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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Holkundkar, Amol R. | - |
dc.date.accessioned | 2024-01-24T09:37:02Z | - |
dc.date.available | 2024-01-24T09:37:02Z | - |
dc.date.issued | 2014-10 | - |
dc.identifier.uri | https://pubs.aip.org/aip/pop/article/21/10/103102/376423 | - |
dc.identifier.uri | http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/13957 | - |
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 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 motion | en_US |
dc.language.iso | en | en_US |
dc.publisher | AIP | en_US |
dc.subject | Physics | en_US |
dc.subject | Doppler effect | en_US |
dc.subject | Magnetic fields | en_US |
dc.subject | Terahertz radiation | en_US |
dc.subject | Insertion device | en_US |
dc.subject | Radiowave and microwave technology | en_US |
dc.subject | Cyclotron resonance | en_US |
dc.subject | Magnetic mirrors | en_US |
dc.title | Magnetic mirror cavities as terahertz 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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