Simulation of Molecular Cloud Collision Dynamics Using Heterogeneous Systems
The results of computer simulation of the process of collision of rotating molecular clouds in the interstellar medium are presented. As matter is compressed, the gas density in the area of their collision increases; this leads to local changes in the shape and fragmentation of clouds. The gas densi...
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| Published in | Journal of applied and industrial mathematics Vol. 17; no. 1; pp. 168 - 175 |
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| Main Authors | , |
| Format | Journal Article |
| Language | English |
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Moscow
Pleiades Publishing
01.03.2023
Springer Nature B.V |
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| Abstract | The results of computer simulation of the process of collision of rotating molecular clouds in the interstellar medium are presented. As matter is compressed, the gas density in the area of their collision increases; this leads to local changes in the shape and fragmentation of clouds. The gas density in the resulting condensations increases by many orders of magnitude, and gravitationally bound domains appear where star clusters can form. The process of star formation is accompanied by considerable spatial and temporal changes in the interstellar gas in these domains, turbulence of the interstellar medium, gravity, and a sharp change in magnetic and radiation fields at the prestellar stage of the evolution of new formations. The rotation of colliding molecular clouds has a great influence on the ongoing processes. The evolution of the matter of protostellar regions from the moment when they begin to form until the moment when they reach stellar density covers a huge range of scales. Simulation of such astrophysical processes on ultra-high resolution computational grids requires a substantial increase in computer power, and optimization of parallel computing on heterogeneous computing systems is required. |
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| AbstractList | The results of computer simulation of the process of collision of rotating molecular clouds in the interstellar medium are presented. As matter is compressed, the gas density in the area of their collision increases; this leads to local changes in the shape and fragmentation of clouds. The gas density in the resulting condensations increases by many orders of magnitude, and gravitationally bound domains appear where star clusters can form. The process of star formation is accompanied by considerable spatial and temporal changes in the interstellar gas in these domains, turbulence of the interstellar medium, gravity, and a sharp change in magnetic and radiation fields at the prestellar stage of the evolution of new formations. The rotation of colliding molecular clouds has a great influence on the ongoing processes. The evolution of the matter of protostellar regions from the moment when they begin to form until the moment when they reach stellar density covers a huge range of scales. Simulation of such astrophysical processes on ultra-high resolution computational grids requires a substantial increase in computer power, and optimization of parallel computing on heterogeneous computing systems is required. |
| Author | Rybakin, B. P. Goryachev, V. D. |
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| Cites_doi | 10.1093/mnras/staa090 10.1016/j.compfluid.2018.03.009 10.1086/510771 10.1051/0004-6361/201628251 10.1038/nature09289 10.3847/1538-4365/ab007f 10.1086/174231 10.1093/mnras/stt203 10.1111/j.1365-2966.2010.16888.x 10.1134/S199508021804011X 10.2458/azu_uapress_9780816531240-ch001 10.1051/0004-6361:20053898 10.1051/0004-6361/201014949 |
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| Keywords | fragmentation of neoformations computational astrophysics collision of molecular clouds parallel programming |
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| References | E. T. Vishniac, “Nonlinear instabilities in shock-bounded slabs,” Astrophys. J. (428), 186–208 (1994). RybakinB.GoryachevV.Parallel algorithms for astrophysics problemsLobachevskii J. Math.2018394562570381195010.1134/S199508021804011X1396.85002 LiG.X.WyrowskiF.MentenK.Revealing a spiral-shaped molecular cloud in our galaxy: Cloud fragmentation under rotation and gravityAstron. & Astrophys.20175989610.1051/0004-6361/201628251 BerneO.MarcelinoN.CernicharoJ.Waves on the surface of the Orion molecular cloudNature Lett.2010466730994794910.1038/nature09289 D. Hubber, C. Batty, A. McLeod, and A. Whitworth, “SEREN—a new SPH code for star and planet formation simulations. Algorithms and test,” Astron. & Astrophys. (529), 1–27 (2011). M. A. Skinner et al., “FORNAX: A flexible code for multiphysics astrophysical simulations astrophys,” J. Suppl. Ser. (241), 7 (2019). “Star formation triggering by cloud-cloud collision,” Publ. Astron. Soc. Jpn. 70 (SP2) (2018). D. Folini and R. Walder, “Supersonic turbulence in shock-bound interaction zones I. Symmetric settings,” Astron. & Astrophys. (459), 1–19 (2006). M. Wolfe, “The OpenACC applications programming interface. Version 2.0. PGInsider,” in Technical News from PGI (2013). T. Kimura and M. Tosa, “Collision of clumpy molecular clouds,” Astron. & Astrophys. (308), 979–987 (1996). RAMSES. https://www.ics.uzh.ch/~teyssier/ramses/RAMSES.html . C. L. Dobbs, M. R. Krumholz, et al., “Formation of molecular clouds and global conditions for star formation,” in Protostars & Planets VI (2014), 3–26. E. R. Parkin and J. M. Pittard, “Numerical heat conduction in hydrodynamical models of colliding hypersonic flows,” Mon. Notices R. Astron. Soc. (406), 2373–2385 (2010). Coarray FORTRAN documentation: https://software.intel.com/content/www/us/en/develop/documentation/fortran-compiler-coarray-tutorial/top.html . D. Calderon et al., “Three-dimensional simulations of clump formation in stellar wind collision,” Mon. Notices R. Astron. Soc. (493), 447–467 (2020). BerneO.MatsumotoY.The Kelvin—Helmholtz instability in Orion: A source of turbulence and chemical mixingAstrophys. J. Lett.2012761L415 E. Vazquez-Semadeni at al., “Molecular cloud evolution. II. From cloud formation to the early stages of star formation in decaying conditions,” Astrophys. J. (657), 870–883 (2007). A. D. McLeod and A. P. Whitworth, “Simulations of the non-linear thin shell instability,” Mon. Notices R. Astron. Soc. (431), 710–721 (2013). HabeA.OhtaK.Gravitational instability induced by a cloud-cloud collision: the case of head-on collision between clouds with different sizes and densitiesPubl. Astron. Soc. Jpn.199244203226 B. Rybakin and V. Goryachev, “Modeling of density stratification and filamentous structure formation in molecular clouds after shock wave collision,” Comput. Fluids (173), 189–194 (2018). 5209_CR5 5209_CR4 5209_CR17 5209_CR7 5209_CR6 5209_CR1 5209_CR14 A. Habe (5209_CR16) 1992; 44 5209_CR13 5209_CR3 5209_CR12 5209_CR11 5209_CR10 O. Berne (5209_CR18) 2010; 466 5209_CR20 G.X. Li (5209_CR2) 2017; 598 O. Berne (5209_CR19) 2012; 761 B. Rybakin (5209_CR15) 2018; 39 5209_CR9 5209_CR8 |
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| SubjectTerms | Collision dynamics Compressed gas Computational grids Computer simulation Domains Evolution Gas density Interstellar chemistry Interstellar gas Interstellar matter Mathematics Mathematics and Statistics Molecular clouds Optimization Protostars Simulation Star & galaxy formation Star clusters Star formation |
| Title | Simulation of Molecular Cloud Collision Dynamics Using Heterogeneous Systems |
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