22–24 Jun 2016
University of Milano-Bicocca
Europe/Rome timezone

TKIDs: MKIDs (not only) for X-ray astronomy

23 Jun 2016, 11:15
25m
U4/08 (University of Milano-Bicocca)

U4/08

University of Milano-Bicocca

Piazza della Scienza, 4 20126 - Milano
Oral Contribution MKIDs for other applications Session 4: MKIDs for other applications - Part 1

Speaker

Dr Gerhard Ulbricht (UCSB)

Description

The Mazin Lab at UC Santa Barbara develops Thermal Kinetic Inductance Detectors (TKIDs) for X-ray imaging spectroscopy. I will present our recent progress developing TKIDs for X-ray imaging spectroscopy in the 0.5 to 20 keV band. TKIDs are optimized for X-ray detection by suspending their inductor and a separate X-ray absorber on a freestanding Si3N4 membrane and by operating them as microcalorimeters. They have the potential to achieve time and energy resolutions comparable to TESs while retaining the passive multiplexibility of MKIDs, thus offering a promising and feasible way to kilo- or even mega-pixel X-ray detector arrays. With considerably saturated prototypes we have already demonstrated a TKID energy resolution of 75 eV at 5.9 keV, and I will elaborate on our plans to further improve our TKID design in order to find out how close to the projected TKID energy resolution of less then 0,1% we can get.

Primary author

Dr Gerhard Ulbricht (UCSB)

Co-authors

Mr Alex B. Walter (UCSB) Prof. Benjamin A. Mazin (UCSB) Mr Clint Bockstiegel (UCSB) Ms Giulia Collura (UCSB) Mr Matthew J. Strader (UCSB) Mr Neelay Fruitwala (UCSB) Mr Paul Szypryt (UCSB) Mr Seth Meeker (UCSB)

Presentation materials