Gamma absorption at increasing energy levels

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SUMMARY

The discussion focuses on gamma absorption modes of matter for energies below 500 MeV, detailing mechanisms such as photoelectric absorption, Compton scattering, electron-positron pair production, and photonuclear absorption. Key energy thresholds include 1.7 MeV for photonuclear absorption in He-4 and 140 MeV for N+γ→N+π interactions. The conversation highlights that electron pair production remains the dominant process in regular matter, with muon pair production being significantly less frequent due to mass differences. The pion production edge, influenced by blueshifted relic radiation, is identified as a critical factor affecting cosmic ray energy limits.

PREREQUISITES
  • Understanding of gamma-ray interactions with matter
  • Familiarity with particle physics concepts such as pair production and resonance
  • Knowledge of energy thresholds relevant to photonuclear reactions
  • Basic principles of cosmic ray physics and energy loss mechanisms
NEXT STEPS
  • Research the mechanisms of photoelectric absorption in detail
  • Explore the implications of muon pair production in high-energy physics
  • Investigate the role of pion production in cosmic ray interactions
  • Study the effects of blueshifted relic radiation on cosmic ray energy limits
USEFUL FOR

Physicists, astrophysicists, and researchers in high-energy particle physics seeking to understand gamma absorption processes and their implications for cosmic ray behavior.

snorkack
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Which are main absorption modes of matter for gamma rays under about 500 MeV? And how strong is the absorption?

For low energies (under 20 MeV) the mechanisms are:
1) Photoelectric absorption - all energies from eV range onwards
2) Compton scattering - all energies enough to displace the electron
3) Electron-positron pair production - starting at 1022 keV
4) Photonuclear absorption - beginning at 1,7 MeV for Be-9, and edges going on to about 20 MeV for He-4

But then on? How absorptive is matter in the range of 40...400 MeV?
The next edges should be:
5) N+γ→N+π, from 140 MeV
6) Muon pair production, from 212 MeV+recoil, which is a lot
7) N+γ→Δ, about 300 MeV, but a broad one because Δ is a resonance, thus wide

Is any of these edges distinguished by a significant intensity compared to the background level of absorption due to 1...4, between the 30...100 MeV range?
 
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Electron pair production stays the dominant process in regular matter. The LHC produces electrons with more than 1 TeV and they still form regular electromagnetic showers.
 
Found estimates for muon pair production. The ratio of electron and muon pair production above threshold turns out to be proportional to inverse square of mass - so 40 000 times less.
But this does not estimate the cross-section for pi meson production - directly or via delta resonance.
How much is that, compared to electron pairs?
 
Pair production is typically several barns (increasing with Z). Inelastic processes with a nucleus are smaller than a barn, and specific reactions are even smaller. I don't have numbers but it is negligible in most cases.
 
mfb said:
Pair production is typically several barns (increasing with Z). Inelastic processes with a nucleus are smaller than a barn, and specific reactions are even smaller. I don't have numbers but it is negligible in most cases.

Well, pion production edge due to blueshifted relic radiation is claimed to be a major limit on cosmic ray range/energy.
How prominent is that pion production edge over positron pair production in order for this claim to be plausible?
 
snorkack said:
Well, pion production edge due to blueshifted relic radiation is claimed to be a major limit on cosmic ray range/energy.
How prominent is that pion production edge over positron pair production in order for this claim to be plausible?
That limits the range of protons. Protons have a weaker electric field than all other nuclei and the photon-electron interactions are completely missing in this scenario. In addition the energy loss from pion production is much larger than the energy loss from electron/positron pair production in this scenario - something that doesn't apply if we care about the photon.
 

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