Abstract
We investigate the response of superfluid Fermi gases to rapid changes of the three-dimensional -wave scattering length by solving the time-dependent Bogoliubov–de Gennes equations. In general the magnitude of the order parameter performs oscillations, which are sometimes called the “Higgs” mode, with the angular frequency , where is the gap in the spectrum of fermionic excitations. First, we excite the oscillations with a linear ramp of and study the evolution of . Second, we continously drive the system with a sinusoidal modulation of . In the first case, the oscillations in damp according to a power law. In the second case, the continued driving causes revivals in the oscillations. In both cases, the excitation of the oscillations causes a reduction in the time-averaged value of . We propose two experimental protocols, based around the two approaches, to measure the frequency and damping of the oscillations, and hence .
- Received 10 September 2012
DOI:https://doi.org/10.1103/PhysRevA.86.053604
©2012 American Physical Society