Photoatomic and photonuclear reactions

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SUMMARY

This discussion focuses on the interactions between gamma photons and atomic nuclei, specifically photoatomic and photonuclear reactions. Key processes include photoelectric absorption and Compton scattering for photoatomic reactions, while photonuclear reactions involve pair production and photoneutron emission. The interaction with Uranium-238 (U238) primarily involves Compton scattering and photoelectric absorption for gamma energies below 1.0222 MeV. Resources such as Glenn F. Knoll's "Radiation Detection and Measurement" provide detailed descriptions of these phenomena and relevant cross-sections.

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  • Understanding of gamma-ray interactions
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  • Knowledge of binding energy calculations
  • Basic principles of radiation detection
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  • Study "Cross-section data for photonuclear reactions" from IAEA resources
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Physicists, nuclear engineers, and researchers in radiation detection and nuclear interactions will benefit from this discussion, particularly those focusing on gamma-ray applications and photonuclear processes.

Stephan_doc
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Grettings to all,
I'm interested to know which are the main interaction between:

1.gamma-atom, also known like photoatomic reactions
2.gamma-nuclei, photonuclear reactions. e.g photofission

Thank you!
 
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Stephan_doc said:
Grettings to all,
I'm interested to know which are the main interaction between:

1.gamma-atom, also known like photoatomic reactions
2.gamma-nuclei, photonuclear reactions. e.g photofission

Thank you!
The photo-atomic reaction implies a gamma-electron reaction. The two possibilities are 1) complete absorption of the gamma photon, photoelectric absorption, in which the electron obtains an energy equivalent to the energy of the gamma less the binding energy of the electron, and 2) scattering, generally known as Compton scattering, in which the gamma photon scatters off the electron with less energy (longer wave length) and the electron absorbs that energy and moves to a higher energy level or is ejected from the atom.

With respect to the nucleus, there are two possibilities: 1) pair production, which has a threshold approximately equal to two electron rest masses (+ some recoil energy of the atom, which is very low because of the nuclear mass) and 2) photoneutron emission, which has a threshold equal to the binding energy of the 'last' neutron, which is just a way of saying the smallest binding energy level. In the case of a deuteron, an interaction with a gamma of sufficient energy (~2.226 MeV), causes photodissociation, and similarly for 9Be, a gamma of ~1.666 MeV causes photoemission of a neutron producing 8Be, which is unstable and which promptly dissociates into 2 alpha particles.
 
Thank you very much for the answer good Astronuc.
Can you tell me where i can find a short description of these phenomena e.g cross section for all nuclides.
For a good understanding i need to write equation of reaction U238+gamma.
Which is main of interaction process between gamma and U238?
 
Stephan_doc said:
Thank you very much for the answer good Astronuc.
Can you tell me where i can find a short description of these phenomena e.g cross section for all nuclides.
For a good understanding i need to write equation of reaction U238+gamma.
Which is main of interaction process between gamma and U238?
The main interaction is energy dependent, but for gammas less than 1.0222 MeV, the main interactions would be Compton scattering and photoelectric absorption.

Chapter 1 Radiation Sources, IV. Sources Of Electromagnetic Radiation, C. Photoneutron sources , p. 23
http://books.google.com/books?id=4vTJ7UDel5IC&lpg=PP1&pg=RA1-PA23#v=onepage&q&f=false

Chapter 2 Radiation Interactions, III. Interaction of Gamma Rays, pp. 47-51

From Glenn F. Knoll, Radiation Detection and Measurement, Fourth Edition, Wiley, 2010
http://www.wiley.com/WileyCDA/WileyTitle/productCd-EHEP001606.html

See also - http://www.bnl.gov/ncss/files/ppt/Gamma%20Ray%20Interactions_%20week%202%20Tuesday%20lecture.ppt

Cross-sections would be available from various laboratories or catalogs of radiation sources, or taken from MCNP code (Los Alamos National Lab), or

IAEA - http://www-nds.iaea.org/photonuclear/
 
Last edited by a moderator:
Thank a lot, these books are very useful.
What formula might be applied to compute binding energy of 'last' neutron or binding energy level for nuclei shells?
When take place reaction such as:(gamma,p), (gamma,He3), (gamma,2n), (gamma,alpha)
 
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