What is the meaning of the term 'prompt muon'?

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Discussion Overview

The discussion centers around the term 'prompt muon' in the context of cosmic rays, exploring the origins and characteristics of these muons, particularly in relation to their production from short-lived particles.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants suggest that prompt muons result from charmed particle decays and other direct processes, which do not exhibit the zenith angle dependence typical of muons from normal processes like pion and kaon decays.
  • There is a discussion about the presence of short-lived particles containing c quarks in the atmosphere, with questions raised about which specific particles contribute to prompt muon production and their mechanisms.
  • One participant proposes that the lack of directional preference for prompt muons may be due to their parent particles not scattering significantly before decaying, unlike those from normal processes that may scatter more based on their zenith angles.
  • Another viewpoint mentions that while prompt muons have a different angular dependence compared to normal processes, they still exhibit some directional preference, particularly in that they do not travel upwards.
  • A participant shares personal experience with accelerator-based experiments involving high-energy proton beams, suggesting similarities with cosmic-ray interactions that produce charm-anticharm pairs leading to prompt muons.

Areas of Agreement / Disagreement

Participants express varying degrees of understanding and hypotheses regarding the nature of prompt muons and their origins, indicating that multiple competing views remain without a clear consensus.

Contextual Notes

There are limitations in the discussion regarding the specific identities of the short-lived particles involved and the mechanisms of their decay processes, which remain unresolved.

Anchovy
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In the context of cosmic rays?
 
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Google knows the answer:
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
 
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.

And these muons arrive at the surface with no directional preference... but I'm not fully clear on why... The \pi, \hspace{1 mm} K that decay to produce the usual atmospheric muons might approach from wide zenith angles, and must therefore pass through much more atmosphere than those from small zenith angles, thus scattering more before they decay... but the parent particles of the prompt muons barely pass through any atmosphere regardless of angle... so they don't tend scatter before they decay? And the muons themselves don't scatter much once they've been created?
 
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.
High-energy collisions can produce heavy quarks, typically as quark+antiquark pair.

Those muons also have a directional preference (most notably, they don't go up), but the angular dependence is different from the normal processes. Their higher typical energy might be related to it.
 
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?)

I'm not familiar with cosmic-ray studies. However, a long time ago I had a small involvement with an accelerator-based "beam dump" experiment in which a high-energy proton beam was sent into a block of metal. Among the many particle-antiparticle pairs produced in such interactions are some charm-anticharm pairs which produce prompt muons. I suspect you have a similar situation with high-energy cosmic-ray interactions.

(edit: mfb beat me to it while I was typing.)
 
OK thanks guys.
 

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