We revisit the energy transfer necessary for the warped reheating scenario in
a two-throat geometry. We study KK mode wavefunctions of the full two-throat
system in the Randall--Sundrum (RS) approximation and find an interesting
subtlety in the calculation of the KK mode tunnelling rate. While wavepacket
tunnelling is suppressed unless the Standard Model throat is very long,
wavefunctions of modes localized in different throats have a non-zero overlap
and energy can be transferred between the throats by interactions between such
KK modes. The corresponding decay rates are calculated and found to be faster
than the tunnelling rates found in previously published works. However, it
turns out that the imaginary parts of the mode frequencies, induced by the
decay, slow the decay rates themselves down. The self-consistent decay rate
turns out to be given by the plane wave tunnelling rate considered previously
in the literature. We then discuss mechanisms that may enhance the energy
transfer between the throats over the RS rates. In particular, we study models
in which the warp factor changes in the UV region less abruptly than in the RS
model, and find that it is easy to build phenomenological models in which the
plane wave tunnelling rate, and hence the KK mode interaction rates, are
enhanced compared to the standard RS setup.Comment: 27 pages + appendices, 5 figures, latex. v2: Discussion of decay in
Section 4 changed: the most dangerous graviton amplitudes are zero, the
results are now more positive for the warped reheating scenario; typos fixed,
discussion cleaned up. v3:corrections in Section 5 (decay rates slowed down),
mild changes of overall conclusion