  Recent evidence for one or more gamma-ray lines at ~ 130 GeV in the Fermi-LAT
data from the Galactic Center has been interpreted as a hint for dark matter
annihilation to Z{\gamma} or H{\gamma} with an annihilation cross section,
<\sigma v> ~ 10^{-27} cm^3 s^{-1} . We test this hypothesis by comparing
synchrotron fluxes due to the electrons and positrons from the decay of the Z
or the H boson only in the Galactic Center against radio data from the same
region in the Galactic Center. We find that the radio data from single dish
telescopes marginally constrain this interpretation of the claimed gamma lines
for a contracted NFW profile. Already-operational radio telescopes such as LWA,
VLA-Low and LOFAR, and future radio telescopes like SKA, which are sensitive to
annihilation cross sections as small as 10^{-28} cm^3 s^{-1}, can confirm or
rule out this scenario very soon. We discuss the assumptions on the dark matter
profile, magnetic fields, and background radiation density profiles, and show
that the constraints are relatively robust for any reasonable assumptions.
Independent of the above said recent developments, we emphasize that our radio
constraints apply to all models where dark matter annihilates to Z{\gamma} or
H{\gamma}.
