BE condensates of weakly interacting bosons in gravity fields

TL;DR

This paper explores Bose-Einstein condensates of weakly interacting bosons in strong gravity fields like black holes and neutron stars, proposing they could be sources of observable gamma rays and related to dark matter interactions.

Contribution

It introduces the concept that BE condensates in gravity fields are stable reservoirs for various bosons and links their decay to observable gamma-ray signals, including potential evidence for Higgs condensates.

Findings

BE condensates can be stable in strong gravity fields.

Decay of condensates may produce observable gamma rays.

DMP collisions in galaxy are insufficient to explain observed gamma rays.

Abstract

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 and W 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 condensates can be emitted outside the horizon for our observation. It is suggested that the recently observed gamma ray peak at 129.8 +- 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 DMPs spread in the galaxy is too small for the incident DMP with the intensity of the cosmic ray energy spectrum.