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Photodisintegration of the Deuteron by 180-Mev and 260-Mev Gamma Rays
16
Citations
3
References
1954
Year
Crystal Counter TelescopePhotometryExperimental Nuclear PhysicsNuclear PhysicsPhysicsGamma-ray EnergiesNatural SciencesNuclear DataEngineeringHigh-energy Nuclear ReactionNuclear Theory260-Mev Gamma RaysLepton-nucleon ScatteringHigh-energy Cosmic RayO Subtraction MethodNuclear Astrophysics
The photodisintegration of the deuteron is observed at gamma-ray energies of 180 Mev and 260 Mev. Both a low-temperature compressed-gas target and a ${\mathrm{D}}_{2}$O-${\mathrm{H}}_{2}$O subtraction method are used. The photoprotons are detected in a crystal counter telescope. Their angular distribution shows a fairly marked forward asymmetry. The total cross sections at 165 and 230 Mev (c.m.) are 54 and 66 \ensuremath{\mu}b, respectively, with an estimated error of 10 percent on the absolute scale.
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