Radiation calculations using LAHET/MCNP/CINDER90 [electronic resource].

Published: Washington, D.C. : United States. Dept. of Energy, 1993.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Physical Description: 10 pages : digital, PDF file
Additional Creators: Los Alamos National Laboratory, United States. Department of Energy, and United States. Department of Energy. Office of Scientific and Technical Information

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Summary

The LAHET Monte Carlo code system has recently been expanded to include high energy hadronic interactions via the FLUKA code, while retaining the original Los Alamos versions of HETC and ISABEL at lower energies. Electrons and photons are transported with EGS4 or ITS, while the MCNP coupled neutron/photon Monte Carlo code provides analysis of neutrons with kinetic energies less than 20 MeV. An interface with the CINDER activation code is now in common use. Various other changes have been made to facilitate analysis of high energy accelerator radiation environments and experimental physics apparatus, such as those found at SSC and RHIC. Current code developments and applications are reviewed.

Report Numbers

E 1.99:la-ur--93-2683
E 1.99: conf-930168--8
conf-930168--8
la-ur--93-2683

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Note

Published through SciTech Connect.
08/01/1993.
"la-ur--93-2683"
" conf-930168--8"
"DE93018298"
Simulating accelerator radiation environments workshop,Santa Fe, NM (United States),11-15 Jan 1993.
Waters, L.S.

Funding Information

W-7405-ENG-36

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