2019
DOI: 10.1038/s41598-019-46835-z
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Dynamics from elastic neutron-scattering via direct measurement of the running time-integral of the van Hove distribution function

Abstract: We present a new neutron-scattering approach to access the van Hove distribution function directly in the time domain, I(t), which reflects the system dynamics. Currently, I(t) is essentially determined from neutron energy-exchange. Our method consists of the straightforward measurement of the running time-integral of I(t), by computing the portion of scattered neutrons corresponding to species at rest within a time t , (conceptually elastic scattering). Previous attempts failed to recog… Show more

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Cited by 8 publications
(23 citation statements)
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“…The longest observation time, corresponding to the inverse of the best energy resolution (narrowest HWHM), is max{t obs } = 1.66/min{dE 1 } = 55 ps, and the shortest observation time, corresponding to the inverse of the broadest energy resolution (largest HWHM), is min{t obs } = 1.66/ max{dE 1 }=0.5 ps. The 1.66 factor for the proper conversion from HWHM to observation time has been explained in our previous work 32 (as well as the "0.6579 meV ps" factor for the proper conversion from energy to time). Also, in the vHI mode, N is the number of neutrons for each "configuration" of the primary spectrometer.…”
Section: Aim Of This Letter and Methodologymentioning
confidence: 65%
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“…The longest observation time, corresponding to the inverse of the best energy resolution (narrowest HWHM), is max{t obs } = 1.66/min{dE 1 } = 55 ps, and the shortest observation time, corresponding to the inverse of the broadest energy resolution (largest HWHM), is min{t obs } = 1.66/ max{dE 1 }=0.5 ps. The 1.66 factor for the proper conversion from HWHM to observation time has been explained in our previous work 32 (as well as the "0.6579 meV ps" factor for the proper conversion from energy to time). Also, in the vHI mode, N is the number of neutrons for each "configuration" of the primary spectrometer.…”
Section: Aim Of This Letter and Methodologymentioning
confidence: 65%
“…www.nature.com/scientificreports www.nature.com/scientificreports/ In fact, it is also possible to further increase the count-gain of vHI by adjusting the energy-width of the secondary spectrometer, dE 2 . It turns out that the vHI approximation holds for secondary spectrometer energy-widths up to four times smaller than the energy-width of the primary spectrometer 32 . This "secondary resolution count-gain" has been computed with our MC code by adjusting the energy-width of the secondary spectrometer to be four times smaller than that of the primary.…”
Section: Resultsmentioning
confidence: 99%
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