  Given that Sr2RuO4 is a two-component p-wave superconductor, there exists the
possibility of well defined collective modes corresponding to fluctuations of
the relative phase and spin-orientation of the two components of the order
parameter. We demonstrate that at temperatures much below Tc, these modes have
energies small compared to the pairing gap scale if the superconductivity
arises primarily from the quasi 1D (dxz and dyz) bands, while it is known that
their energies become comparable to the pairing gap scale if there is a
substantial involvement of the quasi 2D (dxy) band. Therefore, the orbital
origin of the superconductivity can be determined by measuring the energies of
these collective modes.
