The gravity extension for MCNP 6.2

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Abstract

Standard MCNP particle tracking takes place along straight-line trajectories from interaction point to interaction point. There is a feature within MCNP that is planned for deprecation that provides surface boundary conditions for approximating gravity for planetary cases, but this feature is not applicable to a cold neutron beam. A new extension has been developed to track particles along parabolic trajectories with a constant acceleration. MCNP contains 1st and 2nd-order surfaces as well as a special case of 4th-order surfaces for simple tori, and the intersection of parabolic trajectories with these surfaces becomes 2nd, 4th, and 8th-order equations in time, respectively. Solving these equations utilizes a fast algorithm for finding the roots of polynomials. The theory, MCNP input card, and examples of using this new feature will be discussed.

Funding

This material is based upon work supported by the U.S. Department of Energy , Office of Science , Office of Basic Energy Sciences under contract number DE-AC05-00OR22725 .

Keywords

  • MCNP
  • Particle tracking
  • Radiation shielding

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