2024 Vol. 48, No. 6
Display Method: |
			            2024, 48(6): 063001. doi: 10.1088/1674-1137/ad3943 
	   					
		        	
			        
		            	
		        
					Abstract: 
Particle\begin{document}$ \chi_{c0}(3915) $\end{document} ![]()
![]()
\begin{document}$ \omega J/\psi $\end{document} ![]()
![]()
\begin{document}$ B\to K\omega J/\psi $\end{document} ![]()
![]()
\begin{document}$ \gamma\gamma\to\omega J/\psi $\end{document} ![]()
![]()
\begin{document}$ B\to K\omega J/\psi $\end{document} ![]()
![]()
\begin{document}$ \chi_{c0}(3915) $\end{document} ![]()
![]()
\begin{document}$ \omega J/\psi $\end{document} ![]()
![]()
\begin{document}$ \chi_{c0}(3915) $\end{document} ![]()
![]()
\begin{document}$ M=3920.9\pm0.9 $\end{document} ![]()
![]()
\begin{document}$ c^2 $\end{document} ![]()
![]()
\begin{document}$ \Gamma=18.2\pm2.4 $\end{document} ![]()
![]()
		       
		        
		        Particle
			            2024, 48(6): 063101. doi: 10.1088/1674-1137/ad2f22 
	   					
		        	
			        
		            	
		        
					Abstract: 
The finite mass of the heavy quark suppresses the collimated radiations; this is generally referred to as the dead cone effect. In this paper, we study the distribution of hadron multiplicity over the hadron opening angle with respect to the jet axis for various jet flavors. The corresponding measurement can be the most straightforward and simplest approach to explore the dynamical evolution of the radiations in the corresponding jet, which can expose the mass effect. We also propose a transverse energy-weighted angular distribution, which sheds light on the interplay between perturbative and non-perturbative effects in the radiation. Through Monte-Carlo simulations, our calculations show that the dead cone effect can be clearly observed by finding the ratio between the b and light-quark (inclusive) jets; this is expected to be measured at the LHC in the future.
		       
		        
		        
		        
			  
			The finite mass of the heavy quark suppresses the collimated radiations; this is generally referred to as the dead cone effect. In this paper, we study the distribution of hadron multiplicity over the hadron opening angle with respect to the jet axis for various jet flavors. The corresponding measurement can be the most straightforward and simplest approach to explore the dynamical evolution of the radiations in the corresponding jet, which can expose the mass effect. We also propose a transverse energy-weighted angular distribution, which sheds light on the interplay between perturbative and non-perturbative effects in the radiation. Through Monte-Carlo simulations, our calculations show that the dead cone effect can be clearly observed by finding the ratio between the b and light-quark (inclusive) jets; this is expected to be measured at the LHC in the future.
			            2024, 48(6): 063102. doi: 10.1088/1674-1137/ad2f23 
	   					
		        	
			        
		            	
		        
					Abstract: 
We constructed a gauge\begin{document}$ B-L $\end{document} ![]()
![]()
\begin{document}$ D_4\times Z_4\times Z_2 $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			We constructed a gauge
			            2024, 48(6): 063103. doi: 10.1088/1674-1137/ad305f 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, the spectroscopic parameters of exotic molecular states composed of mesons containing two heavy quarks (scalar - axial and pseudoscalar - axial meson combinations) are investigated within the QCD sum rules. Our findings reveal that molecular states containing charm quarks do not form bound states, whereas states with b-quarks can form exotic molecular states. This observation has significant implications for understanding the structure of these exotic states.
		       
		        
		        
		        
			  
			In this study, the spectroscopic parameters of exotic molecular states composed of mesons containing two heavy quarks (scalar - axial and pseudoscalar - axial meson combinations) are investigated within the QCD sum rules. Our findings reveal that molecular states containing charm quarks do not form bound states, whereas states with b-quarks can form exotic molecular states. This observation has significant implications for understanding the structure of these exotic states.
			            2024, 48(6): 063104. doi: 10.1088/1674-1137/ad305d 
	   					
		        	
			        
		            	
		        
					Abstract: 
An approximated solution for the gluon distribution from DGLAP evolution equations with the NLO splitting function in the small-x limit is presented. We first obtain simplified forms of the LO and NLO splitting functions in the small-x limit. With these approximated splitting functions, we obtain the analytical gluon distribution using the Mellin transform. The free parameters in the boundary conditions are obtained by fitting the CJ15 gluon distribution data. We find that the asymptotic behavior of the gluon distribution is consistent with the CJ15 data; however, the NLO results considering the "ladder" structure of gluon emission are slightly better than the LO results. These results indicate that the corrections from NLO have a significant influence on the behavior of the gluon distribution in the small-x region. In addition, we investigate the DGLAP evolution of the proton structure function using the analytical solution of the gluon distribution. The differential structure function reveals that our results have a similar tendency to the CJ15 data at small-x.
		       
		        
		        
		        
			  
			An approximated solution for the gluon distribution from DGLAP evolution equations with the NLO splitting function in the small-x limit is presented. We first obtain simplified forms of the LO and NLO splitting functions in the small-x limit. With these approximated splitting functions, we obtain the analytical gluon distribution using the Mellin transform. The free parameters in the boundary conditions are obtained by fitting the CJ15 gluon distribution data. We find that the asymptotic behavior of the gluon distribution is consistent with the CJ15 data; however, the NLO results considering the "ladder" structure of gluon emission are slightly better than the LO results. These results indicate that the corrections from NLO have a significant influence on the behavior of the gluon distribution in the small-x region. In addition, we investigate the DGLAP evolution of the proton structure function using the analytical solution of the gluon distribution. The differential structure function reveals that our results have a similar tendency to the CJ15 data at small-x.
			            2024, 48(6): 063105. doi: 10.1088/1674-1137/ad33be 
	   					
		        	
			        
		            	
		        
					Abstract: 
This study aims to investigate Lorentz/U(1) gauge symmetry-breaking electrodynamics in the framework of the standard-model extension and analyze the Hamiltonian structure for the theory with a specific dimension\begin{document}$ d\leq 4 $\end{document} ![]()
![]()
\begin{document}$ d\leq 4 $\end{document} ![]()
![]()
		       
		        
		        
			  
			This study aims to investigate Lorentz/U(1) gauge symmetry-breaking electrodynamics in the framework of the standard-model extension and analyze the Hamiltonian structure for the theory with a specific dimension
			            2024, 48(6): 063106. doi: 10.1088/1674-1137/ad2362 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, we systematically investigate collider constraints on effective interactions between Dark Matter (DM) particles and electroweak gauge bosons. We consider the simplified models in which scalar or Dirac fermion DM candidates couple only to electroweak gauge bosons through high dimensional effective operators. Considering the induced DM-quarks and DM-gluons operators from the Renormalization Group Evolution (RGE) running effect, we present comprehensive constraints on the effective energy scale Λ and Wilson coefficients\begin{document}$ C_B(\Lambda),\,C_W(\Lambda) $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			In this study, we systematically investigate collider constraints on effective interactions between Dark Matter (DM) particles and electroweak gauge bosons. We consider the simplified models in which scalar or Dirac fermion DM candidates couple only to electroweak gauge bosons through high dimensional effective operators. Considering the induced DM-quarks and DM-gluons operators from the Renormalization Group Evolution (RGE) running effect, we present comprehensive constraints on the effective energy scale Λ and Wilson coefficients
			            2024, 48(6): 063107. doi: 10.1088/1674-1137/ad30f0 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this paper, we investigate the charmed meson rare decay process\begin{document}$ D^+ \to \pi^+\nu\bar\nu $\end{document} ![]()
![]()
\begin{document}$ \langle\xi_{2;\pi}^n\rangle|_\mu $\end{document} ![]()
![]()
\begin{document}$ \langle \xi_{3;\pi}^{(p,\sigma),n}\rangle|_\mu $\end{document} ![]()
![]()
\begin{document}$ D\to \pi $\end{document} ![]()
![]()
\begin{document}$ f_+^{D\to\pi}(0) = 0.627^{+0.120}_{-0.080} $\end{document} ![]()
![]()
\begin{document}$ z(q^2,t) $\end{document} ![]()
![]()
\begin{document}$ D^+ \to \pi^+ \nu\bar\nu $\end{document} ![]()
![]()
\begin{document}$ \bar D^0 \to \pi^+ e\bar \nu_e $\end{document} ![]()
![]()
\begin{document}$ \bar D^0 \to \pi^+ e\bar \nu_e $\end{document} ![]()
![]()
\begin{document}$ {\cal B}(\bar D^0\to\pi^+e\bar\nu_e) = 0.308^{+0.155}_{-0.066} \times 10^{2} $\end{document} ![]()
![]()
\begin{document}$ \bar D^0\to\pi^+e\bar\nu_e $\end{document} ![]()
![]()
\begin{document}$ q^2 $\end{document} ![]()
![]()
\begin{document}$ D^+ \to \pi^+ \nu\bar\nu $\end{document} ![]()
![]()
\begin{document}${\cal B}(D^+ \to \pi^+ {\nu }{\bar\nu}) = $\end{document} ![]()
![]()
\begin{document}$  1.85^{+0.93}_{-0.46}\times10^{-8}$\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			In this paper, we investigate the charmed meson rare decay process
			            2024, 48(6): 063108. doi: 10.1088/1674-1137/ad34be 
	   					
		        	
			        
		            	
		        
					Abstract: 
Motivated by our previous study [Phys. Rev. D 104(1), 016021 (2021)] on the pionic leading-twist distribution amplitude (DA), we revisit the ρ-meson leading-twist longitudinal DA\begin{document}$ \phi_{2;\rho}^\|(x,\mu) $\end{document} ![]()
![]()
\begin{document}$ \phi_{2;\rho}^\|(x,\mu) $\end{document} ![]()
![]()
\begin{document}$ \phi_{2;\rho}^\|(x,\mu) $\end{document} ![]()
![]()
\begin{document}$ \mu = (1.0, 1.4, 2.0, 3.0)\; {\rm GeV} $\end{document} ![]()
![]()
\begin{document}$ \mu = 1\; {\rm GeV} $\end{document} ![]()
![]()
\begin{document}$ \langle\xi^2\rangle_{2;\rho}^\| = 0.220(6)  $\end{document} ![]()
![]()
\begin{document}$ \langle\xi^4\rangle_{2;\rho}^\| = 0.103(4) $\end{document} ![]()
![]()
\begin{document}$ \langle\xi^6\rangle_{2;\rho}^\| = 0.066(5) $\end{document} ![]()
![]()
\begin{document}$ \langle\xi^8\rangle_{2;\rho}^\| = 0.046(4) $\end{document} ![]()
![]()
\begin{document}$ \langle\xi^{10}\rangle_{2;\rho}^\| = 0.035(3) $\end{document} ![]()
![]()
\begin{document}$ \phi_{2;\rho}^\|(x,\mu) $\end{document} ![]()
![]()
\begin{document}$ A_1(0) = 0.498^{+0.014}_{-0.012} $\end{document} ![]()
![]()
\begin{document}$ A_2(0)=0.460^{+0.055}_{-0.047} $\end{document} ![]()
![]()
\begin{document}$ V(0) = 0.800^{+0.015}_{-0.014} $\end{document} ![]()
![]()
\begin{document}$ r_2 = 0.923^{+0.133}_{-0.119} $\end{document} ![]()
![]()
\begin{document}$ r_V = 1.607^{+0.071}_{-0.071} $\end{document} ![]()
![]()
\begin{document}$ z(t) $\end{document} ![]()
![]()
\begin{document}$ |V_{cd}| $\end{document} ![]()
![]()
\begin{document}$ D\to\rho\ell^+\nu_\ell $\end{document} ![]()
![]()
\begin{document}$ \mathcal{B}(D^0\to \rho^- e^+ \nu_e) = 1.825^{+0.170}_{-0.162}\pm 0.004 $\end{document} ![]()
![]()
\begin{document}$\mathcal{B}(D^+ \to \rho^0 e^+ \nu_e) = $\end{document} ![]()
![]()
\begin{document}$ 2.299^{+0.214}_{-0.204}\pm 0.011$\end{document} ![]()
![]()
\begin{document}$ \mathcal{B}(D^0\to \rho^- \mu^+ \nu_\mu) = 1.816^{+0.168}_{-0.160}\pm 0.004 $\end{document} ![]()
![]()
\begin{document}$\mathcal{B}(D^+ \to \rho^0 \mu^+ \nu_\mu) =2.288^{+0.212}_{-0.201}  \pm 0.011$\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			Motivated by our previous study [Phys. Rev. D 104(1), 016021 (2021)] on the pionic leading-twist distribution amplitude (DA), we revisit the ρ-meson leading-twist longitudinal DA
			            2024, 48(6): 063109. doi: 10.1088/1674-1137/ad34c4 
	   					
		        	
			        
		            	
		        
					Abstract: 
We studied the spectrum and rearrangement decays of S-wave\begin{document}$ cs\bar{c}\bar{s} $\end{document} ![]()
![]()
\begin{document}$ X(4140) $\end{document} ![]()
![]()
\begin{document}$ 1^{++} \;\; cs\bar{c}\bar{s} $\end{document} ![]()
![]()
\begin{document}$ X(3960) $\end{document} ![]()
![]()
\begin{document}$ 0^{++} \;\; cs\bar{c}\bar{s} $\end{document} ![]()
![]()
\begin{document}$ X_0(4140) $\end{document} ![]()
![]()
\begin{document}$ 0^{++} \;\; cs\bar{c}\bar{s} $\end{document} ![]()
![]()
\begin{document}$ cs\bar{c}\bar{s} $\end{document} ![]()
![]()
\begin{document}$ J^{PC}=1^{+-} $\end{document} ![]()
![]()
\begin{document}$ 0^{++} $\end{document} ![]()
![]()
\begin{document}$ 2^{++} $\end{document} ![]()
![]()
		       
		        
		        We studied the spectrum and rearrangement decays of S-wave
			            2024, 48(6): 064001. doi: 10.1088/1674-1137/ad2dc3 
	   					
		        	
			        
		            	
		        
					Abstract: 
TALYS calculations were performed to obtain the theoretical proton capture cross-sections on the p-nuclei. A short review on the status of related experimental studies was also conducted. Some basic properties such as Q-values, Coulomb barrier, Gamow peak, Gamow Window, and decay properties of the parent and daughter nuclei were studied. Various experimental parameters, e.g., beam energy, beam current, targets, and detectors, used in experimental investigations reported in the literature, were tabulated. The results of the TALYS calculations in the Gamow region were compared with the corresponding experimental values wherever available. This study is expected to facilitate the planning of future experiments.
		       
		        
		        
		        
			  
			TALYS calculations were performed to obtain the theoretical proton capture cross-sections on the p-nuclei. A short review on the status of related experimental studies was also conducted. Some basic properties such as Q-values, Coulomb barrier, Gamow peak, Gamow Window, and decay properties of the parent and daughter nuclei were studied. Various experimental parameters, e.g., beam energy, beam current, targets, and detectors, used in experimental investigations reported in the literature, were tabulated. The results of the TALYS calculations in the Gamow region were compared with the corresponding experimental values wherever available. This study is expected to facilitate the planning of future experiments.
			            2024, 48(6): 064002. doi: 10.1088/1674-1137/ad361a 
	   					
		        	
			        
		            	
		        
					Abstract: 
The complete-fusion reaction 204Pb(48Ca,2n)250No was used to study two activities of 250No with distinct half-lives. A total of 1357 events were observed in the SFiNx neutron detection system. The average number of neutrons emitted per spontaneous fission of 250No was determined to be\begin{document}$ (4.1 \pm 0.1) $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			The complete-fusion reaction 204Pb(48Ca,2n)250No was used to study two activities of 250No with distinct half-lives. A total of 1357 events were observed in the SFiNx neutron detection system. The average number of neutrons emitted per spontaneous fission of 250No was determined to be
			            2024, 48(6): 064101. doi: 10.1088/1674-1137/ad30ef 
	   					
		        	
			        
		            	
		        
					Abstract: 
Cluster radioactivity is studied within the generalized liquid drop model (GLDM), in which the shell correction energy, pairing energy, and cluster preformation factor are considered. The calculations show significant improvements and can reproduce the experimental data within a factor of 8.04 after considering these physical effects. In addition, the systematic trend of the cluster preformation factors\begin{document}$ P_c $\end{document} ![]()
![]()
\begin{document}$ N_p N_n $\end{document} ![]()
![]()
\begin{document}$ \log_{10}{P_c} $\end{document} ![]()
![]()
\begin{document}$ N_p N_n $\end{document} ![]()
![]()
Phys. Rev. C 108, 014325 (2023) ], in which \begin{document}$ \log_{10}{P_c} $\end{document} ![]()
![]()
\begin{document}$ N_p N_n $\end{document} ![]()
![]()
\begin{document}$ \log_{10}{P_c} $\end{document} ![]()
![]()
\begin{document}$ N_p N_n $\end{document} ![]()
![]()
\begin{document}$ N_p N_n $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			Cluster radioactivity is studied within the generalized liquid drop model (GLDM), in which the shell correction energy, pairing energy, and cluster preformation factor are considered. The calculations show significant improvements and can reproduce the experimental data within a factor of 8.04 after considering these physical effects. In addition, the systematic trend of the cluster preformation factors
			            2024, 48(6): 064102. doi: 10.1088/1674-1137/ad305c 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, we systematically analyzed the ground state of uranium isotopes from 225 to 240. In our calculations, we used the covariant energy density functional of density-dependent meson exchange interaction (DD-ME2) with separable pairing interaction (TMR). Using the multiple deformation constraint, we calculated the potential energy surface (PES) of the uranium isotopes for both even-even and even-odd nuclei with quadrupole and octupole deformation. Based on our calculation and upon comparing the experimental data and Hartree-Fock-Bogoliubov calculations with Gogny D1S calculation data, the ground state of uranium isotopes with reflection-asymmetric deformation was found to be preferred.
		       
		        
		        
		        
			  
			In this study, we systematically analyzed the ground state of uranium isotopes from 225 to 240. In our calculations, we used the covariant energy density functional of density-dependent meson exchange interaction (DD-ME2) with separable pairing interaction (TMR). Using the multiple deformation constraint, we calculated the potential energy surface (PES) of the uranium isotopes for both even-even and even-odd nuclei with quadrupole and octupole deformation. Based on our calculation and upon comparing the experimental data and Hartree-Fock-Bogoliubov calculations with Gogny D1S calculation data, the ground state of uranium isotopes with reflection-asymmetric deformation was found to be preferred.
			            2024, 48(6): 064103. doi: 10.1088/1674-1137/ad33bd 
	   					
		        	
			        
		            	
		        
					Abstract: 
Traditionally, isoscaling has been interpreted and applied within the framework of the grand canonical ensemble, based on the assumption that fragment production occurs following the attainment of a statistical equilibrium state. However, the influence of the symmetry energy can lead to differences in the neutron and density distribution in neutron-rich nuclei. This in turn may impact the isoscaling parameters (usually denoted by α and β). We examine the isoscaling properties for neutron-rich fragments produced in highly asymmetric systems on inverse kinematics, namely\begin{document}$ ^{40,48} $\end{document} ![]()
![]()
\begin{document}$ ^{58,64} $\end{document} ![]()
![]()
\begin{document}$ ^{9} $\end{document} ![]()
![]()
\begin{document}$ I \equiv N-Z $\end{document} ![]()
![]()
\begin{document}$ |\beta(N)| / \alpha(Z) $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			Traditionally, isoscaling has been interpreted and applied within the framework of the grand canonical ensemble, based on the assumption that fragment production occurs following the attainment of a statistical equilibrium state. However, the influence of the symmetry energy can lead to differences in the neutron and density distribution in neutron-rich nuclei. This in turn may impact the isoscaling parameters (usually denoted by α and β). We examine the isoscaling properties for neutron-rich fragments produced in highly asymmetric systems on inverse kinematics, namely
			            2024, 48(6): 064104. doi: 10.1088/1674-1137/ad2dc1 
	   					
		        	
			        
		            	
		        
					Abstract: 
Numerous experimental and theoretical observations have concluded that the probability of the three fragment emission (ternary fission) or binary fission increases when one proceeds towards the heavy mass region of nuclear periodic table. Many factors affect fragment emission, such as the shell effect, deformation, orientation, and fissility parameter. Binary and ternary fissions are observed for both ground and excited states of the nuclei. The collinear cluster tripartition (CCT) channel of the\begin{document}$ ^{235} $\end{document} ![]()
![]()
\begin{document}$^{\rm th}$\end{document} ![]()
![]()
\begin{document}$ ^{235} $\end{document} ![]()
![]()
\begin{document}$^{\rm th}$\end{document} ![]()
![]()
\begin{document}$ P_0 $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			Numerous experimental and theoretical observations have concluded that the probability of the three fragment emission (ternary fission) or binary fission increases when one proceeds towards the heavy mass region of nuclear periodic table. Many factors affect fragment emission, such as the shell effect, deformation, orientation, and fissility parameter. Binary and ternary fissions are observed for both ground and excited states of the nuclei. The collinear cluster tripartition (CCT) channel of the
			            2024, 48(6): 064105. doi: 10.1088/1674-1137/ad3814 
	   					
		        	
			        
		            	
		        
					Abstract: 
The recent measurements of neutron skins via parity violation in electron scattering have extracted an abnormally thick neutron skin for\begin{document}$ ^{208} $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			The recent measurements of neutron skins via parity violation in electron scattering have extracted an abnormally thick neutron skin for
			            2024, 48(6): 064106. doi: 10.1088/1674-1137/ad361d 
	   					
		        	
			        
		            	
		        
					Abstract: 
Accurately determining the quadrupole deformation parameters of atomic nuclei is crucial for understanding their structural and dynamic properties. This study introduces an innovative approach that combines transfer learning techniques with neural networks to predict the quadrupole deformation parameters of even-even nuclei. With the application of this innovative technique, the quadrupole deformation parameters of 2331 even-even nuclei are successfully predicted within the nuclear region defined by proton numbers\begin{document}$8 \leq Z \leq 134 $\end{document} ![]()
![]()
\begin{document}$N \geq 8$\end{document} ![]()
![]()
\begin{document}$^{48}{\rm{Ca}} + ^{244}{\rm{Pu}}$\end{document} ![]()
![]()
\begin{document}$^{48}{\rm{Ca}} + ^{248}{\rm{Cm}}$\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			Accurately determining the quadrupole deformation parameters of atomic nuclei is crucial for understanding their structural and dynamic properties. This study introduces an innovative approach that combines transfer learning techniques with neural networks to predict the quadrupole deformation parameters of even-even nuclei. With the application of this innovative technique, the quadrupole deformation parameters of 2331 even-even nuclei are successfully predicted within the nuclear region defined by proton numbers
			            2024, 48(6): 065001. doi: 10.1088/1674-1137/ad2e82 
	   					
		        	
			        
		            	
		        
					Abstract: 
The full array of the Large High Altitude Air Shower Observatory (LHAASO) has been in operation since July 2021. For its kilometer-square array (KM2A), we optimized the selection criteria for very high and ultra-high energy γ-rays using data collected from August 2021 to August 2022, resulting in an improvement in significance of the detection in the Crab Nebula of approximately 15%, compared with that of previous cuts. With the implementation of these new selection criteria, the angular resolution was also significantly improved by approximately 10% at tens of TeV. Other aspects of the full KM2A array performance, such as the pointing error, were also calibrated using the Crab Nebula. The resulting energy spectrum of the Crab Nebula in the energy range of 10-1000 TeV are well fitted by a log-parabola model, which is consistent with the previous results from LHAASO and other experiments.
		       
		        
		        
		        
			  
			The full array of the Large High Altitude Air Shower Observatory (LHAASO) has been in operation since July 2021. For its kilometer-square array (KM2A), we optimized the selection criteria for very high and ultra-high energy γ-rays using data collected from August 2021 to August 2022, resulting in an improvement in significance of the detection in the Crab Nebula of approximately 15%, compared with that of previous cuts. With the implementation of these new selection criteria, the angular resolution was also significantly improved by approximately 10% at tens of TeV. Other aspects of the full KM2A array performance, such as the pointing error, were also calibrated using the Crab Nebula. The resulting energy spectrum of the Crab Nebula in the energy range of 10-1000 TeV are well fitted by a log-parabola model, which is consistent with the previous results from LHAASO and other experiments.
			            2024, 48(6): 065101. doi: 10.1088/1674-1137/ad32c0 
	   					
		        	
			        
		            	
		        
					Abstract: 
By considering the concept of a unified single fluid model, referred to as modified Chaplygin gas (MCG), which amalgamates dark energy and dark matter, we explore the thermodynamic characteristics of charged anti-de Sitter (AdS) black holes existing in an unconventional fluid accompanied by MCG. To accomplish this objective, we derive the equations of state by regarding the charge\begin{document}$ Q^{2} $\end{document} ![]()
![]()
\begin{document}$ \psi_{c} $\end{document} ![]()
![]()
\begin{document}$ T_{c} $\end{document} ![]()
![]()
\begin{document}$ Q_{c}^{2} $\end{document} ![]()
![]()
\begin{document}$ Q^{2}-\psi $\end{document} ![]()
![]()
\begin{document}$\dfrac{T_{\min}}{T_{c}}$\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			By considering the concept of a unified single fluid model, referred to as modified Chaplygin gas (MCG), which amalgamates dark energy and dark matter, we explore the thermodynamic characteristics of charged anti-de Sitter (AdS) black holes existing in an unconventional fluid accompanied by MCG. To accomplish this objective, we derive the equations of state by regarding the charge
			            2024, 48(6): 065102. doi: 10.1088/1674-1137/ad34c0 
	   					
		        	
			        
		            	
		        
					Abstract: 
Recently, the emergence of cosmological tension has raised doubts about the consistency of the ΛCDM model. To constrain the neutrino mass within a consistent cosmological framework, we investigate three massive neutrinos with normal hierarchy (NH) and inverted hierarchy (IH) in both the axion-like early dark energy (Axi-EDE) and AdS-EDE models. We use joint datasets including the cosmic microwave background power spectrum from Planck 2018, Pantheon of type Ia supernova, baryon acoustic oscillation, and\begin{document}$ H_0 $\end{document} ![]()
![]()
\begin{document}$\sum m_{\nu,\mathrm{NH}}$\end{document} ![]()
![]()
\begin{document}$\sum m_{\nu,\mathrm{IH}}$\end{document} ![]()
![]()
\begin{document}$\sum m_{\nu,\mathrm{NH}}$\end{document} ![]()
![]()
\begin{document}$\sum m_{\nu,\mathrm{IH}}  $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			Recently, the emergence of cosmological tension has raised doubts about the consistency of the ΛCDM model. To constrain the neutrino mass within a consistent cosmological framework, we investigate three massive neutrinos with normal hierarchy (NH) and inverted hierarchy (IH) in both the axion-like early dark energy (Axi-EDE) and AdS-EDE models. We use joint datasets including the cosmic microwave background power spectrum from Planck 2018, Pantheon of type Ia supernova, baryon acoustic oscillation, and
			            2024, 48(6): 065103. doi: 10.1088/1674-1137/ad34c2 
	   					
		        	
			        
		            	
		        
					Abstract: 
In the frequency band of the Laser Interferometer Space Antenna (LISA), extensive research has been conducted on the impact of foreground confusion noise generated by galactic binaries within the Milky Way Galaxy. Additionally, recent evidence of a stochastic signal, announced by the NANOGrav, EPTA, PPTA, CPTA, and InPTA, indicates that the stochastic gravitational-wave background (SGWB) generated by supermassive black hole binaries (SMBHBs) can contribute strong background noise within the LISA band. Given the presence of such strong noise, it is expected to have significant impacts on LISA's scientific missions. In this study, we investigate the impacts of the SGWB generated by SMBHBs on the detection of individual massive black hole binaries, verified galactic binaries, and extreme mass ratio inspirals in the context of LISA. We find it essential to resolve and eliminate the excess noise from the SGWB to guarantee the success of LISA's missions.
		       
		        
		        
		        
			  
			In the frequency band of the Laser Interferometer Space Antenna (LISA), extensive research has been conducted on the impact of foreground confusion noise generated by galactic binaries within the Milky Way Galaxy. Additionally, recent evidence of a stochastic signal, announced by the NANOGrav, EPTA, PPTA, CPTA, and InPTA, indicates that the stochastic gravitational-wave background (SGWB) generated by supermassive black hole binaries (SMBHBs) can contribute strong background noise within the LISA band. Given the presence of such strong noise, it is expected to have significant impacts on LISA's scientific missions. In this study, we investigate the impacts of the SGWB generated by SMBHBs on the detection of individual massive black hole binaries, verified galactic binaries, and extreme mass ratio inspirals in the context of LISA. We find it essential to resolve and eliminate the excess noise from the SGWB to guarantee the success of LISA's missions.
			            2024, 48(6): 065104. doi: 10.1088/1674-1137/ad361c 
	   					
		        	
			        
		            	
		        
					Abstract: 
We study the dynamics of the critical collapse of a spherically symmetric scalar field. Approximate analytic expressions for the metric functions and matter field in the large-radius region are obtained. In the central region, owing to the boundary conditions, the equation of motion for the scalar field is reduced to the flat-spacetime form.
		       
		        
		        
		        
			  
			We study the dynamics of the critical collapse of a spherically symmetric scalar field. Approximate analytic expressions for the metric functions and matter field in the large-radius region are obtained. In the central region, owing to the boundary conditions, the equation of motion for the scalar field is reduced to the flat-spacetime form.
			            2024, 48(6): 065105. doi: 10.1088/1674-1137/ad34bf 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this work, the optical appearance of an asymmetric thin-shell wormhole with a Bardeen profile is studied. To initiate the process, we need to construct an asymmetric thin-shell wormhole utilizing the cut-and-paste technique proposed by Visser and subsequently ascertain its pertinent physical quantities such as the radius of the photon sphere and critical impact parameters for different values of magnetic charge g. Then, the effective potential and motion behavior of photons are also investigated within the framework of asymmetric thin-shell wormholes with a Bardeen profile. It can be found that the effective potential, ray trajectory, and azimuthal angle of the thin-shell wormhole exhibit a strong correlation with the mass ratio of black holes. By considering the accretion disk as the sole background light source, we observe additional photon rings and lensing bands in the optical appearance of the asymmetric thin-shell wormhole with a Bardeen profile compared to those exhibited by the Bardeen black hole. One can find that there is an increase in the size of the specific additional light bands with increasing magnetic charge g, which is different from the black hole case. These exceptionally luminous rings can serve as a robust criterion for the identification and characterization of the thin-shell wormhole spacetime.
		       
		        
		        
		        
			  
			In this work, the optical appearance of an asymmetric thin-shell wormhole with a Bardeen profile is studied. To initiate the process, we need to construct an asymmetric thin-shell wormhole utilizing the cut-and-paste technique proposed by Visser and subsequently ascertain its pertinent physical quantities such as the radius of the photon sphere and critical impact parameters for different values of magnetic charge g. Then, the effective potential and motion behavior of photons are also investigated within the framework of asymmetric thin-shell wormholes with a Bardeen profile. It can be found that the effective potential, ray trajectory, and azimuthal angle of the thin-shell wormhole exhibit a strong correlation with the mass ratio of black holes. By considering the accretion disk as the sole background light source, we observe additional photon rings and lensing bands in the optical appearance of the asymmetric thin-shell wormhole with a Bardeen profile compared to those exhibited by the Bardeen black hole. One can find that there is an increase in the size of the specific additional light bands with increasing magnetic charge g, which is different from the black hole case. These exceptionally luminous rings can serve as a robust criterion for the identification and characterization of the thin-shell wormhole spacetime.
			            2024, 48(6): 065106. doi: 10.1088/1674-1137/ad32be 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, we extend the surface growth approach for bulk reconstruction into the AdS spacetime with a boundary in the AdS/BCFT correspondence. We show that the geometry in the entanglement wedge with a boundary can be constructed from the direct growth of bulk extremal surfaces layer by layer. Furthermore, we observe that the surface growth configuration in BCFT can be connected with the defect multi scale entanglement renormalization ansatz (MERA) tensor network. Additionally, we investigate the entanglement of purification within the surface growth process, which not only reveals more refined structure of entanglement entropy in the entanglement wedge but also suggests a selection rule for surface growth in the bulk reconstruction.
		       
		        
		        
		        
			  
			In this study, we extend the surface growth approach for bulk reconstruction into the AdS spacetime with a boundary in the AdS/BCFT correspondence. We show that the geometry in the entanglement wedge with a boundary can be constructed from the direct growth of bulk extremal surfaces layer by layer. Furthermore, we observe that the surface growth configuration in BCFT can be connected with the defect multi scale entanglement renormalization ansatz (MERA) tensor network. Additionally, we investigate the entanglement of purification within the surface growth process, which not only reveals more refined structure of entanglement entropy in the entanglement wedge but also suggests a selection rule for surface growth in the bulk reconstruction.
			            2024, 48(6): 065107. doi: 10.1088/1674-1137/ad361e 
	   					
		        	
			        
		            	
		        
					Abstract: 
High-energy photons may oscillate with axion-like particles (ALPs) when they propagate through the Milky Way's magnetic field, resulting in an alteration in the observed photon energy spectrum. Ultra-high energy gamma-ray spectra, measured by the Large High Altitude Air Shower Observatory (LHAASO) up to\begin{document}$ {\cal{O}}(1)\; {\rm{PeV}} $\end{document} ![]()
![]()
\begin{document}$ g_{a\gamma} $\end{document} ![]()
![]()
\begin{document}$ 1.4\times 10^{-10} $\end{document} ![]()
![]()
\begin{document}$ {\rm GeV}^{-1} $\end{document} ![]()
![]()
\begin{document}$ \sim 4\times 10^{-7} \; {\rm{eV}} $\end{document} ![]()
![]()
\begin{document}$ 7.5\times 10^{-11} $\end{document} ![]()
![]()
\begin{document}$ {\rm GeV}^{-1} $\end{document} ![]()
![]()
\begin{document}$ \sim 4 \times 10^{-7}\; {\rm{eV}} $\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			High-energy photons may oscillate with axion-like particles (ALPs) when they propagate through the Milky Way's magnetic field, resulting in an alteration in the observed photon energy spectrum. Ultra-high energy gamma-ray spectra, measured by the Large High Altitude Air Shower Observatory (LHAASO) up to
			            2024, 48(6): 065108. doi: 10.1088/1674-1137/ad34bd 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this paper, we undertake a detailed study of real scalar inflation using LATTICEEASY simulations to investigate preheating phenomena. Generally, the scalar inflation potential with non-minimal coupling can be approximated using a quartic potential. We observe that the evolutionary behavior of this potential remains unaffected by the coupling coefficient. Furthermore, the theoretical predictions for the scalar spectral index (\begin{document}$n_s$\end{document} ![]()
![]()
\begin{document}$N_{\rm pre}$\end{document} ![]()
![]()
\begin{document}$n_s$\end{document} ![]()
![]()
		       
		        
		        
		        
			  
			In this paper, we undertake a detailed study of real scalar inflation using LATTICEEASY simulations to investigate preheating phenomena. Generally, the scalar inflation potential with non-minimal coupling can be approximated using a quartic potential. We observe that the evolutionary behavior of this potential remains unaffected by the coupling coefficient. Furthermore, the theoretical predictions for the scalar spectral index (
			            2024, 48(6): 065109. doi: 10.1088/1674-1137/ad361f 
	   					
		        	
			        
		            	
		        
					Abstract: 
We obtain an exact solution for spherically symmetric Letelier AdS black holes immersed in perfect fluid dark matter (PFDM). Considering the cosmological constant as the positive pressure of the system and volume as its conjugate variable, we analyze the thermodynamics of our black holes in the extended phase space. Owing to the background clouds of strings parameter (a) and the parameter endowed with PFDM (β), we analyze the Hawking temperature, entropy, and specific heat. Furthermore, we investigate the relationship between the photon sphere radius and phase transition for the Letelier AdS black holes immersed in PFDM. Through the analysis, with a particular condition, non-monotonic behaviors are found between the photon sphere radius, impact parameter, PFDM parameter, temperature, and pressure. We can regard the changes in both the photon sphere radius and impact parameter before and after phase transition as the order parameter; their critical exponents near the critical point are equal to the same value, 1/2, similar to that in ordinary thermal systems. This indicates that a universal relation of gravity may exist near the critical point for a black hole thermodynamic system.
		       
		        
		        
		        
			  
			We obtain an exact solution for spherically symmetric Letelier AdS black holes immersed in perfect fluid dark matter (PFDM). Considering the cosmological constant as the positive pressure of the system and volume as its conjugate variable, we analyze the thermodynamics of our black holes in the extended phase space. Owing to the background clouds of strings parameter (a) and the parameter endowed with PFDM (β), we analyze the Hawking temperature, entropy, and specific heat. Furthermore, we investigate the relationship between the photon sphere radius and phase transition for the Letelier AdS black holes immersed in PFDM. Through the analysis, with a particular condition, non-monotonic behaviors are found between the photon sphere radius, impact parameter, PFDM parameter, temperature, and pressure. We can regard the changes in both the photon sphere radius and impact parameter before and after phase transition as the order parameter; their critical exponents near the critical point are equal to the same value, 1/2, similar to that in ordinary thermal systems. This indicates that a universal relation of gravity may exist near the critical point for a black hole thermodynamic system.
ISSN 1674-1137 CN 11-5641/O4
Original research articles, Ietters and reviews Covering theory and experiments in the fieids of
- Particle physics
- Nuclear physics
- Particle and nuclear astrophysics
- Cosmology
Author benefits
- A SCOAP3 participating journal - free Open Access publication for qualifying articles
- Average 24 days to first decision
- Fast-track publication for selected articles
- Subscriptions at over 3000 institutions worldwide
- Free English editing on all accepted articles
News
	
- Chinese Physics C Outstanding Reviewer Award 2023
- Impact factor of Chinese Physics C is 3.6 in 2022
- 2022 CPC Outstanding Reviewer Awards
- The 2023 Chinese New Year-Office closure
- ãChinese Physics CãBEST PAPER AWARDS 2022
Cover Story
    
- Cover Story (Issue 9, 2025): Precise measurement of Ïc0 resonance parameters and branching fractions of Ïc0,c2âÏï¼Ïï¼/ K+K-
- Cover Story (Issue 8, 2025) A Novel Perspective on Spacetime Perturbations: Bridging Riemannian and Teleparallel Frameworks
- Cover Story (Issue 7, 2025) Evidence of the negative parity linear chain states in 16C
- Cover Story (Issue 1, 2025) Comments on Prediction of Energy Resolution inthe JUNO Experiment
- Cover Story (Issue 12, 2024) | Doubly heavy meson puzzle: precise prediction of the mass spectra and hadronic decay with coupled channel effects to hunt for beauty-charm family











 
    	     
		    

