0000000000374614

AUTHOR

Shang Li

showing 2 related works from this author

Determination of local defect density in diamond by double electron-electron resonance

2021

Magnetic impurities in diamond influence the relaxation properties and thus limit the sensitivity of magnetic, electric, strain, and temperature sensors based on nitrogen-vacancy color centers. Diamond samples may exhibit significant spatial variations in the impurity concentrations hindering the quantitative analysis of relaxation pathways. Here, we present a local measurement technique which can be used to determine the concentration of various species of defects by utilizing double electron-electron resonance. This method will help to improve the understanding of the physics underlying spin relaxation and guide the development of diamond samples, as well as offering protocols for optimiz…

Quantum PhysicsMaterials scienceCondensed Matter - Mesoscale and Nanoscale PhysicsRelaxation (NMR)FOS: Physical sciencesResonanceDiamond02 engineering and technologyElectronengineering.material021001 nanoscience & nanotechnology01 natural sciencesMolecular physicsElectron resonanceImpurityMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciencesengineeringddc:530Quantum Physics (quant-ph)010306 general physics0210 nano-technologySpin relaxationPhysical Review B
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Search for gamma-ray spectral lines with the DArk Matter Particle Explorer

2021

The DArk Matter Particle Explorer (DAMPE) is well suitable for searching for monochromatic and sharp $\gamma$-ray structures in the GeV$-$TeV range thanks to its unprecedented high energy resolution. In this work, we search for $\gamma$-ray line structures using five years of DAMPE data. To improve the sensitivity, we develop two types of dedicated data sets (including the BgoOnly data which is the first time to be used in the data analysis for the calorimeter-based gamma-ray observatories) and adopt the signal-to-noise ratio optimized regions of interest (ROIs) for different DM density profiles. No line signals or candidates are found between 10 and 300 GeV in the Galaxy. The constraints o…

High Energy Astrophysical Phenomena (astro-ph.HE)Line-like structureHigh Energy Physics - Experiment (hep-ex)MultidisciplinaryAstrophysics::High Energy Astrophysical PhenomenaDAMPE Dark matter Gamma-ray Line-like structureSettore FIS/01 - Fisica SperimentaleDAMPEDark matterFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaGamma-rayHigh Energy Physics - ExperimentScience Bulletin
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