2025 Vol. 49, No. 2
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2025, 49(2): 023001. doi: 10.1088/1674-1137/ad8baf
Abstract:
In this study, we employed the heavy quark expansion model with the kinetic scheme to evaluate\begin{document}$ \alpha_S(m_c^2) $\end{document} ![]()
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, the strong coupling constant at the charm quark mass \begin{document}$ m_c $\end{document} ![]()
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, using data o...
In this study, we employed the heavy quark expansion model with the kinetic scheme to evaluate
2025, 49(2): 023101. doi: 10.1088/1674-1137/ad8ec2
Abstract:
The direct CP asymmetry in the weak decay process of hadrons is commonly attributed to the weak phase of the CKM matrix and the indeterminate strong phase. We propose a method to generate a significant phase difference through the interference betwee...
The direct CP asymmetry in the weak decay process of hadrons is commonly attributed to the weak phase of the CKM matrix and the indeterminate strong phase. We propose a method to generate a significant phase difference through the interference betwee...
2025, 49(2): 023102. doi: 10.1088/1674-1137/ad9259
Abstract:
The total cross sections of the process\begin{document}$ e^+ e^-\to \Lambda_c^+ \bar{\Lambda}_c^- $\end{document} ![]()
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close to the threshold are calculated within the vector meson dominance model. It is found that the theoretical results can describe th...
The total cross sections of the process
2025, 49(2): 023103. doi: 10.1088/1674-1137/ad9898
Abstract:
Two near-threshold peaking structures with spin-parities of\begin{document}$ J^{PC}=0^{++} $\end{document} ![]()
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were recently discovered by the LHCb Collaboration in the \begin{document}$ D_s^+D_s^- $\end{document} ![]()
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invariant mass distribution of the deca...
Two near-threshold peaking structures with spin-parities of
2025, 49(2): 023104. doi: 10.1088/1674-1137/ad8ec3
Abstract:
We investigated the ground state (1S), radially excited states (2S) and (3S), and orbitally excited state (1P) for the heavy charmonia (\begin{document}$ c \bar c $\end{document} ![]()
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) and bottomonia (\begin{document}$ b \bar b $\end{document} ![]()
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) mesons in ...
We investigated the ground state (1S), radially excited states (2S) and (3S), and orbitally excited state (1P) for the heavy charmonia (
2025, 49(2): 023105. doi: 10.1088/1674-1137/ad9893
Abstract:
This paper is the extension of our previous work entitled ''Searching a systematics for nonfactorizable contributions to\begin{document}$ {B^ - } $\end{document} ![]()
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and \begin{document}$ {\bar B^0} $\end{document} ![]()
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hadronic decays''. Obtaining the facto...
This paper is the extension of our previous work entitled ''Searching a systematics for nonfactorizable contributions to
2025, 49(2): 023106. doi: 10.1088/1674-1137/ad94e0
Abstract:
We present improved predictions of a class of event-shape distributions called angularity for a contribution from an effective operator\begin{document}$ H\to gg $\end{document} ![]()
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in Higgs hadronic decay that suffers from large perturbative uncertainti...
We present improved predictions of a class of event-shape distributions called angularity for a contribution from an effective operator
2025, 49(2): 023107. doi: 10.1088/1674-1137/ad9d1d
Abstract:
Precise determination of the Higgs boson self-couplings is essential for understanding the mechanism underlying electroweak symmetry breaking. However, owing to the limited number of Higgs boson pair events at the LHC, only loose constraints have bee...
Precise determination of the Higgs boson self-couplings is essential for understanding the mechanism underlying electroweak symmetry breaking. However, owing to the limited number of Higgs boson pair events at the LHC, only loose constraints have bee...
2025, 49(2): 023108. doi: 10.1088/1674-1137/ad99b1
Abstract:
Tsallis nonextensive statistics is applied to study the transport coefficients of strongly interacting matter within the Polyakov chiral\begin{document}$S U(3) $\end{document} ![]()
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quark mean field model (PCQMF). Nonextensivity is introduced within the P...
Tsallis nonextensive statistics is applied to study the transport coefficients of strongly interacting matter within the Polyakov chiral
2025, 49(2): 024101. doi: 10.1088/1674-1137/ad9016
Abstract:
We conduct a new investigation of the correlation at saturation (subsaturation) density between the density dependence of symmetry energy and the percentage of the energy-weighted sum rule (EWSR) exhausted by pygmy dipole resonances (PDR) in 68Ni and...
We conduct a new investigation of the correlation at saturation (subsaturation) density between the density dependence of symmetry energy and the percentage of the energy-weighted sum rule (EWSR) exhausted by pygmy dipole resonances (PDR) in 68Ni and...
2025, 49(2): 024102. doi: 10.1088/1674-1137/ad9146
Abstract:
The ground-state bands in the\begin{document}$ N=152 $\end{document} ![]()
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isotones 254No, 255Lr, and 256Rf are investigated using the cranked shell model (CSM), with pairing correlations treated via the particle-number-conserving (PNC) method. The experi...
The ground-state bands in the
2025, 49(2): 024103. doi: 10.1088/1674-1137/ad9895
Abstract:
Using the inelastic scattering of charmed strange mesons by open-charm mesons in hadronic matter produced in Pb-Pb collisions at the Large Hadron Collider, we study the production of\begin{document}$\psi (4040)$\end{document} ![]()
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, \begin{document}$\psi ...
Using the inelastic scattering of charmed strange mesons by open-charm mesons in hadronic matter produced in Pb-Pb collisions at the Large Hadron Collider, we study the production of
2025, 49(2): 024104. doi: 10.1088/1674-1137/ad8e40
Abstract:
This study investigated the tetrahedral structure in 80Zr and Lambda (Λ) impurity effect in\begin{document}$ ^{81}_{\; \Lambda} $\end{document} ![]()
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Zr using the multidimensionally constrained relativistic Hartree-Bogoliubov model. The ground states of bo...
This study investigated the tetrahedral structure in 80Zr and Lambda (Λ) impurity effect in
2025, 49(2): 024105. doi: 10.1088/1674-1137/ad99b0
Abstract:
Although a 3rd-order difference formula has often been employed to investigate the odd-even staggering (OES) in experimental cross sections, other formulas can also be very useful. In this work, three formulas, the 2nd, 4th, and 5th-order difference ...
Although a 3rd-order difference formula has often been employed to investigate the odd-even staggering (OES) in experimental cross sections, other formulas can also be very useful. In this work, three formulas, the 2nd, 4th, and 5th-order difference ...
2025, 49(2): 024106. doi: 10.1088/1674-1137/ad9f43
Abstract:
Assuming the equilibrium of the Quantum Chromodynamics (QCD) system, we investigate the critical behavior of the sixth-, eighth-, and tenth-order susceptibilities of the net-baryon number through mapping the results in the three-dimensional Ising mod...
Assuming the equilibrium of the Quantum Chromodynamics (QCD) system, we investigate the critical behavior of the sixth-, eighth-, and tenth-order susceptibilities of the net-baryon number through mapping the results in the three-dimensional Ising mod...
2025, 49(2): 025101. doi: 10.1088/1674-1137/ad8bb0
Abstract:
We investigate the accretion of Vlasov gas onto a static, spherically symmetric black hole (BH) influenced by the Kalb–Ramond (KR) field, focusing on the effects of Lorentz symmetry breaking (LSB) parameters. We employ the Maxwell–Jüttner distributio...
We investigate the accretion of Vlasov gas onto a static, spherically symmetric black hole (BH) influenced by the Kalb–Ramond (KR) field, focusing on the effects of Lorentz symmetry breaking (LSB) parameters. We employ the Maxwell–Jüttner distributio...
2025, 49(2): 025102. doi: 10.1088/1674-1137/ad873d
Abstract:
As a generalization of Einstein's theory, Horava-Lifshitz gravity has attracted significant interest owing to its healthy ultraviolet behavior. In this paper, we analyze the impact of the Horava-Lifshitz corrections on the gravitomagnetic field. We p...
As a generalization of Einstein's theory, Horava-Lifshitz gravity has attracted significant interest owing to its healthy ultraviolet behavior. In this paper, we analyze the impact of the Horava-Lifshitz corrections on the gravitomagnetic field. We p...
2025, 49(2): 025103. doi: 10.1088/1674-1137/ad9148
Abstract:
By incorporating first-order QED effects, we explored the shadows of Kerr-Newman black holes with a magnetic charge through the numerical backward ray-tracing method. Our investigation encompassed both the direct influence of the electromagnetic fiel...
By incorporating first-order QED effects, we explored the shadows of Kerr-Newman black holes with a magnetic charge through the numerical backward ray-tracing method. Our investigation encompassed both the direct influence of the electromagnetic fiel...
2025, 49(2): 025104. doi: 10.1088/1674-1137/ad9453
Abstract:
In this paper, we explore the quasinormal modes (QNMs) of a black hole surrounded by a fluid of strings within the framework of Rastall gravity. We analyze the behavior of scalar, electromagnetic, and gravitational perturbations, focusing on the infl...
In this paper, we explore the quasinormal modes (QNMs) of a black hole surrounded by a fluid of strings within the framework of Rastall gravity. We analyze the behavior of scalar, electromagnetic, and gravitational perturbations, focusing on the infl...
2025, 49(2): 025105. doi: 10.1088/1674-1137/ad972c
Abstract:
We investigate the second order energy density perturbation\begin{document}$ \delta^{(2)} $\end{document} ![]()
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induced by small-scale Gaussian and local-type non-Gaussian primordial curvature perturbations. The relative abundance of primordial black hole...
We investigate the second order energy density perturbation
2025, 49(2): 025106. doi: 10.1088/1674-1137/ad93b8
Abstract:
In this paper, we propose a method of fixing the leading behaviors of three dimensional geometries from the dual CFT2 entanglement entropies. We employ only the holographic principle and do not use any assumption about the AdS/CFT correspondence and ...
In this paper, we propose a method of fixing the leading behaviors of three dimensional geometries from the dual CFT2 entanglement entropies. We employ only the holographic principle and do not use any assumption about the AdS/CFT correspondence and ...
2025, 49(2): 025107. doi: 10.1088/1674-1137/ad9894
Abstract:
This manuscript investigates a Schwarzschild black hole surrounded by perfect fluid dark matter embedded in a cloud of strings. The effects of its surroundings on thermodynamics, timelike and null geodesics, shadows, and quasinormal modes are analyze...
This manuscript investigates a Schwarzschild black hole surrounded by perfect fluid dark matter embedded in a cloud of strings. The effects of its surroundings on thermodynamics, timelike and null geodesics, shadows, and quasinormal modes are analyze...
2025, 49(2): 025108. doi: 10.1088/1674-1137/ad93b7
Abstract:
In this paper, using Hamiltonian formalism, we obtain solutions for constant-roll inflation according to the noncommutativity and the non-minimal coupling field of the Lagrangian. We consider three different types of couplings: power-law, exponential...
In this paper, using Hamiltonian formalism, we obtain solutions for constant-roll inflation according to the noncommutativity and the non-minimal coupling field of the Lagrangian. We consider three different types of couplings: power-law, exponential...
2025, 49(2): 025109. doi: 10.1088/1674-1137/ad9899
Abstract:
A white hole is simply a region of spacetime described by general relativity. Black holes are often assumed to form through star collapses. Based on such an assumption, the white hole region does not present. Recent research on quantum gravity indica...
A white hole is simply a region of spacetime described by general relativity. Black holes are often assumed to form through star collapses. Based on such an assumption, the white hole region does not present. Recent research on quantum gravity indica...
2025, 49(2): 025110. doi: 10.1088/1674-1137/ad99b2
Abstract:
We investigated the impact of\begin{document}$f(R,L_m,T)$\end{document} ![]()
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gravity on the internal structure of compact stars, expecting this theory to manifest prominently in the high-density cores of such stars. We considered the algebraic function \...
We investigated the impact of
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