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Title: Relativistic modeling capabilities in PERSEUS extended MHD simulation code for HED plasmas

Abstract

We discuss the incorporation of relativistic modeling capabilities into the PERSEUS extended MHD simulation code for high-energy-density (HED) plasmas, and present the latest hybrid X-pinch simulation results. The use of fully relativistic equations enables the model to remain self-consistent in simulations of such relativistic phenomena as X-pinches and laser-plasma interactions. By suitable formulation of the relativistic generalized Ohm’s law as an evolution equation, we have reduced the recovery of primitive variables, a major technical challenge in relativistic codes, to a straightforward algebraic computation. Our code recovers expected results in the non-relativistic limit, and reveals new physics in the modeling of electron beam acceleration following an X-pinch. Through the use of a relaxation scheme, relativistic PERSEUS is able to handle nine orders of magnitude in density variation, making it the first fluid code, to our knowledge, that can simulate relativistic HED plasmas.

Authors:
 [1];  [2]
  1. 438 Rhodes Hall, Cornell University, Ithaca, NY, 14853 (United States)
  2. Cornell University, Ithaca, NY, 14853 (United States)
Publication Date:
OSTI Identifier:
22390832
Resource Type:
Journal Article
Journal Name:
AIP Conference Proceedings
Additional Journal Information:
Journal Volume: 1639; Journal Issue: 1; Conference: 9. International Conference on Dense Z Pinches, Napa, CA (United States), 3-7 Aug 2014; Other Information: (c) 2014 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0094-243X
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; ACCELERATION; COMPUTERIZED SIMULATION; ELECTRON BEAMS; ENERGY DENSITY; LASERS; LINEAR PINCH DEVICES; MAGNETOHYDRODYNAMICS; P CODES; PLASMA; PLASMA DENSITY; PLASMA SIMULATION; RELATIVISTIC RANGE; RELAXATION

Citation Formats

Hamlin, Nathaniel D., E-mail: nh322@cornell.edu, and Seyler, Charles E., E-mail: ces7@cornell.edu. Relativistic modeling capabilities in PERSEUS extended MHD simulation code for HED plasmas. United States: N. p., 2014. Web. doi:10.1063/1.4904782.
Hamlin, Nathaniel D., E-mail: nh322@cornell.edu, & Seyler, Charles E., E-mail: ces7@cornell.edu. Relativistic modeling capabilities in PERSEUS extended MHD simulation code for HED plasmas. United States. https://doi.org/10.1063/1.4904782
Hamlin, Nathaniel D., E-mail: nh322@cornell.edu, and Seyler, Charles E., E-mail: ces7@cornell.edu. Mon . "Relativistic modeling capabilities in PERSEUS extended MHD simulation code for HED plasmas". United States. https://doi.org/10.1063/1.4904782.
@article{osti_22390832,
title = {Relativistic modeling capabilities in PERSEUS extended MHD simulation code for HED plasmas},
author = {Hamlin, Nathaniel D., E-mail: nh322@cornell.edu and Seyler, Charles E., E-mail: ces7@cornell.edu},
abstractNote = {We discuss the incorporation of relativistic modeling capabilities into the PERSEUS extended MHD simulation code for high-energy-density (HED) plasmas, and present the latest hybrid X-pinch simulation results. The use of fully relativistic equations enables the model to remain self-consistent in simulations of such relativistic phenomena as X-pinches and laser-plasma interactions. By suitable formulation of the relativistic generalized Ohm’s law as an evolution equation, we have reduced the recovery of primitive variables, a major technical challenge in relativistic codes, to a straightforward algebraic computation. Our code recovers expected results in the non-relativistic limit, and reveals new physics in the modeling of electron beam acceleration following an X-pinch. Through the use of a relaxation scheme, relativistic PERSEUS is able to handle nine orders of magnitude in density variation, making it the first fluid code, to our knowledge, that can simulate relativistic HED plasmas.},
doi = {10.1063/1.4904782},
url = {https://www.osti.gov/biblio/22390832}, journal = {AIP Conference Proceedings},
issn = {0094-243X},
number = 1,
volume = 1639,
place = {United States},
year = {2014},
month = {12}
}