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Search for Light Dark Matter with Quadratic Interactions in Standard Model Fields

NYU Physics via YouTube

Overview

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Explore a physics seminar presentation examining innovative search methods for light dark matter with quadratic interactions, delivered by Da Liu from the University of Pittsburgh. Learn about the theoretical framework where light dark matter interacts quadratically with Standard Model fields, resulting in effective interactions between dark matter and nucleon fields below QCD confinement scale. Understand how these interactions create potential barriers affecting dark matter wind around ordinary matter, potentially causing bounce-back effects and inducing measurable pressure forces. Delve into various experimental constraints including Supernova cooling, Big Bang Nucleosynthesis, and gravitational inverse square law tests, while discovering potential detection methods through space-based weak equivalence principle experiments. Cover key topics including field-like vs particle-like dark matter models, acceleration effects, geometric limits, shielding effects, and practical experimental approaches using torsion balances, microscopes, and Galileo-type tests.

Syllabus

Intro
Dark Matter: field-like or particle like
Light Scalar Dark Matter Model
Acceleration induced by DM wind
Geometric Limit
Slow scattering limit: large skin depth
Shielding effect: potential barrier
Supernova Cooling Bound: Raffelt criterion
BBN in a Nutshell
BBN: Helium-4
Bound from Gravitational inverse-square law
Possible experiments: Torsion Balance
Torsion Balance: Dark Matter
Possible experiments: Microscope
Possible experiments: Galileo Galilei
Summary in One Plot
Conclusion
Sensitivity No shielding
Two conditions for the maximal force

Taught by

NYU Physics

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