COSEv: A collective oscillation simulation engine for neutrinos

被引:15
作者
George, Manu [1 ]
Lin, Chun-Yu [2 ]
Wu, Meng-Ru [1 ,3 ]
Liu, Tony G. [1 ]
Xiong, Zewei [4 ]
机构
[1] Acad Sinica, Inst Phys, Taipei 11529, Taiwan
[2] Natl Ctr High Performance Comp, Natl Appl Res Labs, Hsinchu Sci Pk, Hsinchu City 30076, Taiwan
[3] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan
[4] GSI Helmholtzzentrum Schwerionenforsch, Planckstr 1, D-64291 Darmstadt, Germany
基金
欧洲研究理事会;
关键词
Neutrino; Flavor conversion; Etc; HIGH-ORDER; SCHEMES;
D O I
10.1016/j.cpc.2022.108588
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
We introduce the implementation details of the simulation code COSEv, which numerically solves a set of non-linear partial differential equations that govern the dynamics of neutrino collective flavor conversions. We systematically provide the details of both finite difference method supported by Kreiss-Oliger dissipation and finite volume method with seventh order weighted essentially non-oscillatory scheme. To ensure the reliability of the code, we perform comparison of the simulation results with theoretically obtainable solutions. In order to understand and characterize the error accumulation behavior of the implementations when neutrino self-interactions are switched on, we also analyze the evolution of the deviation of the conserved quantities for different values of simulation parameters. We report the performance of our code with both CPUs and GPUs. The public version of the COSEv package is available at https://github .com /COSEnu /COSEnu. Program summaryProgram Title: COSEvCPC Library link to program files: https://doi .org /10 .17632 /d4dhg2sths .1Developer's repository link: https://github .com /COSEnu /COSEnu Code Ocean capsule: https://codeocean .com /capsule /7929908 Licensing provisions: BSD 3-clauseProgramming language: C++, Python 3.0+Supplementary material: https://cosenu .github .io /cosenu _docs/ Nature of problem: Collective neutrino flavor oscillations is a novel but generic phenomenon that occurs in cosmological and astrophysical environments dense in neutrinos. Understanding this phenomenon requires solving the corresponding quantum kinetic transport equation, which is a set of nonlinear and hyperbolic partial differential equations.Solution method: We adopt the method of lines to solve the hyperbolic partial differential equations in our program. The spatial derivatives are evaluated using either the finite difference method supported by 3rd order Kreiss-Oliger dissipation or the finite volume method with 7th order WENO scheme. The time integration is performed using the explicit 4th order Runge-Kutta method. Parallelization with OpenMP or OpenACC is supported.(c) 2022 Elsevier B.V. All rights reserved.
引用
收藏
页数:13
相关论文
共 57 条
[1]  
Abbar S., 2021, ARXIV
[2]   Fast neutrino flavor conversion modes in multidimensional core-collapse supernova models: The role of the asymmetric neutrino distributions [J].
Abbar, Sajad ;
Duan, Huaiyu ;
Sumiyoshi, Kohsuke ;
Takiwaki, Tomoya ;
Volpe, Maria Cristina .
PHYSICAL REVIEW D, 2020, 101 (04)
[3]   Fast neutrino flavor conversion: Roles of dense matter and spectrum crossing [J].
Abbar, Sajad ;
Duan, Huaiyu .
PHYSICAL REVIEW D, 2018, 98 (04)
[4]  
[Anonymous], 2013, Time-Dependent Problems and Difference Methods
[5]   Fast collective neutrino oscillations inside the neutrino sphere in core-collapse supernovae [J].
Azari, Milad Delfan ;
Yamada, Shoichi ;
Morinaga, Taiki ;
Nagakura, Hiroki ;
Furusawa, Shun ;
Harada, Akira ;
Okawa, Hirotada ;
Iwakami, Wakana ;
Sumiyoshi, Kohsuke .
PHYSICAL REVIEW D, 2020, 101 (02)
[6]   Monotonicity preserving weighted essentially non-oscillatory schemes with increasingly high order of accuracy [J].
Balsara, DS ;
Shu, CW .
JOURNAL OF COMPUTATIONAL PHYSICS, 2000, 160 (02) :405-452
[7]   Linearized flavor-stability analysis of dense neutrino streams [J].
Banerjee, Arka ;
Dighe, Amol ;
Raffelt, Georg .
PHYSICAL REVIEW D, 2011, 84 (05)
[8]   Fast Flavor Depolarization of Supernova Neutrinos [J].
Bhattacharyya, Soumya ;
Dasgupta, Basudeb .
PHYSICAL REVIEW LETTERS, 2021, 126 (06)
[9]   Late-time behavior of fast neutrino oscillations [J].
Bhattacharyya, Soumya ;
Dasgupta, Basudeb .
PHYSICAL REVIEW D, 2020, 102 (06)
[10]   Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments [J].
Capozzi, Francesco ;
Saviano, Ninetta .
UNIVERSE, 2022, 8 (02)