94 research outputs found
Chiral Dirac-like fermion in spin-orbit-free antiferromagnetic semimetals
Dirac semimetal is a phase of matter, whose elementary excitation is
described by the relativistic Dirac equation. In the limit of zero mass, its
parity-time symmetry enforces the Dirac fermion in the momentum space, which is
composed of two Weyl fermions with opposite chirality, to be non-chiral.
Inspired by the flavor symmetry in particle physics, we theoretically propose a
massless Dirac-like equation yet linking two Weyl fields with the identical
chirality by assuming SU(2) isospin symmetry, independent of the space-time
rotation exchanging the two fields. Dramatically, such symmetry is hidden in
certain solid-state spin-1/2 systems with negligible spin-orbit coupling, where
the spin degree of freedom is decoupled with the lattice. Therefore, the
existence of the corresponding quasiparticle, dubbed as flavor Weyl fermion,
cannot be explained by the conventional (magnetic) space group framework. The
four-fold degenerate flavor Weyl fermion manifests linear dispersion and a
Chern number of 2, leading to a robust network of topologically protected Fermi
arcs throughout the Brillouin zone. For material realization, we show that the
transition-metal chalcogenide CoNb3S6 with experimentally confirmed collinear
antiferromagnetic order is ideal for flavor Weyl semimetal under the
approximation of vanishing spin-orbit coupling. Our work reveals a counterpart
of the flavor symmetry in magnetic electronic systems, leading to further
possibilities of emergent phenomena in quantum materials.Comment: 27 pages and 5 figure
Spin-group symmetry in magnetic materials with negligible spin-orbit coupling
Symmetry formulated by group theory plays an essential role with respect to
the laws of nature, from fundamental particles to condensed matter systems.
Here, by combining symmetry analysis and tight-binding model calculations, we
elucidate that the crystallographic symmetries of a vast number of magnetic
materials with light elements, in which the neglect of relativistic spin-orbit
coupling (SOC) is an appropriate approximation, are considerably larger than
the conventional magnetic groups. Thus, a symmetry description that involves
partially-decoupled spin and spatial rotations, dubbed as spin group, is
required. Spin group permits more symmetry operations and thus more energy
degeneracies that are disallowed by the magnetic groups. One consequence of the
spin group is the new anti-unitary symmetries that protect SOC-free Z_2
topological phases with unprecedented surface node structures. Our work not
only manifests the physical reality of materials with weak SOC, but also shed
light on the understanding of all solids with and without SOC by a unified
group theory.Comment: To appear in Phys. Rev. X; main text includes 34 pages, 1 table and 5
figure
Machine Learning Enabled Prediction of Mechanical Properties of Tungsten Disulfide Monolayer
One of two-dimensional transition metal dichalcogenide materials, tungsten disulfide (WS2), has aroused much research interest, and its mechanical properties play an important role in a practical application. Here the mechanical properties of h-WS2 and t-WS2 monolayers in the armchair and zigzag directions are evaluated by utilizing the molecular dynamics (MD) simulations and machine learning (ML) technique. We mainly focus on the effects of chirality, system size, temperature, strain rate, and random vacancy defect on mechanical properties, including fracture strain, fracture strength, and Young’s modulus. We find that the mechanical properties of h-WS2 surpass those of t-WS2 due to the different coordination spheres of the transition metal atoms. It can also be observed that the fracture strain, fracture strength, and Young’s modulus decrease when temperature and vacancy defect ratio are enhanced. The random forest (RF) supervised ML algorithm is employed to model the correlations between different impact factors and target outputs. A total number of 3600 MD simulations are performed to generate the training and testing dataset for the ML model. The mechanical properties of WS2 (i.e., target outputs) can be predicted using the trained model with the knowledge of different input features, such as WS2 type, chirality, temperature, strain rate, and defect ratio. The mean square errors of ML predictions for the mechanical properties are orders of magnitude smaller than the actual values of each property, indicating good training results of the RF model
MetaRadar: Indoor Localization by Reconfigurable Metamaterials
Indoor localization has drawn much attention owing to its potential for
supporting location based services. Among various indoor localization
techniques, the received signal strength (RSS) based technique is widely
researched. However, in conventional RSS based systems where the radio
environment is unconfigurable, adjacent locations may have similar RSS values,
which limits the localization precision. In this paper, we present MetaRadar,
which explores reconfigurable radio reflection with a surface/plane made of
metamaterial units for multi-user localization. By changing the reflectivity of
metamaterial, MetaRadar modifies the radio channels at different locations, and
improves localization accuracy by making RSS values at adjacent locations have
significant differences. However, in MetaRadar, it is challenging to build
radio maps for all the radio environments generated by metamaterial units and
select suitable maps from all the possible maps to realize a high accuracy
localization. To tackle this challenge, we propose a compressive construction
technique which can predict all the possible radio maps, and propose a
configuration optimization algorithm to select favorable metamaterial
reflectivities and the corresponding radio maps. The experimental results show
a significant improvement from a decimeter-level localization error in the
traditional RSS-based systems to a centimeter-level one in MetaRadar
Non-default Component of Sovereign Emerging Market Yield Spreads and its Determinants: Evidence from Credit Default Swap Market
This article shows that a sizable component of emerging market sovereign yield spreads is due to factors other than default risk, such as liquidity. The author estimates the non-default component of the yield spreads as the basis between the actual credit default swap (CDS) premium and the hypothetical CDS premium implied by emerging market bond yields. On average, the basis is large and positive for speculative-grade bonds and slightly negative for investment-grade bonds. The large positive basis for speculative-grade bonds supports the existence of speculation in the CDS market when the underlying's credit quality is bad. The author studies the effects of bond liquidity, liquidity in the CDS market, equity market performance, and macroeconomic variables on the non-default component of the emerging market yield spreads. The results show that bond liquidity has a significant and positive effect on the CDS–bond basis of investment-grade bonds. The results suggest that the liquid bonds of investment-grade bonds are more expensive relative to the prices implied their CDS premiums. However, the results are somewhat mixed and even contrary for the speculative-grade bond sample
Sciences for The 2.5-meter Wide Field Survey Telescope (WFST)
The Wide Field Survey Telescope (WFST) is a dedicated photometric survey
facility under construction jointly by the University of Science and Technology
of China and Purple Mountain Observatory. It is equipped with a primary mirror
of 2.5m in diameter, an active optical system, and a mosaic CCD camera of 0.73
Gpix on the main focus plane to achieve high-quality imaging over a field of
view of 6.5 square degrees. The installation of WFST in the Lenghu observing
site is planned to happen in the summer of 2023, and the operation is scheduled
to commence within three months afterward. WFST will scan the northern sky in
four optical bands (u, g, r, and i) at cadences from hourly/daily to
semi-weekly in the deep high-cadence survey (DHS) and the wide field survey
(WFS) programs, respectively. WFS reaches a depth of 22.27, 23.32, 22.84, and
22.31 in AB magnitudes in a nominal 30-second exposure in the four bands during
a photometric night, respectively, enabling us to search tremendous amount of
transients in the low-z universe and systematically investigate the variability
of Galactic and extragalactic objects. Intranight 90s exposures as deep as 23
and 24 mag in u and g bands via DHS provide a unique opportunity to facilitate
explorations of energetic transients in demand for high sensitivity, including
the electromagnetic counterparts of gravitational-wave events detected by the
second/third-generation GW detectors, supernovae within a few hours of their
explosions, tidal disruption events and luminous fast optical transients even
beyond a redshift of 1. Meanwhile, the final 6-year co-added images,
anticipated to reach g about 25.5 mag in WFS or even deeper by 1.5 mag in DHS,
will be of significant value to general Galactic and extragalactic sciences.
The highly uniform legacy surveys of WFST will also serve as an indispensable
complement to those of LSST which monitors the southern sky.Comment: 46 pages, submitted to SCMP
Cumulative increased risk of incident type 2 diabetes mellitus with increasing triglyceride glucose index in normal-weight people: The Rural Chinese Cohort Study
Machine Learning Enabled Prediction of Mechanical Properties of Tungsten Disulfide Monolayer
One of two-dimensional transition metal dichalcogenide materials, tungsten disulfide (WS2), has aroused much research interest, and its mechanical properties play an important role in a practical application. Here the mechanical properties of h-WS2 and t-WS2 monolayers in the armchair and zigzag directions are evaluated by utilizing the molecular dynamics (MD) simulations and machine learning (ML) technique. We mainly focus on the effects of chirality, system size, temperature, strain rate, and random vacancy defect on mechanical properties, including fracture strain, fracture strength, and Young’s modulus. We find that the mechanical properties of h-WS2 surpass those of t-WS2 due to the different coordination spheres of the transition metal atoms. It can also be observed that the fracture strain, fracture strength, and Young’s modulus decrease when temperature and vacancy defect ratio are enhanced. The random forest (RF) supervised ML algorithm is employed to model the correlations between different impact factors and target outputs. A total number of 3600 MD simulations are performed to generate the training and testing dataset for the ML model. The mechanical properties of WS2 (i.e., target outputs) can be predicted using the trained model with the knowledge of different input features, such as WS2 type, chirality, temperature, strain rate, and defect ratio. The mean square errors of ML predictions for the mechanical properties are orders of magnitude smaller than the actual values of each property, indicating good training results of the RF model
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