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Neutrino mass in radiatively-broken scale-invariant models · Around

2007

Neutrino mass in radiatively-broken scale-invariant models

Foot, Robert, Kobakhidze, Archil, McDonald, Kristian. L. et al.

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Understand

Scale invariance may be a classical symmetry which is broken radiatively.

This provides a simple way to stabilize the scale of electroweak symmetry breaking against radiative corrections.
The simplest phenomenologically successful model of this type involves the addition of one real scalar field to the standard model.
In this minimal model the electroweak Higgs can be interpreted as the pseudo-Goldstone boson of broken scale invariance.

Built on

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Similar

K. S. Babu, Phys. Lett. B 203
1988
Cited alongside, same era.
D. Chang, W. Y. Keung and P. B. Pal, Phys. Rev. Lett. 61
1988
Cited alongside, same era.
J. Preskill, S. P. Trivedi, F. Wilczek and M. B. Wise, Nucl. Phys. B 363
1991
Cited alongside, same era.
R. Hempfling, Phys. Lett. B 379
1996
Cited alongside, same era.
R. Foot, A. Kobakhidze and R. R. Volkas, Phys. Lett. B, in press, arXiv:0704.1165 [hep-ph]
Original
Cited in the paper.
R. Foot, A. Kobakhidze, K. L. McDonald and R. R. Volkas, arXiv:0709.2750 [hep-ph]
Original
Cited in the paper.
K. L. McDonald and B. H. J. McKellar, arXiv:hep-ph/0309270
Cited in the paper.

Then

K. S. Babu and C. Macesanu, Phys. Rev. D 67
2003
Later among the works it cites.
K. A. Meissner and H. Nicolai, Phys. Lett. B 648
2007
Closest in time.
J. R. Espinosa and M. Quiros, Phys. Rev. D 76
2007
Closest in time.
W. F. Chang, J. N. Ng and J. M. S. Wu, Phys. Rev. D 75
2007
Closest in time.

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