Numerical Modeling of Hydrodynamic Turbulence with Self-gravity on Intel Xeon Phi KNL-Reference-Cited by-同舟云学术

Numerical Modeling of Hydrodynamic Turbulence with Self-gravity on Intel Xeon Phi KNL

Published:2019 Issue: Volume: Page:309-322
ISSN:1865-0929
Container-title:Communications in Computer and Information Science
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Author:

Kulikov Igor^ORCID,Chernykh Igor,Berendeev Evgeny,Protasov Victor,Serenko Alexander,Prigarin Vladimir,Ulyanichev Ivan,Karavaev Dmitry,Vorobyov Eduard,Tutukov Alexander

Publisher

Springer International Publishing

Link

http://link.springer.com/content/pdf/10.1007/978-3-030-28163-2_22

Reference34 articles.

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2. Heitsch, F., Mac Low, M.-M., Klessen, R.: Gravitational Collapse in turbulent molecular clouds II. Magnetohydrodynamical turbulence. Astrophys. J. 547, 280–291 (2001). https://doi.org/10.1086/318335

3. Beresnyak, A., Xu, H., Li, H., Schlickeiser, R.: Magnetohydrodynamic turbulence and cosmic-ray reacceleration in galaxy clusters. Astrophys. J. Suppl. Ser. 771, 131 (2013). https://doi.org/10.1088/0004-637X/771/2/131

4. Kim, W., Ostriker, E.: Amplification, saturation, and Q Thresholds for runaway: growth of self-gravitating structures in models of magnetized galactic gas disks. Astrophys. J. 559, 70–95 (2001). https://doi.org/10.1086/322330

5. Alig, C., Burkert, A., Johansson, P., Schartmann, M.: Simulations of direct collisions of gas clouds with the central black hole. Mon. Not. Roy. Astron. Soc. 412(1), 469–486 (2011). https://doi.org/10.1111/j.1365-2966.2010.17915.x

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