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High Pressure Carbon Behavior Induced from Carbide Hugoniots

Published online by Cambridge University Press:  10 February 2011

T. Sekine
Affiliation:
National Institute for Research in Inorganic Materials, 1–1 Namiki, Tsukuba 305, JAPAN, [email protected]
E. Takazawa
Affiliation:
National Institute for Research in Inorganic Materials, 1–1 Namiki, Tsukuba 305, JAPAN, [email protected]
T. Kobayashi
Affiliation:
National Institute for Research in Inorganic Materials, 1–1 Namiki, Tsukuba 305, JAPAN, [email protected]
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Abstract

Investigations of Hugoniots the diamond-type carbides(various SiC) and NaCl-type carbides such as TiC give some insights into the high-pressure carbon behaviors. The experimental results of phase transitions of a-SiC and β-SiC, together with those of diamond-structure Si, imply that the candidate as post-diamond phase has sixfold coordination and that a possible transition pressure is about 1–2 TPa. The NaCl-type carbide Hugoniots indicate that sixfold coordinated C is very stable at high pressures. The partial molar volume of carbon in the NaCl-type carbides ranges between 1.4 to 2.6 cnvVg-atom C at 1 atm and reaches about 2.8 cm3/g-atom C at 100 GPa. Taking into account structural variations of the corresponding metals, the volume of the sixfold coordinated C is estimated to be 1.7 cm3/g-atom C, about half of that of diamond, and the post-diamond phase appears to be extremely hard.

Type
Research Article
Copyright
Copyright © Materials Research Society 1998

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References

REFERENCES

1. Yin, M.T., Phys. Rev. B30, 1973 (1984);Google Scholar
Biswas, R., Martin, R.M., Needs, R.J., and Nielsen, O.H., Phys. Rev., B30, 3210 (1984):Google Scholar
Fahy, S. and Louie, S.G., Phys. Rev., B36, 3373(1987).Google Scholar
2. McMahan, A.K., Phys. Rev. B30, 5835 (1984).Google Scholar
3. Scandolo, S., Chiaretti, G.L., and Tosatti, E., Phys. Rev. B53, 5051(1996).Google Scholar
4. Yoshida, M., Onodera, A., Ueno, M., Takemura, K., and Shimomura, O., Phys. Rev. B48, 10587 (1993).Google Scholar
5. Sekine, T., Tashiro, S., Kobayashi, T., and Matsumura, T., in Shock Waves in Condensed Matter-1995, ed. by Schmidt, S.C. and Tao, W.C.(AIP, New York, 1996), pp. 12011204.Google Scholar
6. Sekine, T. and Kobayashi, T., Phys. Rev. B55, 8034 (1997).Google Scholar
7. Ootani, S. and Ishizawa, Y., Prog. Crystal. Growth Charact., 23, 153 (1991).Google Scholar
8. Sekine, T., Fat'yanov, O.V., Kobayashi, T., Ootani, S., and Suzuki, I., Proc. 21st. Intern. Symp. Shock Waves, (in press).Google Scholar
9. Grady, D.E., J. Appl. Phys., 75, 197 (1994).Google Scholar
10. Gust, W.H., Holt, A.C., and Royce, E.B., J. Appl. Phys., 44, 550 (1973).Google Scholar
11. McQueen, R.G., Marsh, S.P., Taylor, J.W., Fritz, J.N., and Carter, W.J., in High-Velocity Impact Phenomena, ed. by Kinslow, R. (Academic Press, New York, 1970), pp. 293417.Google Scholar
12. Karch, K. and Bechstedt, F., Phys. Rev. B53, 13400 (1996);Google Scholar
Chang, K.J. and Cohen, M.L., Phys. Rev., B35, 8196 (1987).Google Scholar
13. Marsh, S.P., ed. LASL Shock Hugoniot Data, (University of California Press, Berkeley, 1980), p. 658.Google Scholar
14. Xia, H., Parthasarathy, G., Luo, H., Vohra, Y.K., and Ruoff, A.L., Phys. Rev. B42, p. 6736 (1990);Google Scholar
Xia, H., Duelos, S.J., Ruoff, A.L., and Vohra, Y.K., Phys. Rev. Lett., 64, 204 (1990);Google Scholar
Jayaraman, A., Klement, W. Jr, and Kennedy, G.C., Phys. Rev. 131[2], 644 (1963).Google Scholar
15. Shannon, R.D., Acta Crystal., A32, 751 (1976);Google Scholar
Shannon, R.D. and Prewitt, C.P., Acta Crystal., B25, 925(1969).Google Scholar
16. Toth, L.E., in Transition Metal Carbides and Nitrides, (Academic Press, New York, 1971), pp. 128.Google Scholar