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 |