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Among solutions of the strong CP problem, the "invisible" axion in the narrow axion window is argued to be the remaining possibility among natural solutions on the smallness of $\bar{\theta}$.
J.E. Kim, Phys. Rev. Lett
1980
Earlier work this paper cites.
P. Sikivie, Phys. Rev. Lett
1982
Earlier work this paper cites.
G. Lazarides and Q. Shafi, Phys. Lett. B
1982
Earlier work this paper cites.
E. Witten, Phys. Lett. B
1984
Earlier work this paper cites.
M. B. Green and J. Schwarz, Phys. Lett. B
1984
Earlier work this paper cites.
J. E. Kim, Phys. Lett. B
1984
Cited alongside, same era.
K. Choi and J.E. Kim, Phys. Rev. Lett
1985
Cited alongside, same era.
E. Witten, Phys. Lett. B
1985
Cited alongside, same era.
K. Choi and J. E. Kim, Phys. Lett. B
1985
Cited alongside, same era.
J. J. Atick, L. Dixon, and A. Sen, Nucl. Phys. B
1987
Cited alongside, same era.
G. ’t Hooft, Nucl. Phys. B
Cited in the paper.
J. E. Kim, B. Kyae, and S. Nam, arXiv:1703.05345 [hep-ph]
Cited in the paper.
J. J. Atick and A. Sen, Nucl. Phys. B
1988
Later among the works it cites.
J. E. Kim, Y. K. Semertzidis, and S. Tsujikawa, Front. Phys
2014
Later among the works it cites.
J.E. Kim, Phys. Lett. B
2016
Later among the works it cites.
For a recent review, see, J. E. Kim, “Fate of global symmetries in cosmology: QCD axion, quintessential axion and trans-Planckian inflaton decay-constant”, 2017
2017
Closest in time.
J. E. Kim, Phys. Rev. D
2017
Closest in time.
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