The scalar field associated with fluctuations in the positions of the two branes, the ``radion'', plays an important role determining the cosmology and collider phenomenology of the Randall-Sundrum solution to the hierarchy problem. It is now well known th

V µ

V ν

h m i 2M 2V

v (B +D )ηµν

Figure 4:Feynman rules for three-point gauge boson couplings including curvature-Higgs mixing.and

Z 2=1+6ξγ2(1−6ξ)(24)

tan 2θ=12ξγZ m 2h

4M 2W +t

s .(27)

Using Eqs.(23)–(25),the coefficient can be written as

(A +C )2+(B +D )2=1+ 1−6ξ