A5061366321- Pulsars and Gravitational Waves Research
- High-Energy Particle Collisions Research
- Quantum Chromodynamics and Particle Interactions
- Nuclear physics research studies
- Cosmology and Gravitation Theories
- Gamma-ray bursts and supernovae
- Particle physics theoretical and experimental studies
- Geophysics and Gravity Measurements
- High-pressure geophysics and materials
- Black Holes and Theoretical Physics
- Nuclear reactor physics and engineering
- Nuclear Physics and Applications
- Cold Atom Physics and Bose-Einstein Condensates
- Solar and Space Plasma Dynamics
- Radioactive Decay and Measurement Techniques
- Additive Manufacturing Materials and Processes
- Aluminum Alloys Composites Properties
- Genomics and Rare Diseases
- Particle Detector Development and Performance
- Quantum Electrodynamics and Casimir Effect
- Relativity and Gravitational Theory
- Astro and Planetary Science
- NF-κB Signaling Pathways
- Astrophysics and Cosmic Phenomena
- Cutaneous lymphoproliferative disorders research
Materials Technology (United Kingdom)
2025
Inner Mongolia University
2023-2024
Shanghai Jiao Tong University
2018-2024
Central China Normal University
2022-2024
International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles
2024
High Energy Accelerator Research Organization
2024
AGH University of Krakow
2023
Campbell Collaboration
2023
Czech Academy of Sciences, Institute of Psychology
2023
Institute of Physics
2021
The neutron skin thickness $\Delta r_{\rm{np}}$ of heavy nuclei is essentially determined by the symmetry energy density slope $L({\rho })$ at $\rho_c = 0.11~{\rm {fm}^{-3}}\approx 2/3\rho_0$ ($\rho_0$ nuclear saturation density), roughly corresponding to average finite nuclei. PREX collaboration recently reported a model-independent extraction r^{208}_{\rm{np}} 0.283 \pm 0.071$ fm for $^{208}$Pb, suggesting rather stiff $E_{\rm{sym}}({\rho with $L({\rho_c }) \ge 52$ MeV. We show that cannot...
Transverse momentum ($p_{T}$) generation in relativistic heavy ion collisions is sensitive to the initial geometry and final-state bulk evolution. We demonstrate with hydrodynamic calculations that mean $p_T$ ratio ($R_{\langle p_{T}\rangle}$) between highly similar isobar $^{96}_{44}$Ru+$^{96}_{44}$Ru $^{96}_{40}$Zr+$^{96}_{40}$Zr insensitive evolution remains small difference nuclear structure (neutron skin deformation) Ru Zr nuclei.We further find deformation can produce an...
Particle production in ultrarelativistic heavy ion collisions depends on the details of nucleon density distributions colliding nuclei. We demonstrate that charged hadron multiplicity isobaric at energies provide a novel approach to determine poorly known neutron and thus skin thickness finite nuclei, which can turn put stringent constraints nuclear symmetry energy.
While the equation of state (EOS) symmetric nuclear matter (SNM) at suprasaturation densities has been relatively well constrained from heavy-ion collisions, EOS high-density neutron-rich is still largely uncertain due to poorly known behavior symmetry energy. Using constraints on SNM collisions together with data finite nuclei and existence $2\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$ neutron stars electromagnetic observations, we show that energy cannot be too soft, which leads lower...
Based on the accurately calibrated interaction FSUGold, we show that including isovector scalar $\delta$ meson and its coupling to isoscalar $\sigma$ in relativistic mean field (RMF) model can soften symmetry energy $E_{\rm{sym}}(n)$ at intermediate densities while stiffen high densities. We find this new RMF be simultaneously compatible with (1) constraints equation of state symmetric nuclear matter suprasaturation from flow data heavy-ion collisions, (2) neutron skin thickness $^{208}$Pb...
Within a confining quark matter model which considers phenomenologically the confinement and asymptotic freedom as well chiral symmetry restoration deconfinement at high baryon density, we find that if up-down ($ud$QM) is more stable than nuclear strange (SQM), maximum mass of static stars with $ud$QM $2.87M_{\odot}$ under agreement both constraints on star tidal deformability from gravitational wave signal GW170817 mass-radius PSR J0030+0451 J0740+6620 measured by NICER. In contrast,...
Neutron skin thickness ($\mathrm{\ensuremath{\Delta}}{r}_{\mathrm{np}}$) of nuclei and the inferred nuclear symmetry energy are critical importance to physics astrophysics. It is traditionally measured by processes with significant theoretical uncertainties. We recently proposed an indirect measurement $\mathrm{\ensuremath{\Delta}}{r}_{\mathrm{np}}$ charged hadron multiplicities in central isobaric collisions at relativistic energies, which sensitive densities. In this Letter, we propose a...
In this work, we explore the properties of isospin asymmetric quark matter in stars (QSs). The chemical potential, asymmetry, symmetry energy, equation state (EOS) strange (SQM), and maximum mass QSs are also studied by using different phenomenological models. Our results indicate that parameter space models for energy EOS star can be reduced considering recent mass-radius estimates PSR $\mathrm{J}0740+6620$, $\mathrm{J}0030+0451$, 4U 1702-429, central compact within supernova remnant HESS J1731-347.
<title>Abstract</title> Metallic materials typically experience significant strength degradation at elevated temperatures. Traditional strengthening methods, which rely on thermally stable particle dispersion, exhibit limited effectiveness owing to the challenges in suppressing activated dislocation motion. This work introduces a novel strategy for achieving exceptional high-temperature through nanoscale eutectic cellular network (ECN) enabled by additive manufacturing. A near-eutectic...
Abstract In this work, we extend the quasiparticle model to include chemical potential dependence of coupling constant g and consider density-dependent bag $$B_m$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>B</mml:mi> <mml:mi>m</mml:mi> </mml:msub> </mml:math> in order satisfy asymptotic freedom feature. By satisfying absolutely stable condition at zero temperature, draw stability region strange quark matter (SQM) describe recently discovered pulsars PSR...
Abstract We investigate the thermodynamical properties of color-flavor locked (CFL) quark matter at zero temperature, finite and strong magnetic field by using quasiparticle model. find that considering CFL phase can significantly change equation state (EOS) as well in stars (QSs) temperature or under within In particular, our results have shown we provide large QSs from model satisfying both upper limit $$\Lambda _{1.4}<800$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">...
Using the very recently reported mass of PSR J0740+6620 together with data finite nuclei and constraints on equation state symmetric nuclear matter at suprasaturation densities from flow in heavy-ion collisions, we show that symmetry energy Esym(n) cannot be supersoft so it becomes negative neutron stars (NSs) thus may make NS have a pure core. This is contrast to fact using 2.01 ± 0.04M⊙ J0348+0432 as maximum rule out high-density Esym(n). Furthermore, find stiffer based existence 2.14M⊙...
We investigate the isospin properties of strange quark matter (SQM) and stars (QSs) in framework isospin-dependent confining (ICQM) model confined-isospin density-dependent mass (CIDDM) model. Within these two phenomenological models, we study symmetry energy, stability matter, fractions, asymmetry, asymmetry SQM, mass-radius relation stars. find that including dependence can significantly influence matter. Recently, LIGO-Virgo collaboration reported their detection gravitational wave (GW)...
Within a confining quark matter model which considers phenomenologically the confinement and asymptotic freedom as well chiral symmetry restoration deconfinement at high baryon density, we find that if up-down ($ud$QM) is more stable than nuclear strange (SQM), maximum mass of static stars with $ud$QM $2.87M_{\odot}$ under agreement both constraints on star tidal deformability from gravitational wave signal GW170817 mass-radius PSR J0030+0451 J0740+6620 measured by NICER. In contrast,...
Abstract We present detailed forecasts for the constraints on characteristics of primordial magnetic fields (PMFs) generated prior to recombination that will be obtained with LiteBIRD satellite. The are driven by some main physical effects PMFs CMB anisotropies: gravitational magnetically-induced perturbations; thermal and ionization history Universe; Faraday rotation imprint polarization spectra; non-Gaussianities induced in anisotropies. represents a sensitive probe PMFs. explore different...
Based on an extended Skyrme interaction that includes the terms in relative momenta up to sixth order, corresponding so-called pseudopotential next-to-next-to-next-to leading order (N3LO), we derive expressions of Hamiltonian density and single nucleon potential under general non-equilibrium conditions which can be applied transport model simulations heavy-ion collisions induced by neutron-rich nuclei. While conventional interactions, include second predict incorrect behavior as a function...
We study the thermodynamic properties of color-flavored-locked (CFL) quark matter in finite temperature and strong magnetic field cases within confined-isospin-density-dependent-mass model. find that considering CFL phase star (QS) can significantly influence equation state as well QSs at or under fields. In particular, our results indicate polytropic index becomes anisotropic fields decreases with increment mass different isentropic stages QSs.
Background Kabuki syndrome (KS) is a rare developmental disorder characterised by multiple congenital anomalies and intellectual disability. UTX (ubiquitously transcribed tetratricopeptide repeat, X chromosome), which encodes histone demethylase, one of the two major pathogenic risk genes for KS. Although disability key phenotype KS, role in cognitive function remains unclear. Currently, no targeted therapies are available Aims This study aimed to investigate how regulates cognition, explore...
Anti-epidermal growth factor receptor (EGFR) therapy–associated cutaneous toxicity is a syndrome characterized by papulopustular rash, local inflammation, folliculitis, and microbial infection, resulting in decrease quality of life dose interruption. However, no effective clinical intervention available for this adverse effect. Here, we report the atrophy dermal white adipose tissue (dWAT), highly plastic with various skin-specific functions, correlates rash occurrence exacerbation murine...
Transverse momentum ($p_{T}$) generation in relativistic heavy ion collisions is sensitive to the initial geometry and final-state bulk evolution. We demonstrate with hydrodynamic calculations that mean $p_T$ ratio ($R_{\langle p_{T}\rangle}$) between highly similar isobar $^{96}_{44}$Ru+$^{96}_{44}$Ru $^{96}_{40}$Zr+$^{96}_{40}$Zr insensitive evolution remains small difference nuclear structure (neutron skin deformation) Ru Zr nuclei.We further find deformation can produce an...