2024 Vol. 48, No. 4
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2024, 48(4): 041001. doi: 10.1088/1674-1137/ad2361
Abstract:
The attractive interaction between\begin{document}$ J/\psi $\end{document} ![]()
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and \begin{document}$ \psi(3770) $\end{document} ![]()
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has to be strong enough if X(6900) is of the molecule type. We argue that since \begin{document}$ \psi(3770) $\end{document} ![]()
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...
The attractive interaction between
2024, 48(4): 043001. doi: 10.1088/1674-1137/ad20d5
Abstract:
In this study, we conducted a search for dark matter using a part of the data recorded by the CMS experiment during run-I of the LHC in 2012 with a center of mass energy of 8 TeV and an integrated luminosity of 11.6 fb−1. These data were gathered fro...
In this study, we conducted a search for dark matter using a part of the data recorded by the CMS experiment during run-I of the LHC in 2012 with a center of mass energy of 8 TeV and an integrated luminosity of 11.6 fb−1. These data were gathered fro...
2024, 48(4): 043002. doi: 10.1088/1674-1137/ad1fe6
Abstract:
Luminosity monitoring at\begin{document}$ e^+e^- $\end{document} ![]()
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colliders was investigated using \begin{document}$\mathrm{SANC}$\end{document} ![]()
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Monte Carlo event generator \begin{document}$\mathrm{ReneSANCe}$\end{document} ![]()
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and integrator \begin{docu...
Luminosity monitoring at
2024, 48(4): 043003. doi: 10.1088/1674-1137/ad2675
Abstract:
In this study, the possibility of observing a solar neutrino background in a future neutrinoless double beta decay experiment using a high-pressure gaseous 82SeF6 TPC is investigated. Various contributions are simulated, and possible features that co...
In this study, the possibility of observing a solar neutrino background in a future neutrinoless double beta decay experiment using a high-pressure gaseous 82SeF6 TPC is investigated. Various contributions are simulated, and possible features that co...
2024, 48(4): 043101. doi: 10.1088/1674-1137/ad17b0
Abstract:
The leptonic di-flavor violation (LFV) processes\begin{document}$ \mu^\pm \mu^\pm \rightarrow e^\pm e^\pm $\end{document} ![]()
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and \begin{document}$ \mu^\pm \mu^\pm \rightarrow \tau^\pm \tau^\pm $\end{document} ![]()
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and leptonic di-number violation (LNV) proc...
The leptonic di-flavor violation (LFV) processes
2024, 48(4): 043102. doi: 10.1088/1674-1137/ad1a0b
Abstract:
Recently, the LHCb experimental group found an exotic state\begin{document}$ T^+_{cc} $\end{document} ![]()
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from the \begin{document}$ pp \to D^0D^0\pi^+ + X $\end{document} ![]()
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process. A key question is whether it is just a molecule or may have a confined t...
Recently, the LHCb experimental group found an exotic state
2024, 48(4): 043103. doi: 10.1088/1674-1137/ad25f5
Abstract:
We investigate the possibility of detecting the leptophilic gauge boson\begin{document}$ Z_x $\end{document} ![]()
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predicted by the \begin{document}$ U(1)_{L_e-L_\mu} $\end{document} ![]()
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model via the processes \begin{document}$ e^+e^-\rightarrow \ell^+\ell^-...
We investigate the possibility of detecting the leptophilic gauge boson
2024, 48(4): 043104. doi: 10.1088/1674-1137/ad205f
Abstract:
Employing a 4-form ansatz of 11-dimensional supergravity over a non-dynamical\begin{document}$AdS_4 \times S^7/Z_k$\end{document} ![]()
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background and setting the internal space as an \begin{document}$S^1$\end{document} ![]()
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Hopf fibration on \begin{document}$...
Employing a 4-form ansatz of 11-dimensional supergravity over a non-dynamical
2024, 48(4): 043105. doi: 10.1088/1674-1137/ad243e
Abstract:
In this study, we reanalyze the top-quark pair production at next-to-next-to-leading order (NNLO) in quantum chromodynamics (QCD) at future\begin{document}$ e^+e^- $\end{document} ![]()
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colliders using the Principle of Maximum Conformality (PMC) method. T...
In this study, we reanalyze the top-quark pair production at next-to-next-to-leading order (NNLO) in quantum chromodynamics (QCD) at future
2024, 48(4): 044001. doi: 10.1088/1674-1137/ad243f
Abstract:
Baryon numbers are theorized to be carried by valence quarks in the standard QCD picture of the baryon structure. Another theory proposed an alternative baryon number carrier, a non-perturbative Y-shaped configuration of the gluon field, called the b...
Baryon numbers are theorized to be carried by valence quarks in the standard QCD picture of the baryon structure. Another theory proposed an alternative baryon number carrier, a non-perturbative Y-shaped configuration of the gluon field, called the b...
2024, 48(4): 044101. doi: 10.1088/1674-1137/ad20d4
Abstract:
The influence of the tensor interaction of nucleons on the characteristics of neutron-rich silicon and nickel isotopes was studied in this work. Tensor forces are considered within the framework of the Hartree-Fock approach with the Skyrme interactio...
The influence of the tensor interaction of nucleons on the characteristics of neutron-rich silicon and nickel isotopes was studied in this work. Tensor forces are considered within the framework of the Hartree-Fock approach with the Skyrme interactio...
2024, 48(4): 044102. doi: 10.1088/1674-1137/ad243d
Abstract:
In this study, proton emission half-lives were investigated for deformed proton emitters with\begin{document}$ 53\leq Z \leq 83 $\end{document} ![]()
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based on the presented deformed Gamow-like model, where the deformation effect was included in the Coulom...
In this study, proton emission half-lives were investigated for deformed proton emitters with
2024, 48(4): 044103. doi: 10.1088/1674-1137/ad1fe3
Abstract:
This study explores the ground-state characteristics of neutron-rich sodium isotopes, encompassing two-neutron separation energies, root-mean-square radii, quadrupole moments of proton and neutron distributions, single-particle levels of bound and re...
This study explores the ground-state characteristics of neutron-rich sodium isotopes, encompassing two-neutron separation energies, root-mean-square radii, quadrupole moments of proton and neutron distributions, single-particle levels of bound and re...
Astrophysical S-factor and reaction rate for 15N(p,γ)16O within the modified potential cluster model

2024, 48(4): 044104. doi: 10.1088/1674-1137/ad1fe7
Abstract:
We study radiative\begin{document}$ p^{15} {\rm{N}}$\end{document} ![]()
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capture on the ground state of 16O at stellar energies within the framework of a modified potential cluster model (MPCM) with forbidden states, including low-lying resonances. The in...
We study radiative
2024, 48(4): 044105. doi: 10.1088/1674-1137/ad21e9
Abstract:
In this study, α-particle preformation factors in heavy and superheavy nuclei from 220Th to 294Og are investigated. By combing experimental α decay energies and half-lives, the α-particle preformation factors\begin{document}$ P_{\alpha} $\end{docu...
In this study, α-particle preformation factors in heavy and superheavy nuclei from 220Th to 294Og are investigated. By combing experimental α decay energies and half-lives, the α-particle preformation factors
2024, 48(4): 045101. doi: 10.1088/1674-1137/ad1cda
Abstract:
Cosmic rays can interact with the solar atmosphere and produce a slew of secondary messengers, making the Sun a bright gamma-ray source in the sky. Detailed observations with Fermi-LAT have shown that these interactions must be strongly affected by s...
Cosmic rays can interact with the solar atmosphere and produce a slew of secondary messengers, making the Sun a bright gamma-ray source in the sky. Detailed observations with Fermi-LAT have shown that these interactions must be strongly affected by s...
2024, 48(4): 045102. doi: 10.1088/1674-1137/ad1feb
Abstract:
In this study, we investigated the astronomical implications of Rastall gravity, particularly its behavior amidst a radiation field compared to Reissner-Nordström (RN) black holes. We found a crucial correlation between the dynamics of the accretion ...
In this study, we investigated the astronomical implications of Rastall gravity, particularly its behavior amidst a radiation field compared to Reissner-Nordström (RN) black holes. We found a crucial correlation between the dynamics of the accretion ...
2024, 48(4): 045103. doi: 10.1088/1674-1137/ad1b3c
Abstract:
The CNO cycle is the main source of energy in stars more massive than our Sun. This process defines the energy production, the duration of which can be used to determine the lifetime of massive stars. The cycle is an important tool for determining th...
The CNO cycle is the main source of energy in stars more massive than our Sun. This process defines the energy production, the duration of which can be used to determine the lifetime of massive stars. The cycle is an important tool for determining th...
2024, 48(4): 045104. doi: 10.1088/1674-1137/ad1dcd
Abstract:
In this paper, we propose a hybrid metric Palatini approach in which the Palatini scalar curvature is non minimally coupled to the scalar field. We derive Einstein's field equations, i.e., the equations of motion of the scalar field. Furthermore, the...
In this paper, we propose a hybrid metric Palatini approach in which the Palatini scalar curvature is non minimally coupled to the scalar field. We derive Einstein's field equations, i.e., the equations of motion of the scalar field. Furthermore, the...
2024, 48(4): 045105. doi: 10.1088/1674-1137/ad2360
Abstract:
In this paper, we present several explicit reconstructions for the aether scalar tensor (AeST) theory derived from the background of the Friedmann-Lemaître-Robertson-Walker cosmological evolution. It is shown that the Einstein-Hilbert Lagrangian with...
In this paper, we present several explicit reconstructions for the aether scalar tensor (AeST) theory derived from the background of the Friedmann-Lemaître-Robertson-Walker cosmological evolution. It is shown that the Einstein-Hilbert Lagrangian with...
2024, 48(4): 045106. doi: 10.1088/1674-1137/ad2b4f
Abstract:
We discuss the gravitational wave (GW) spectra predicted from the electroweak scalegenesis of the Higgs portal type with a large number of dark chiral flavors, which many flavor QCD would underlie and give the dynamical explanation of the negative Hi...
We discuss the gravitational wave (GW) spectra predicted from the electroweak scalegenesis of the Higgs portal type with a large number of dark chiral flavors, which many flavor QCD would underlie and give the dynamical explanation of the negative Hi...
2024, 48(4): 045107. doi: 10.1088/1674-1137/ad260a
Abstract:
The study of Kerr geodesics has a long history, particularly for those occurring within the equatorial plane, which are generally well-understood. However, when compared with the classification introduced by one of the authors [Phys. Rev. D 105, 0240...
The study of Kerr geodesics has a long history, particularly for those occurring within the equatorial plane, which are generally well-understood. However, when compared with the classification introduced by one of the authors [Phys. Rev. D 105, 0240...
2024, 48(4): 045108. doi: 10.1088/1674-1137/ad2a5f
Abstract:
Glitches represent a category of non-Gaussian and transient noise that frequently intersects with gravitational wave (GW) signals, thereby exerting a notable impact on the processing of GW data. The inference of GW parameters, crucial for GW astronom...
Glitches represent a category of non-Gaussian and transient noise that frequently intersects with gravitational wave (GW) signals, thereby exerting a notable impact on the processing of GW data. The inference of GW parameters, crucial for GW astronom...
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