0000000000778526

AUTHOR

Hendrik Bekker

showing 2 related works from this author

Quantum sensitivity limits of nuclear magnetic resonance experiments searching for new fundamental physics

2021

Nuclear magnetic resonance is a promising experimental approach to search for ultra-light axion-like dark matter. Searches such as the cosmic axion spin-precession experiments (CASPEr) are ultimately limited by quantum-mechanical noise sources, in particular, spin-projection noise. We discuss how such fundamental limits can potentially be reached. We consider a circuit model of a magnetic resonance experiment and quantify three noise sources: spin-projection noise, thermal noise, and amplifier noise. Calculation of the total noise spectrum takes into account the modification of the circuit impedance by the presence of nuclear spins, as well as the circuit back-action on the spin ensemble. S…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Materials Science (miscellaneous)Dark matterFOS: Physical sciences01 natural sciencesNoise (electronics)010305 fluids & plasmasNuclear magnetic resonanceHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530Sensitivity (control systems)Electrical and Electronic Engineering010306 general physicsAxionQuantumElectrical impedanceSpin-½PhysicsQuantum PhysicsSpinsInstrumentation and Detectors (physics.ins-det)Atomic and Molecular Physics and OpticsCondensed Matter - Other Condensed MatterHigh Energy Physics - PhenomenologyQuantum Physics (quant-ph)Other Condensed Matter (cond-mat.other)
researchProduct

Spectral signatures of axionlike dark matter

2022

We derive spectral line shapes of the expected signal for a haloscope experiment searching for axionlike dark matter. The knowledge of these line shapes is needed to optimize an experimental design and data analysis procedure. We extend the previously known results for the axion-photon and axion-gluon couplings to the case of gradient (axion-fermion) coupling. A unique feature of the gradient interaction is its dependence not only on magnitudes but also on directions of velocities of galactic halo particles, which leads to the directional sensitivity of the corresponding haloscope. We also discuss the daily and annual modulations of the gradient signal caused by the Earth's rotational and o…

High Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)FOS: Physical sciencesddc:530530Astrophysics - Cosmology and Nongalactic AstrophysicsHigh Energy Physics - ExperimentPhysics - Atomic PhysicsPhysical Review
researchProduct