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Prospects for Axion Detection

Published online by Cambridge University Press:  04 August 2017

John Moody
John Moody*
Affiliation:
Institute for Theoretical Physics, UCSB

Extract

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Axions are a natural consequence of the only known solution of the ‘Strong CP Problem.’ The axion represents a minimal U(1) extension to the standard SU(3) × SU(2) × U(1) model of the strong and electroweak interactions and furthermore appears very frequently in the contexts of SUSY GUTs, Kaluza-Klein, Superstring, Technicolor, and other unified models. As such, the axion is perhaps the best motivated conjectured particle.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 117: Dark Matter in the Universe , 1987 , pp. 494 - 495
Copyright
Copyright © Reidel 1987 

References

1. Weinberg, S., Phys. Rev. Lett. 40, 223 (1977); Wilczek, F., Phys. Rev. Lett. 40, 279 (1977).CrossRefGoogle Scholar
2. Peccei, R.D. and Quinn, H., Phys. Rev. Lett. 38, 1440 (1977).Google Scholar
3. Donnelly, T., et al., Phys. Rev. D18, 1607 (1978).Google Scholar
4. Fukugita, M., Watamura, S., Yoshimura, M., Phys. Rev. Lett. 48, 1522 (1982), and Phys. Rev. D26, 1840 (1982); Krauss, L., Moody, J., Wilczek, F., Phys. Lett. 144B, 391 (1984); Iwamoto, N., Phys. Rev. Lett. 53, 1198 (1984); Morris, D. (LBL report 18690, 1984).Google Scholar
5. Kim, J.E., Phys. Rev. Lett. 43, 103 (1979); Dine, M., Fischler, W., and Srednicki, M., Phys. Lett. 104B, 199 (1981); Shifman, M., Vainshtein, A., and Zakharov, V., Nucl. Phys. B166, 493 (1980).Google Scholar
6. Preskill, J., Wise, M.B., and Wilczek, F., Phys. Lett. 120B, 127 (1983); Abbott, L.F. and Sikivie, P., Phys. Lett. 120B, 133 (1983); Dine, M. and Fischler, W., Phys. Lett. 120B, 137 (1983).Google Scholar
7. Sikivie, P., Phys. Rev. Lett. 51, 1415 (1983), and 52, 695, (1984).Google Scholar
8. Krauss, L., Moody, J., Wilczek, F., and Morris, D., ITP preprint NSF-ITP-85-76.Google Scholar
9. Sikivie, P., University of Florida preprint (1985).Google Scholar
10. Melissinos, A., et al., private communication (1985); Sikivie, P., Sullivan, N., Tanner, D., Experimental proposal (1984); Lubin, P., Morris, D. and Pennypacker, C., Experimental Proposal (1985).Google Scholar
11. Morris, D., LBL Report LBL-17915 (1984).Google Scholar
12. Krauss, L., Moody, J., Wilczek, F., and Morris, D., ITP preprint NSF-ITP-85-08.Google Scholar
13. Slonczewski, J., IBM preprint (1985); private communications of Bennett, C., Coleman, S. and Fortson, N. Google Scholar
14. Private communications of Bennett, C., Chapline, G., Fortson, N., Moody, J., Morris, D., Slonczewski, J., Snyderman, N., and Wilczek, F. Google Scholar
15. Moody, J. and Wilczek, F., Phys. Rev. D30, 130 (1984).Google Scholar