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 |