What Does It Mean for a Fireball to Be Opaque to Pair Production?

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SUMMARY

The discussion centers on the concept of "opacity to pair production" in the context of fireballs and high-energy astrophysics. It establishes that an opaque source prevents high-energy photons from escaping due to increased optical depth, which is a function of photon energy. The interaction γγ' → e+ e- illustrates how very high-energy photons interact with cosmic infrared photons, leading to attenuation and rendering the universe opaque to such emissions at TeV energies. This phenomenon significantly limits the visibility of extragalactic sources of multi-TeV radiation, particularly at distances of 1 Gpc and redshifts z 0.2.

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  • Understanding of pair production in particle physics
  • Familiarity with optical depth and its implications in astrophysics
  • Knowledge of high-energy photon interactions, specifically at TeV energies
  • Basic concepts of cosmic infrared background radiation
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  • Research the process of pair production and its significance in high-energy astrophysics
  • Study the effects of optical depth on photon escape in astrophysical sources
  • Explore the implications of cosmic infrared background radiation on high-energy photon detection
  • Investigate the capabilities and limitations of current telescopes in detecting TeV radiation
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Astronomers, astrophysicists, and students studying high-energy astrophysics, particularly those interested in the interactions of photons and the implications for observing distant cosmic sources.

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What does "to be opaque to pair production" mean?
(I'm talking about fireball).
I know what a pair production is but I can't get the crucial point: does it mean the photons don't collide?
If it is so that means an opaque-to-p.p.- source have a greater luminosity (emits more photons) than a non opaque source ...
but it can't be because the optical depth is usually an increasing function of the photon energy, and therefore, a large optical depth would prevent the escape of high-energy photons from the source...
 
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Physics news on Phys.org
From : http://press.princeton.edu/chapters/s9092.pdf

"Ultravioletand X-ray fluxes from compact sources are often attenuated by
photoelectric absorption from intervening neutral or ionized matter, including absorption by Milky Way gas. At TeV energies, the Ultraviolet and X-ray fluxes fromcompact sources are often attenuated by photoelectric absorption from intervening neutral or ionized matter, including absorption by Milky Way gas. At TeV energies, the universe
becomes opaque to pair production attenuation of very high-energy photons
(γ ) on cosmic infrared photons(γ')
. This process, represented by the reaction
γγ' → e+ e-
prevents us from seeing extragalactic sources of multi-
TeVradiation at distances 1 Gpc (redshifts z 0.2). The highest-energy
cosmic photon yet detected was at ≈90 TeVfrom a Milagro source [9]. At
100 TeV energies and higher, telescopes yet lack sufficient sensitivity to
detect cosmic sources or the plane of our Galaxy."


Bob S
 

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