The Quadratic Zeeman Effect in Moderately Strong Magnetic Fields

1987 ◽  
Vol 497 (1 Chaotic Pheno) ◽  
pp. 22-36 ◽  
Author(s):  
SHANNON L. COFFEY ◽  
ANDRÉ DEPRIT ◽  
BRUCE MILLER ◽  
CAROL A. WILLIAMS
Keyword(s):  
Magnetic Fields ◽  
Zeeman Effect ◽  
Strong Magnetic Fields ◽  
Quadratic Zeeman Effect

scholarly journals The study of the magnetic properties of matter strong magnetic fields.—I.—The balance and its properties

1931 ◽  
Vol 131 (816) ◽  
pp. 224-243 ◽  
Keyword(s):  
Magnetic Susceptibility ◽  
Magnetic Fields ◽  
Room Temperature ◽  
Direct Method ◽  
Magnetic Moments ◽  
Zeeman Effect ◽  
Inhomogeneous Magnetic Field ◽  
Present Communication ◽  
Strong Magnetic Fields ◽  
Short Times

In several previous communications the author has described a method by which magnetic fields up to 300,000 gauss could be obtained for a duration of time of the order of 1/100 of a second. It was shown that these magnetic fields, in spite of the shortness of their duration, can be applied to the study of different phenomena such as the change of resistance, the Zeeman effect, and others. The present paper describes a number of investigations which have been made on different substances, extending the application of intense magnetic fields to the study of magnetic susceptibility and magnetostriction. The interest in measuring the susceptibility of different substances in strong magnetic fields lies mainly in seeing whether the linear law of magnetisation for ordinary para- and diamagnetic substances holds for higher fields, and also in the investigation of the saturation of paramagnetic bodies at low temperatures, with a view to determining the elementary magnetic moments. In the present communication a method of measuring the magnetic susceptibility is described and experimental results are given which verify the linear law of magnetisation for several paramagnetic and diamagnetic substances. The saturation of iron and nickel in strong fields is also studied. As will be seen later, the possibility of making these measurements in such a small fraction of time results from the increased magnitude of the phenomenon itself. The most direct method for measuring the magnetic susceptibility is to record the force on a magnetised body in an inhomogeneous magnetic field. In the usual experiments at room temperature this force is only a few hundred dynes, but when fields reach the magnitude of 300 kilogauss the force becomes several grams, and is then sufficiently large to be measured with fair accuracy even in short times of the order of 1/100 of a second. In this paper a special type of balance will be described by which these measurements are made possible.

The Zeeman Effect in Strong Magnetic Fields

Nature ◽  
1924 ◽  
Vol 114 (2860) ◽  
pp. 273-273 ◽  
Author(s):  
P. KAPITZA ◽  
H. W. B. SKINNER
Keyword(s):  
Magnetic Fields ◽  
Zeeman Effect ◽  
Strong Magnetic Fields

scholarly journals The Quadratic Zeeman Effect for CI Lines-Application to the Spectrum of EG 129

1979 ◽  
Vol 53 ◽  
pp. 322-323
Author(s):  
I. Bues ◽  
G. Varvatis
Keyword(s):  
Magnetic Fields ◽  
Field Strength ◽  
Correction Factor ◽  
Energy Levels ◽  
Zeeman Effect ◽  
Visible Region ◽  
Quadratic Zeeman Effect

Garstang and Kemic (1974) derived formulae for the splitting of hydrogen and helium lines in the presence of large magnetic fields. We applied their method in calculating the eigenvectors for some transitions of neutral carbon, where a correction factor for the coupling and mixing of the energy levels has to be applied. For CI – lines in the visible region of the spectrum, well separated components can be expected for a field strength up to 2 • 107G. Fig. 1 shows the splitting of three lines for B = 107 G.

scholarly journals Hochtemperatur-Mikrowellenspektrometer für Zeeman-Effekt-Messungen an diamagnetischen Molekeln

1973 ◽  
Vol 28 (3-4) ◽  
pp. 458-463
Author(s):  
R. Honerjäger ◽  
R. Tischer
Keyword(s):  
Magnetic Susceptibility ◽  
High Temperature ◽  
Magnetic Fields ◽  
Zeeman Effect ◽  
Absorption Cell ◽  
Vibrational States ◽  
Magnetic Susceptibility Anisotropy ◽  
Strong Magnetic Fields ◽  
Upper Limit ◽  
Microwave Spectrometer

AbstractA high-temperature microwave spectrometer has been developed for Zeeman effect measurements in strong magnetic fields up to 50 kG. The absorption cell is placed in a superconducting solenoid and can be heated as high as 1200 °C. The gJ-factor and the magnetic susceptibility anisotropy of TIF, CsF and CsCl, the gJ-factor of CsBr, and an upper limit for the value of the gJ-factor of CsI have been measured. The molecules CsF and CsCl were also studied in higher vibrational states.

scholarly journals The Zeeman and Paschen-Back effects in strong magnetic fields

1938 ◽  
Vol 167 (928) ◽  
pp. 1-15 ◽  
Author(s):  
Piotr Leonidovich Kapitza ◽  
P. G. Strelkov ◽  
E. Laurman
Keyword(s):  
Magnetic Fields ◽  
Experimental Error ◽  
Applied Field ◽  
Zeeman Effect ◽  
Spectral Lines ◽  
Strong Magnetic Fields ◽  
Current Impulse ◽  
Accumulator Battery ◽  
Small Capacity ◽  
The Magnetic Field

The Zeeman effect in strong magnetic fields was first studied by Kapitza and Skinner (1925), the fields being obtained by a method developed by one of us (Kapitza 1924), in which an accumulator battery of small capacity was discharged through a coil. In this way it was possible to obtain magnetic fields up to 140,000 gauss during a time of 1/100 sec. It turned out that in such fields the majority of the spectral lines which were studied, split up (within the limits of experimental error) proportionally to the applied field, in accordance with the theory which had previously been verified only in weaker magnetic fields. An exception, however, was the zinc line at 4680 A, which gave a splitting about 10% greater than that predicted by the theory, this discrepancy being outside the limits of experimental error. Since then the method of producing strong magnetic fields has been considerably developed (Kapitza 1927); instead of the discharge of an accumulator the powerful current impulse from a short-circuited generator has been used, which has made possible the production of fields more than twice as great as those formerly obtained, and moreover, in considerably larger volumes. A the same time the technique of measuring the magnetic field has also been improved. Using these improvements we have made a new investigation of the Zeeman effect in fields up to 320,000 gauss, in which we have been able to increase considerably the accuracy of the measurements, and to explain the cause of the discrepancies previously found. We have also been able to investigate the Paschen-Back effect and to verify the theory of this effect.

Polarized Radiation from White Dwarfs and Atoms in Strong Magnetic Fields

1974 ◽  
Vol 53 ◽  
pp. 287-300
Author(s):  
R. F. O'Connell
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Cross Section ◽  
White Dwarfs ◽  
Zeeman Effect ◽  
Initial Response ◽  
Model Atmosphere ◽  
Radiation Absorption ◽  
Strong Magnetic Fields ◽  
Polarized Radiation

We present the recent results of our continuing program of investigation of the behavior of matter in strong to super-strong magnetic fields (B ∼ 106−1012 G). This work was motivated by the discovery of strong magnetic fields (B ∼ 107 G) in some white dwarfs and the likely existence of super-strong fields (B ∼ 1012 G) in pulsars. Magnetic white dwarfs were discovered from observations of the continuous spectrum and one of the most intriguing challenges for the theorist is to provide an explanation for the observed wavelength dependence of the fractional circularly and linearly polarized radiation. Our initial response to this question was the determination of an exact solution of Kemp's harmonic oscillator model. These results are used as input to the ATLAS model atmosphere program and then comparison is made with observations. The disparities still existing between theory and observation convince us of the necessity for developing a new model of the continuum radiation, two likely possibilities being photoionization and free-free absorption. This leads us to present a general formulation of radiation absorption and emission processes in a magnetic field. Next we calculate the cross section for the photoionization, correct to first order in B. For the purpose of obtaining exact results for this cross section, the effect of a magnetic field on the energy spectrum and wave functions of hydrogen, helium, etc. must be obtained. The results for hydrogen are presented here. They will be useful also in determining accurate values for the displacements due to the quadratic Zeeman effect in the line spectra of DA stars, particularly for the higher excited states.

scholarly journals Hot-star wind models with magnetically split line blanketing

2018 ◽  
Vol 620 ◽  
pp. A176 ◽  
Author(s):  
J. Krtička
Keyword(s):  
Magnetic Fields ◽  
Zeeman Effect ◽  
Zeeman Splitting ◽  
Magnetic Line ◽  
Hot Stars ◽  
Strong Magnetic Fields ◽  
Flux Variability ◽  
Line Splitting ◽  
Line Force ◽  
The Magnetic Field

Fraction of hot stars posses strong magnetic fields that channel their radiatively driven outflows. We study the influence of line splitting in the magnetic field (Zeeman effect) on the wind properties. We use our own global wind code with radiative transfer in the comoving frame to understand the influence of the Zeeman splitting on the line force. We show that the Zeeman splitting has a negligible influence on the line force for magnetic fields that are weaker than about 100 kG. This means that the wind mass-loss rates and terminal velocities are not affected by the magnetic line splitting for magnetic fields as are typically found on the surface of nondegenerate stars. Neither have we found any strong flux variability that would be due to the magnetically split line blanketing.

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