Delayed-particles from photonuclear library interactions. Intel-based and PowerPC-based executables are included. For plotting geometry, cross-sections, or results, X11 must be installed on your PC. Pions, muons, and kaons are treated only by physics models. Analyzes a HISTP history file and generates double-differential particle production cross sections for primary beam interactions.
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Data library only driven transport for n,p,e by default. It was first released to the public in as version 2. Please note that included MCNPX executables run only on the machines listed below in section 9 of this abstract. C and Fortran 90 compilers are mdnp6 to compile.
The Cygwin environment may be obtained at no cost from the web site http: Photonuclear interactions from 1. Each of these files contains precompiled executables and corresponding binary data libraries for bertin and phtlib. Included executables and reference templates for output and tally files used in the MCNP5 regression test suite were generated for Linux and Windows with the mfnp6 compilers: While maintenance and bug fixes will continue for MCNP5 v.
Photonuclear physics is available for a limited number of isotopes. The only graphics support for this release is X11 http: The gcc C compiler is used for all versions.
Export control regulations restrict mcnnp6 distribution of Fortran source code.
Explicit tracking of all charged particles in magnetic fields. For details, see LA-UR The code has improved support for newer Fortran 90 compilers.
For plotting geometry, cross-sections, or results, X11 must be installed on your PC. Included executables and reference templates for output and tally files used in the MCNP5 regression test suite were generated for Linux and Windows with the following compilers:. Converts output of mesh and radiography tallies to input for external graphics programs. In addition, variance reduction schemes such as secondary particle biasingand new tallies have been created specific to the intermediate and high energy physics ranges.
In fact, this initial production release of MCNP6 v. For photons, the code accounts for incoherent and coherent scattering, the possibility of fluorescent emission after photoelectric absorption, and absorption in electron-positron pair production.
Up to 14 GB may be required during file expansion. A separate test library of cross sections is used for running regression sample problems, but the test library is not suitable for real problems. Note that some compilers are not yet suitable for compiling a threaded version of MCNP5.
Delayed-particles from photonuclear library interactions. Electrons from 1 keV - 1 GeV. Electron transport does not cmnp6 the effects of external or self-induced electromagnetic fields. Windows executables, with Intel Users should be aware that this first production release does contain several limitations.
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It is expected that users of this initial release apply MCNP6 to the problems that they know well and have some intuition about, and report back to the MCNP6 team email mcnp6 lanl.
The capability to calculate keff eigenvalues for fissile systems remains a standard feature. An X-windows server is required to display the X11 graphics.
MCNPX runs under Unix, Linux, and Windows operating systems and has been implemented on various bit and bit workstations and personal computers.
Mncp6 standard features that make MCNP very versatile and easy to use include a powerful general source, criticality source, and surface source; both geometry and output tally plotters; a rich collection of variance reduction techniques; a flexible tally structure; and an extensive collection of cross-section data.
Verification of MCNP5 - 1.