1897
DOI: 10.1080/14786449708621028
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VII. Doublets and triplets in the spectrum produced by external magnetic forces

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Cited by 54 publications
(22 citation statements)
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“…The x = 1/B that satisfy equation (26) give all the new maxima and minima in the MO at T = 0. Notice that at zero temperature β → ∞ and equation (26) implies x → x n , as expected.…”
Section: Mo Extrema Shiftmentioning
confidence: 97%
See 1 more Smart Citation
“…The x = 1/B that satisfy equation (26) give all the new maxima and minima in the MO at T = 0. Notice that at zero temperature β → ∞ and equation (26) implies x → x n , as expected.…”
Section: Mo Extrema Shiftmentioning
confidence: 97%
“…The new extrema will be located at x = x l − pδ l , where δ l is the corresponding shift and p = 1(−1) for the maxima (minima). In this way we can rewrite equation (26) as a function of δ l and the considered peak x l :…”
Section: Mo Extrema Shiftmentioning
confidence: 99%
“…Moreover, for each of these sidebands the frequency spacing between the two subpeaks grows larger as |α| increases. The observed sideband splitting leads to energy spectra for the amplified quantum noise that are qualitatively analogous to energy spectra of electrons under the Zeeman splitting of the spectral lines in a gas, which occurs in the presence of a strong magnetic field [31].…”
Section: Impact Of the Amplitude Of The Dispersion Oscillationmentioning
confidence: 92%
“…In the Landau gauge we have A = −Bye x , and the momentum changes following the Peierls substitution [26] p → p − eA. Considering the Zeeman effect [27], the term µ · B = µ B gBs z /2 is added to H, where s z = 2S z / is the Pauli matrix acting in the spin state. We omit the nearestand next-nearest neighbor Rashba SOIs, denoted as λ R1 and λ R2 in [11], since they are negligible in comparison to the intrinsic SOI λ SO .…”
Section: Energy Spectrummentioning
confidence: 99%