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Ab initio computations from 78Ni towards 70Ca along neutron number N = 50 沿中子数 N = 50 从 78Ni 到 70Ca 的 Ab initio 计算
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-11 DOI: 10.1016/j.physletb.2024.139010

We present coupled-cluster computations of nuclei with neutron number N=50 “south” of 78Ni using nucleon-nucleon and three-nucleon forces from chiral effective field theory. We find an erosion of the magic number N=50 toward 70Ca manifesting itself by an onset of deformation and increased complexity in the ground states. For 78Ni, we predict a low-lying rotational band consistent with recent data, which up until now has been a challenge for ab initio nuclear models. Ground states are deformed in 76Fe, 74Cr, and 72Ti, although the spherical states are too close in energy to unambiguously identify the shape of the ground state within the uncertainty estimates. In 70Ca, the potential energy landscape from quadrupole-constrained Hartree-Fock computations flattens, and the deformation becomes less rigid. We also compute the low-lying spectra and B(E2) values for these neutron-rich N=50 nuclei.

我们利用手性有效场理论中的核子-核子力和三核子力,对 78Ni "以南 "中子数 N=50 的原子核进行了耦合-簇计算。我们发现神奇数字 N=50 在向 70Ca 移动的过程中会受到侵蚀,表现为基态开始变形,复杂性增加。对于 78Ni,我们预测出了一个与最新数据相一致的低洼旋转带,到目前为止,这一直是原子核模型所面临的挑战。在 76Fe、74Cr 和 72Ti 中,基态发生了变形,尽管球形态的能量过于接近,无法在不确定性估计范围内明确确定基态的形状。在 70Ca 中,四极约束哈特里-福克(Hartree-Fock)计算得出的势能图变得平缓,变形也变得不那么刚硬。我们还计算了这些富中子 N=50 核的低洼谱和 B(E2) 值。
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引用次数: 0
Gamma-ray signal from ZN≥3 dark matter-companion models 来自 ZN≥3 暗物质-伴星模型的伽马射线信号
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-10 DOI: 10.1016/j.physletb.2024.139011

In Ref. [10], we proposed to replace the final dark matter (DM) particle in the semi-annihilation mode DM+DMantiDM+Higgs boson with its ZN3 companion, thus reducing DM number density without DM-nucleon scattering. In this work, we study the indirect detection signals from DM annihilation, the Higgs boson pair with one of them from the companion decay being on- or off- shell, depending on the DM-companion mass splitting. We generate the photon spectrum by using PYTHIA8 and study the properties of the spectrum, to find that the hard part of the spectrum in our model is mainly shaped by the direct Higgs boson and thus does not differ much from that of the conventional semi-annihilation mode. Using the Fermi-LAT data of dwarf spheroidal galaxies, we derive the current limit of the DM annihilation cross section for DM+DMcompanion+Higgs boson, and for the relatively light DM, it reaches the typical thermal cross section. However, for the TeV scale DM, we have to rely on the Cherenkov Telescope Array, which is able to rule out the whole parameter space except for the coannihilation region.

在 Ref.中,我们提出了在半湮灭模式下用伴星取代最终暗物质(DM)粒子,从而在不发生DM-核散射的情况下降低DM的数量密度。在这项工作中,我们研究了来自DM湮灭的间接探测信号,希格斯玻色子对与其中一个来自伴星衰变的希格斯玻色子对是在壳内还是壳外,这取决于DM-伴星的质量分裂。我们利用PYTHIA8生成了光子谱,并研究了光子谱的性质,发现在我们的模型中,光子谱的硬部分主要是由直接希格斯玻色子形成的,因此与传统的半湮灭模式差别不大。利用矮球状星系的费米-LAT数据,我们推导出了DM湮灭截面的当前极限,对于相对较轻的DM,它达到了典型的热截面。然而,对于TeV尺度的DM,我们必须依靠切伦科夫望远镜阵列,它能够排除除共湮灭区域以外的整个参数空间。
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引用次数: 0
Mapping low-lying states and B(E2;01+→21+) in even-even nuclei with machine learning 用机器学习绘制偶偶数原子核中的低洼状态和[式省略]图谱
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-10 DOI: 10.1016/j.physletb.2024.139013

A machine-learning algorithm, Light Gradient Boosting Machine, was applied for the first time to investigate the fundamental experimental observables in even-even nuclei over the Segrè chart. Specifically, we focused on the excitation energies of the 21+ and 41+ states, and the reduced electric quadrupole transition probability B(E2;01+21+). Present obtained results well reproduced experimental data within an accuracy of 1.07, 1.05, and 1.14 times for the 21+ and 41+ states as well as B(E2;01+21+), respectively, being significantly precise than the results from any state-of-the-art nuclear models and from any machine-learning-based approaches. The predictive capability of our machine learning methodology was further validated using 17 newly measured data points which were not used in the training set. Taking O, Ca, Sn, and Pb isotopes as examples, it has been found that our methodology precisely captures both the isotopic trend and absolute values, surpassing all theoretical models hitherto. Our findings reveal the double-magic nature of 100Sn and the disappearance of the N=20 shell in 28O.

我们首次采用了一种机器学习算法--光梯度提升机(Light Gradient Boosting Machine)--来研究偶偶数原子核在塞格雷图上的基本实验观测数据。具体来说,我们重点研究了和状态的激发能量以及还原电四极转换概率。目前所获得的结果很好地再现了实验数据,对于和态以及Ⅴ态,精确度分别为1.07倍、1.05倍和1.14倍,比任何最先进的核模型和基于机器学习的方法的结果都要精确得多。我们使用 17 个新测量的数据点进一步验证了机器学习方法的预测能力。以 O、Ca、Sn 和 Pb 同位素为例,我们发现我们的方法精确地捕捉到了同位素趋势和绝对值,超越了迄今为止所有的理论模型。我们的研究结果揭示了 Sn 的双重魔力和 O 的外壳消失。
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引用次数: 0
CPT and Lorentz symmetry tests with hydrogen using a novel in-beam hyperfine spectroscopy method applicable to antihydrogen experiments 使用适用于反氢实验的新型束内超细光谱法进行氢的 CPT 和洛伦兹对称性测试
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-10 DOI: 10.1016/j.physletb.2024.139012

We present a Rabi-type measurement of two ground-state hydrogen hyperfine transitions performed in two opposite external magnetic field directions. This puts first constraints at the level of

on a set of coefficients of the Standard Model Extension, which were not measured by previous experiments. Moreover, we introduce a novel method, applicable to antihydrogen hyperfine spectroscopy in a beam, that determines the zero-field hyperfine transition frequency from the two transitions measured at the same magnetic field. Our value,
, is in agreement with literature at a relative precision of 0.44 ppb. This is the highest precision achieved on hydrogen in a beam, improving over previous results by a factor of 6.

我们介绍了在两个相反的外磁场方向上对两个基态氢超频跃迁进行的拉比式测量。这首次在水平上对标准模型扩展的一组系数施加了约束,而以前的实验并没有测量到这些系数。此外,我们还介绍了一种适用于光束中反氢超细光谱分析的新方法,它可以根据在相同磁场下测量到的两个跃迁来确定零场超细跃迁频率。我们的值为 ,与文献一致,相对精度为 0.44 ppb。这是在光束中对氢实现的最高精度,比以前的结果提高了 6 倍。
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引用次数: 0
Reconstruction of Bremsstrahlung γ-rays spectrum in heavy ion reactions with Richardson-Lucy algorithm 用理查森-卢西算法重构重离子反应中的轫致辐射 γ 射线光谱
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-07 DOI: 10.1016/j.physletb.2024.139009

The high momentum tail (HMT) in the momentum distribution of nucleons above the Fermi surface has been regarded as an evidence of short-range correlations (SRCs) in atomic nuclei. It has been showcased recently that the np Bremsstrahlung radiation in heavy ion reactions can be used to extract HMT information. The Richardson-Lucy (RL) algorithm is introduced to the reconstruction of the original Bremsstrahlung γ-ray energy spectrum from experimental measurements. By solving the inverse problem of the detector response to the γ-rays, the original energy spectrum of the Bremsstrahlung γ in 25 MeV/u 86Kr + 124Sn has been reconstructed and compared to the isospin- and momentum-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) simulations. The analysis based on hypothesis test suggests the existence of the HMT of nucleons in nuclei, in accordance with the previous conclusions. With its effectiveness being demonstrated, it is feasible to apply the RL algorithm in future experiments of measuring the Bremsstrahlung γ-rays in heavy ion reactions.

费米表面上方核子动量分布中的高动量尾(HMT)一直被视为原子核中短程相关性(SRC)的证据。最近的研究表明,重离子反应中的 np 轫致辐射可以用来提取 HMT 信息。理查森-卢西(RL)算法被引入到从实验测量中重建原始轫致辐射γ能谱的过程中。通过求解探测器对γ射线响应的逆问题,重建了 25 MeV/u 86Kr + 124Sn 中轫致辐射γ的原始能谱,并与等空间和动量相关的玻尔兹曼-厄林-乌伦贝克(IBUU)模拟进行了比较。基于假设检验的分析表明,原子核中存在核子的 HMT,这与之前的结论一致。由于证明了其有效性,在未来测量重离子反应中的轫致辐射 γ 射线的实验中应用 RL 算法是可行的。
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引用次数: 0
The m-component super KP hierarchy in Kac-van de Leur version Kac-van de Leur 版本中的 m 分量超 KP 层次结构
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-06 DOI: 10.1016/j.physletb.2024.139005

In this paper, the m-component super KP hierarchy in form of free superfermions is constructed by Clifford superalgebra. The super bosonic counterpart of this hierarchy is described by using the vertex operators. Based on this, some super Hirota equations are determined and the bilinear identity is expressed by super Baker functions and tau function. Darboux transformation in terms of superfermions is also discussed.

本文通过克利福德超代数构建了自由超费米子形式的 m 分超 KP 层次。利用顶点算子描述了这一层次结构的超玻色对应物。在此基础上,确定了一些超广达方程,并用超贝克函数和 tau 函数表达了双线性特性。此外,还讨论了超费米子的达尔布克斯变换。
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引用次数: 0
On character expansion and Gaussian regularization of Itzykson-Zuber measure 关于伊齐克森-祖贝尔度量的特征扩展和高斯正则化
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-06 DOI: 10.1016/j.physletb.2024.139006

Character expansions are among the most important approaches to modern quantum field theory, which substitute integrals by combinations of peculiar special functions from the Schur-Macdonald family. These formulas allow various deformations, which are not transparent in integral formulation. We analyze from this point of view the Itzykson-Zuber integral over unitary matrices which is exactly solvable, but difficult to deform in β and (q,t) directions. Character expansion straightforwardly resolves this problem. However, taking averages with the so defined measure can look problematic, because integrals of individual expansion terms often diverge and well defined is only the sum of them. We explain a way to overcome this problem by Gaussian regularization, which can have a broad range of further applications.

特性展开是现代量子场论最重要的方法之一,它用舒尔-麦克唐纳家族的特殊函数组合代替积分。这些公式允许各种变形,而这些变形在积分公式中是不透明的。我们从这个角度分析了单位矩阵上的伊齐克森-祖贝尔积分,它是完全可解的,但难以在 β 和 (q,t) 方向上变形。特性展开直接解决了这一问题。然而,用这样定义的度量取平均值可能会有问题,因为单个扩展项的积分往往会发散,而定义良好的只是它们的和。我们解释了一种通过高斯正则化来克服这一问题的方法,它可以有更广泛的应用。
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引用次数: 0
Perturbative results of matrix elements of the axial current and their relation with the axial anomaly 轴向电流矩阵元素的扰动结果及其与轴向异常的关系
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-06 DOI: 10.1016/j.physletb.2024.138999

In the Standard Model of particle physics, the axial current is not conserved, due both to fermion masses and to the axial anomaly. Using perturbative quantum chromodynamics, we calculate matrix elements of the local and non-local axial current for a gluon target, clarifying their connection with the axial anomaly. In so doing, we also reconsider classic results obtained in the context of the nucleon spin sum rule as well as recent results for off-forward kinematics. An important role is played by the infrared regulator, for which we put a special emphasis on the nonzero quark mass. We highlight cancellations that take place between contributions from the axial anomaly and the quark mass, and we elaborate on the relation of those cancellations with the conservation of angular momentum.

在粒子物理的标准模型中,由于费米子质量和轴向反常,轴向电流是不守恒的。利用微扰量子色动力学,我们计算了胶子目标的局部和非局部轴向电流的矩阵元素,澄清了它们与轴向反常的联系。在此过程中,我们还重新考虑了在核子自旋和规则背景下获得的经典结果,以及偏前运动学的最新结果。红外调节器发挥了重要作用,我们特别强调了非零夸克质量。我们强调了轴向反常贡献和夸克质量之间的抵消,并详细阐述了这些抵消与角动量守恒的关系。
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引用次数: 0
Hadronic scattering effects on Λ polarization in relativistic heavy ion collisions 强子散射对相对论重离子碰撞中Λ极化的影响
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-05 DOI: 10.1016/j.physletb.2024.139004

The Λ hyperon spin flip and non-flip cross sections are calculated in a simple hadronic model by including both the s-channel process involving the spin 3/2, positive parity Σ(1358) resonance and the t-channel process via the exchange of a scalar σ meson. Because of its large mass, the Λ spin flip to non-flip cross sections is negligibly small in the t-channel process compared to the constant value of 1/3.5 in the s-channel process. With the s-channel Λπ spin-dependent cross sections included in a schematic kinetic model, the effects of hadronic scatterings on the Λ spin polarization in Au-Au collisions at sNN=7.7 GeV are studied. It is found that the Λ spin polarization only decreases by 7-12% during the hadronic stage of these collisions, which justifies the assumption in theoretical studies that compare the Λ polarization calculated at the chemical freezeout to the measured one at the kinetic freezeout.

我们在一个简单的强子模型中计算了Λ超子自旋翻转和非翻转的截面,包括涉及自旋3/2、正奇偶共振的-通道过程和通过标量介子交换的-通道过程。由于Λ介子的质量很大,与-沟道过程中1/3.5的恒定值相比,-沟道过程中Λ自旋翻转到非翻转的截面小得可以忽略不计。在一个示意性动力学模型中包含了-沟道自旋相关截面,研究了在GeV的金-金对撞中强子散射对Λ自旋极化的影响。研究发现,在这些对撞的强子阶段,Λ自旋极化只降低了7-12%,这证明了理论研究中的假设是正确的,即把化学冻结时计算的Λ极化与动力学冻结时测量的Λ极化进行比较。
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引用次数: 0
Rotating and accelerating AdS black holes in Einstein-Gauss-Bonnet gravity 爱因斯坦-高斯-波奈引力中的旋转和加速 AdS 黑洞
IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-09-04 DOI: 10.1016/j.physletb.2024.139000

We present new, exact, rotating and accelerating solutions within the framework of five-dimensional Einstein-Gauss-Bonnet theory at the Chern-Simons point. The rotating solutions describe black holes characterized by a single rotation parameter, a mass parameter, and two extra integration constants that can be interpreted as hairs of a gravitational nature. It is noteworthy that the rotation cannot be removed by a large diffeomorphism. We also extend our procedure to dimension seven, providing a new rotating solution with two rotation parameters pertaining to cubic Lovelock theory with a unique vacuum.

我们在五维爱因斯坦-高斯-波奈理论的框架内提出了新的、精确的、旋转和加速解。旋转解描述的黑洞具有一个旋转参数、一个质量参数和两个额外的积分常数,可以解释为引力性质的毛发。值得注意的是,大衍射无法消除旋转。我们还将程序扩展到七维,提供了一个新的旋转解,它有两个旋转参数,与具有唯一真空的立方拉弗洛克理论有关。
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引用次数: 0
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Physics Letters B
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