Quantum Materials for Dark Matter Detection

Europe/Stockholm
122:026 (Nordita, Stockholm)

122:026

Nordita, Stockholm

Alexander Balatsky (Nordita), Alfredo Ferella (Stockholm University), Felix Kahlhoefer (RWTH Aachen University), Jan Conrad (Stockholm University), Martin Winkler (Stockholm University), Mathew Lawson (Stockholm University), Mathias Geilhufe (Nordita), Riccardo Catena (Chalmers), Timon Emken (Chalmers)
Description

Venue

Nordita, Stockholm, Sweden

Scope

Recently, the evidence for the existence of a significant component of matter in the Universe which is not visible by conventional telescopes has become indisputable. To date, the nature of this matter, coined dark matter (DM), is still unknown. Currently, the most popular theoretical model of dark matter introduces a new type of elementary particle created in the early Universe, dubbed Weakly Interacting Massive particle (WIMP). The predicted mass of WIMPs ranges from GeV to TeV, with an interaction strengths roughly on the weak scale. In recent years, searches for this GeV mass DM have reached sensitivities that probe the current paradigm and the absence of positive signals motivate the widening of the search window. One particular line of research is the focus on light and ultra-light dark matter, i.e. sub-GeV mass dark matter from a hidden dark sector with a new force interacting with the standard model or ultra-light DM with mass range from 10-22 eV to keV. The arguably most popular example of the latter class is the axion, invoked to solve the apparent absence of CP violation in Quantum Chromo Dynamics. Detection of these particles poses new challenges to potential sensor materials: very small energy depositions, magnetic properties and anisotropic response to particle interactions for example become crucial requirements. The challenge of finding suitable materials fits well with recent developments in solid state physics: Motivated by the exponential growth of computational power and the resulting data, we witness the rapid adoption of functional materials prediction within the framework of materials informatics. Here, methods adapted from computer science based on data-mining and machine learning are applied to identify materials with requested target properties.

The program will contain two introductory lectures: one on solid state physics for particle physicists (by Alexander Balatsky) and one vice versa (by Riccardo Catena).

[Timetable - available from start of the conference]

Application

If you want to apply for participation in the conference, please fill in the application form. You will be informed by the organizers shortly after the application deadline whether your application has been approved. Due to space restrictions, the total number of participants is limited. (Invited speakers are of course automatically approved, but need to register anyway.)

Application deadline: 22 November 2019

There is no registration fee.

Sponsored by:

Nordita KTH - Royal Institute of Technology Stockholm University

    • 1
      Opening 132:028

      132:028

      Nordita, Stockholm

    • 2
      Introductory Talk: Dark Matter Direct Detection for Condensed Matter Physicists 132:028

      132:028

      Nordita, Stockholm

      Speaker: Riccardo Catena
    • 3
      Coffee break 132:028

      132:028

      Nordita, Stockholm

    • 4
      Light Dark Matter Search with XENON1T 132:028

      132:028

      Nordita, Stockholm

      Speaker: Jelle Aalbers (Stockholm University)
    • 5
      Lunch Albanova cafeteria

      Albanova cafeteria

      Nordita, Stockholm

    • 6
      New Routes and Materials Design for Sub-GeV Dark Matter Detection 132:028

      132:028

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      Speaker: Sinead Griffin
    • 7
      Graphene and its applications to cosmology: the PTOLEMY project 132:028

      132:028

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      Speaker: Alfredo Ferella
    • 8
      Coffee break 132:028

      132:028

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    • 9
      Introductory Talk: Condensed Matter for Particle Physicists 132:028

      132:028

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      Speaker: Alexander Balatsky
    • 10
      Reception 122:026

      122:026

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    • 11
      Quasiparticles and Axion Dark Matter: the Plasma Haloscope 132:028

      132:028

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      Speaker: Matthew Lawson
    • 12
      Coffee break 132:028

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    • 13
      How atoms respond to general dark matter-electron interactions 132:028

      132:028

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      Speaker: Timon Emken
    • 14
      Lunch Albanova cafeteria

      Albanova cafeteria

      Nordita, Stockholm

    • 15
      Sub-MeV Dark Matter Detection with Dirac Materials 132:028

      132:028

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      Speaker: Martin Winkler
    • 16
      Finding FIMPs 132:028

      132:028

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      Speaker: Saniya Heeba
    • 17
      Coffee break 132:028

      132:028

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    • 18
      Light dark matter detection in paleo detectors 132:028

      132:028

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      Speaker: Andzej Drukier
    • 19
      Coffee break 132:028

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    • 20
      Light dark matter detection with superfluid from EFT 132:028

      132:028

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      Speaker: Sichun Sun
    • 21
      Lunch Albanova cafeteria

      Albanova cafeteria

      Nordita, Stockholm

    • 22
      Discussion 132:028

      132:028

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    • 23
      Closing 132:028

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      Nordita, Stockholm