25 19:41
,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.作者: transdermal 時(shí)間: 2025-3-25 20:21
,Die eigenen Ressourcen zutage f?rdern,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).作者: institute 時(shí)間: 2025-3-26 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.作者: 加入 時(shí)間: 2025-3-26 08:18 作者: atopic 時(shí)間: 2025-3-26 10:59 作者: 樂(lè)意 時(shí)間: 2025-3-26 13:33 作者: 小卷發(fā) 時(shí)間: 2025-3-26 19:05
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.作者: Mosaic 時(shí)間: 2025-3-26 23:32
Highly Excited States,rengths of white dwarfs or neutron stars, can be realized for highly excited states (.. > 30, e.g.) even in terrestrial laboratory field strengths of several Tesla. The discussion of the influence of strong laboratory magnetic fields on . of the hydrogen atom is the subject of this chapter.作者: 受傷 時(shí)間: 2025-3-27 03:27
Die Tatkraft der vier Basisemotionen,(3.1) can be classified according to .-parity . and the .component .. of orbital angular momentum, which are exact symmetries of ., but in general no further separation of the two-dimensional problem is possible.作者: senile-dementia 時(shí)間: 2025-3-27 05:33 作者: 思想 時(shí)間: 2025-3-27 11:37 作者: 騙子 時(shí)間: 2025-3-27 14:31 作者: 表示向下 時(shí)間: 2025-3-27 20:44
Interacting Charged Particles in Uniform Magnetic Fields,tential . at the position .. of particle . is abbreviated by .. = ..). In this section no special gauge is adopted. The Hamiltonian of the system is given by . where the potential energy . of the interaction is assumed to be momentum independent and translationally invariant. Generally, the conserve作者: 排名真古怪 時(shí)間: 2025-3-28 00:32
Methods of Solution for the Magnetized Coulomb Problem,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 作者: tolerance 時(shí)間: 2025-3-28 02:12 作者: Notorious 時(shí)間: 2025-3-28 06:23 作者: Chemotherapy 時(shí)間: 2025-3-28 10:35 作者: 喃喃訴苦 時(shí)間: 2025-3-28 15:15
Stationary Lines and White Dwarf Spectra,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作者: BRACE 時(shí)間: 2025-3-28 20:59
Relativistic Effects, Nuclear Mass Effects, and Landau-Excited States,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
