| Display title | Physics:Luminosity (scattering theory) |
| Default sort key | Luminosity (scattering theory) |
| Page length (in bytes) | 6,421 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 421692 |
| Page content language | en - English |
| Page content model | wikitext |
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| Page creator | imported>WikiGary |
| Date of page creation | 01:07, 8 February 2024 |
| Latest editor | imported>WikiGary |
| Date of latest edit | 01:07, 8 February 2024 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | In scattering theory and accelerator physics, luminosity (L) is the ratio of the number of events detected (dN) in a certain period of time (dt) to the cross-section (σ):
$ L={\frac {1}{\sigma }}{\frac {dN}{dt}}. $
It has the dimensions of events per time per area, and is usually expressed in the cgs... |
