2022 Vol. 46, No. 11
Display Method: |
2022, 46(11): 111001. doi: 10.1088/1674-1137/ac827c
Abstract:
The isotopic cross sections of residual nuclei produced in fragmentation reactions of 18O projectiles impinging on a carbon target at energies near 260 MeV/nucleon were measured at the HIRFL facility in Lanzhou (China). A full identification of atomic and mass numbers of fragments was achieved from the determination of their magnetic rigidity, energy loss, and time of flight. The production cross sections for a dozen of nitrogen, carbon, and boron isotopes were determined with uncertainties below 30% for most of the cases. The obtained cross sections for N and B isotopes show a rather good agreement with previous experimental data obtained with different projectile energies. The cross sections for some C isotopes seem to exhibit a dependence on the projectile energy. A comparison of the data and several theoretical model calculations are presented.
The isotopic cross sections of residual nuclei produced in fragmentation reactions of 18O projectiles impinging on a carbon target at energies near 260 MeV/nucleon were measured at the HIRFL facility in Lanzhou (China). A full identification of atomic and mass numbers of fragments was achieved from the determination of their magnetic rigidity, energy loss, and time of flight. The production cross sections for a dozen of nitrogen, carbon, and boron isotopes were determined with uncertainties below 30% for most of the cases. The obtained cross sections for N and B isotopes show a rather good agreement with previous experimental data obtained with different projectile energies. The cross sections for some C isotopes seem to exhibit a dependence on the projectile energy. A comparison of the data and several theoretical model calculations are presented.
2022, 46(11): 111002. doi: 10.1088/1674-1137/ac945c
Abstract:
The cross sections of\begin{document}$ e^+e^- \rightarrow K^+K^-J/\psi $\end{document} ![]()
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\begin{document}$ ^{-1} $\end{document} ![]()
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\begin{document}$ 4225.3\pm2.3\pm21.5 $\end{document} ![]()
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\begin{document}$ 72.9\pm6.1\pm30.8 $\end{document} ![]()
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\begin{document}$ Y(4230) $\end{document} ![]()
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\begin{document}$ Y(4500) $\end{document} ![]()
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\begin{document}$ 4484.7\pm13.3\pm24.1 $\end{document} ![]()
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\begin{document}$ 111.1\pm30.1\pm15.2 $\end{document} ![]()
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\begin{document}$ \Gamma(Y(4230)\to e^+ e^-) \mathcal{B}(Y(4230) \to K^+ K^- J/\psi) $\end{document} ![]()
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The cross sections of
2022, 46(11): 112001. doi: 10.1088/1674-1137/ac84ca
Abstract:
It is currently widely accepted that gluons, while massless at the level of the fundamental QCD Lagrangian, acquire an effective mass through the non-Abelian implementation of the classic Schwinger mechanism. The key dynamical ingredient that triggers the onset of this mechanism is the formation of composite massless poles inside the fundamental vertices of the theory. These poles enter the evolution equation of the gluon propagator and nontrivially affect the way the Slavnov-Taylor identities of the vertices are resolved, inducing a smoking-gun displacement in the corresponding Ward identities. In this article, we present a comprehensive review of the pivotal concepts associated with this dynamical scenario, emphasizing the synergy between functional methods and lattice simulations and highlighting recent advances that corroborate the action of the Schwinger mechanism in QCD.
It is currently widely accepted that gluons, while massless at the level of the fundamental QCD Lagrangian, acquire an effective mass through the non-Abelian implementation of the classic Schwinger mechanism. The key dynamical ingredient that triggers the onset of this mechanism is the formation of composite massless poles inside the fundamental vertices of the theory. These poles enter the evolution equation of the gluon propagator and nontrivially affect the way the Slavnov-Taylor identities of the vertices are resolved, inducing a smoking-gun displacement in the corresponding Ward identities. In this article, we present a comprehensive review of the pivotal concepts associated with this dynamical scenario, emphasizing the synergy between functional methods and lattice simulations and highlighting recent advances that corroborate the action of the Schwinger mechanism in QCD.
2022, 46(11): 113001. doi: 10.1088/1674-1137/ac7f21
Abstract:
Various Higgs factories are proposed to study the Higgs boson precisely and systematically in a model- independent way. In this study, the Particle Flow Network and ParticleNet techniques are used to classify the Higgs decays into multicategories, and the ultimate goal is to realize an "end-to-end" analysis. A Monte Carlo simulation study is performed to demonstrate the feasibility, and the performance looks rather promising. This result could be the basis of a "one-stop" analysis to measure all the branching fractions of the Higgs decays simultaneously.
Various Higgs factories are proposed to study the Higgs boson precisely and systematically in a model- independent way. In this study, the Particle Flow Network and ParticleNet techniques are used to classify the Higgs decays into multicategories, and the ultimate goal is to realize an "end-to-end" analysis. A Monte Carlo simulation study is performed to demonstrate the feasibility, and the performance looks rather promising. This result could be the basis of a "one-stop" analysis to measure all the branching fractions of the Higgs decays simultaneously.
2022, 46(11): 113002. doi: 10.1088/1674-1137/ac80b4
Abstract:
The integrated luminosities of data samples collected in the BESIII experiment in 2016–2017 at center-of-mass energies between 4.19 and 4.28 GeV are measured with a precision better than 1% by analyzing large-angle Bhabha scattering events. The integrated luminosities of old datasets collected in 2010–2014 are updated by considering corrections related to detector performance, offsetting the effect of newly discovered readout errors in the electromagnetic calorimeter, which can haphazardly occur.
The integrated luminosities of data samples collected in the BESIII experiment in 2016–2017 at center-of-mass energies between 4.19 and 4.28 GeV are measured with a precision better than 1% by analyzing large-angle Bhabha scattering events. The integrated luminosities of old datasets collected in 2010–2014 are updated by considering corrections related to detector performance, offsetting the effect of newly discovered readout errors in the electromagnetic calorimeter, which can haphazardly occur.
2022, 46(11): 113003. doi: 10.1088/1674-1137/ac84cc
Abstract:
From December 2019 to June 2021, the BESIII experiment collected approximately 5.85 fb−1 of data at center-of-mass energies between 4.61 and 4.95 GeV. This is the highest collision energy BEPCII has reached to date. The accumulated\begin{document}$e^+e^-$\end{document} ![]()
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\begin{document}$\Lambda_{c}^{+}\bar{\Lambda}_{c}^{-}$\end{document} ![]()
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\begin{document}$e^+e^-$\end{document} ![]()
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\begin{document}$\sim$\end{document} ![]()
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From December 2019 to June 2021, the BESIII experiment collected approximately 5.85 fb−1 of data at center-of-mass energies between 4.61 and 4.95 GeV. This is the highest collision energy BEPCII has reached to date. The accumulated
2022, 46(11): 113101. doi: 10.1088/1674-1137/ac80ef
Abstract:
The physical state of\begin{document}$ \rho-\omega-\phi $\end{document} ![]()
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\begin{document}$ \omega \rightarrow \pi^{+}\pi^{-} $\end{document} ![]()
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\begin{document}$ \phi \rightarrow \pi^{+}\pi^{-} $\end{document} ![]()
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\begin{document}$ \rho-\omega $\end{document} ![]()
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\begin{document}$ \rho-\phi $\end{document} ![]()
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\begin{document}$ \omega-\phi $\end{document} ![]()
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\begin{document}$ CP $\end{document} ![]()
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\begin{document}$ CP $\end{document} ![]()
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\begin{document}$ B^{0}\rightarrow \pi^+\pi^{-}\eta^{(')} $\end{document} ![]()
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\begin{document}$ \pi^+\pi^{-} $\end{document} ![]()
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\begin{document}$ \omega $\end{document} ![]()
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\begin{document}$ \phi $\end{document} ![]()
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\begin{document}$ CP $\end{document} ![]()
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The physical state of
2022, 46(11): 113102. doi: 10.1088/1674-1137/ac80f0
Abstract:
Although\begin{document}$ d^*(2380) $\end{document} ![]()
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\begin{document}$ d^*(2380) $\end{document} ![]()
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\begin{document}$ p{\bar{p}}\to d^*(2380){\bar{p}}{\bar{n}} $\end{document} ![]()
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\begin{document}$ {\bar{{\rm{P}}}} $\end{document} ![]()
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\begin{document}$ {d^*} $\end{document} ![]()
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\begin{document}$ p{\bar{p}}\to d^*(2380){\bar{p}}{\bar{n}} $\end{document} ![]()
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\begin{document}$ \Delta{\bar{\Delta}} $\end{document} ![]()
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\begin{document}$ nb $\end{document} ![]()
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\begin{document}$ {\bar{\Delta}}{\bar{\Delta}}\to {\bar{p}}{\bar{n}} $\end{document} ![]()
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\begin{document}$ {\bar{d^*}}\to {\bar{p}}{\bar{n}} $\end{document} ![]()
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\begin{document}$ 3\%\sim 4\% $\end{document} ![]()
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\begin{document}$ {\bar{{\rm{P}}}} $\end{document} ![]()
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\begin{document}$ {\bar{p}} $\end{document} ![]()
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\begin{document}$ {\bar{n}} $\end{document} ![]()
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\begin{document}$ {\bar{d^*}} $\end{document} ![]()
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Although
2022, 46(11): 113103. doi: 10.1088/1674-1137/ac814e
Abstract:
Previous studies have indicated that the peak of the quarkonium entropy at the deconfinement transition can be related to the entropic force, which would induce the dissociation of heavy quarkonium. In this study, we investigated the entropic force in a rotating hot and dense medium using AdS/CFT correspondence. It was found that the inclusion of angular velocity increases the entropic force, thus enhancing quarkonium dissociation, while chemical potential has the same effect. The results imply that the quarkonium dissociates easier in rotating medium compared with the static case.
Previous studies have indicated that the peak of the quarkonium entropy at the deconfinement transition can be related to the entropic force, which would induce the dissociation of heavy quarkonium. In this study, we investigated the entropic force in a rotating hot and dense medium using AdS/CFT correspondence. It was found that the inclusion of angular velocity increases the entropic force, thus enhancing quarkonium dissociation, while chemical potential has the same effect. The results imply that the quarkonium dissociates easier in rotating medium compared with the static case.
2022, 46(11): 113104. doi: 10.1088/1674-1137/ac827b
Abstract:
The associated production of a dark particle and photon, represented as a mono-γ event, is a promising channel to probe particle content and dynamics in the dark sector. In this study, we investigate the properties of the mono-γ production of vector dark matter at future\begin{document}$ e^+e^- $\end{document} ![]()
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The associated production of a dark particle and photon, represented as a mono-γ event, is a promising channel to probe particle content and dynamics in the dark sector. In this study, we investigate the properties of the mono-γ production of vector dark matter at future
2022, 46(11): 113105. doi: 10.1088/1674-1137/ac82e1
Abstract:
In the standard model effective field theory, operators involving the top quark are generally difficult to probe and can generate sizable loop contributions to electroweak precision observables measured by past and future lepton colliders. Could the high precision of electroweak measurements compensate for loop suppression and provide competitive reaches on these operators? Would the inclusion of these contributions introduce too many additional parameters for a meaningful global electroweak analysis to be performed? In this paper, we perform a detailed phenomenological study to address these two important questions. Focusing on eight dimension-6 operators that generate anomalous couplings between electroweak gauge bosons and third-generation quarks, we calculate their one loop contributions to\begin{document}$ e^+e^- \to f\bar{f} $\end{document} ![]()
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\begin{document}$ e^-e^+ \to WW $\end{document} ![]()
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In the standard model effective field theory, operators involving the top quark are generally difficult to probe and can generate sizable loop contributions to electroweak precision observables measured by past and future lepton colliders. Could the high precision of electroweak measurements compensate for loop suppression and provide competitive reaches on these operators? Would the inclusion of these contributions introduce too many additional parameters for a meaningful global electroweak analysis to be performed? In this paper, we perform a detailed phenomenological study to address these two important questions. Focusing on eight dimension-6 operators that generate anomalous couplings between electroweak gauge bosons and third-generation quarks, we calculate their one loop contributions to
2022, 46(11): 113106. doi: 10.1088/1674-1137/ac8653
Abstract:
We systematically study the magnetic dipole moments of multiquark states. In this study, the magnetic dipole moments of possible\begin{document}$ B^- B^{*-} $\end{document} ![]()
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\begin{document}$ B^0 B^{*-} $\end{document} ![]()
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\begin{document}$ B^- B^{*0} $\end{document} ![]()
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\begin{document}$ B^0 B^{*0} $\end{document} ![]()
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\begin{document}$ B_s^0 B^{*-} $\end{document} ![]()
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\begin{document}$ B^- B_s^{*0} $\end{document} ![]()
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\begin{document}$ B_s^{0} B^{*0} $\end{document} ![]()
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\begin{document}$ B^0 B_s^{*0} $\end{document} ![]()
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\begin{document}$ B^0_s B_s^{*0} $\end{document} ![]()
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\begin{document}$ J^P = 1^+ $\end{document} ![]()
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We systematically study the magnetic dipole moments of multiquark states. In this study, the magnetic dipole moments of possible
2022, 46(11): 113107. doi: 10.1088/1674-1137/ac8652
Abstract:
In this study, we calculate the transition form factors of\begin{document}$ \Lambda_b $\end{document} ![]()
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\begin{document}$ \Lambda_c $\end{document} ![]()
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\begin{document}$ \Lambda_b $\end{document} ![]()
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\begin{document}$ \Lambda_c $\end{document} ![]()
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\begin{document}$ \Lambda_c^* $\end{document} ![]()
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\begin{document}$ \Lambda_b \rightarrow \Lambda_c $\end{document} ![]()
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\begin{document}$ \Lambda_b $\end{document} ![]()
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\begin{document}$ \Lambda_b \rightarrow \Lambda_c $\end{document} ![]()
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\begin{document}$ \Lambda_b \to \Lambda_c \ell\mu $\end{document} ![]()
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\begin{document}$ R_{\Lambda_c} $\end{document} ![]()
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\begin{document}$ R_{\Lambda_c} $\end{document} ![]()
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In this study, we calculate the transition form factors of
Determination of the half-life of 184gRe and the isomeric ratio of 184m, gRe induced by D-T neutrons
2022, 46(11): 114001. doi: 10.1088/1674-1137/ac7f88
Abstract:
The isomeric ratio of 184m, gRe and the half-life of 184gRe were measured in the 185Re (n, 2n) 184Re reaction at 14.8 MeV, and the uncertainty was discussed in detail. The measurements were performed using the activation method implemented for a rhenium sample using the K-400 neutron generator at the Chinese Academy of Engineering Physics (CAEP). Isomeric state and ground state nuclei of 184Re were identified by their γ-ray spectra. To eliminate the effect of the γ-ray emitted from the isomer on the counting of the ground state characteristic peaks, the isomeric ratio of 184m, gRe was calculated to be 0.29 ± 0.11 according to the neutron activation cross-section formula. This result is consistent with previous data within the uncertainty and can be used to determine parameters that characterize the dependence of the level density on the excitation energy and angular momentum. Through exponential function fitting and a detailed discussion of the uncertainty evaluation, the half-life of 184gRe was determined as 35.43 ± 0.16 d, which is consistent with the currently recommended value; however, the uncertainty assessment of the latter was barely documented. In addition, this study indicates that the half-life of the ground state can be obtained by eliminating the contamination of γ-rays emitted from the isomer, which provides the possibility of determining the half-lives of nuclides containing isomers.
The isomeric ratio of 184m, gRe and the half-life of 184gRe were measured in the 185Re (n, 2n) 184Re reaction at 14.8 MeV, and the uncertainty was discussed in detail. The measurements were performed using the activation method implemented for a rhenium sample using the K-400 neutron generator at the Chinese Academy of Engineering Physics (CAEP). Isomeric state and ground state nuclei of 184Re were identified by their γ-ray spectra. To eliminate the effect of the γ-ray emitted from the isomer on the counting of the ground state characteristic peaks, the isomeric ratio of 184m, gRe was calculated to be 0.29 ± 0.11 according to the neutron activation cross-section formula. This result is consistent with previous data within the uncertainty and can be used to determine parameters that characterize the dependence of the level density on the excitation energy and angular momentum. Through exponential function fitting and a detailed discussion of the uncertainty evaluation, the half-life of 184gRe was determined as 35.43 ± 0.16 d, which is consistent with the currently recommended value; however, the uncertainty assessment of the latter was barely documented. In addition, this study indicates that the half-life of the ground state can be obtained by eliminating the contamination of γ-rays emitted from the isomer, which provides the possibility of determining the half-lives of nuclides containing isomers.
2022, 46(11): 114002. doi: 10.1088/1674-1137/ac8227
Abstract:
The results of experiments on measuring the energy spectra of alpha particles in reactions with heavy ions are presented. The measurements were performed using the high-resolution magnetic analyzer MAVR with beams of 48Ca (280 MeV) and 56Fe (320 and 400 MeV) on 181Ta and 238U targets at an angle of 0°. A strong dependence of the double differential cross sections for production of alpha particles on the atomic number of the target nucleus was observed, which indicates that fast alpha particles are mainly emitted from the target nucleus; this conclusion was also confirmed by calculations within the time-dependent Schrödinger equation approach. An analysis of the obtained experimental data was carried out within the model of moving sources modified to consider the kinematic limits for two-body and three-body exit channels.
The results of experiments on measuring the energy spectra of alpha particles in reactions with heavy ions are presented. The measurements were performed using the high-resolution magnetic analyzer MAVR with beams of 48Ca (280 MeV) and 56Fe (320 and 400 MeV) on 181Ta and 238U targets at an angle of 0°. A strong dependence of the double differential cross sections for production of alpha particles on the atomic number of the target nucleus was observed, which indicates that fast alpha particles are mainly emitted from the target nucleus; this conclusion was also confirmed by calculations within the time-dependent Schrödinger equation approach. An analysis of the obtained experimental data was carried out within the model of moving sources modified to consider the kinematic limits for two-body and three-body exit channels.
2022, 46(11): 114101. doi: 10.1088/1674-1137/ac7eb3
Abstract:
In this study, we investigate formulas of the number of states with a given total spin I and isospin T for n nucleons in a single-j shell denoted by\begin{document}$ D_{IT} (j, n) $\end{document} ![]()
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\begin{document}$ D_{IT} (j, n) $\end{document} ![]()
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In this study, we investigate formulas of the number of states with a given total spin I and isospin T for n nucleons in a single-j shell denoted by
2022, 46(11): 114102. doi: 10.1088/1674-1137/ac7fe6
Abstract:
Color screening and parton inelastic scattering modify the heavy-quark antiquark potential in mediums consisting of particles from quantum chromodynamics (QCD), leading to the suppression of quarkonium production in relativistic heavy-ion collisions. Owing to the small charm/anti-charm (\begin{document}$ c\bar{c} $\end{document} ![]()
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\begin{document}$ c\bar{c} $\end{document} ![]()
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\begin{document}$ c\bar{c} $\end{document} ![]()
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\begin{document}$ c\bar{c} $\end{document} ![]()
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\begin{document}$ c\bar{c} $\end{document} ![]()
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\begin{document}$R_{pA}$\end{document} ![]()
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\begin{document}$ J/\psi $\end{document} ![]()
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\begin{document}$ \psi(2S) $\end{document} ![]()
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\begin{document}$ \sqrt{s_{NN}}=5.02 $\end{document} ![]()
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Color screening and parton inelastic scattering modify the heavy-quark antiquark potential in mediums consisting of particles from quantum chromodynamics (QCD), leading to the suppression of quarkonium production in relativistic heavy-ion collisions. Owing to the small charm/anti-charm (
2022, 46(11): 114103. doi: 10.1088/1674-1137/ac7fe8
Abstract:
In the present work, we systematically study the α-decay half-lives of uranium (Z=92) isotopes based on the Gamow model with a screened electrostatic barrier. There are only two adjustable parameters in our model i.e. the parameter g and the screening parameter t in the Hulthen potential for considering the screened electrostatic effect of the Coulomb potential. The calculated results are in good agreement with experimental data, and the corresponding root-mean-square (rms) deviations of uranium isotopes with α transition orbital angular momentum l=0 and l=2 are 0.141 and 0.340, respectively. Moreover, we extend this model to predict α-decay half-lives of uranium isotopes whose α decay is energetically allowed or observed but not yet quantified in NUBASE2020. For comparison, the modified Hatsukawa formula (XLZ), the unified Royer formula (DZR), the universal decay law (UDL) and the Viola–Seaborg–Sobiczewski formula (VSS) are also used. The predictions are basically consistent with each other. Meanwhile, the results also indicate that N=126 shell closure is still robust at Z=92 and the spectroscopic factor\begin{document}$ S_{\alpha} $\end{document} ![]()
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In the present work, we systematically study the α-decay half-lives of uranium (Z=92) isotopes based on the Gamow model with a screened electrostatic barrier. There are only two adjustable parameters in our model i.e. the parameter g and the screening parameter t in the Hulthen potential for considering the screened electrostatic effect of the Coulomb potential. The calculated results are in good agreement with experimental data, and the corresponding root-mean-square (rms) deviations of uranium isotopes with α transition orbital angular momentum l=0 and l=2 are 0.141 and 0.340, respectively. Moreover, we extend this model to predict α-decay half-lives of uranium isotopes whose α decay is energetically allowed or observed but not yet quantified in NUBASE2020. For comparison, the modified Hatsukawa formula (XLZ), the unified Royer formula (DZR), the universal decay law (UDL) and the Viola–Seaborg–Sobiczewski formula (VSS) are also used. The predictions are basically consistent with each other. Meanwhile, the results also indicate that N=126 shell closure is still robust at Z=92 and the spectroscopic factor
2022, 46(11): 114104. doi: 10.1088/1674-1137/ac80ee
Abstract:
In this study, we adopt the self-consistent Hartree-Fock-Bogoliubov (HFB) theory with the proton-neutron quasi-particle random phase approximation (pnQRPA) based on the Skyrme force for calculation of the β− decay half-lives for nuclei with N ~ 82 and 126 on possible r-process paths. In the calculations, the Skyrme interaction (e.g., SKO') is adopted, and the tensor interaction is added self-consistently in both HFB and QRPA calculations. We systematically study how the half-life is changed by varying the strength of the triplet-even (TE) and triplet-odd (TO) components as well as the IS pairing. We find that a variation in strength of the IS pairing of approximately 20% does not produce a substantial effect on β-decay rates with or without the tensor force, while a strength variation of the TO tensor force considerably affects the change in the β-decay half-lives for the very neutron rich N ~ 82 and 126 isotonic chains. In addition, with the inclusion of the tensor force, the GT decay becomes dominant for very neutron-rich nuclei.
In this study, we adopt the self-consistent Hartree-Fock-Bogoliubov (HFB) theory with the proton-neutron quasi-particle random phase approximation (pnQRPA) based on the Skyrme force for calculation of the β− decay half-lives for nuclei with N ~ 82 and 126 on possible r-process paths. In the calculations, the Skyrme interaction (e.g., SKO') is adopted, and the tensor interaction is added self-consistently in both HFB and QRPA calculations. We systematically study how the half-life is changed by varying the strength of the triplet-even (TE) and triplet-odd (TO) components as well as the IS pairing. We find that a variation in strength of the IS pairing of approximately 20% does not produce a substantial effect on β-decay rates with or without the tensor force, while a strength variation of the TO tensor force considerably affects the change in the β-decay half-lives for the very neutron rich N ~ 82 and 126 isotonic chains. In addition, with the inclusion of the tensor force, the GT decay becomes dominant for very neutron-rich nuclei.
2022, 46(11): 114105. doi: 10.1088/1674-1137/ac82e2
Abstract:
The critical parameters of the liquid-gas phase transition of symmetric nuclear matter are computed using the Brueckner-Hartree-Fock method at finite temperature by employing different realistic nucleon-nucleon potentials. Temperature effects on single-particle potentials, defect functions, and three-body forces are discussed in detail. Results obtained from the full procedure and frozen-correlations approximation are compared. We find critical temperatures of approximately 14 to 19 MeV and critical densities in the range of\begin{document}$ 0.05 $\end{document} ![]()
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\begin{document}$ 0.08{\;\mathrm{fm}^{-3}} $\end{document} ![]()
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The critical parameters of the liquid-gas phase transition of symmetric nuclear matter are computed using the Brueckner-Hartree-Fock method at finite temperature by employing different realistic nucleon-nucleon potentials. Temperature effects on single-particle potentials, defect functions, and three-body forces are discussed in detail. Results obtained from the full procedure and frozen-correlations approximation are compared. We find critical temperatures of approximately 14 to 19 MeV and critical densities in the range of
2022, 46(11): 114106. doi: 10.1088/1674-1137/ac82e3
Abstract:
The dibaryon concept for nuclear force is presented, assuming that the attraction between nucleons at medium distances is mainly due to the s-channel exchange of an intermediate six-quark (dibaryon) state. To construct the respective NN interaction model, a microscopic six-quark description of the NN system is used, in which symmetry aspects play a special role. It is shown that the NN interaction in all important partial waves can be described by the superposition of long-range t-channel one-pion exchange and s-channel exchange by an intermediate dibaryon. The model developed in this study provides a good description of both elastic phase shifts and inelasticities of NN scattering in all S, P, D, and F partial waves at energies from zero to 600–800 MeV and even higher. The parameters of the intermediate six-quark states, corresponding to the best fit of NN scattering data, are found to be consistent with the parameters of the known dibaryon resonances in those NN partial configurations, where their existence has been experimentally confirmed. Predictions for new dibaryon states are given as well.
The dibaryon concept for nuclear force is presented, assuming that the attraction between nucleons at medium distances is mainly due to the s-channel exchange of an intermediate six-quark (dibaryon) state. To construct the respective NN interaction model, a microscopic six-quark description of the NN system is used, in which symmetry aspects play a special role. It is shown that the NN interaction in all important partial waves can be described by the superposition of long-range t-channel one-pion exchange and s-channel exchange by an intermediate dibaryon. The model developed in this study provides a good description of both elastic phase shifts and inelasticities of NN scattering in all S, P, D, and F partial waves at energies from zero to 600–800 MeV and even higher. The parameters of the intermediate six-quark states, corresponding to the best fit of NN scattering data, are found to be consistent with the parameters of the known dibaryon resonances in those NN partial configurations, where their existence has been experimentally confirmed. Predictions for new dibaryon states are given as well.
2022, 46(11): 115001. doi: 10.1088/1674-1137/ac8539
Abstract:
Neutron-induced nuclear recoil background is critical to dark matter searches in the PandaX-4T liquid xenon experiment. In this study, we investigate the features of neutron background in liquid xenon and evaluate its contribution in single scattering nuclear recoil events using three methods. The first method is fully based on Monte Carlo simulations. The last two are data-driven methods that also use multiple scattering signals and high energy signals in the data. In the PandaX-4T commissioning data with an exposure of 0.63 tonne-year, all these methods give a consistent result, i.e., there are\begin{document}$ 1.15\pm0.57 $\end{document} ![]()
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Neutron-induced nuclear recoil background is critical to dark matter searches in the PandaX-4T liquid xenon experiment. In this study, we investigate the features of neutron background in liquid xenon and evaluate its contribution in single scattering nuclear recoil events using three methods. The first method is fully based on Monte Carlo simulations. The last two are data-driven methods that also use multiple scattering signals and high energy signals in the data. In the PandaX-4T commissioning data with an exposure of 0.63 tonne-year, all these methods give a consistent result, i.e., there are
2022, 46(11): 115101. doi: 10.1088/1674-1137/ac7f22
Abstract:
In this study, we obtain wormhole solutions in the recently proposed extension of symmetric teleparallel gravity, known as\begin{document}$ f(Q,T) $\end{document} ![]()
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\begin{document}$ f(Q,T) $\end{document} ![]()
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\begin{document}$ f(Q,T) $\end{document} ![]()
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\begin{document}$ f(Q,T)=\alpha Q+\beta T $\end{document} ![]()
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\begin{document}$ f(Q,T)=Q+\lambda Q^2+\eta T $\end{document} ![]()
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\begin{document}$ f(Q,T) $\end{document} ![]()
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In this study, we obtain wormhole solutions in the recently proposed extension of symmetric teleparallel gravity, known as
2022, 46(11): 115102. doi: 10.1088/1674-1137/ac814d
Abstract:
Considering the quantum electrodynamics (QED) effect, we study the phase transition and Ruppeiner geometry of Euler-Heisenberg anti-de Sitter black holes in the extended phase space. For negative and small positive QED parameters, we observe a small/large black hole phase transition and reentrant phase transition, respectively, whereas a large positive value of the QED parameter ruins the phase transition. Phase diagrams for each case are explicitly shown. Then, we construct the Ruppeiner geometry in thermodynamic parameter space. Different features of the corresponding scalar curvature are shown for both the small/large black hole phase transition and reentrant phase transition cases. Of particular interest is the additional region of positive scalar curvature, indicating a dominant repulsive interaction among black hole microstructures, for the black hole with a small positive QED parameter. Furthermore, universal critical phenomena are observed for the scalar curvature of Ruppeiner geometry. These results indicate that the QED parameter has a crucial influence on the black hole phase transition and microstructure.
Considering the quantum electrodynamics (QED) effect, we study the phase transition and Ruppeiner geometry of Euler-Heisenberg anti-de Sitter black holes in the extended phase space. For negative and small positive QED parameters, we observe a small/large black hole phase transition and reentrant phase transition, respectively, whereas a large positive value of the QED parameter ruins the phase transition. Phase diagrams for each case are explicitly shown. Then, we construct the Ruppeiner geometry in thermodynamic parameter space. Different features of the corresponding scalar curvature are shown for both the small/large black hole phase transition and reentrant phase transition cases. Of particular interest is the additional region of positive scalar curvature, indicating a dominant repulsive interaction among black hole microstructures, for the black hole with a small positive QED parameter. Furthermore, universal critical phenomena are observed for the scalar curvature of Ruppeiner geometry. These results indicate that the QED parameter has a crucial influence on the black hole phase transition and microstructure.
2022, 46(11): 115103. doi: 10.1088/1674-1137/ac84cb
Abstract:
Recent advances in nuclear theory and new astrophysical observations have led to the need for specific theoretical models applicable to dense-matter physics phenomena. Quantum chromodynamics (QCD) predicts the existence of non-nucleonic degrees of freedom at high densities in neutron-star matter, such as quark matter. Within a confining quark matter model, which consists of homogeneous, neutral 3-flavor interacting quark matter with\begin{document}$ \mathcal{O}(m_s^4) $\end{document} ![]()
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Recent advances in nuclear theory and new astrophysical observations have led to the need for specific theoretical models applicable to dense-matter physics phenomena. Quantum chromodynamics (QCD) predicts the existence of non-nucleonic degrees of freedom at high densities in neutron-star matter, such as quark matter. Within a confining quark matter model, which consists of homogeneous, neutral 3-flavor interacting quark matter with
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