Antiproton flux and cross-sections in antideuterium production

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  • Thread starter Thread starter LeInvertedPenguine
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    Cross-section Flux
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SUMMARY

The discussion centers on antideuterium production and its relevance to dark matter detection, specifically addressing the concept of cross-sections in particle physics. Cross-sections are defined as the probability of a specific interaction occurring, such as annihilation into Standard Model channels or scattering events involving dark matter. Participants confirm that a high signal-to-background ratio is anticipated in antiproton flux, which is significant for probing dark matter candidates. The conversation highlights the need for context regarding dark matter models and detection methods to fully understand the implications of antiproton and antideuterium fluxes.

PREREQUISITES
  • Understanding of particle physics terminology, specifically "cross-section" and "signal-to-background ratio".
  • Familiarity with dark matter detection methods and models.
  • Knowledge of Standard Model interactions in particle physics.
  • Basic comprehension of antiproton and antideuterium production processes.
NEXT STEPS
  • Research "cross-section calculations in particle physics" for a deeper understanding of interaction probabilities.
  • Explore "dark matter detection techniques" to learn about various methodologies used in experiments.
  • Study "antiproton and antideuterium production mechanisms" to grasp their roles in cosmic ray physics.
  • Investigate "signal-to-background ratio optimization" in experimental physics to enhance detection strategies.
USEFUL FOR

Physicists, researchers in particle physics, and students studying dark matter detection and cosmic ray interactions will benefit from this discussion.

LeInvertedPenguine
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Hello!

I`m currently reading an article about antideuterium production and dark matter detection. The article often uses the term cross-section, like for example: “Assuming an annihilation cross section into a particular Standard Model Channel” and “Probe scattering cross sections through the recoil of dark matter off of target nuclei”. I would be very grateful if someone could clarify this term to me in this context. Also, is it correct that we can expect an high signal-to-background ratio in the antiproton flux alongside the expected antideuterium flux and do we use this actively when probing for dark matter candidates?
 
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I wrote an article about cross sections. They are connected to the probability that a process happens.

Your second question is missing too much context. Which dark matter model are you looking at, what would be the detection method, and so on?
 
Thank you, I will definitely take a look at the article.

I suppose the latter sort of answers my question as well. I take the request for more context that the increased antiproton flux is nothing we generally search for across a wide range of models. Since I don’t know enough to elaborate on it, I will leave it for now until I am able to ask about something that makes sense.
Thank you so much for your reply.
 

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