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View article: Evidence for Topological States and a Lifshitz Transition in Metastable 2<i>M</i>‐WSe<sub>2</sub>
Evidence for Topological States and a Lifshitz Transition in Metastable 2<i>M</i>‐WSe<sub>2</sub> Open
In recent years, T d transition metal dichalcogenides have been heavily explored for their type‐II Weyl topology, gate‐tunable superconductivity, and nontrivial edge states in the monolayer limit. Here, the Fermi surface characteristics an…
View article: Colossal Terahertz Emission with Ultrafast Tunability Based on Van der Waals Ferroelectric NbOI<sub>2</sub>
Colossal Terahertz Emission with Ultrafast Tunability Based on Van der Waals Ferroelectric NbOI<sub>2</sub> Open
Terahertz (THz) technology is critical for quantum material physics, biomedical imaging, ultrafast electronics, and next‐generation wireless communications. However, standing in the way of widespread applications is the scarcity of efficie…
View article: Colossal terahertz emission with ultrafast tunability based on van der Waals ferroelectric NbOI$_2$
Colossal terahertz emission with ultrafast tunability based on van der Waals ferroelectric NbOI$_2$ Open
Terahertz (THz) technology is critical for quantum material physics, biomedical imaging, ultrafast electronics, and next-generation wireless communications. However, standing in the way of widespread applications is the scarcity of efficie…
View article: Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii
Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii Open
The core mass of galaxy clusters is both an important anchor of the radial mass distribution profile and probe of structure formation. With thousands of strong lensing galaxy clusters being discovered by current and upcoming surveys, timel…
View article: Nanoscale covariance magnetometry with diamond quantum sensors
Nanoscale covariance magnetometry with diamond quantum sensors Open
Nitrogen vacancy (NV) centers in diamond are atom-scale defects that can be used to sense magnetic fields with high sensitivity and spatial resolution. Typically, the magnetic field is measured by averaging sequential measurements of singl…
View article: Nanoscale covariance magnetometry with diamond quantum sensors
Nanoscale covariance magnetometry with diamond quantum sensors Open
Nitrogen vacancy (NV) centers in diamond are atom-scale defects that can be used to sense magnetic fields with high sensitivity and spatial resolution. Typically, the magnetic field is measured by averaging sequential measurements of singl…
View article: Nanoscale covariance magnetometry with diamond quantum sensors
Nanoscale covariance magnetometry with diamond quantum sensors Open
Nitrogen vacancy (NV) centers in diamond are atom-scale defects with long spin coherence times that can be used to sense magnetic fields with high sensitivity and spatial resolution. Typically, the magnetic field projection at a single poi…
View article: The Strongest Cluster Lenses: An Analysis of the Relation between Strong Gravitational Lensing Strength and the Physical Properties of Galaxy Clusters
The Strongest Cluster Lenses: An Analysis of the Relation between Strong Gravitational Lensing Strength and the Physical Properties of Galaxy Clusters Open
Strong gravitational lensing provides unique opportunities to investigate the mass distribution at the cores of galaxy clusters and to study high-redshift galaxies. Using 110 strong-lensing models of 74 cluster fields from the Hubble Front…
View article: Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii
Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii Open
The core mass of galaxy clusters is both an important anchor of the radial mass distribution profile and a probe of structure formation. With thousands of strong lensing galaxy clusters being discovered by current and upcoming surveys, tim…