Timeline for Cherenkov radiation
Current License: CC BY-SA 4.0
11 events
| when toggle format | what | by | license | comment | |
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| Nov 27, 2020 at 15:14 | history | edited | Frederic Thomas | CC BY-SA 4.0 |
Improved a typesetting of a formula and its introducing sentence.
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| Jun 11, 2020 at 9:33 | history | edited | CommunityBot |
Commonmark migration
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| Nov 3, 2017 at 23:37 | comment | added | L. Maynard | @Arthur you're welcome. I am not sure what your level is but take a look at lss.fnal.gov/archive/2011/pub/fermilab-pub-11-688-ppd.pdf. I do not know too much more about this myself though I will know a lot more after next year. | |
| Nov 3, 2017 at 10:55 | comment | added | Nemo | @L.Maynard, Thank you! I appreciate. What type of interaction exist between neutrino and the nucleus? Why does neutrino need a nucleus in order to interact that way? | |
| Nov 2, 2017 at 21:48 | comment | added | L. Maynard | @Arthur I have added some more information into the question itself. Japan's Super-Kamiokande neutrino detector is of interest in this regard. | |
| Nov 2, 2017 at 21:46 | history | edited | L. Maynard | CC BY-SA 3.0 |
Expanded physical description, expanded description of neutrinos
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| Nov 2, 2017 at 21:41 | comment | added | Chris♦ | @Arthur High energy neutrinos can interact with matter to produce electrons, muons, or tau leptons, depending on the flavor and energy of the neutrinos. | |
| Nov 2, 2017 at 21:35 | history | edited | L. Maynard | CC BY-SA 3.0 |
Expanded physical description
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| Nov 2, 2017 at 14:21 | comment | added | Nemo | "It is actually resultant electrons and muons that emit the Cherenkov radiation. " What resultant electrons and muons? Where do they come from? | |
| Oct 31, 2017 at 19:19 | vote | accept | Nemo | ||
| Oct 30, 2017 at 2:37 | history | answered | L. Maynard | CC BY-SA 3.0 |