  Analysis of the Fermi-LAT data has revealed two extended structures above and
below the Galactic Centre emitting gamma rays with a hard spectrum, the
so-called Fermi bubbles. Hadronic models attempting to explain the origin of
the Fermi bubbles predict the emission of high-energy neutrinos and gamma rays
with similar fluxes. The ANTARES detector, a neutrino telescope located in the
Mediterranean Sea, has a good visibility to the Fermi bubble regions. Using
data collected from 2008 to 2011 no statistically significant excess of events
is observed and therefore upper limits on the neutrino flux in TeV range from
the Fermi bubbles are derived for various assumed energy cutoffs of the source.
