MADMAX: A new way of probing QCD Axion Dark Matter with a Dielectric Haloscope - Foundations

24 Jul 2017, 14:00
15m
Executive Learning Center

Executive Learning Center

Contributed talk New Technologies New Technologies

Speaker

Stefan Knirck (Max-Planck-Institute for Physics, Munich, Germany)

Description

WISPy Dark Matter candidates have increasingly come under focus of scientific interest. In particular the QCD Axion might also be able to solve other fundamental problems such as strong CP-violation and could be responsible for inflation and structure formation in the early universe. Galactic Axions, Axion-Like-Particels and Hidden Photons can be converted to photons employing a surface boundary of different dielectric constants under a strong magnetic field. Combining many such surfaces, one can enhance this conversion significantly utilizing constructive interference. The proposed MADMAX setup containing 80 high dielectric discs in a 10T magnetic field might probe the well-motivated mass range of (40-400)µeV, a range which is inaccessible by existing cavity searches. We present the foundations of this approach, discussing implications on the accuracy of disc placement, dark matter velocity effects and expected sensitivity.

Primary authors

Allen Christopher Caldwell (Max-Planck-Institut fur Physik (DE)) Mr Chris Gooch (Max-Planck-Institute for Physics, Germany, Munich) Mr Armen Hambarzumjan (Max-Planck-Institute for Physics, Germany, Munich) Stefan Knirck (Max-Planck-Institute for Physics, Munich, Germany) Bela Majorovits (MPI for Physics) Alexander Millar (Max Planck Institute for Phyiscs) Georg Raffelt (MPI Physik, Munich) Javier Redondo (LMU/MPP Munich) Olaf Reimann (Max Planck Institute) Frank Simon (Max-Planck-Institut fuer Physik) Frank Daniel Steffen (Max-Planck-Institute of Physics)

Presentation materials