2012

Comment on "Could the Excess Seen at 124-126 GeV Be due to the Randall-Sundrum Radion?"

Tang, Yong

Understand

In recent Letter by Cheung et al.[PRL {\bf 108},141602(2012)], one very interesting suggestion for the excess around 125 GeV seen at the LHC is a RS radion with $\Lambda_\phi=680$GeV.

In this note, we show that taking constraints on the RS graviton into account, it is unlikely to have a 125 GeV RS radion with $\Lambda_\phi=680$GeV and accommodate with both experimental and theoretically constraints.

Built on

L. Randall and R. Sundrum, Phys. Rev. Lett. 83
1999
Earlier work this paper cites.
W. D. Goldberger and M. B. Wise, Phys. Rev. Lett. 83
1999
Earlier work this paper cites.
H. Davoudiasl, J. L. Hewett and T. G. Rizzo, Phys. Rev. D 63
2001
Earlier work this paper cites.

Similar

K. Agashe, H. Davoudiasl, G. Perez and A. Soni, Phys. Rev. D 76
Original
2007
Cited alongside, same era.
S. Chatrchyan et al
Original
2011
Cited alongside, same era.
G. Aad et al
Original
2012
Cited alongside, same era.
S. Chatrchyan et al
Original
Cited in the paper.

Then

K. Cheung and T. -C. Yuan, Phys. Rev. Lett. 108, 141602
Original
2012
Closest in time.
The ATLAS Collaboration, ATLAS-CONF-2012-007
2012
Closest in time.

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