Gamma absorption at increasing energy levels

In summary, the main absorption modes of matter for gamma rays under about 500 MeV are photoelectric absorption, Compton scattering, electron-positron pair production, and photonuclear absorption. In the range of 40-400 MeV, other modes such as N+γ→N+π, muon pair production, and N+γ→Δ become more dominant. However, in regular matter, electron pair production remains the dominant process. The cross-section for pi meson production is typically several barns and is negligible in most cases. The pion production edge is claimed to be a major limit on cosmic ray range/energy, but this is only plausible if it is more prominent than positron pair production.
  • #1
snorkack
2,190
477
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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  • #2
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.
 
  • #3
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?
 
  • #4
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.
 
  • #5
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?
 
  • #6
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.
 

What is gamma absorption?

Gamma absorption is the process in which gamma rays, a type of electromagnetic radiation, are absorbed by matter.

How does gamma absorption change at increasing energy levels?

As the energy levels of gamma rays increase, the probability of absorption also increases. This means that at higher energy levels, more gamma rays are likely to be absorbed by matter.

What factors affect gamma absorption at increasing energy levels?

There are several factors that can affect gamma absorption at increasing energy levels, including the density and composition of the absorbing material, the distance the gamma rays travel, and the strength of the gamma ray source.

What are some applications of studying gamma absorption at increasing energy levels?

Studying gamma absorption at increasing energy levels can provide valuable information about the properties and behavior of matter, and can be used in fields such as nuclear physics, medical imaging, and environmental monitoring.

How is gamma absorption at increasing energy levels measured?

Gamma absorption at increasing energy levels is typically measured using specialized equipment such as gamma ray detectors or spectrometers. These devices can detect and measure the intensity of gamma rays at different energy levels, allowing scientists to study their absorption patterns.

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