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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Holkundkar, Amol R. | - |
dc.date.accessioned | 2024-01-25T03:53:07Z | - |
dc.date.available | 2024-01-25T03:53:07Z | - |
dc.date.issued | 2014-06 | - |
dc.identifier.uri | https://arxiv.org/abs/1406.0398 | - |
dc.identifier.uri | http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/13969 | - |
dc.description.abstract | We 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.iso | en | en_US |
dc.publisher | ARXIV | en_US |
dc.subject | Physics | en_US |
dc.subject | Optics (physics.optics) | en_US |
dc.subject | Classical Physics (physics.class-ph) | en_US |
dc.title | Magnetic mirror cavities as THz radiation sources and a means of quantifying radiation friction | en_US |
dc.type | Article | en_US |
Appears in Collections: | Department of Physics |
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