2025 Vol. 49, No. 7
Display Method: |
			            2025, 49(7): 071001. doi: 10.1088/1674-1137/adc120 
	   					
		        	
			        
		            	
		        
					Abstract: 
We propose the weak magnetic effect, which emerges as the dissipative correction to the quark phase space distribution function in quark-gluon plasma close to local thermal equilibrium, as a novel contribution to the observed Lambda hyperon local spin polarization. A finite field strength that is consistent with previous estimates of the magnetic field in heavy-ion collisions can be used to xplain the experimentally observed Lambda local spin polarization through all centrality classes. Moreover, the weak magnetic effect plays an unambiguous role in the ordering between the second-order and third-order modulations of experimental Lambda local spin polarization.
		       
		        
		        
		        
			  
			We propose the weak magnetic effect, which emerges as the dissipative correction to the quark phase space distribution function in quark-gluon plasma close to local thermal equilibrium, as a novel contribution to the observed Lambda hyperon local spin polarization. A finite field strength that is consistent with previous estimates of the magnetic field in heavy-ion collisions can be used to xplain the experimentally observed Lambda local spin polarization through all centrality classes. Moreover, the weak magnetic effect plays an unambiguous role in the ordering between the second-order and third-order modulations of experimental Lambda local spin polarization.
			            2025, 49(7): 071002. doi: 10.1088/1674-1137/adcc8f 
	   					
		        	
			        
		            	
		        
					Abstract: 
The angular distribution of elastic scattering is highly sensitive to the surface region of the nucleus, making it a powerful tool for measuring the neutron skin thickness. Utilizing the CDM3Y6 double-folding potential, we extracted the neutron skin thickness of\begin{document}$ ^{124} $\end{document} ![]()
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\begin{document}$ ^{12} $\end{document} ![]()
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\begin{document}$ ^{124} $\end{document} ![]()
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\begin{document}$ 0.168_{\text{−}0.019}^{+0.025} $\end{document} ![]()
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\begin{document}$ 0.177 \pm 0.022 $\end{document} ![]()
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\begin{document}$ L = 39.0_{\text{−}16.5}^{+20.8} $\end{document} ![]()
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\begin{document}$L = 46.1  \pm   18.7$\end{document} ![]()
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			The angular distribution of elastic scattering is highly sensitive to the surface region of the nucleus, making it a powerful tool for measuring the neutron skin thickness. Utilizing the CDM3Y6 double-folding potential, we extracted the neutron skin thickness of
			            2025, 49(7): 073001. doi: 10.1088/1674-1137/adc88d 
	   					
		        	
			        
		            	
		        
					Abstract: 
Utilizing 4.5\begin{document}$ \text{fb}^{-1} $\end{document} ![]()
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\begin{document}$ e^+e^- $\end{document} ![]()
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\begin{document}$ \Lambda_{c}^{+}\to\Sigma^{0} K^{+}\pi^{0} $\end{document} ![]()
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\begin{document}$ \Lambda_{c}^{+}\to\Sigma^{0}K^{+} \pi^+ \pi^- $\end{document} ![]()
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\begin{document}$ 5.0\times 10^{-4} $\end{document} ![]()
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\begin{document}$ \Lambda_{c}^{+}\to\Sigma^{0} K^{+}\pi^{0} $\end{document} ![]()
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\begin{document}$ 6.5\times 10^{-4} $\end{document} ![]()
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\begin{document}$ \Lambda_c^{+}\to\Sigma^0K^{+}\pi^{+}\pi^{-} $\end{document} ![]()
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			Utilizing 4.5
			            2025, 49(7): 073101. doi: 10.1088/1674-1137/adcc8a 
	   					
		        	
			        
		            	
		        
					Abstract: 
We study the new\begin{document}$Z'$\end{document} ![]()
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\begin{document}$h_0$\end{document} ![]()
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\begin{document}$H_0$\end{document} ![]()
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\begin{document}$\mu^+\mu^- \to (Z, Z') \to Zh_0, ZH_0$\end{document} ![]()
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\begin{document}$Zh_0, ZH_0$\end{document} ![]()
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\begin{document}$\sqrt{s}=3, 4, 6, 10, 30$\end{document} ![]()
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\begin{document}${\cal{L}}=2, 4, 6, 10, 30$\end{document} ![]()
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\begin{document}${ {\rm{ab}}^{-1}}$\end{document} ![]()
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\begin{document}$h_0$\end{document} ![]()
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\begin{document}$H_0$\end{document} ![]()
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\begin{document}$\mu^+\mu^- \to (Z, Z') \to Zh_0, ZH_0$\end{document} ![]()
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			We study the new
			            2025, 49(7): 073102. doi: 10.1088/1674-1137/adc084 
	   					
		        	
			        
		            	
		        
					Abstract: 
This work conducts a comprehensive analysis of the mass spectra and decay properties of bottomonium states using a relativistic screened potential model. The mass spectrum, decay constants,\begin{document}$ E1 $\end{document} ![]()
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\begin{document}$ M1 $\end{document} ![]()
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\begin{document}$ \Upsilon(10355) $\end{document} ![]()
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\begin{document}$ \Upsilon(10580) $\end{document} ![]()
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\begin{document}$ \Upsilon(10860) $\end{document} ![]()
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\begin{document}$ \Upsilon(11020) $\end{document} ![]()
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\begin{document}$ S-D $\end{document} ![]()
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\begin{document}$ \Upsilon(10355) $\end{document} ![]()
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\begin{document}$ 3S-2D $\end{document} ![]()
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\begin{document}$ \Upsilon(10580) $\end{document} ![]()
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\begin{document}$ \Upsilon(10753) $\end{document} ![]()
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\begin{document}$ 4S-3D $\end{document} ![]()
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\begin{document}$ \Upsilon(10860) $\end{document} ![]()
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\begin{document}$ \Upsilon(11020) $\end{document} ![]()
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\begin{document}$ 5S-4D $\end{document} ![]()
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			This work conducts a comprehensive analysis of the mass spectra and decay properties of bottomonium states using a relativistic screened potential model. The mass spectrum, decay constants,
			            2025, 49(7): 073103. doi: 10.1088/1674-1137/adcb29 
	   					
		        	
			        
		            	
		        
					Abstract: 
We analyze the recent data from the BESIII collaboration on the\begin{document}$ X(3872) $\end{document} ![]()
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\begin{document}$ J/\psi\pi^+\pi^- $\end{document} ![]()
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\begin{document}$ D^0\bar{D}^0\pi^0 $\end{document} ![]()
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\begin{document}$ X(3872) $\end{document} ![]()
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\begin{document}$ D\bar D^* $\end{document} ![]()
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\begin{document}$ J/\psi\pi^+\pi^- $\end{document} ![]()
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\begin{document}$ D^0\bar{D}^0\pi^0 $\end{document} ![]()
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\begin{document}$ X(3872) $\end{document} ![]()
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			We analyze the recent data from the BESIII collaboration on the
			            2025, 49(7): 073104. doi: 10.1088/1674-1137/add5c5 
	   					
		        	
			        
		            	
		        
					Abstract: 
We explore the properties of vector dark matter (DM) particles that predominantly interact with Standard Model (SM) electroweak gauge bosons using an effective field theory approach. The study emphasizes effective contact interactions, invariant under the SM gauge group, between vector DM and SM-neutral electroweak gauge bosons. Focusing on interaction terms up to dimension-eight, we establish constraints on the model parameters based on the observed DM relic density and indirect detection signals. We also examine the prospects for dark matter-nucleon scattering in direct detection experiments. In addition, we analyze the sensitivity of low-energy LEP data to the pair production of light DM particles (with masses up to 80 GeV). Finally, we assess the potential of the proposed International Linear Collider to probe these effective operators through the detection of DM particles produced in association with mono-photons.
		       
		        
		        
		        
			  
			We explore the properties of vector dark matter (DM) particles that predominantly interact with Standard Model (SM) electroweak gauge bosons using an effective field theory approach. The study emphasizes effective contact interactions, invariant under the SM gauge group, between vector DM and SM-neutral electroweak gauge bosons. Focusing on interaction terms up to dimension-eight, we establish constraints on the model parameters based on the observed DM relic density and indirect detection signals. We also examine the prospects for dark matter-nucleon scattering in direct detection experiments. In addition, we analyze the sensitivity of low-energy LEP data to the pair production of light DM particles (with masses up to 80 GeV). Finally, we assess the potential of the proposed International Linear Collider to probe these effective operators through the detection of DM particles produced in association with mono-photons.
			            2025, 49(7): 074001. doi: 10.1088/1674-1137/adc7e5 
	   					
		        	
			        
		            	
		        
					Abstract: 
Bremsstrahlung fluxes for irradiating tantalum samples were formed by irradiating a tungsten converter with an electron beam having energy up to 130 MeV. The relative yields and flux-averaged cross-sections of multinucleon photonuclear reactions that emit up to nine neutrons in 181Ta nuclei were determined. Monte Carlo simulations for studying the yields of photonuclear reactions were performed using Geant4 and TALYS-2.0 codes. The obtained experimental results were compared with available literature data and calculated results. The comparison showed that the values of the relative reaction yield and flux-averaged cross-section coincide with the literature data, considering the different geometries of the experiments. The calculated results coincide with the experimental ones only for reactions that emit up to five neutrons from the nucleus.
		       
		        
		        
		        
			  
			Bremsstrahlung fluxes for irradiating tantalum samples were formed by irradiating a tungsten converter with an electron beam having energy up to 130 MeV. The relative yields and flux-averaged cross-sections of multinucleon photonuclear reactions that emit up to nine neutrons in 181Ta nuclei were determined. Monte Carlo simulations for studying the yields of photonuclear reactions were performed using Geant4 and TALYS-2.0 codes. The obtained experimental results were compared with available literature data and calculated results. The comparison showed that the values of the relative reaction yield and flux-averaged cross-section coincide with the literature data, considering the different geometries of the experiments. The calculated results coincide with the experimental ones only for reactions that emit up to five neutrons from the nucleus.
			            2025, 49(7): 074002. doi: 10.1088/1674-1137/adc122 
	   					
		        	
			        
		            	
		        
					Abstract: 
In-ring nuclear reactions induced by light-ions, which are characterized by low-momentum sensitivity and low background, play an important role in nuclear structure and astrophysics investigations. Recently, the in-ring proton-nucleus elastic scattering measurements at low momentum transfer based on the internal hydrogen-gas-jet target have been successfully performed at the Cooler Storage Ring of the Heavy Ion Research Facility in Lanzhou (HIRFL-CSR). In this proceeding, we present the progress of matter radius measurements using the small-angle differential cross sections of proton-nucleus elastic scattering at HIRFL-CSR.
		       
		        
		        
		        
			  
			In-ring nuclear reactions induced by light-ions, which are characterized by low-momentum sensitivity and low background, play an important role in nuclear structure and astrophysics investigations. Recently, the in-ring proton-nucleus elastic scattering measurements at low momentum transfer based on the internal hydrogen-gas-jet target have been successfully performed at the Cooler Storage Ring of the Heavy Ion Research Facility in Lanzhou (HIRFL-CSR). In this proceeding, we present the progress of matter radius measurements using the small-angle differential cross sections of proton-nucleus elastic scattering at HIRFL-CSR.
			            2025, 49(7): 074003. doi: 10.1088/1674-1137/adbad0 
	   					
		        	
			        
		            	
		        
					Abstract: 
The Nuclotron-based Ion Collider fAcility (NICA), currently under construction at JINR, is expected to conduct its first beam tests in the second half of 2025. The NICA project is designed to provide colliding beams for investigating heavy stripped ion collisions at energies of 4.5 GeV/u. The NICA accelerator complex comprises several components: the operational heavy ion linac HILAC with an energy of 3.2 MeV/u, superconducting Booster synchrotron with a maximum energy of 600 MeV/u, superconducting Nuclotron synchrotron capable of accelerating gold ions to 3.9 GeV/u, and two storage rings with two interaction points currently under installation. The system includes two electron cooling units—one in the Booster synchrotron with a maximum electron energy of 60 keV, and another in the Collider with two electron beams, each with a maximum energy of 2.5 MeV. Additionally, two stochastic cooling systems are integrated into the setup. The status of the NICA accelerator complex, including its cooling systems, is presented. Experimental results from electron cooling studies conducted during the commissioning of the injection complex are reported. Plans for the further development and application of the electron and stochastic cooling systems are also described.
		       
		        
		        
		        
			  
			The Nuclotron-based Ion Collider fAcility (NICA), currently under construction at JINR, is expected to conduct its first beam tests in the second half of 2025. The NICA project is designed to provide colliding beams for investigating heavy stripped ion collisions at energies of 4.5 GeV/u. The NICA accelerator complex comprises several components: the operational heavy ion linac HILAC with an energy of 3.2 MeV/u, superconducting Booster synchrotron with a maximum energy of 600 MeV/u, superconducting Nuclotron synchrotron capable of accelerating gold ions to 3.9 GeV/u, and two storage rings with two interaction points currently under installation. The system includes two electron cooling units—one in the Booster synchrotron with a maximum electron energy of 60 keV, and another in the Collider with two electron beams, each with a maximum energy of 2.5 MeV. Additionally, two stochastic cooling systems are integrated into the setup. The status of the NICA accelerator complex, including its cooling systems, is presented. Experimental results from electron cooling studies conducted during the commissioning of the injection complex are reported. Plans for the further development and application of the electron and stochastic cooling systems are also described.
			            2025, 49(7): 074004. doi: 10.1088/1674-1137/adcb96 
	   					
		        	
			        
		            	
		        
					Abstract: 
The distribution of nuclei produced in the 40Ar + 232Th reaction has been studied at the gas-filled recoil separator (SHANS2) at the China Accelerator Facility for Superheavy Elements (CAFE2). The bombardment was carried out at a beam energy of 205 MeV with the detection system installed at the focal plane. Forty-four isotopes heavier than 208Pb were observed. These isotopes were identified as the transfer reaction (or target-like) products, and their relative cross-sections were extracted. Based on the mass distribution of these products, we exclude the possibility that they were produced by fusion-fission reactions; thus, they may originate from quasi-fission of the 40Ar + 232Th reaction.
		       
		        
		        
		        
			  
			The distribution of nuclei produced in the 40Ar + 232Th reaction has been studied at the gas-filled recoil separator (SHANS2) at the China Accelerator Facility for Superheavy Elements (CAFE2). The bombardment was carried out at a beam energy of 205 MeV with the detection system installed at the focal plane. Forty-four isotopes heavier than 208Pb were observed. These isotopes were identified as the transfer reaction (or target-like) products, and their relative cross-sections were extracted. Based on the mass distribution of these products, we exclude the possibility that they were produced by fusion-fission reactions; thus, they may originate from quasi-fission of the 40Ar + 232Th reaction.
					Software defined radio for on-line interaction with beam processes in the heavy ion storage ring ESR 
								
				
		         
								
			            2025, 49(7): 074005. doi: 10.1088/1674-1137/adcc01 
	   					
		        	
			        
		            	
		        
					Abstract: 
The application of software defined radio in on-line interactions with the beam processes of the heavy ion storage ring is presented. We discusse how this new technique can enhance the beam time efficiency and create new measurement possibilities. A specific example to halt the accelerator running if a rare stored particle is identified on-line is discussed.
		       
		        
		        
		        
			  
			The application of software defined radio in on-line interactions with the beam processes of the heavy ion storage ring is presented. We discusse how this new technique can enhance the beam time efficiency and create new measurement possibilities. A specific example to halt the accelerator running if a rare stored particle is identified on-line is discussed.
			            2025, 49(7): 074006. doi: 10.1088/1674-1137/add099 
	   					
		        	
			        
		            	
		        
					Abstract: 
The opportunities and challenges of performing transfer reactions in inverse kinematics using the 16,18O beams at the experimental Cooler Storage Ring (CSRe) of the Heavy Ion Research Facility in Lanzhou (HIRFL) with the internal gas-jet target are discussed herein. The kinematics, differential cross sections for various transfer reactions using the 16,18O beam with incident energies of 30 and 100 MeV/nucleon, and the H2- or D2-gas-jet targets are compared. The 16O beam at 100 MeV/nucleon with an intensity of ≥106 pps interacting with the H2-gas-jet target is recommended as the first transfer reaction at HIRFL-CSRe.
		       
		        
		        
		        
			  
			The opportunities and challenges of performing transfer reactions in inverse kinematics using the 16,18O beams at the experimental Cooler Storage Ring (CSRe) of the Heavy Ion Research Facility in Lanzhou (HIRFL) with the internal gas-jet target are discussed herein. The kinematics, differential cross sections for various transfer reactions using the 16,18O beam with incident energies of 30 and 100 MeV/nucleon, and the H2- or D2-gas-jet targets are compared. The 16O beam at 100 MeV/nucleon with an intensity of ≥106 pps interacting with the H2-gas-jet target is recommended as the first transfer reaction at HIRFL-CSRe.
			            2025, 49(7): 074007. doi: 10.1088/1674-1137/add09a 
	   					
		        	
			        
		            	
		        
					Abstract: 
The cross sections of the 148Sm(n,α)145Nd reaction were measured for the first time at neutron energies ranging from 4.8 to 5.3 MeV. The experiment was carried out on the Van de Graaff accelerator EG–5 at the Frank Laboratory of Neutron Physics, Joint Institute for Nuclear Research. Fast neutrons were produced via the 2H(d,n)3He reaction with a deuterium gas target. A twin gridded ionization chamber was used as the charged particle detector, with back–to–back 148Sm samples mounted on tantalum backings at the common cathode. The absolute neutron flux was measured using the 238U3O8 sample. The obtained cross section data were compared with those from existing nuclear data libraries and theoretical calculations using the TALYS–1.96 code. The present results for the 148Sm(n,α)145Nd reaction are expected to resolve discrepancies among various nuclear evaluation data.
		       
		        
		        
		        
			  
			The cross sections of the 148Sm(n,α)145Nd reaction were measured for the first time at neutron energies ranging from 4.8 to 5.3 MeV. The experiment was carried out on the Van de Graaff accelerator EG–5 at the Frank Laboratory of Neutron Physics, Joint Institute for Nuclear Research. Fast neutrons were produced via the 2H(d,n)3He reaction with a deuterium gas target. A twin gridded ionization chamber was used as the charged particle detector, with back–to–back 148Sm samples mounted on tantalum backings at the common cathode. The absolute neutron flux was measured using the 238U3O8 sample. The obtained cross section data were compared with those from existing nuclear data libraries and theoretical calculations using the TALYS–1.96 code. The present results for the 148Sm(n,α)145Nd reaction are expected to resolve discrepancies among various nuclear evaluation data.
			            2025, 49(7): 074008. doi: 10.1088/1674-1137/add70d 
	   					
		        	
			        
		            	
		        
					Abstract: 
A new inelastic excitation and cluster-decay experiment was conducted to investigate the negative-parity linear-chain structure in 16C. The helium and beryllium isotopes emitted from the highly excited states of 16C and the recoil target deuteron were detected in coincidence. The 16C excitation-energy spectra associated with different decay paths were reconstructed using the invariant mass method. Owing to the newly reconfigured detector setup, the detection acceptance was extended to a higher excitation-energy range, allowing a number of new resonant states to be observed beyond the previously reported\begin{document}$ \pi^2\sigma^2 $\end{document} ![]()
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\begin{document}$ 1^- $\end{document} ![]()
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\begin{document}$ 3^- $\end{document} ![]()
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\begin{document}$ 5^- $\end{document} ![]()
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\begin{document}$ 7^- $\end{document} ![]()
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			A new inelastic excitation and cluster-decay experiment was conducted to investigate the negative-parity linear-chain structure in 16C. The helium and beryllium isotopes emitted from the highly excited states of 16C and the recoil target deuteron were detected in coincidence. The 16C excitation-energy spectra associated with different decay paths were reconstructed using the invariant mass method. Owing to the newly reconfigured detector setup, the detection acceptance was extended to a higher excitation-energy range, allowing a number of new resonant states to be observed beyond the previously reported
			            2025, 49(7): 074101. doi: 10.1088/1674-1137/adc3fd 
	   					
		        	
			        
		            	
		        
					Abstract: 
To explore the possible existence of nuclear chirality in the\begin{document}$ A\approx 60 $\end{document} ![]()
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\begin{document}$ \pi f_{7/2}^{-1} \otimes \nu g_{9/2}^{1} $\end{document} ![]()
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\begin{document}$ V_{pn} $\end{document} ![]()
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\begin{document}$ E(I) $\end{document} ![]()
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\begin{document}$ \Delta E(I) $\end{document} ![]()
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\begin{document}$ B(M1) $\end{document} ![]()
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\begin{document}$ B(E2) $\end{document} ![]()
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\begin{document}$ S(I) $\end{document} ![]()
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\begin{document}$ \mathscr{J} $\end{document} ![]()
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\begin{document}$ \pi f_{7/2}^{-1} \otimes \nu g_{9/2}^{1} $\end{document} ![]()
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\begin{document}$ \beta=0.25 $\end{document} ![]()
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\begin{document}$ \gamma=34^{\circ} $\end{document} ![]()
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\begin{document}$\mathscr{J}= $\end{document} ![]()
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\begin{document}$ 10\; \hbar^2/\rm MeV$\end{document} ![]()
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\begin{document}$ \Delta E(I) $\end{document} ![]()
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\begin{document}$ S(I) $\end{document} ![]()
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\begin{document}$ V_{pn} $\end{document} ![]()
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\begin{document}$ V_{pn} $\end{document} ![]()
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\begin{document}$ \mathscr{P}(\theta,\varphi) $\end{document} ![]()
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			To explore the possible existence of nuclear chirality in the
			            2025, 49(7): 074102. doi: 10.1088/1674-1137/adc4ca 
	   					
		        	
			        
		            	
		        
					Abstract: 
This article describes a series of studies on the effect of the rotation of the fissile 236U nucleus in the 235U(n,f) process induced by monochromatic polarized neutrons with energies of 62 meV and 270 meV. The studied effect is expressed as a shift in the anisotropic angular distribution of γ-rays emitted by excited fission fragments by a small angle relative to the deformation axis of the fissile nucleus when the neutron beam polarization direction is reversed. All measurements were performed at the Heinz Mayer-Leibniz research neutron source (FRM II reactor) of the Munich Technical University in Garching on the polarized neutron beam of the POLI instrument. To generalize all results obtained on ROT effects for fission γ-rays, the results of earlier studies by the ITEP group for cold neutrons are re-processed, and the result obtained by the PNPI group for thermal neutrons is also presented.
		       
		        
		        
		        
			  
			This article describes a series of studies on the effect of the rotation of the fissile 236U nucleus in the 235U(n,f) process induced by monochromatic polarized neutrons with energies of 62 meV and 270 meV. The studied effect is expressed as a shift in the anisotropic angular distribution of γ-rays emitted by excited fission fragments by a small angle relative to the deformation axis of the fissile nucleus when the neutron beam polarization direction is reversed. All measurements were performed at the Heinz Mayer-Leibniz research neutron source (FRM II reactor) of the Munich Technical University in Garching on the polarized neutron beam of the POLI instrument. To generalize all results obtained on ROT effects for fission γ-rays, the results of earlier studies by the ITEP group for cold neutrons are re-processed, and the result obtained by the PNPI group for thermal neutrons is also presented.
			            2025, 49(7): 074103. doi: 10.1088/1674-1137/adc7e4 
	   					
		        	
			        
		            	
		        
					Abstract: 
This paper presents a comprehensive investigation of the true ternary fission of the\begin{document}$ ^{248}\text{Cf} $\end{document} ![]()
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\begin{document}$ \text{TCM} $\end{document} ![]()
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\begin{document}$ \text{WKB} $\end{document} ![]()
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\begin{document}$ Z = 20 $\end{document} ![]()
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\begin{document}$ Z = 52 $\end{document} ![]()
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\begin{document}$ A_{1} $\end{document} ![]()
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\begin{document}$ A_{2} $\end{document} ![]()
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\begin{document}$ A_{3} $\end{document} ![]()
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\begin{document}${V {\text{-}} Q}$\end{document} ![]()
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\begin{document}$ T_{\frac{1}{2}} $\end{document} ![]()
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\begin{document}$ Z_{1} $\end{document} ![]()
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\begin{document}$ Z_{2} $\end{document} ![]()
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\begin{document}$ Z_{3} $\end{document} ![]()
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			This paper presents a comprehensive investigation of the true ternary fission of the
			            2025, 49(7): 074104. doi: 10.1088/1674-1137/adc2da 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, the evolution of nuclear shape and rotational behavior along the yrast line in even-even\begin{document}$ ^{126-136} {\rm{Ba}}$\end{document} ![]()
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\begin{document}$ \beta_2, \gamma, \beta_4 $\end{document} ![]()
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\begin{document}$ ^{126-136} {\rm{Ba}}$\end{document} ![]()
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\begin{document}$ ^{130} {\rm{Ba}}$\end{document} ![]()
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\begin{document}$ \pi(h_{11/2})^2 $\end{document} ![]()
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\begin{document}$ \nu(h_{11/2})^2 $\end{document} ![]()
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\begin{document}$ \gamma > 0^{\circ} $\end{document} ![]()
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\begin{document}$ \gamma < 0^{\circ} $\end{document} ![]()
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			In this study, the evolution of nuclear shape and rotational behavior along the yrast line in even-even
			            2025, 49(7): 074105. doi: 10.1088/1674-1137/adc097 
	   					
		        	
			        
		            	
		        
					Abstract: 
In the present work, based on a Gamow-like model, considering the deformation effect of Coulomb potential, where the effective nuclear radius constant is parameterized, we systematically investigate the cluster radioactivity half-lives of 25 trans-lead nuclei. For comparison, a universal decay law (UDL) proposed by Qi et al. [Phys. Rev. C 80, 044326 (2009)], a new semi-empirical formula for exotic cluster decay proposed by Balasubramaniam et al. [Phys. Rev. C 70, 017301 (2004)], and a scaling law proposed by Horoi [J. Phys. G: Nucl. Part. Phys. 30, 945 (2004)] are also used. The calculated results within the deformed Gamow-like model are in better agreement with the experimental half-lives. The deformation effect is also discussed within both the Gamow-like and deforemed Gamow-like models. Moreover, we extend this model to predict the cluster radioactivity half-lives of 49 nuclei whose decay energies are energetically allowed or observed but not yet quantified in NUBASE2020.
		       
		        
		        
		        
			  
			In the present work, based on a Gamow-like model, considering the deformation effect of Coulomb potential, where the effective nuclear radius constant is parameterized, we systematically investigate the cluster radioactivity half-lives of 25 trans-lead nuclei. For comparison, a universal decay law (UDL) proposed by Qi et al. [Phys. Rev. C 80, 044326 (2009)], a new semi-empirical formula for exotic cluster decay proposed by Balasubramaniam et al. [Phys. Rev. C 70, 017301 (2004)], and a scaling law proposed by Horoi [J. Phys. G: Nucl. Part. Phys. 30, 945 (2004)] are also used. The calculated results within the deformed Gamow-like model are in better agreement with the experimental half-lives. The deformation effect is also discussed within both the Gamow-like and deforemed Gamow-like models. Moreover, we extend this model to predict the cluster radioactivity half-lives of 49 nuclei whose decay energies are energetically allowed or observed but not yet quantified in NUBASE2020.
			            2025, 49(7): 074106. doi: 10.1088/1674-1137/adc121 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, we explore the possibilities of the formation of bound states of neutral pseudoscalar mesons\begin{document}$ \eta, \eta', D^{0} $\end{document} ![]()
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\begin{document}$ \bar{D^{0}}, B^{0}, \bar{B^{0}} $\end{document} ![]()
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\begin{document}$ \bar{K^{0}} $\end{document} ![]()
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\begin{document}$ ^{12} {\rm{C}}$\end{document} ![]()
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\begin{document}$ ^{16} {\rm{O}}$\end{document} ![]()
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\begin{document}$ ^{40} {\rm{C}}{\rm{a}}$\end{document} ![]()
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\begin{document}$ ^{208} {\rm{Pb}}$\end{document} ![]()
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\begin{document}$S U $\end{document} ![]()
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\begin{document}$S U$\end{document} ![]()
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\begin{document}$\eta,\; D^{0}$\end{document} ![]()
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\begin{document}$ \bar{D^{0}}, B^{0}, \bar{B^{0}} $\end{document} ![]()
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\begin{document}$ \bar{K^{0}} $\end{document} ![]()
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\begin{document}$ \eta ' $\end{document} ![]()
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			In this study, we explore the possibilities of the formation of bound states of neutral pseudoscalar mesons
			            2025, 49(7): 074107. doi: 10.1088/1674-1137/adc11e 
	   					
		        	
			        
		            	
		        
					Abstract: 
An axially quadruple-octupole deformed relativistic Hartree-Fock (O-RHF) model with density-dependent meson-nucleon couplings is developed in this study. In this model, the reflection symmetry is not preserved, and the integro-differential Dirac equations are solved by expanding the Dirac spinor on the spherical Dirac Woods-Saxon basis. The reliability of the newly developed O-RHF model is demonstrated by taking the octupole nucleus\begin{document}$ ^{144} {\rm{Ba}}$\end{document} ![]()
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\begin{document}$ ^{144} {\rm{Ba}}$\end{document} ![]()
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\begin{document}$ i = 1,2,3 $\end{document} ![]()
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\begin{document}$ ^{144} {\rm{Ba}}$\end{document} ![]()
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\begin{document}$ 1i_{13/2} $\end{document} ![]()
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\begin{document}$ 1h_{11/2} $\end{document} ![]()
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\begin{document}$ ^{144} {\rm{Ba}}$\end{document} ![]()
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\begin{document}$ ^{144} {\rm{Ba}}$\end{document} ![]()
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\begin{document}$ ^{144} {\rm{Ba}}$\end{document} ![]()
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			An axially quadruple-octupole deformed relativistic Hartree-Fock (O-RHF) model with density-dependent meson-nucleon couplings is developed in this study. In this model, the reflection symmetry is not preserved, and the integro-differential Dirac equations are solved by expanding the Dirac spinor on the spherical Dirac Woods-Saxon basis. The reliability of the newly developed O-RHF model is demonstrated by taking the octupole nucleus
			            2025, 49(7): 074108. doi: 10.1088/1674-1137/add25a 
	   					
		        	
			        
		            	
		        
					Abstract: 
For even Th and U nuclei, the description of the energies of yrast bands in the Harris variable moment of inertia model is studied in its phenomenological application. For some of these nuclei, the results obtained in the microscopic version of the interacting boson model (IBM) are presented, in which high-spin excitation modes are also considered. For other nuclei, in scenarios where high-spin orbits are not highly significant in describing the properties of yrast bands, in addition to the Harris model, the IBM with a full standard Hamiltonian constructed only from s and d bosons is utilized. Because the Harris model is considered with no more than four parameters, it can be used for both heavy and superheavy nuclei to approximate the energies of high-spin states. This study on the properties of nuclei using various models reveals the possibilities of describing different behaviors of the moments of inertia in the IBM and outlines additional criteria for the implementation of band crossing.
		       
		        
		        
		        
			  
			For even Th and U nuclei, the description of the energies of yrast bands in the Harris variable moment of inertia model is studied in its phenomenological application. For some of these nuclei, the results obtained in the microscopic version of the interacting boson model (IBM) are presented, in which high-spin excitation modes are also considered. For other nuclei, in scenarios where high-spin orbits are not highly significant in describing the properties of yrast bands, in addition to the Harris model, the IBM with a full standard Hamiltonian constructed only from s and d bosons is utilized. Because the Harris model is considered with no more than four parameters, it can be used for both heavy and superheavy nuclei to approximate the energies of high-spin states. This study on the properties of nuclei using various models reveals the possibilities of describing different behaviors of the moments of inertia in the IBM and outlines additional criteria for the implementation of band crossing.
			            2025, 49(7): 074109. doi: 10.1088/1674-1137/adc65b 
	   					
		        	
			        
		            	
		        
					Abstract: 
The ground state properties of finite, bulk matter, and neutron stars are investigated using a proposed effective interaction (HPU4) of the relativistic mean field model (RMF) that incorporates self and cross-couplings of σ, ω, and ρ mesons with nucleons. This interaction has been constructed by fitting data on binding energies and charge radii of finite nuclei, neutron skin (\begin{document}$\Delta r_{{np}}$\end{document} ![]()
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\begin{document}$ ^{48} {\rm{Ca}}$\end{document} ![]()
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\begin{document}$\Delta r_{np}$\end{document} ![]()
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\begin{document}$ ^{48} {\rm{Ca}}$\end{document} ![]()
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\begin{document}$ J_{0} $\end{document} ![]()
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\begin{document}$ L_{0} $\end{document} ![]()
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\begin{document}$ ^{208} {\rm{Pb}}$\end{document} ![]()
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\begin{document}$ ^{48} {\rm{Ca}}$\end{document} ![]()
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\begin{document}$ J_{0} $\end{document} ![]()
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\begin{document}$ L_{0} $\end{document} ![]()
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\begin{document}$ K_{\text{sym}} $\end{document} ![]()
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\begin{document}$ R_{1.4} $\end{document} ![]()
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\begin{document}$ g_{\rho N} $\end{document} ![]()
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\begin{document}$ \sigma\rho_{\mu}\rho^{\mu} $\end{document} ![]()
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\begin{document}$ \sigma^{2}\rho_{\mu}\rho^{\mu} $\end{document} ![]()
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			The ground state properties of finite, bulk matter, and neutron stars are investigated using a proposed effective interaction (HPU4) of the relativistic mean field model (RMF) that incorporates self and cross-couplings of σ, ω, and ρ mesons with nucleons. This interaction has been constructed by fitting data on binding energies and charge radii of finite nuclei, neutron skin (
			            2025, 49(7): 074110. doi: 10.1088/1674-1137/add5d0 
	   					
		        	
			        
		            	
		        
					Abstract: 
Shape competition and coexistence between the pear- and the tetrahedral-shape octupole deformations in actinide nuclei is investigated by employing the realistic nuclear mean-field theory with the phenomenological, so-called 'universal' Woods-Saxon Hamiltonian with newly adjusted parameters containing no parametric correlations. Both types of octupole deformations exhibit significant effects in\begin{document}$ N=132 $\end{document} ![]()
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\begin{document}$ N=134 $\end{document} ![]()
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\begin{document}$ N=136 $\end{document} ![]()
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\begin{document}$ N=134 $\end{document} ![]()
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\begin{document}$ N=136 $\end{document} ![]()
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\begin{document}$^{218}_{\;\;86}{\rm{Rn}}_{132} $\end{document} ![]()
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\begin{document}$^{222}_{\;\;88}{\rm{Ra}}_{134} $\end{document} ![]()
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\begin{document}$^{222}_{\;\;86}{\rm{Rn}}_{136} $\end{document} ![]()
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			Shape competition and coexistence between the pear- and the tetrahedral-shape octupole deformations in actinide nuclei is investigated by employing the realistic nuclear mean-field theory with the phenomenological, so-called 'universal' Woods-Saxon Hamiltonian with newly adjusted parameters containing no parametric correlations. Both types of octupole deformations exhibit significant effects in
			            2025, 49(7): 074111. doi: 10.1088/1674-1137/adcf8e 
	   					
		        	
			        
		            	
		        
					Abstract: 
This paper discusses the structure and stability of quark stars (QSs) made of interacting quark matter. The discussion accounts for color superconductivity and perturbative QCD corrections. By combining this EoS with the Tolman-Oppenheimer-Volkoff (TOV) equations, we explore the mass-radius (\begin{document}$ M-R $\end{document} ![]()
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\begin{document}$ R^2 $\end{document} ![]()
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\begin{document}$ f(R) = R + a R^2 $\end{document} ![]()
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\begin{document}$ R^2 $\end{document} ![]()
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\begin{document}$ M-\rho_c $\end{document} ![]()
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\begin{document}$ 2M_{\odot} $\end{document} ![]()
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			This paper discusses the structure and stability of quark stars (QSs) made of interacting quark matter. The discussion accounts for color superconductivity and perturbative QCD corrections. By combining this EoS with the Tolman-Oppenheimer-Volkoff (TOV) equations, we explore the mass-radius (
			            2025, 49(7): 074112. doi: 10.1088/1674-1137/adcf8f 
	   					
		        	
			        
		            	
		        
					Abstract: 
The effects of the tensor force on the\begin{document}$2\nu\beta\beta$\end{document} ![]()
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\begin{document}$0\nu\beta\beta$\end{document} ![]()
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\begin{document}$^{76}{\rm{Ge}}$\end{document} ![]()
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\begin{document}$^{82}{\rm{Se}}$\end{document} ![]()
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\begin{document}$^{130}{\rm{Te}}$\end{document} ![]()
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\begin{document}$^{136}{\rm{Xe}}$\end{document} ![]()
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\begin{document}$J^{\pi}=0^{\pm}\sim 10^{\pm}$\end{document} ![]()
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\begin{document}$2\nu\beta\beta$\end{document} ![]()
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\begin{document}$0\nu\beta\beta$\end{document} ![]()
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\begin{document}$^{76}{\rm{Ge}}$\end{document} ![]()
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\begin{document}$^{82}{\rm{Se}}$\end{document} ![]()
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\begin{document}$^{130}{\rm{Te}}$\end{document} ![]()
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\begin{document}$^{136}{\rm{Xe}}$\end{document} ![]()
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\begin{document}$0\nu\beta\beta$\end{document} ![]()
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\begin{document}$1^+$\end{document} ![]()
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\begin{document}$2\nu\beta\beta$\end{document} ![]()
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\begin{document}$0\nu\beta\beta$\end{document} ![]()
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			The effects of the tensor force on the
			            2025, 49(7): 075101. doi: 10.1088/1674-1137/adcc8d 
	   					
		        	
			        
		            	
		        
					Abstract: 
Quasars serve as important cosmological probes; constructing accurate luminosity relations for them is essential for their use in cosmology. If the coefficients of such luminosity relations vary with redshift, they could introduce biases into cosmological constraints derived from quasars. In this paper, we conduct a detailed analysis of the redshift variation in the X-ray and ultraviolet (UV) luminosity (\begin{document}$ L_\mathrm{X} $\end{document} ![]()
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\begin{document}$ L_\mathrm{UV} $\end{document} ![]()
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\begin{document}$ L_\mathrm{X} $\end{document} ![]()
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\begin{document}$ L_\mathrm{UV} $\end{document} ![]()
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\begin{document}$ L_\mathrm{X} $\end{document} ![]()
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\begin{document}$ L_\mathrm{UV} $\end{document} ![]()
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\begin{document}$ L_\mathrm{X} $\end{document} ![]()
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\begin{document}$ L_\mathrm{UV} $\end{document} ![]()
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			Quasars serve as important cosmological probes; constructing accurate luminosity relations for them is essential for their use in cosmology. If the coefficients of such luminosity relations vary with redshift, they could introduce biases into cosmological constraints derived from quasars. In this paper, we conduct a detailed analysis of the redshift variation in the X-ray and ultraviolet (UV) luminosity (
			            2025, 49(7): 075102. doi: 10.1088/1674-1137/adc7e1 
	   					
		        	
			        
		            	
		        
					Abstract: 
Due to quantum gravitational effects, Barrow proposed that the black hole horizon is "fractalized" into a sphereflake. Based on this idea, in this work we investigate the phase structure and stability of Einstein-Power-Yang-Mills (EPYM) AdS black holes in the restricted phase space, assuming the black hole event horizon has a fractal structure. From the first law of thermodynamics for EPYM AdS black holes in the restricted phase space, we find that the mass parameter should be interpreted as the internal energy. Moreover, the Smarr relation for this system in the restricted phase space is not a homogeneous function due to the fractal structure, which differs significantly from the corresponding relation in the extended phase space. The presence of a fractal structure can be regarded as a probe for phase transitions. Interestingly, for a fixed central charge in the EPYM AdS black hole system with a fractal structure, a supercritical phase transition also exists, similar to the case in the standard EPYM AdS black hole system. Furthermore, we investigate the effects of the fractal parameter ∆ and non-linear Yang-Mills parameter γ on the thermodynamical stability of this system are also investigated.
		       
		        
		        
		        
			  
			Due to quantum gravitational effects, Barrow proposed that the black hole horizon is "fractalized" into a sphereflake. Based on this idea, in this work we investigate the phase structure and stability of Einstein-Power-Yang-Mills (EPYM) AdS black holes in the restricted phase space, assuming the black hole event horizon has a fractal structure. From the first law of thermodynamics for EPYM AdS black holes in the restricted phase space, we find that the mass parameter should be interpreted as the internal energy. Moreover, the Smarr relation for this system in the restricted phase space is not a homogeneous function due to the fractal structure, which differs significantly from the corresponding relation in the extended phase space. The presence of a fractal structure can be regarded as a probe for phase transitions. Interestingly, for a fixed central charge in the EPYM AdS black hole system with a fractal structure, a supercritical phase transition also exists, similar to the case in the standard EPYM AdS black hole system. Furthermore, we investigate the effects of the fractal parameter ∆ and non-linear Yang-Mills parameter γ on the thermodynamical stability of this system are also investigated.
			            2025, 49(7): 075103. doi: 10.1088/1674-1137/adc2db 
	   					
		        	
			        
		            	
		        
					Abstract: 
Compact binary systems lose orbital energy and momentum because of gravitational radiation. Based on the mass and mass-current multipole moments of the binary system with the spin vector defined by Bohé et al. [Class. Quantum Grav. 30, 075017 (2013)], we calculate the loss rates of energy, angular momentum and linear momentum induced by the next-to-leading spin-orbit effects. For the case of circular orbit, the formulations the these losses are formulated in terms of orbital frequency.
		       
		        
		        
			  
			Compact binary systems lose orbital energy and momentum because of gravitational radiation. Based on the mass and mass-current multipole moments of the binary system with the spin vector defined by Bohé et al. [Class. Quantum Grav. 30, 075017 (2013)], we calculate the loss rates of energy, angular momentum and linear momentum induced by the next-to-leading spin-orbit effects. For the case of circular orbit, the formulations the these losses are formulated in terms of orbital frequency.
			            2025, 49(7): 075104. doi: 10.1088/1674-1137/adc3fc 
	   					
		        	
			        
		            	
		        
					Abstract: 
In this study, we investigate the optical appearance of a charged black hole in the Kalb-Ramond background, incorporating a Lorentz-violating parameter\begin{document}$ l=0.01 $\end{document} ![]()
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\begin{document}$ l=0 $\end{document} ![]()
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\begin{document}$ l=0.05 $\end{document} ![]()
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\begin{document}$ l=0.1 $\end{document} ![]()
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			In this study, we investigate the optical appearance of a charged black hole in the Kalb-Ramond background, incorporating a Lorentz-violating parameter
			            2025, 49(7): 075105. doi: 10.1088/1674-1137/adc188 
	   					
		        	
			        
		            	
		        
					Abstract: 
This study explores black holes in general relativity (GR) coupled with nonlinear electrodynamics (NED) in the presence of perfect fluid dark matter (PFDM). We derive a singular black hole solution and investigate its thermodynamic properties, including the black hole temperature, entropy, and specific heat capacity of the black hole spacetime. The analysis of energy conditions reveals deviations from standard GR, with PFDM affecting the weak and strong energy conditions. The study further examines the impact of NED and PFDM on the innermost stable circular orbit (ISCO), demonstrating that PFDM shifts the ISCO radius and that the combined effects of NED and PFDM field parameters sufficiently influence orbital stability. Our analysis of the black hole shadow reveals that PFDM increases the shadow radius, while a higher charge reduces it, leading to modifications in potential astrophysical observables. The thermodynamic behavior of the black hole exhibits phase transitions marked by changes in heat capacity, indicating possible stability regimes. Moreover, we derive equations for black hole shadow size and study the spacetime effects on the shadow. These results provide a framework for testing alternative gravity theories and understanding the role of exotic matter in strong gravitational fields. Finally, we compare the constraints on NED and PFDM field parameters derived from our black hole model with the Event Horizon Telescope (EHT) observations of M87* and Sgr A*, providing observational limits on deviations from GR.
		       
		        
		        
		        
			  
			This study explores black holes in general relativity (GR) coupled with nonlinear electrodynamics (NED) in the presence of perfect fluid dark matter (PFDM). We derive a singular black hole solution and investigate its thermodynamic properties, including the black hole temperature, entropy, and specific heat capacity of the black hole spacetime. The analysis of energy conditions reveals deviations from standard GR, with PFDM affecting the weak and strong energy conditions. The study further examines the impact of NED and PFDM on the innermost stable circular orbit (ISCO), demonstrating that PFDM shifts the ISCO radius and that the combined effects of NED and PFDM field parameters sufficiently influence orbital stability. Our analysis of the black hole shadow reveals that PFDM increases the shadow radius, while a higher charge reduces it, leading to modifications in potential astrophysical observables. The thermodynamic behavior of the black hole exhibits phase transitions marked by changes in heat capacity, indicating possible stability regimes. Moreover, we derive equations for black hole shadow size and study the spacetime effects on the shadow. These results provide a framework for testing alternative gravity theories and understanding the role of exotic matter in strong gravitational fields. Finally, we compare the constraints on NED and PFDM field parameters derived from our black hole model with the Event Horizon Telescope (EHT) observations of M87* and Sgr A*, providing observational limits on deviations from GR.
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