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On the Large-Scale Structures Formed by Wakes of Open Cosmic Strings

Published online by Cambridge University Press:  12 April 2016

Tetsuya Hara
Affiliation:
Department of physics, Kyoto Sangyo University, Kyoto 603
Shoji Morioka
Affiliation:
Department of physics, Kyoto Sangyo University, Kyoto 603
Shigeru Miyoshi
Affiliation:
Institute of Astronomy, Cambridge, UK

Extract

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Large-scale structures of the universe have been variously described as sheetlike, filamentary, cellular, bubbles or spongelike. Recently cosmic strings become one of viable candidates for galaxy formation scenario, and some of the large-scale structures seem to be simply explained by the open cosmic strings).

Type
VIII. Classical Theory of Multiplets
Copyright
Copyright © NASA 1990

References

1) Lapparent, V. de, Geller, M. J. and Huchra, J. P., Astrophys. J. 302(1986), L1.CrossRefGoogle Scholar
2) Haynes, M. P. and Giovanelli, R., Astrophys. J. 306 (1986), L55.CrossRefGoogle Scholar
3) Vilenkin, A., Phys. Rep. 121 (1985), 263.CrossRefGoogle Scholar
4) Silk, J. and Vilenkin, A., Phys. Rev. Lett. 53(1984), 1700.Google Scholar
5) Vachaspati, T., Phys. Rev. Lett. 57(1986), 1655.Google Scholar
6) Hara, T. and Miyoshi, S., Prog. Theor. Phys. 81(1989), 1187.Google Scholar
7) Hara, T. and Miyoshi, S., Prog. Theor. Phys. 77(1987), 1152.Google Scholar
8) Hara, T. and Miyoshi, S., Prog. Theor. Phys. 78(1987), 1081.CrossRefGoogle Scholar
9) Stebbins, A. et al. Astrophys. J. 322(1987), 1.Google Scholar
10) Rees, M. J., Mon. Not. R. Astron. Soc. 222(1986), 27p.Google Scholar
11) Albrecht, A. and Turok, N., Phys. Rev. Lett. 54(1985), 1868.Google Scholar
12) Hara, T. and Miyoshi, S., preprintGoogle Scholar
13) Hockney, R.W. and Eastwood, J.W., “Computer Simulation Using Particles” (1981; MacGraw Hill, New York).Google Scholar