The Bose-Einstein ( BE ) condensates of weakly interacting bosons in a strong gravity field , such as AGN ( Active Galactic Nuclei ) , BHs ( black holes ) and neutron stars , are discussed .
Being bound systems in gravity fields , these are stable reservoirs for the Higgs bosons , and vector bosons of Z ^ { 0 } and W ^ { \pm } as well as supersymmetric bosons .
Upon gravitational disturbances , such as a gravitational collapse , these objects are relieved from the BE condensate bound states and decay or interact with each other freely .
Using the repulsive nature of gravity at short distances which was obtained by the present author as quantum corrections to gravity , the particles produced by the decays or interactions of the bosons liberated from BE codensates can be emitted outside the horizon for our observation .
It is suggested that the recently observed gamma ray peak at 129.8 \pm 2.4 GeV from FERMI Large Area Telescope may be evidence for the existence of the Higgs boson condensates .
The BE condensates of supersymmetric bosons are the most likely sources for the gamma rays from DMP ( dark matter particle ) and anti-DMP collisions .
It is shown that the said process from the DMPs spread in the galaxy is too small for the incident DMP with the intensity of the cosmic ray energy spectrum .