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Acta Physica Polonica B最新文献

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Beta-decay Half-life Uncertainty of the Extremely Neutron-rich Nuclei Due to Nuclear-mass Deviation 由核质量偏差引起的极富中子核的β衰变半衰期不确定性
IF 0.5 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2023-01-01 DOI: 10.5506/aphyspolb.54.8-a3
N. Ly, N. Duy, N. K. Uyen, L. Khiem
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引用次数: 0
Bound-free Pair Production Mechanism in Pb–(p) Collisions at the LHC Pb - (p)在大型强子对撞机中的无束缚对产生机制
IF 0.5 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2023-01-01 DOI: 10.5506/aphyspolb.54.4-a4
M. Yilmaz Şengül
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引用次数: 0
Fission Fragment Mass and Kinetic Energy Yields of Fermium Isotopes 镄同位素的裂变碎片质量和动能产率
4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2023-01-01 DOI: 10.5506/aphyspolb.54.9-a2
K. Pomorski, A. Dobrowolski, B. Nerlo-Pomorska, M. Warda, A. Zdeb, J. Bartel, H. Molique, C. Schmitt, Z.G. Xiao, Y.J. Chen, L.L. Liu
A rapidly converging 4-dimensional Fourier shape parametrization is used to model the fission process of heavy nuclei. Potential energy landscapes are computed within the macroscopic-microscopic approach, on top of which the multi-dimensional Langevin equation is solved to describe the fission dynamics. Charge equilibration at scission and de-excitation by neutron evaporation of the primary fragments after scission is investigated. The model describes various observables, including fission-fragment mass, charge, and kinetic energy yields, as well as post-scission neutron multiplicities and, most importantly, their correlations, which are crucial to unravel the complexity of the fission process. The parameters of the dynamical model were tuned to reproduce experimental data obtained from thermal neutron-induced fission of $^{235}$U, which allows us to discuss the transition from asymmetric to symmetric fission along the Fm isotopic chain.
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引用次数: 1
The Rigorous Test of the Generalized Brink–Axel Hypothesis in the (A=138) Nuclear Mass Region 广义Brink-Axel假说在(A=138)核质量区的严格检验
IF 0.5 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2023-01-01 DOI: 10.5506/aphyspolb.54.8-a1
B. V. Kheswa
The generalized Brink–Axel (gBA) hypothesis suggests that the γ -ray strength function ( γ SF) of a nucleus only depends on the γ -ray energy, and not on the properties of the initial and final excitation energy levels between which the nucleus decays. This hypothesis has been tested in various studies and it is still controversial. In this study, the gBA hypothesis was tested in the A = 138 nuclear mass region by rigorously investigating the dependence of the γ SF of 138 La on both initial and final excitation energies. The results showed that the shape and absolute value of the γ SF are independent of the initial and final excitation energy. Therefore, the results of this work are in support of the generalized Brink–Axel hypothesis.
广义Brink-Axel (gBA)假设表明,原子核的γ射线强度函数(γ SF)仅取决于γ射线能量,而不取决于原子核衰变所处的初始和最终激发能级的性质。这一假设已在各种研究中得到验证,但仍存在争议。在A = 138核质量区,通过严格研究138la的γ SF对初始和最终激发能的依赖,验证了gBA假设。结果表明,γ SF的形状和绝对值与初始激发能和最终激发能无关。因此,本工作的结果支持广义Brink-Axel假设。
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引用次数: 0
Analysis of (^{6})Li((^{3})He,(d)^{7})Be Transfer Reaction for Different Approaches 不同途径下(^{6}) Li((^{3}) He, (d)^{7}) Be转移反应的分析
IF 0.5 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2023-01-01 DOI: 10.5506/aphyspolb.54.5-a1
M. Aygun, Z. Aygun, N. Karaali
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引用次数: 0
Nuclear Structure of Proton-rich (^{20-23})Mg Isotopes 富质子的核结构(^{20-23}) Mg同位素
IF 0.5 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2023-01-01 DOI: 10.5506/aphyspolb.54.1-a3
M. Hadi, A. A. Al-Sa’ad
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引用次数: 0
Exorcizing Ghosts from the Vacuum Spectra in String-inspired Nonlocal Tachyon Condensation 弦激发非局域速子凝聚中真空光谱幽灵的驱除
4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2023-01-01 DOI: 10.5506/aphyspolb.54.9-a4
Florian Nortier
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引用次数: 1
On the Dynamics of Delayed and Non-delayed Fractional-order and Distributed-order Consumer Models 延迟与非延迟分数阶与分布阶消费者模型的动力学研究
IF 0.5 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2023-01-01 DOI: 10.5506/aphyspolb.54.7-a2
M.A. Abd Rabo, G. Mahmoud, S. Aly, T. Abed-Elhameed
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引用次数: 0
Defect Wormhole: A Traversable Wormhole Without Exotic Matter 缺陷虫洞:一个没有外来物质的可穿越虫洞
IF 0.5 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-12-30 DOI: 10.5506/APhysPolB.54.5-A3
F. Klinkhamer
We present a traversable-wormhole solution of the gravitational field equation of General Relativity without need of exotic matter (exotic matter can, for example, have negative energy density and vanishing isotropic pressure). Instead of exotic matter, the solution relies on a 3-dimensional"spacetime defect"characterized by a locally vanishing metric determinant.
我们提出了广义相对论引力场方程的可穿越虫洞解,而不需要奇异物质(例如,奇异物质可以具有负能量密度和消失的各向同性压力)。该解决方案依赖于以局部消失的度量行列式为特征的三维“时空缺陷”,而不是奇异物质。
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引用次数: 10
Should Unstable Quantum Field Theories be Lorentz-invariant? 不稳定量子场论应该是洛伦兹不变量吗?
IF 0.5 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-12-19 DOI: 10.5506/APhysPolB.53.11-A4
L. Gavassino
An unstable field theory is what we obtain when we linearise the equations of an interacting field theory near an unstable state. Theories of this kind are adopted to model the onset of spontaneous symmetry breakings, when the fields are sitting on the top of the Mexican hat, and they start to “roll down” to the bottom. At present, there exists no rigorous proof that unstable quantum field theories are Lorentz-invariant (in the sense of Wigner’s theorem). Here, we show that they shouldn’t be. In fact, unstable theories always have a limited regime of applicability, and they are valid only for a very short time. As consequence, there is a preferred simultaneity hyperplane, along which the unstable theory is everywhere applicable, while a generic observer (whose four-velocity is not orthogonal to such hyperplane) must use the full non-linear theory. In summary: the current quantization schemes are “ok”, independently from whether they lead to a Lorentz-invariant theory.
当我们将不稳定状态附近的相互作用场理论的方程线性化时,我们得到了不稳定场理论。这类理论被用来模拟自发对称断裂的发生,当田地坐在墨西哥帽的顶部时,它们开始“向下滚动”到底部。目前,还没有严格的证据证明不稳定量子场理论是洛伦兹不变量(在Wigner定理的意义上)。在这里,我们证明了它们不应该是。事实上,不稳定理论的适用性总是有限的,而且它们只在很短的时间内有效。因此,存在一个优选的同时超平面,沿着该超平面,不稳定理论在任何地方都适用,而一般的观测器(其四个速度不正交于这样的超平面)必须使用全非线性理论。总之:当前的量化方案是“好的”,独立于它们是否导致洛伦兹不变量理论。
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引用次数: 0
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Acta Physica Polonica B
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