Comparison of Acceleration Methods in a Radiation Transport Code With Adaptive Mesh Refinement

被引:7
|
作者
Garcia-Fernandez, Carlos [1 ]
Velarde, Pedro [1 ]
Cotelo, Manuel [1 ]
机构
[1] Univ Politecn Madrid, Inst Fus Nucl, E-28006 Madrid, Spain
关键词
Adaptive mesh refinement (AMR); diffusion synthetic acceleration (DSA); radiation transport; synthetic acceleration; transport synthetic acceleration (TSA); DIFFUSION SYNTHETIC ACCELERATION; ITERATIVE METHODS; HYDRODYNAMICS;
D O I
10.1109/TPS.2010.2052109
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
New considerations about the acceleration of an iterative process to couple the radiation transport equation and the equation of matter temperature are presented in this paper. Two synthetic acceleration methods [diffusion synthetic acceleration (DSA) and transport synthetic acceleration (TSA)] have been studied and analyzed, showing its strengths and weaknesses. This study is applied to an adaptive mesh refinement (AMR) context, concluding in a better performance of DSA for coarse level resolutions with higher S(n), while TSA is better for finer level boxes and smaller S(n) cases. These conclusions are applied to accelerate the resolution of an AMR problem.
引用
收藏
页码:2359 / 2366
页数:8
相关论文
共 50 条
  • [1] The Black Hole Accretion Code: adaptive mesh refinement and constrained transport
    Sanchez, H. R. Olivares
    Porth, O.
    Mizuno, Y.
    12TH INTERNATIONAL CONFERENCE ON NUMERICAL MODELING OF SPACE PLASMA FLOWS: ASTRONUM-2017, 2018, 1031
  • [2] Constrained transport and adaptive mesh refinement in the Black Hole Accretion Code
    Olivares, Hector
    Porth, Oliver
    Davelaar, Jordy
    Most, Elias R.
    Fromm, Christian M.
    Mizuno, Yosuke
    Younsi, Ziri
    Rezzolla, Luciano
    ASTRONOMY & ASTROPHYSICS, 2019, 629
  • [3] Tree-based solvers for adaptive mesh refinement code flash - II: radiation transport module TreeRay
    Wuensch, Richard
    Walch, Stefanie
    Dinnbier, Frantisek
    Seifried, Daniel
    Haid, Sebastian
    Klepitko, Andre
    Whitworth, Anthony P.
    Palous, Jan
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 505 (03) : 3730 - 3754
  • [4] ENZO: AN ADAPTIVE MESH REFINEMENT CODE FOR ASTROPHYSICS
    Bryan, Greg L.
    Norman, Michael L.
    O'Shea, Brian W.
    Abel, Tom
    Wise, John H.
    Turk, Matthew J.
    Reynolds, Daniel R.
    Collins, David C.
    Wang, Peng
    Skillman, Samuel W.
    Smith, Britton
    Harkness, Robert P.
    Bordner, James
    Kim, Ji-hoon
    Kuhlen, Michael
    Xu, Hao
    Goldbaum, Nathan
    Hummels, Cameron
    Kritsuk, Alexei G.
    Tasker, Elizabeth
    Skory, Stephen
    Simpson, Christine M.
    Hahn, Oliver
    Oishi, Jeffrey S.
    So, Geoffrey C.
    Zhao, Fen
    Cen, Renyue
    Li, Yuan
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2014, 211 (02):
  • [5] Comparison of refinement criteria for structured adaptive mesh refinement
    Li, Shengtai
    JOURNAL OF COMPUTATIONAL AND APPLIED MATHEMATICS, 2010, 233 (12) : 3139 - 3147
  • [6] AMRA:: An Adaptive Mesh Refinement hydrodynamic code for astrophysics
    Plewa, T
    Müller, E
    COMPUTER PHYSICS COMMUNICATIONS, 2001, 138 (02) : 101 - 127
  • [7] RAM: A relativistic adaptive mesh refinement hydrodynamics code
    Zhang, WQ
    MacFadyen, AI
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2006, 164 (01): : 255 - 279
  • [8] N-body code with adaptive mesh refinement
    Yahagi, H
    Yoshi, Y
    ASTROPHYSICAL JOURNAL, 2001, 558 (01): : 463 - 475
  • [9] N-body code with adaptive mesh refinement
    Yahagi, H
    Yoshii, Y
    ASTROPHYSICAL SUPERCOMPUTING USING PARTICLE SIMULATIONS, 2003, (208): : 465 - 466
  • [10] Cosmological hydrodynamics code with dynamically adaptive mesh refinement
    Yahagi, H
    Yoshii, Y
    PHYSICS OF GALAXY FORMATION, PROCEEDINGS, 2001, 222 : 419 - 422