Probing Dark Matter Particle Properties with Ultra-High-Resolution CMB Lensing

APA

Sehgal, N. (2019). Probing Dark Matter Particle Properties with Ultra-High-Resolution CMB Lensing. Perimeter Institute for Theoretical Physics. https://pirsa.org/19090017

MLA

Sehgal, Neelima. Probing Dark Matter Particle Properties with Ultra-High-Resolution CMB Lensing. Perimeter Institute for Theoretical Physics, Sep. 06, 2019, https://pirsa.org/19090017

BibTex

          @misc{ scivideos_PIRSA:19090017,
            doi = {10.48660/19090017},
            url = {https://pirsa.org/19090017},
            author = {Sehgal, Neelima},
            keywords = {Cosmology, Particle Physics, Strong Gravity},
            language = {en},
            title = {Probing Dark Matter Particle Properties with Ultra-High-Resolution CMB Lensing},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2019},
            month = {sep},
            note = {PIRSA:19090017 see, \url{https://scivideos.org/pirsa/19090017}}
          }
          

Neelima Sehgal Stony Brook University

Abstract

I will discuss a novel and powerful way to probe dark matter particle properties using deep, high-resolution cosmic microwave background (CMB) gravitational lensing measurements. These measurements can distinguish between cold dark matter and alternative dark matter models that can explain observational puzzles of small-scale structure. I will also discuss a new experiment being developed, called CMB-HD, that can achieve this science and also open new windows on the early Universe, gas and galaxy evolution, planetary studies, and the transient sky.