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Phys. Rev. B 74, 012101 (2006) [4 pages]

Simulation of shock-induced melting of Ni using molecular dynamics coupled to a two-temperature model

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L. Koči1, E. M. Bringa2, D. S. Ivanov3, J. Hawreliak2, J. McNaney2, A. Higginbotham4, L. V. Zhigilei5, A. B. Belonoshko6,7, B. A. Remington2, and R. Ahuja1,6
1Condensed Matter Theory, Physics Department, University of Uppsala, Box 530, SE-751 21 Uppsala, Sweden
2Lawrence Livermore National Laboratory, Livermore, California 94550, USA
3National Centre for Laser Applications, Galway, Ireland
4Department of Physics, Clarendon Laboratory, University of Oxford, Oxford OX1 3PU, United Kingdom
5Department of Materials Science and Engineering, University of Virginia, Charlottesville, Virginia 22903, USA
6Applied Material Physics, Department of Materials Science and Engineering, Royal Institute of Technology, 100 44 Stockholm, Sweden
7Condensed Matter Theory, Alba Nova University Center, Physics Department, Royal Institute of Technology, 100 44 Stockholm, Sweden

Received 29 December 2005; revised 27 April 2006; published 6 July 2006

Using nonequilibrium molecular dynamics (MD) simulations we study shock-induced melting in Ni with an embedded atom method (EAM). Dynamic melting is probed by the pair correlation function, and we find a melting lattice temperature of Tmelt=6400±300 K for a melting pressure of Pmelt=275±10 GPa. When a combined MD+TTM (two-temperature model) approach is used to include electronic heat conduction and electron-phonon coupling, Pmelt and Tmelt change. For a given pressure, the temperature behind the shock decreases due to electronic heat diffusion into the cold, unshocked material. This cooling of the material behind the shock slightly increases the melting pressure compared to simulations without electronic heat conduction and electron-phonon coupling. The decrease in the temperature behind the shock front is enhanced if the electron-phonon coupling is artificially made larger. We also explore the feasibility of using x-ray diffraction to detect melting.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.74.012101
DOI:
10.1103/PhysRevB.74.012101
PACS:
62.50.+p