Anchovy
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In the context of cosmic rays?
The term 'prompt muon' refers to muons produced from charmed particle decays and other direct processes, known as X-processes, which do not exhibit zenith angle dependence typical of muons from normal processes like pion and kaon decays. These prompt muons are generated from short-lived particles containing c quarks that decay rapidly, resulting in muons that arrive at the surface of the Earth without directional preference. The discussion highlights the differences in angular dependence and energy levels between prompt muons and those from conventional atmospheric processes.
PREREQUISITESPhysicists, researchers in particle physics, and students studying cosmic rays and high-energy interactions will benefit from this discussion.
Muons resulting from charmed particle decays and other so-called prompt or direct processes, often referred to as X-processes, do not manifest the zenith angle dependence which is characteristic for muons from so-called normal processes, i.e., from pion and kaon decays
High-energy collisions can produce heavy quarks, typically as quark+antiquark pair.Anchovy said:Ahh, good find. So there are short-lived particles containing c quarks in the atmosphere (which ones specifically and what are they doing there in the first place?) that rapidly decay (hence 'prompt') to muons.
Anchovy said:So there are short-lived particles containing c quarks in the atmosphere (which ones specifically and what are they doing there in the first place?)