MBG reproduces cosmic inflation naturally from its 5D entropic equations once interacting massless scalars resolve a QFT-derived time-interaction inconsistency.
”Dark Matter Dynamics and Indirect Detection”
2 Pith papers cite this work. Polarity classification is still indexing.
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abstract
Non-baryonic, or "dark," matter is believed to be a major component of the total mass budget of the universe. We review the candidates for particle dark matter and discuss the prospects for direct detection (via interaction of dark matter particles with laboratory detectors) and indirect detection (via observations of the products of dark matter self-annihilations), focusing in particular on the Galactic center, which is among the most promising targets for indirect detection studies. The gravitational potential at the Galactic center is dominated by stars and by the supermassive black hole, and the dark matter distribution is expected to evolve on sub-parsec scales due to interaction with these components. We discuss the dominant interaction mechanisms and show how they can be used to rule out certain extreme models for the dark matter distribution, thus increasing the information that can be gleaned from indirect detection searches.
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Orbit-averaged DM energy exchange for S4714 reaches stellar luminosity at σ_χp ~ 10^{-36} cm² (MeV-GeV) and σ_χe ~ 5×10^{-38} cm² (sub-MeV) for spiked DM profiles.
citing papers explorer
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Entropy considerations in Many-Body Gravity and General Relativity, and the impact on cosmic inflation
MBG reproduces cosmic inflation naturally from its 5D entropic equations once interacting massless scalars resolve a QFT-derived time-interaction inconsistency.
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Dark matter energy exchange in stars orbiting supermassive black holes
Orbit-averaged DM energy exchange for S4714 reaches stellar luminosity at σ_χp ~ 10^{-36} cm² (MeV-GeV) and σ_χe ~ 5×10^{-38} cm² (sub-MeV) for spiked DM profiles.