  The energy in the solar acoustic spectrum is known to be correlated with
flares, but it is not known if the same is true for stellar flares? In order to
answer this question, we have analyzed 73 flares in 39 solar-like stars. These
flares were identified in the 854 solar-like stars observed by the Kepler
spacecraft that have stellar parameters measured with asteroseismology. Though
we were not able to identify a statistically significant enhancement of the
energy in the high-frequency part of the post-flare acoustic spectra compared
to the pre-flare spectra of these stars, we did identify a larger variability
between the energy in the high-frequency part of the post- and pre-flare
acoustic spectra compared to spectra taken at random times.
