output
20152026
most citedNovel Bayesian neural network based approach for nuclear charge radii

80 citations

90 papers

nucl-ex2026

Indirect Measurement of the Factor for at Gamow Energies via the Trojan Horse Method with Near-0 degree Spectator Detection

Chengbo Li, Huiming Jia, Qungang Wen +8

The astrophysical S*(E) factor for the 12C+12C reaction within the Gamow window plays a pivotal role in modeling stellar carbon burning and explosive nucleosynthesis scenarios. How…

nucl-ex2026

measurement of the reaction at astrophysical energies via the Trojan horse method with quasi-free breakup

Chengbo Li, Huiming Jia, Qungang Wen +9

The 12C(12C,a)20Ne reaction at astrophysical energies is crucial for understanding the carbon burning process in massive star and explosive astrophysical scenarios like Type Ia sup…

cs.AI2026

SymDiag: Explainable Diagnosis for LLM Reasoning via Neuro-Symbolic Verification

Wenyao Cui, Huaping Zhang, Yongyi Huang +6

Large language models (LLMs) increasingly serve as data-driven reasoners, yet their chains-of-thought (CoT) can be unfaithful even when final answers are correct. Most existing ``v…

cs.RO2026

Disentangling Visuo-Tactile Foresight: Oracle-Guided Interface Discovery for World Action Models

Zihang Yao, Chaoyue Ding, Yingying Yu

Contact-rich manipulation remains challenging because successful control depends on physical interaction cues that are often weakly observable from vision alone. Recent tactile wor…

astro-ph.GA2026

The complex kinematics of the young stars orbiting the supermassive black hole in the Galactic center can be explained by the presence of an intermediate mass companion of Sgr A

Xiaochen Zheng, Long Wang, Douglas N. C. Lin +2

The sub-parsec proximity around the Sgr A supermassive black hole (SMBH) in the center of the Milky Way contains an inner cluster of eccentric S-stars with randomly oriente…

astro-ph.SR2026

GSC 08227-00723: An Unusually Large PSH Excess AH Pic Candidate

Xin Li, Yongkang Sun

Nova-like variables are high-accretion-rate cataclysmic variables (CVs) that, in contrast to dwarf novae, do not undergo outbursts caused by thermal-viscous instability. However, a…

gr-qc2026

High Sensitivity Methodologies to Detect Radio Band Gravitational Waves

Wei Hong, Peng He, Tong-Jie Zhang +2

Gravitational waves (GWs) can resonate with magnetic fields through the Gertsenshtein-Zeldovich effect, producing electromagnetic signals at the same frequency. In pulsar magnetosp…

astro-ph.HE2025★ 7 cited

SN 2022acko: a low-luminosity SNe IIP with signs of early circumstellar interaction

Lin Han, Zhang Jujia, Wang Xiaofeng +13

We present optical-ultraviolet photometry and optical spectra for the type II supernova (SN) 2022acko. The spectroscopic observations span phases from 1.5 to 60 days…

hep-ph2025

Effect of super-Gaussian pulse shape on pair production in chirped electric field with spatial inhomogeneity

Xiao-Ting Xu, Le-Le Chen, Rong-an Tang +3

Pair production in spatially inhomogeneous chirped electric fields with super-Gaussian pulse shape is investigated using the Dirac-Heisenberg-Wigner formalism, and the effect of su…

physics.app-ph2025★ 2 cited

Magneto-photoelectrochemical 2D heterojunction platform for biosensing detection

Tao Wang, Nan Zhang, Hongjie Huang +12

Photoelectrochemical (PEC) biosensors exhibit significant potential for biomolecule detection due to their high sensitivity and low background noise. However, their performance is…

nucl-th2025★ 2 cited

Implication of shell quenching in scandium isotopes around N=20

Rong An, Xiang Jiang, Na Tang +2

Shell closure structures are commonly observed phenomena associated with nuclear charge radii throughout the nuclide chart. Inspired by recent studies demonstrating that the abrupt…

physics.flu-dyn2025★ 13 cited

Sensitivity of three-dimensional boundary-layer stability to intrinsic uncertainties of fluid properties: a study on supercritical CO2

Jie Ren, Yongxiang Wu, Xuerui Mao +2

The intrinsic uncertainty of fluid properties, including the equation of state, viscosity, and thermal conductivity, on boundary layer stability has scarcely been addressed. When a…

astro-ph.CO2025

Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks

Tianchi Zhang, Tianxiang Mao, Wenxiao Xu +1

The concentration of dark matter haloes is closely linked to their mass accretion history. We utilize the halo mass accretion histories from large cosmological N-body simulations a…

hep-ph2024★ 2 cited

Berry phase in axion physics, SM global structure, and generalized symmetries

Qing-Hong Cao, Shuailiang Ge, Yandong Liu +1

We investigate the Berry phase arising from axion-photon and axion-fermion interactions. The effective Hamiltonians in both systems share the same form, enabling a unified descript…

physics.soc-ph2024★ 4 cited

Continuous agent-based modeling of adult-child pairs based on a pseudo-energy: Relevance for public safety and egress efficiency

Chuan-Zhi Thomas Xie, Tie-Qiao Tang, Alexandre Nicolas

Pushes, falls, stampedes, and crushes are safety hazards that emerge from the collective motion of crowds, but might be avoided by better design and guidance. While pedestrian dyna…

astro-ph.HE2024★ 6 cited

Forecasting Supernova Observations with the CSST: I. Photometric Samples

Chengqi Liu, Youhua Xu, Xianmin Meng +8

The China Space Station Telescope (CSST, also known as Xuntian) is a serviceable two-meter-aperture wide-field telescope operating in the same orbit as the China Space Station. The…

hep-ph2024★ 6 cited

Distinguishing Dirac from Majorana Heavy Neutrino at Future Lepton Colliders

Qing-Hong Cao, Kun Cheng, Yandong Liu

We propose to identify whether a sterile neutrino is Dirac-type or Majorana-type by counting the peak of the rapidity distribution at lepton colliders. Our method requires only one…

nucl-th2023★ 13 cited

New quantification of symmetry energy from neutron skin thicknesses of Ca and Pb

Rong An, Shuai Sun, Li-Gang Cao +1

Precise knowledge of the nuclear symmetry energy can be tentatively calibrated through multimessenger constraints. The neutron skin thickness of a heavy nucleus is one of the most…

nucl-th2023★ 17 cited

Improved description of nuclear charge radii: Global trends beyond shell closure

Rong An, Xiang Jiang, Na Tang +2

Charge radii measured with high accuracy provide a stringent benchmark for characterizing nuclear structure phenomena. In this work, the systematic evolution of charge radii for nu…

astro-ph.GA2023★ 6 cited

Potential Impact of the Sagittarius Dwarf Galaxy on the Formation of Young O-rich Stars

Tiancheng Sun, Shaolan Bi, Xunzhou Chen +11

The Milky Way underwent significant transformations in its early history, characterised by violent mergers and satellite galaxy accretion. However, recent observations reveal notab…

astro-ph.HE2023★ 37 cited

Circumstellar Material Ejected Violently by A Massive Star Immediately before its Death

Jujia Zhang, Han Lin, Xiaofeng Wang +7

Type II supernovae represent the most common stellar explosions in the Universe, for which the final stage evolution of their hydrogen-rich massive progenitors towards core-collaps…

cond-mat.supr-con2023★ 25 cited

Pressure-induced Superconductivity and Topological Quantum Phase Transitions in the Topological Semimetal ZrTe2

Shihao Zhu, Juefei Wu, Peng Zhu +18

Topological transition metal dichalcogenides (TMDCs) have attracted much attention due to its potential applications in spintronics and quantum computations. In this work, we syste…

cond-mat.mes-hall2023★ 12 cited

Coupling of hole double quantum dot in planar germanium to a microwave cavity

Yuan Kang, Zong-Hu Li, Zhen-Zhen Kong +10

In recent years, notable progress has been made in the study of hole qubits in planar germanium, and circuit quantum electrodynamics (circuit QED) has emerged as a promising approa…

cond-mat.mes-hall2023★ 14 cited

Single spin qubit geometric gate in a silicon quantum dot

Rong-Long Ma, Ao-Ran Li, Chu Wang +11

Preserving qubit coherence and maintaining high-fidelity qubit control under complex noise environment is an enduring challenge for scalable quantum computing. Here we demonstrate…