17–22 Jun 2018
DESY in Hamburg
Europe/Berlin timezone

Constraints On Bosonic Dark Matter From Ultralow-Field Nuclear Magnetic Resonance (CASPEr)

21 Jun 2018, 14:50
20m
Auditorium (DESY in Hamburg)

Auditorium

DESY in Hamburg

Notkestraße 85 22607 Hamburg Germany
Presentation Plenary presentations

Speaker

Mr Antoine Garcon (Helmholtz Institute Mainz)

Description

The nature of dark matter, the invisible substance that makes up over $80$% of the matter in the universe, is one of the most intriguing mysteries of modern physics. Elucidating the nature of dark matter would profoundly impact our understanding of cosmology and particle physics, providing key insights into physics beyond the Standard Model. Recent theories of couplings between dark matter and nuclear spins have opened the possibility of directly detecting axion, axion-like and dark-photon dark matter via NMR spectroscopy [1]: as nuclear spins move through the galactic dark-matter halo, the spins couple to dark-matter particles and behave as if they were in an oscillating magnetic field, potentially generating a dark-matter-driven NMR signal. The Cosmic Axion Spin Precession Experiment (CASPEr) is multi-faceted NMR search for such particles [2]. Here, we will review a CASPEr experiment based on zero- to ultralow-field NMR (ZULF NMR [3]). We first review the physical principles enabling the detection of dark-matter via ZULF NMR and introduce the off-resonance-based measurement scheme used for such detection [4]. We expect dark-matter particles to induce modulation of the $J$-coupling energy levels of the NMR sample. Axions and dark-photons could then be detected by searching for frequency-modulation induced sidebands in the well-defined ZULF NMR spectrum of labelled formic acid. We then describe the current ZULF NMR apparatus and present an exotic data processing scheme, which enables the possibility to perform coherent averaging of transient NMR signals induced by sources of unknown frequencies such as dark matter. Finally, we present our latest results on ultralight-axion dark-matter acquired through this search. [1] P. W. Graham and S. Rajendran, Phys. Rev. D, (88), 035023 (2013) [2] D. Budker et al., Phys. Rev. X, (4), 1-10 (2014) [3] J.W. Blanchard, D. Budker, eMagRes, (5), 5-3 (2016) [4] A. Garcon et al., IOP Quantum Science and Technology, (3), 1 (2017)

Summary

Results of an axion dark-matter search via ultralow-field nuclear magnetic resonance: CASPEr ZULF.

Primary author

Mr Antoine Garcon (Helmholtz Institute Mainz)

Co-authors

Dr Arne Wickenbrock (Johannes Gutenberg-Universität) Prof. Dmitry Budker (Helmholtz Institute) Mr Gary Centers (Helmholtz Institute, Mainz) Dr John W. Blanchard (Helmholtz Institute Mainz) Marina Gil (Mrs.) Mr Nataniel L. Figueroa (HIM)

Presentation materials