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dc.contributor.authorHolkundkar, Amol R.-
dc.date.accessioned2024-01-24T09:37:02Z-
dc.date.available2024-01-24T09:37:02Z-
dc.date.issued2014-10-
dc.identifier.urihttps://pubs.aip.org/aip/pop/article/21/10/103102/376423-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/13957-
dc.description.abstractWe propose a radiation source based on a magnetic mirror cavity. Relativistic electrons are simulated entering the cavity and their trajectories and resulting emission spectra are calculated. The uniformity of the particle orbits is found to result in a frequency comb in terahertz range, the precise energies of which are tunable by varying the electron's γ-factor. For very high energy particles, radiation friction causes the spectral harmonics to broaden and we suggest this as a possible way to verify competing classical equations of motionen_US
dc.language.isoenen_US
dc.publisherAIPen_US
dc.subjectPhysicsen_US
dc.subjectDoppler effecten_US
dc.subjectMagnetic fieldsen_US
dc.subjectTerahertz radiationen_US
dc.subjectInsertion deviceen_US
dc.subjectRadiowave and microwave technologyen_US
dc.subjectCyclotron resonanceen_US
dc.subjectMagnetic mirrorsen_US
dc.titleMagnetic mirror cavities as terahertz radiation sources and a means of quantifying radiation frictionen_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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