| 1. | The spectrum of the scattered photons is termed the Raman spectrum.
|
| 2. | If the scattered photon still has enough energy, the process may be repeated.
|
| 3. | This is done by creating a photon of known wavelength and measuring the wavelength of the scattered photon.
|
| 4. | In particular the minimum uncertainty is when the scattered photon has limit energy equal to the incident observing energy.
|
| 5. | With a bright star the scattered photons are sufficient to expose the film and make a slightly larger image.
|
| 6. | Momentum and energy conservation require that these are equal to the momentum and energy loss of the scattered photon.
|
| 7. | Compared to a confocal microscope, photon detection is much more effective since even scattered photons contribute to the usable signal.
|
| 8. | A hemispherical semiconductor would also work, with the flat back-surface serving as a mirror to back-scattered photons.
|
| 9. | This constraint arises from the fact that in RIXS the scattered photons do not add or remove charge from the system under study.
|
| 10. | It is a photon-in / photon-out spectroscopy where one measures both the energy and momentum change of the scattered photon.
|
मोबाइल