Radiation from matter-antimatter annihilation in the quark nugget model of dark matter
V.V. Flambaum, I.B. Samsonov

TL;DR
This paper investigates the interactions of matter with antimatter quark nuggets in the dark matter model, showing that electron-positron annihilation is suppressed and proposing alternative mechanisms for observed galactic gamma-ray signals.
Contribution
It demonstrates that the strong electric field of anti-quark nuggets prevents electron-positron annihilation, challenging previous explanations for galactic 511 keV photons and suggesting new mechanisms involving proton interactions.
Findings
Electron-positron annihilation probability is reduced by five orders of magnitude.
Electron interactions cannot explain the galactic 511 keV photon observations.
Proton annihilation and pion decay may account for observed gamma-ray signals.
Abstract
We revisit the properties of positron cloud in quark nugget (QN) model of dark matter (DM). In this model, dark matter particles are represented by compact composite objects composed of a large number of quarks or antiquarks with total baryon number . These particles have a very small number density in our galaxy which makes them "dark" to all DM detection experiments and cosmological observations. In this scenario, anti-quark nuggets play special role because they may manifest themselves in annihilation with visible matter. We study electron-positron annihilation in collisions of free electrons, hydrogen and helium gases with the positron cloud of anti-quark nuggets. We show that a strong electric field of anti-quark nuggets destroys positronium, hydrogen and helium atoms and prevents electrons from penetrating deeply in positron cloud, thus reducing the probability of…
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