Difference between revisions of "MCNPX"
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− | == | + | [[Category:Software]] |
+ | {|<!--CONFIGURATION: REQUIRED--> | ||
+ | |{{#vardefine:app|MCNPX}} | ||
+ | |{{#vardefine:url|http://mcnpx.lanl.gov/}} | ||
+ | <!--CONFIGURATION: OPTIONAL (|1}} means it's ON)--> | ||
+ | |{{#vardefine:conf|}} <!--CONFIGURATION--> | ||
+ | |{{#vardefine:exe|}} <!--ADDITIONAL INFO--> | ||
+ | |{{#vardefine:pbs|1}} <!--PBS SCRIPTS--> | ||
+ | |{{#vardefine:policy|}} <!--POLICY--> | ||
+ | |{{#vardefine:testing|}} <!--PROFILING--> | ||
+ | |{{#vardefine:faq|}} <!--FAQ--> | ||
+ | |{{#vardefine:citation|1}} <!--CITATION--> | ||
+ | |{{#vardefine:installation|}} <!--INSTALLATION--> | ||
+ | |} | ||
+ | <!--BODY--> | ||
+ | <!--Description--> | ||
+ | {{#if: {{#var: url}}| | ||
+ | {{App_Description|app={{#var:app}}|url={{#var:url}}|name={{#var:app}}}}|}} | ||
− | + | MCNPX , Monte Carlo N-Particle eXtended, is a general-purpose Monte Carlo radiation transport code for modeling the interaction of radiation with everything. It extends the capabilities of MCNP4C3 to nearly all particles, nearly all energies, and to nearly all applications without an additional computational time penalty. | |
Please note, MCNPX is installed on HPC Center's RedHat EL6 systems. Please read the section of "Execution Instructions..." below for information on how to access the software. | Please note, MCNPX is installed on HPC Center's RedHat EL6 systems. Please read the section of "Execution Instructions..." below for information on how to access the software. | ||
− | == | + | <!--Modules--> |
+ | ==Required Modules== | ||
+ | ===Serial=== | ||
+ | * intel | ||
+ | * mcnpx | ||
− | + | ==System Variables== | |
− | < | + | * AMBERHOME |
− | + | <!--Configuration--> | |
− | </ | + | {{#if: {{#var: conf}}|==Configuration== |
+ | See the [[{{PAGENAME}}_Configuration]] page for {{#var: app}} configuration details. | ||
+ | |}} | ||
+ | <!--Run--> | ||
+ | {{#if: {{#var: exe}}|==Additional Information== | ||
+ | WRITE_ADDITIONAL_INSTRUCTIONS_ON_RUNNING_THE_SOFTWARE_IF_NECESSARY | ||
+ | |}} | ||
+ | <!--PBS scripts--> | ||
+ | {{#if: {{#var: pbs}}|==PBS Script Examples== | ||
+ | See the [[{{PAGENAME}}_PBS]] page for {{#var: app}} PBS script examples. | ||
+ | |}} | ||
+ | <!--Policy--> | ||
+ | {{#if: {{#var: policy}}|==Usage Policy== | ||
+ | WRITE USAGE POLICY HERE (Licensing, usage, access). | ||
+ | |}} | ||
+ | <!--Performance--> | ||
+ | {{#if: {{#var: testing}}|==Performance== | ||
+ | WRITE_PERFORMANCE_TESTING_RESULTS_HERE | ||
+ | |}} | ||
+ | <!--Faq--> | ||
+ | {{#if: {{#var: faq}}|==FAQ== | ||
+ | *'''Q:''' **'''A:'''|}} | ||
+ | <!--Citation--> | ||
+ | {{#if: {{#var: citation}}|==Citation== | ||
+ | ===Serial Version=== | ||
+ | If you publish research that uses {{#var:app}} you have to cite it as follows: <br/> | ||
+ | D.A. Case, T.A. Darden, T.E. Cheatham, III, C.L. Simmerling, J. Wang, R.E. Duke, R. Luo, R.C. Walker, W. Zhang, K.M. Merz, B. Roberts, S. Hayik, A. Roitberg, G. Seabra, J. Swails, A.W. Goetz, I. Kolossvai, K.F. Wong, F. Paesani, J. Vanicek, R.M. Wolf, J. Liu, X. Wu, S.R. Brozell, T. Steinbrecher, H. Gohlke, Q. Cai, X. Ye, J. Wang, M.-J. Hsieh, G. Cui, D.R. Roe, D.H. Mathews, M.G. Seetin, R. Salomon-Ferrer, C. Sagui, V. Babin, T. Luchko, S. Gusarov, A. Kovalenko, and P.A. Kollman (2012), AMBER 12, University of California, San Francisco. | ||
− | + | ===GPU Version=== | |
+ | If you make use of any of this GPU support in your work please use the following citations: <br/> | ||
− | + | Andreas W. Goetz; Mark J. Williamson; Dong Xu; Duncan Poole; Scott Le Grand; & Ross C. Walker* "Routine microsecond molecular dynamics simulations with AMBER - Part I: Generalized Born", J. Chem. Theory Comput., 2012, 8 (5), pp 1542-1555 , DOI: 10.1021/ct200909j | |
− | + | ||
− | + | D.A. Case, T.A. Darden, T.E. Cheatham, III, C.L. Simmerling, J. Wang, R.E. Duke, R. Luo, R.C. Walker, W. Zhang, K.M. Merz, B. Roberts, S. Hayik, A. Roitberg, G. Seabra, J. Swails, A.W. Goetz, I. Kolossvai, K.F. Wong, F. Paesani, J. Vanicek, R.M. Wolf, J. Liu, X. Wu, S.R. Brozell, T. Steinbrecher, H. Gohlke, Q. Cai, X. Ye, J. Wang, M.-J. Hsieh, G. Cui, D.R. Roe, D.H. Mathews, M.G. Seetin, R. Salomon-Ferrer, C. Sagui, V. Babin, T. Luchko, S. Gusarov, A. Kovalenko, and P.A. Kollman (2012), AMBER 12, University of California, San Francisco. | |
− | + | |}} | |
− | + | <!--Installation--> | |
− | + | {{#if: {{#var: installation}}|==Installation== | |
− | + | See the [[{{PAGENAME}}_Install]] page for {{#var: app}} installation notes.|}} | |
− | + | <!--Turn the Table of Contents and Edit paragraph links ON/OFF--> | |
− | + | __NOTOC____NOEDITSECTION__ | |
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Revision as of 15:27, 15 January 2013
Description
MCNPX , Monte Carlo N-Particle eXtended, is a general-purpose Monte Carlo radiation transport code for modeling the interaction of radiation with everything. It extends the capabilities of MCNP4C3 to nearly all particles, nearly all energies, and to nearly all applications without an additional computational time penalty.
Please note, MCNPX is installed on HPC Center's RedHat EL6 systems. Please read the section of "Execution Instructions..." below for information on how to access the software.
Required Modules
Serial
- intel
- mcnpx
System Variables
- AMBERHOME
PBS Script Examples
See the MCNPX_PBS page for MCNPX PBS script examples.
Citation
Serial Version
If you publish research that uses MCNPX you have to cite it as follows:
D.A. Case, T.A. Darden, T.E. Cheatham, III, C.L. Simmerling, J. Wang, R.E. Duke, R. Luo, R.C. Walker, W. Zhang, K.M. Merz, B. Roberts, S. Hayik, A. Roitberg, G. Seabra, J. Swails, A.W. Goetz, I. Kolossvai, K.F. Wong, F. Paesani, J. Vanicek, R.M. Wolf, J. Liu, X. Wu, S.R. Brozell, T. Steinbrecher, H. Gohlke, Q. Cai, X. Ye, J. Wang, M.-J. Hsieh, G. Cui, D.R. Roe, D.H. Mathews, M.G. Seetin, R. Salomon-Ferrer, C. Sagui, V. Babin, T. Luchko, S. Gusarov, A. Kovalenko, and P.A. Kollman (2012), AMBER 12, University of California, San Francisco.
GPU Version
If you make use of any of this GPU support in your work please use the following citations:
Andreas W. Goetz; Mark J. Williamson; Dong Xu; Duncan Poole; Scott Le Grand; & Ross C. Walker* "Routine microsecond molecular dynamics simulations with AMBER - Part I: Generalized Born", J. Chem. Theory Comput., 2012, 8 (5), pp 1542-1555 , DOI: 10.1021/ct200909j
D.A. Case, T.A. Darden, T.E. Cheatham, III, C.L. Simmerling, J. Wang, R.E. Duke, R. Luo, R.C. Walker, W. Zhang, K.M. Merz, B. Roberts, S. Hayik, A. Roitberg, G. Seabra, J. Swails, A.W. Goetz, I. Kolossvai, K.F. Wong, F. Paesani, J. Vanicek, R.M. Wolf, J. Liu, X. Wu, S.R. Brozell, T. Steinbrecher, H. Gohlke, Q. Cai, X. Ye, J. Wang, M.-J. Hsieh, G. Cui, D.R. Roe, D.H. Mathews, M.G. Seetin, R. Salomon-Ferrer, C. Sagui, V. Babin, T. Luchko, S. Gusarov, A. Kovalenko, and P.A. Kollman (2012), AMBER 12, University of California, San Francisco.