Anti-D-brane as Dark Matter in Warped String Compactification
Shinji Mukohyama

TL;DR
This paper proposes that anti-D-branes in warped string compactifications can serve as dark matter candidates, with potential production mechanisms linked to D/anti-D interactions during inflation.
Contribution
It introduces a novel dark matter candidate arising from anti-D-branes in warped geometries and explores their production scenarios within string theory.
Findings
Anti-D-branes near the throat bottom behave like dark matter.
Possible production mechanisms include D/anti-D interactions during inflation.
The model connects string theory objects with cosmological dark matter.
Abstract
It is pointed out that in the warped string compactification, motion of anti-D-branes near the bottom of a throat behaves like dark matter. Several scenarios for production of the dark matter are suggested, including one based on the D/anti-D interaction at the late stage of D/anti-D inflation.
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