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Time-delayed coinci-dence technique for subnatural-width spec-troscopy as an inter-ference phenomenon

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dc.contributor Казанский федеральный университет
dc.contributor.author Shakhmuratov Rustem Nazimovich
dc.contributor.author Vagizov Farit Gabdulhakovich
dc.date.accessioned 2020-03-23T12:03:34Z
dc.date.available 2020-03-23T12:03:34Z
dc.date.issued 2019
dc.identifier.citation Shakhmuratov R. N. Time-delayed coincidence technique for subnatural-width spectroscopy as an inter-ference phenomenon / R. N. Shakhmuratov F. G. Vagizov // Phys. Rev. A. - 2019. - Vol. 99. No.3. - P. 033831-11
dc.identifier.issn 1050-2947
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/158233
dc.description.abstract A single photon, emitted in a transition between two states, has a frequency distribution of intensity that is given by a Lorentzian if the transition is only naturally broadened and the period of observation T is long compared to the lifetime T1 of the excited state. However, when the observation time T is short or comparable to T1, the frequency spectrum is appreciably broadened. If only the delayed part of the emitted radiation field is detected, then the radiation spectrum does not change. However, if the radiation field is transmitted through a resonant absorber and then detected, the transmission spectrum of the delayed radiation field is narrowed. We show that this narrowing is due to the interference of the spectral components of the incident and coherently scattered fields. Experimental spectra of absorption of Mössbauer radiation, obtained by the coincidence technique, confirm this conclusion.
dc.language.iso en
dc.relation.ispartofseries PHYS REV A
dc.rights открытый доступ
dc.subject single photon
dc.subject Mössbauer radiation
dc.subject interference
dc.subject line narrowing
dc.subject.other Физика
dc.title Time-delayed coinci-dence technique for subnatural-width spec-troscopy as an inter-ference phenomenon
dc.type Article
dc.contributor.org Химический институт им. А.М. Бутлерова
dc.description.pages 033831-1-033831-11
dc.relation.ispartofseries-issue 3
dc.relation.ispartofseries-volume 99
dc.pub-id 204459
dc.identifier.doi 10.1103/PhysRevA.99.033831


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