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frontiers of physics 2016(6)
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Ultra-strong shock waves are of fundamental interest to astrophysics,inertial confinement fusion and compressible turbulences. A number of physicalor chemical transitions, such as phase transitions, reactions, dissociation andionization, are intrigued in a small region at the vicinity of the shock front,which has a thickness of several mean free paths. Non-equilibrium moleculardynamics simulations of ultra-strong shock waves in dense helium are carriedout as an example to illustrate the dynamics and microscopic structures of theshock front. For more details, please refer to the article “Molecular dynamicssimulations of microscopic structure of ultra strong shock waves in densehelium” by Hao Liu, et al., Front. Phys. 11(6), 115206 (2016). [Photo credits:Hao Liu and Wei Kang, Center for Applied Physics and Technology, PekingUniversity] hock waves are of fundamental interest to astrophysics,inertial confinement fusion and compressible turbulences. A number of physicalor chemical transitions, such as phase transitions, reactions, dissociation andionization, are intrigued in a small region at the vicinity of the shock front,which has a thickness of several mean free paths. Non-
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Molecular dynamics simulations of microscopic structure of ultra strong shock waves in dense helium Hao Liu, Wei Kang, Qi Zhang, Yin Zhang, Huilin Duan, X. T. He Front. Phys. 2016, 11 (6): 115206 . DOI: 10.1007/s11467-016-0590-5 |
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