PIRSA:18050001

Video URL

https://pirsa.org/18050001

Microwave Kinetic Inductance Detectors for Exoplanets and Light Dark Matter

Mazin, B. (2018). Microwave Kinetic Inductance Detectors for Exoplanets and Light Dark Matter. Perimeter Institute for Theoretical Physics. https://pirsa.org/18050001

Mazin, Benjamin. Microwave Kinetic Inductance Detectors for Exoplanets and Light Dark Matter. Perimeter Institute for Theoretical Physics, May. 01, 2018, https://pirsa.org/18050001 

          @misc{ scivideos_PIRSA:18050001,
            doi = {10.48660/18050001},
            url = {https://pirsa.org/18050001},
            author = {Mazin, Benjamin},
            keywords = {Particle Physics},
            language = {en},
            title = {Microwave Kinetic Inductance Detectors for Exoplanets and Light Dark Matter},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2018},
            month = {may},
            note = {PIRSA:18050001 see, \url{https://scivideos.org/pirsa/18050001}}
          }

Benjamin Mazin University of California, Santa Barbara

Talk numberPIRSA:18050001
DOI10.48660/18050001
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Microwave Kinetic Inductance Detectors, or MKIDs, are superconducting detector arrays that can measure the energy and arrival time of individual optical through near-IR photons without read noise or dark counts.  I will discuss our recent work and results from the first two MKID Integral Field Spectrographs (IFSs) for high contrast imaging, DARKNESS/SDC at the Palomar 200" and MEC/SCExAO on Subaru. I will then look at the future of MKIDs and their potential on 30-m class telescopes like the TMT, and explore a fascinating new application in the detection of light scalar dark matter.