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Visualization for physics analysis improvement and applications in BESIII
Modern particle physics experiments usually rely on highly complex and large-scale spectrometer devices. In high energy physics experiments,...
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The path to \(\hbox {N}^3\hbox {LO}\) parton distributions
We extend the existing leading (LO), next-to-leading (NLO), and next-to-next-to-leading order (NNLO) NNPDF4.0 sets of parton distribution functions...
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Gravitons in a gravitational plane wave
Gravitational plane waves (when Ricci flat) belong to the VSI family. The achronym VSI stands for vanishing scalar invariants , meaning that all...
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Localized surface plasmon resonance enhanced photodetector: Physical model, enhanced mechanism and applications
Localized surface plasmon resonance (LSPR) is an intriguing phenomenon that can break diffraction limitations and exhibit excellent light-confinement...
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Observational constraints on the emergent universe with non-linear equation of state and interacting fluids
We investigate a flat emergent universe (EU) with a nonlinear equation of state equivalent to three different composition of fluids. In the EU...
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Self-aligned TiOx-based 3D vertical memristor for a high-density synaptic array
The emerging nonvolatile memory, three-dimensional vertical resistive random-access memory (VRRAM), inspired by the vertical NAND structure, has been...
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Framed DDF operators and the general solution to Virasoro constraints
We define the framed DDF operators by introducing the concept of local frames in the usual formulation of DDF operators. In doing so it is possible...
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A study of interacting NTADE and SMHDE models via cosmological parameters within rastall gravity
This article explores the characteristics of interacting new Tsallis agegraphic dark energy (NTADE) and Sharma–Mittal holographic dark energy (SMHDE)...
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Spherical orbits around Kerr–Newman and Ghosh black holes
We conduct a comprehensive study on spherical orbits around two types of black holes: Kerr–Newman black holes, which are charged, and Ghosh black...
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Cosmic accretion shocks as a tool to measure the dark matter mass of galaxy clusters
Cosmological accretion shocks created during the formation of galaxy clusters are a ubiquitous phenomenon all around the universe. These shocks and...
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Generation and characterization of customized Laguerre–Gaussian beams with arbitrary profiles
We experimentally demonstrate the generation of customized Laguerre–Gaussian (LG) beams whose intensity maxima are localized around any desired...
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Nonlocal QED and lepton g-2 anomalies
Quantum electrodynamics is generally extended to a nonlocal QED by introducing the correlation functions. The gauge link is introduced to guarantee...
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Can the angular scale of cosmic homogeneity be used as a cosmological test?
In standard cosmology, the cosmic homogeneity scale is the transition scale above which the patterns arising from non-uniformities – such as groups...
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Support for fragile porous dust in a gravitationally self-regulated disk around IM Lup
Protoplanetary disks, the birthplace of planets, are expected to be gravitationally unstable in their early phase of evolution. IM Lup, a well-known...
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An estimate of the impact rate on Mars from statistics of very-high-frequency marsquakes
The number density of impact craters on a planetary surface is used to determine its age, which requires a model for the production rate of craters...
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Nonmetric geometric flows and quasicrystalline topological phases for dark energy and dark matter in \(f(Q)\) cosmology
We elaborate on nonmetric geometric flow theory and metric-affine gravity with applications in modern cosmology. Two main motivations for our...