2024 Vol. 48, No. 3
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			            2024, 48(3): 033101. doi: 10.1088/1674-1137/ad13f6 
	   					
		        	
			        
		            	
		        
					Abstract: 
We study the decays of\begin{document}$ \Lambda_b \to \Lambda(\to p \pi^-) \ell ^+ \ell^- $\end{document} ![]()
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\begin{document}$ \ell = (e, \mu, \tau) $\end{document} ![]()
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\begin{document}$ \Lambda_b $\end{document} ![]()
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\begin{document}$ \Lambda_b \to \Lambda(\to p \pi^-) \tau^+ \tau^- $\end{document} ![]()
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\begin{document}$ \Lambda_b \to \Lambda(\to p \pi^-) \mu^+ \mu^- $\end{document} ![]()
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\begin{document}$ \Lambda_b \to \Lambda(\to p \pi^-) \tau^+ \tau^- $\end{document} ![]()
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\begin{document}$ K_{10} $\end{document} ![]()
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\begin{document}$ \Lambda_b \to \Lambda(\to p \pi^-) \mu^+ \mu^- $\end{document} ![]()
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\begin{document}$ \Lambda_b $\end{document} ![]()
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			We study the decays of
			            2024, 48(3): 033102. doi: 10.1088/1674-1137/ad1a98 
	   					
		        	
			        
		            	
		        
					Abstract: 
We present a complete study on the\begin{document}$ J/\psi $\end{document} ![]()
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\begin{document}$ c\bar{c} $\end{document} ![]()
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\begin{document}$ {}^{3}S_1^{[1]} $\end{document} ![]()
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\begin{document}$ {}^{1}S_0^{[8]} $\end{document} ![]()
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\begin{document}$ {}^{1}S_0^{[8]} $\end{document} ![]()
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			We present a complete study on the
			            2024, 48(3): 033103. doi: 10.1088/1674-1137/ad102b 
	   					
		        	
			        
		            	
		        
					Abstract: 
In the standard model QCD Lagrangian, a term of CP violating gluon density is theoretically expected to have a physical coefficient\begin{document}$ \bar{\theta} $\end{document} ![]()
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\begin{document}$ \bar{\theta} $\end{document} ![]()
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\begin{document}$ \bar{\theta} $\end{document} ![]()
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\begin{document}$ \bar{\theta} $\end{document} ![]()
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			In the standard model QCD Lagrangian, a term of CP violating gluon density is theoretically expected to have a physical coefficient
			            2024, 48(3): 033104. doi: 10.1088/1674-1137/ad181c 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, we apply the QCD sum rules to investigate the vector fully-light tetraquark states with an explicit P-wave between the diquark and antidiquark pairs. We observed that the\begin{document}$ C\gamma_\alpha\otimes\stackrel{\leftrightarrow}{\partial}_\mu\otimes\gamma^\alpha C $\end{document} ![]()
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\begin{document}$ C\gamma_\alpha\otimes\stackrel{\leftrightarrow}D_\mu\otimes\gamma^\alpha C $\end{document} ![]()
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\begin{document}$ 2.16 \pm 0.14 \,{\rm{GeV}} $\end{document} ![]()
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\begin{document}$ Y(2175)/\phi(2170) $\end{document} ![]()
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\begin{document}$J^{PC}=1^{--}$\end{document} ![]()
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\begin{document}$ qs\bar{q}\bar{s} $\end{document} ![]()
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\begin{document}$ ss\bar{s}\bar{s} $\end{document} ![]()
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\begin{document}$ C\gamma_\mu\otimes \stackrel{\leftrightarrow}{\partial}_\alpha \otimes\gamma^\alpha C + C\gamma^\alpha \otimes\stackrel{\leftrightarrow}{\partial}_\alpha \otimes\gamma_\mu $\end{document} ![]()
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\begin{document}$ C\gamma_\mu\otimes \stackrel{\leftrightarrow}D_\alpha \otimes\gamma^\alpha C +  C\gamma^\alpha \otimes\stackrel{\leftrightarrow}D_\alpha \otimes\gamma_\mu $\end{document} ![]()
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\begin{document}$ X(2200) $\end{document} ![]()
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\begin{document}$ X(2400) $\end{document} ![]()
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\begin{document}$ 2.20 $\end{document} ![]()
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\begin{document}$ 2.40\,{\rm{GeV}} $\end{document} ![]()
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\begin{document}$ 2.16-3.13\,{\rm{GeV}} $\end{document} ![]()
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\begin{document}$ 2.16-3.16\,{\rm{GeV}} $\end{document} ![]()
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			In this study, we apply the QCD sum rules to investigate the vector fully-light tetraquark states with an explicit P-wave between the diquark and antidiquark pairs. We observed that the
			            2024, 48(3): 033105. doi: 10.1088/1674-1137/ad13f5 
	   					
		        	
			        
		            	
		        
					Abstract: 
In the low energy realization of the quirk assisted Standard Model, the couplings between the exotic particles "quirks" and gauge bosons may contribute to the W mass and muon\begin{document}$ g-2 $\end{document} ![]()
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\begin{document}$ m_F $\end{document} ![]()
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\begin{document}$ g-2 $\end{document} ![]()
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			In the low energy realization of the quirk assisted Standard Model, the couplings between the exotic particles "quirks" and gauge bosons may contribute to the W mass and muon
			            2024, 48(3): 033106. doi: 10.1088/1674-1137/ad1b3d 
	   					
		        	
			        
		            	
		        
					Abstract: 
A new method based on the maximum entropy principle for reconstructing the parton distribution function (PDF) from moments is proposed. Unlike traditional methods, the new method does not require any artificial assumptions. For the case of moments with errors, we introduce Gaussian functions to soften the constraints of moments. Through a series of tests, the effectiveness and reconstruction efficiency of this new method are evaluated comprehensively, demonstrating that this method is reasonable and can achieve high-quality reconstruction with at least the first six moments as input. Finally, we select a set of lattice quantum chromodynamics (QCD) results regarding moments as input and provide reasonable reconstruction results for the pion.
		       
		        
		        
		        
			  
			A new method based on the maximum entropy principle for reconstructing the parton distribution function (PDF) from moments is proposed. Unlike traditional methods, the new method does not require any artificial assumptions. For the case of moments with errors, we introduce Gaussian functions to soften the constraints of moments. Through a series of tests, the effectiveness and reconstruction efficiency of this new method are evaluated comprehensively, demonstrating that this method is reasonable and can achieve high-quality reconstruction with at least the first six moments as input. Finally, we select a set of lattice quantum chromodynamics (QCD) results regarding moments as input and provide reasonable reconstruction results for the pion.
			            2024, 48(3): 033107. doi: 10.1088/1674-1137/ad1cdb 
	   					
		        	
			        
		            	
		        
					Abstract: 
An analytical study with respect to the nonlinear corrections for the nuclear gluon distribution function in the next-to-leading order approximation at small x is presented. We consider the nonlinear corrections to the nuclear gluon distribution functions at low values of x and\begin{document}$ Q^{2} $\end{document} ![]()
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\begin{document}$ F_{2}(x,Q^{2}) $\end{document} ![]()
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\begin{document}$ Q_{0}^{2}=1.69\; {\rm{GeV}}^2 $\end{document} ![]()
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\begin{document}$ Q_{0}^{2} $\end{document} ![]()
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			An analytical study with respect to the nonlinear corrections for the nuclear gluon distribution function in the next-to-leading order approximation at small x is presented. We consider the nonlinear corrections to the nuclear gluon distribution functions at low values of x and
			            2024, 48(3): 034001. doi: 10.1088/1674-1137/ad1678 
	   					
		        	
			        
		            	
		        
					Abstract: 
The elastic scattering angular distributions of\begin{document}$ ^{13} $\end{document} ![]()
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\begin{document}$ ^{14} $\end{document} ![]()
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\begin{document}$ ^{208} $\end{document} ![]()
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			The elastic scattering angular distributions of
			            2024, 48(3): 034002. doi: 10.1088/1674-1137/ad1a0a 
	   					
		        	
			        
		            	
		        
					Abstract: 
The ground-state mass excess of the\begin{document}$ T_{z}=-2 $\end{document} ![]()
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\begin{document}$ ^{22} $\end{document} ![]()
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\begin{document}$ 18103(10) $\end{document} ![]()
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\begin{document}$ 1^+ $\end{document} ![]()
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\begin{document}$ ^{22} $\end{document} ![]()
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\begin{document}$ ^{22} $\end{document} ![]()
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\begin{document}$ 1^+ $\end{document} ![]()
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\begin{document}$ ^{22} $\end{document} ![]()
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\begin{document}$ ^{22} $\end{document} ![]()
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\begin{document}$ -625(51) $\end{document} ![]()
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\begin{document}$ -330(51) $\end{document} ![]()
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\begin{document}$ \pi s_{1/2} $\end{document} ![]()
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			The ground-state mass excess of the
			            2024, 48(3): 034003. doi: 10.1088/1674-1137/ad147e 
	   					
		        	
			        
		            	
		        
					Abstract: 
A study of the inelastic scattering of neutrons with an energy of\begin{document}$ 14.1 $\end{document} ![]()
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\begin{document}$ _{4} $\end{document} ![]()
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\begin{document}$ _{3} $\end{document} ![]()
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\begin{document}$ _{12} $\end{document} ![]()
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\begin{document}$ ^{16} $\end{document} ![]()
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\begin{document}$ ^{31} $\end{document} ![]()
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\begin{document}$ ^{32} $\end{document} ![]()
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\begin{document}$ 14.1 $\end{document} ![]()
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\begin{document}$ ^{31} $\end{document} ![]()
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			A study of the inelastic scattering of neutrons with an energy of
			            2024, 48(3): 034101. doi: 10.1088/1674-1137/ad181b 
	   					
		        	
			        
		            	
		        
					Abstract: 
Recent measurements of the two neutrino double beta decay high precision electron spectra, combined with charge exchange or β-decay experimental data, have revealed severe constraints across current nuclear many body calculations. Our calculations show that the quasi-particle random phase approximation (QRPA) approach can adequately reproduce the measured spectra for the two open shell nuclei,\begin{document}$ ^{82} $\end{document} ![]()
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\begin{document}$ ^{100} $\end{document} ![]()
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\begin{document}$ ^{136} $\end{document} ![]()
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\begin{document}$ g_A $\end{document} ![]()
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\begin{document}$ ^{136} $\end{document} ![]()
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			Recent measurements of the two neutrino double beta decay high precision electron spectra, combined with charge exchange or β-decay experimental data, have revealed severe constraints across current nuclear many body calculations. Our calculations show that the quasi-particle random phase approximation (QRPA) approach can adequately reproduce the measured spectra for the two open shell nuclei,
			            2024, 48(3): 034102. doi: 10.1088/1674-1137/ad18d2 
	   					
		        	
			        
		            	
		        
					Abstract: 
Wobbling motion in a system comprising a triaxial rotor and a single quasiparticle is studied employing the particle-rotor model. The energy spectra, wobbling frequencies, electromagnetic transition probabilities, g-factors, angular momentum components, spin coherent state maps, and static quadrupole moments are investigated. These investigations were conducted with regard to the Fermi surface transitioning from the lowest\begin{document}$ h_{11/2} $\end{document} ![]()
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\begin{document}$ \gamma=20^\circ $\end{document} ![]()
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			Wobbling motion in a system comprising a triaxial rotor and a single quasiparticle is studied employing the particle-rotor model. The energy spectra, wobbling frequencies, electromagnetic transition probabilities, g-factors, angular momentum components, spin coherent state maps, and static quadrupole moments are investigated. These investigations were conducted with regard to the Fermi surface transitioning from the lowest
			            2024, 48(3): 034103. doi: 10.1088/1674-1137/ad1582 
	   					
		        	
			        
		            	
		        
					Abstract: 
Recently, the synthesis of new elements above Z = 118 has been a hot topic in nuclear physics. Meanwhile, the α-decay chain is expected to be the unique tool to identify these heaviest nuclei. We have systematically calculated the α-decay energies and half-lives on the same footing for superheavy nuclei (SHN) within the cluster model along with a slightly modified Woods-Saxon (W.S.) potential as the nuclear potential. Based on the available experimental data, the key radius parameter (R) in the α-core potential is determined via the systematic trend from the α-decay and isotopic chains. The α-decay energy (\begin{document}$Q _{\alpha} $\end{document} ![]()
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\begin{document}$ ^{293,294} $\end{document} ![]()
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\begin{document}$ ^{294} $\end{document} ![]()
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			Recently, the synthesis of new elements above Z = 118 has been a hot topic in nuclear physics. Meanwhile, the α-decay chain is expected to be the unique tool to identify these heaviest nuclei. We have systematically calculated the α-decay energies and half-lives on the same footing for superheavy nuclei (SHN) within the cluster model along with a slightly modified Woods-Saxon (W.S.) potential as the nuclear potential. Based on the available experimental data, the key radius parameter (R) in the α-core potential is determined via the systematic trend from the α-decay and isotopic chains. The α-decay energy (
			            2024, 48(3): 034104. doi: 10.1088/1674-1137/ad1a97 
	   					
		        	
			        
		            	
		        
					Abstract: 
A new empirical formula for the astrophysical S-factor has been suggested as a function of the Coulomb interaction parameter, center of mass energy, and barrier height. About 22 fusion reactions with 40,48Ca as projectiles were considered for different targets, leading to compound nuclei with atomic and mass numbers varying between 40\begin{document}$ \le Z \le  $\end{document} ![]()
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\begin{document}$ 88 \le A \le 278$\end{document} ![]()
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			A new empirical formula for the astrophysical S-factor has been suggested as a function of the Coulomb interaction parameter, center of mass energy, and barrier height. About 22 fusion reactions with 40,48Ca as projectiles were considered for different targets, leading to compound nuclei with atomic and mass numbers varying between 40
			            2024, 48(3): 034105. doi: 10.1088/1674-1137/ad18d3 
	   					
		        	
			        
		            	
		        
					Abstract: 
We investigate the effects of the σ meson mass (\begin{document}$ m_\sigma $\end{document} ![]()
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\begin{document}$ \Delta I/I $\end{document} ![]()
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\begin{document}$ \rho_{t} $\end{document} ![]()
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\begin{document}$ P_{t} $\end{document} ![]()
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\begin{document}$ \Delta I/I $\end{document} ![]()
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\begin{document}$\Delta I/I\geq7$\end{document} ![]()
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\begin{document}$ \rho_{t} $\end{document} ![]()
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\begin{document}$ P_{t} $\end{document} ![]()
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\begin{document}$ m_\sigma $\end{document} ![]()
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\begin{document}$ m_\sigma $\end{document} ![]()
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\begin{document}$\Delta I/I\geq7$\end{document} ![]()
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			We investigate the effects of the σ meson mass (
			            2024, 48(3): 034106. doi: 10.1088/1674-1137/ad1b3e 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, we utilize the complexity-action duality to study the evolution of complexity in a holographic QCD model at finite temperature and chemical potential. By inserting a fundamental string as a probe, we investigated the properties of complexity growth in this Einstein-Maxwell-scalar gravity system, which is affected by the string velocity, chemical potential, and temperature. Our results show that the complexity growth is maximized when the probe string is stationary, and it decreases as the velocity of the string increases. When the string approaches relativistic velocities, the complexity growth always increases monotonically with respect to the chemical potential. Furthermore, we find that the complexity growth can be used to identify phase transitions and crossovers in the model.
		       
		        
		        
		        
			  
			In this study, we utilize the complexity-action duality to study the evolution of complexity in a holographic QCD model at finite temperature and chemical potential. By inserting a fundamental string as a probe, we investigated the properties of complexity growth in this Einstein-Maxwell-scalar gravity system, which is affected by the string velocity, chemical potential, and temperature. Our results show that the complexity growth is maximized when the probe string is stationary, and it decreases as the velocity of the string increases. When the string approaches relativistic velocities, the complexity growth always increases monotonically with respect to the chemical potential. Furthermore, we find that the complexity growth can be used to identify phase transitions and crossovers in the model.
			            2024, 48(3): 034107. doi: 10.1088/1674-1137/ad1925 
	   					
		        	
			        
		            	
		        
					Abstract: 
Key nuclear inputs for the astrophysical r-process simulations are the weak interaction rates. Consequently, the accuracy of these inputs directly affects the reliability of nucleosynthesis modeling. The majority of the stellar rates, used in simulation studies are calculated by invoking the Brink-Axel (BA) hypothesis. The BA hypothesis assumes that the strength functions of all parent excited states are the same as for the ground state, only shifted in energies. However, the BA hypothesis has to be tested against microscopically calculated state-by-state rates. In this project, we study the impact of the BA hypothesis on calculated stellar\begin{document}$ \beta^{-} $\end{document} ![]()
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\begin{document}$ \beta^{-} $\end{document} ![]()
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\begin{document}$\rho{{\rm Y}}_{e}$\end{document} ![]()
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\begin{document}$\rm g/cm^{3}$\end{document} ![]()
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\begin{document}$ GK $\end{document} ![]()
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\begin{document}$ \beta^{-} $\end{document} ![]()
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\begin{document}$ \beta^{-} $\end{document} ![]()
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			Key nuclear inputs for the astrophysical r-process simulations are the weak interaction rates. Consequently, the accuracy of these inputs directly affects the reliability of nucleosynthesis modeling. The majority of the stellar rates, used in simulation studies are calculated by invoking the Brink-Axel (BA) hypothesis. The BA hypothesis assumes that the strength functions of all parent excited states are the same as for the ground state, only shifted in energies. However, the BA hypothesis has to be tested against microscopically calculated state-by-state rates. In this project, we study the impact of the BA hypothesis on calculated stellar
			            2024, 48(3): 034108. doi: 10.1088/1674-1137/ad1d4b 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, a microscopic shell-model description of the low-lying collective states in the weakly deformed nucleus\begin{document}$ ^{106} $\end{document} ![]()
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\begin{document}$S U(3)$\end{document} ![]()
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			In this study, a microscopic shell-model description of the low-lying collective states in the weakly deformed nucleus
			            2024, 48(3): 035101. doi: 10.1088/1674-1137/ad1a0c 
	   					
		        	
			        
		            	
		        
					Abstract: 
General relativity has been very successful since its proposal more than a century ago. However, various cosmological observations and theoretical consistency still motivate us to explore extended gravity theories. Horndeski gravity stands out as one attractive theory by introducing only one scalar field. Here we formulate the post-Newtonian effective field theory of Horndeski gravity and investigate the conservative dynamics of inspiral compact binary systems. We calculate the leading effective Lagrangian for a compact binary and obtain the periastron advance per period. In particular, we apply our analytical calculation to two binary systems, PSR B 1534+12 and PSR J0737-3039, and constrain the relevant model parameters. This theoretical framework can also be systematically extended to higher orders.
		       
		        
		        
		        
			  
			General relativity has been very successful since its proposal more than a century ago. However, various cosmological observations and theoretical consistency still motivate us to explore extended gravity theories. Horndeski gravity stands out as one attractive theory by introducing only one scalar field. Here we formulate the post-Newtonian effective field theory of Horndeski gravity and investigate the conservative dynamics of inspiral compact binary systems. We calculate the leading effective Lagrangian for a compact binary and obtain the periastron advance per period. In particular, we apply our analytical calculation to two binary systems, PSR B 1534+12 and PSR J0737-3039, and constrain the relevant model parameters. This theoretical framework can also be systematically extended to higher orders.
			            2024, 48(3): 035102. doi: 10.1088/1674-1137/ad1ed8 
	   					
		        	
			        
		            	
		        
					Abstract: 
Black holes (BHs) exhibiting coordinate singularities but lacking essential singularities throughout the spacetime are referred to as regular black holes (RBHs). The initial formulation of RBHs was presented by Bardeen, who considered the Einstein equation coupled with a nonlinear electromagnetic field. In this study, we investigate the gravitational perturbations, including the axial and polar sectors, of the Bardeen (Anti-) de Sitter black holes. We derive the master equations with source terms for both axial and polar perturbations and subsequently compute the quasinormal modes (QNMs) through numerical methods. For the Bardeen de Sitter black hole, we employ the 6th-order WKB approach. The numerical results reveal that the isospectrality is broken in this case. Conversely, the QNM frequencies are calculated using the HH method for the Bardeen Anti-de Sitter black hole.
		       
		        
		        
		        
			  
			Black holes (BHs) exhibiting coordinate singularities but lacking essential singularities throughout the spacetime are referred to as regular black holes (RBHs). The initial formulation of RBHs was presented by Bardeen, who considered the Einstein equation coupled with a nonlinear electromagnetic field. In this study, we investigate the gravitational perturbations, including the axial and polar sectors, of the Bardeen (Anti-) de Sitter black holes. We derive the master equations with source terms for both axial and polar perturbations and subsequently compute the quasinormal modes (QNMs) through numerical methods. For the Bardeen de Sitter black hole, we employ the 6th-order WKB approach. The numerical results reveal that the isospectrality is broken in this case. Conversely, the QNM frequencies are calculated using the HH method for the Bardeen Anti-de Sitter black hole.
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
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