2019
DOI: 10.1016/j.jpcs.2017.12.034
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Nuclear magnetic relaxation and Knight shift due to orbital interaction in Dirac electron systems

Abstract: We study the nuclear magnetic relaxation rate and Knight shift in the presence of the orbital and quadrupole interactions for three-dimensional Dirac electron systems (e.g., bismuth-antimony alloys). By using recent results of the dynamic magnetic susceptibility and permittivity, we obtain rigorous results of the relaxation rates (1/T 1 ) orb and (1/T 1 ) Q , which are due to the orbital and quadrupole interactions, respectively, and show that (1/T 1 ) Q gives a negligible contribution compared with (1/T 1 ) o… Show more

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Cited by 29 publications
(57 citation statements)
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References 38 publications
(83 reference statements)
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“…Putting together the inter‐ and intraband contribution, the real part of the response function reads asRe[Πab(q) ]=qaqb12π2vnormalF(ln[Wfalse|μfalse|]1415)for a ≠ b . This qualitatively agrees with the result from the previous studies . We also evaluated Equation numerically and compared with Equation .…”
Section: Explicit Formula Of the Response Function At Zero Temperaturesupporting
confidence: 89%
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“…Putting together the inter‐ and intraband contribution, the real part of the response function reads asRe[Πab(q) ]=qaqb12π2vnormalF(ln[Wfalse|μfalse|]1415)for a ≠ b . This qualitatively agrees with the result from the previous studies . We also evaluated Equation numerically and compared with Equation .…”
Section: Explicit Formula Of the Response Function At Zero Temperaturesupporting
confidence: 89%
“…This qualitatively agrees with the result from the previous studies. [18,21,26,27] We also evaluated Equation (16) numerically and compared with Equation (27). The agreement is perfect which is shown in Figure 1.…”
Section: Real Partmentioning
confidence: 82%
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“…A recent model of spin-orbit-based NMR relaxation in 3D Dirac and Weyl systems accounts for this behavior very well. In this theory [24,25], fluctuations in Dirac-type orbital currents are responsible for the relaxation. The orbital hyperfine interaction introduces a 1/k 2 contribution to the momentum sum determining 1/T 1 T [24,26], thus connecting to fluctuations that are more extended in space than the typical local contributions, explaining the site-independence.…”
mentioning
confidence: 99%