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Detector R&D Klik om de tekststijl van het model te bewerken - - PowerPoint PPT Presentation

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Detector R&D Klik om de tekststijl van het model te bewerken Tweede niveau Derde niveau Vierde niveau Vijfde niveau Niels van Bakel Vista Update October 21, 2020 Vista Update October 19 - 2020 1 DR&D

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SLIDE 1

Vista Update – October 19 - 2020

  • Klik om de tekststijl van het model te bewerken
  • Tweede niveau
  • Derde niveau
  • Vierde niveau
  • Vijfde niveau

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Detector R&D

Vista Update – October 21, 2020

Niels van Bakel

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SLIDE 2

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

DR&D Group

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Current staff count:

  • Niels v Bakel, Martin v

Beuzekom, Martin Fransen, Jory Sonneveld, and Matteo Tacca

Experimental groups:

  • Kazu Akiba (LHCb), Hella

Snoek (Atlas), Alessandro Grelli (Alice), Alessandro Bertolini (GW), Conor Mow-Lowry (GW), Bas Swinkels (GW)

Detector R&D strategy 2017:

  • Smart and fast pixel detectors
  • Gravitational wave detector instrumentation
  • Collaborate with high-tech industry
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SLIDE 3

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

DR&D strategy

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ET Pathfinder Virgo upgrade LISA

ECFA Detector Panel Report 2018

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SLIDE 4

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

Looking back

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Vista25 in 2017

⬆ 🌷

  • ⬆ = increased, need

funding and skills

  • 🌷 = not very

successful

  • 👎 = now a strength!
  • 🙃 = via spin-offs
  • 😑 = equal

😑 👎 🙃

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SLIDE 5

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

Looking back

5

Vista25 in 2017

🙃 🙃

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SLIDE 6

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

Fast semi-conductor detectors

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  • Future pixels need fast timing, and high readout bandwidth
  • Pay off from our chip and readout system developments
  • Develop ‘fastest’ pixel electronics
  • 4D Tracking & Time resolved imaging

Fast chips

  • A first step: ~100 ps timing
  • Ideas on 20 ps resolution exist

Fast sensors Fast readout

  • 160 Gbps data out
  • 1 TB per minute per chip

sub-ns

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SLIDE 7

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

LHC Memo to Nikhef management

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  • Current Nikhef and DR&D goals for fast

timing

  • Hybrid technology: interest from LHCb & Atlas,

develop fast sensors

  • MAPS technology: interest from Alice & Atlas
  • Both need fast timing circuits in CMOS, fast data

links, and radiation hardness

  • Electronics Department
  • Interested in 28 nm CMOS technology for fast

timing and fast data links

  • Will follow CERN MAPS technology: currently 180

nm but will move to 65 nm

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SLIDE 8

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

  • Fast timing pixel chips ➯ “Timepix -like”
  • To be combined with novel fast sensor layers
  • First standard blocks for Alice LS3 MAPS
  • Start soon with circuitry for ‘fast’ MAPS
  • Serializers for increasing data rates in scientific instruments
  • In radiation environments
  • Low-noise low-power readout for MEMS accelerometers

ASIC developments

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Involved in Medipix, RD50 & RD53, AIDA-Inova, and CERN EP strategic R&D work packages

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SLIDE 9

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

Fast semi-conductor detectors (now)

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  • Future pixels need fast timing, and high readout bandwidth
  • Pay off from our chip and readout system developments
  • Develop ‘fastest’ pixel electronics ⇨ Hybrid & MAPS detectors
  • 4D Tracking

Fast chips

  • A first step: ~100 ps timing
  • Ideas on 20 ps resolution exist

Fast readout

  • 160 Gbps data out
  • 1 TB per minute per chip

Fast sensors Fast MAPS

sub-ns

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SLIDE 10

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

Suspensions & Seismic sensors

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  • Develop the most sensitive and compact accelerometer in

the low-frequency regime

➡ Applications in subsurface imaging for geothermal development & space navigation

  • Active & passive suspension systems
  • Ultimately apply these at the Einstein Telescope

6D Isolator

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SLIDE 11

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

Infrastructure - Optical lab

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  • Frequency dependent squeezing
  • Test optical and mechanical

components

  • Study higher-order-modes and non-

gaussian beams

  • Different beam profiles with

compatible mirrors

  • Improve sensing and controls schemes
  • Small IFO with suspended mirrors
  • Student projects

Go beyond the current limit of fundamental noises

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SLIDE 12

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

  • Signal detection and Alignment
  • First batch of Quadrant Photo Diodes for LISA (August 2020)
  • Will lead to photo diode development for Einstein Telescope

Wavefront cameras for GW detectors

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Instrumentation for Advanced Virgo, ET Pathfinder, Einstein Telescope, and LISA

4 pixels to N x N

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SLIDE 13

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

ECFA-EPS 2019 (Newsletter #3)

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  • Long term commitments
  • Focus @ Nikhef
  • Strong network
  • Discussed in Vista?!
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SLIDE 14

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

ECFA-EPS 2019 (Newsletter #3)

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  • Not only for LHC LS3/

LS4 but also for FCC or ILC

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SLIDE 15

NWO site visit – Monday September 19 - 2017 Vista Update – October 21, 2020

  • Focus & critical mass
  • Fast timing takes off
  • After years of investments in chip and readout R&D
  • Critical mass ⇨ on forefront!
  • Start Monolothic detector development
  • Extended R&D on GW instrumentation
  • Active member of LISA space mission
  • Decrease x-ray imaging activities in 2021

Recap

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