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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/13969
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dc.contributor.authorHolkundkar, Amol R.-
dc.date.accessioned2024-01-25T03:53:07Z-
dc.date.available2024-01-25T03:53:07Z-
dc.date.issued2014-06-
dc.identifier.urihttps://arxiv.org/abs/1406.0398-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/13969-
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 tuneable 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 motion.en_US
dc.language.isoenen_US
dc.publisherARXIVen_US
dc.subjectPhysicsen_US
dc.subjectOptics (physics.optics)en_US
dc.subjectClassical Physics (physics.class-ph)en_US
dc.titleMagnetic mirror cavities as THz radiation sources and a means of quantifying radiation frictionen_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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