Self-Interacting Dark Matter with Naturally Light Mediator
Ernest Ma (UC Riverside)

TL;DR
This paper proposes a renormalizable dark matter model with light mediators to address the cusp-core problem in dwarf galaxies, using two scalar singlets under a broken global symmetry.
Contribution
It introduces a novel, complete renormalizable model for self-interacting dark matter with a naturally light mediator.
Findings
The model achieves natural light mediators compatible with electroweak scale dark matter.
It provides a theoretical framework for resolving small-scale structure issues.
The model maintains renormalizability and consistency with known physics.
Abstract
A promising proposal for resolving the cusp-core anomaly in the density profile of dwarf galaxies is to allow dark matter to interact with itself through a light mediator of mass much less than a GeV. The theoretical challenge is to have a complete renormalizable theory where this happens naturally even though dark matter itself may be of the electroweak scale, i.e. 100 GeV to 1 TeV. I propose here such a model, with just two neutral complex scalar singlets under a softly broken dark global U(1) symmetry.
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