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Production cross-sections and Radiative Decay widths of Heavy Quarkonia in magnetized matter 磁化物质中重夸克子的产生、截面和辐射衰变宽度
Pub Date : 2023-09-29 DOI: 10.1142/s0218301323500489
Amruta Mishra, Ankit Kumar
We study the production cross-sections and radiative decay widths of heavy quarkonia (charmonia and bottomonia) in magnetized nuclear matter. The production cross-sections of the $psi(3770)$ and $Upsilon(4S)$, from the $Dbar D$ and $Bbar B$ scatterings respectively, are studied from the medium modifications of the masses and partial decay widths to open charm (bottom) mesons, of these heavy flavor mesons. Within a chiral effective model, the masses of the vector and pseudoscalar charmonium (bottomonium) states are calculated from the medium modification of a dilaton field, $chi$, which mimics the gluon condensates of QCD. In the presence of a magnetic field, there is mixing of the pseudoscalar (P) meson and the longitudinal component of the vector (V) meson (PV mixing), which leads to appreciable modifications of their masses. The radiative decay widths of the vector (V) heavy quarkonia to the pseudoscalar (P) mesons ($J/psirightarrow eta_c(1S) gamma$, $psi(2S)rightarrow eta_c(2S) gamma$ and $psi(1D)rightarrow eta_c(2S) gamma$ for the charm sector and $Upsilon(NS)rightarrow eta_b(NS)gamma$, $N$=1,2,3,4, for the bottom sector) in the magnetized asymmetric nuclear matter are also investigated in the present work. The difference in the mass of the transverse component from the longitudinal component of the vector meson, arising due to PV mixing, is observed as a double peak structure in the invariant mass spectrum of the production cross-section of $psi(3770)$. The modifications of the production cross-sections as well as the radiative decay widths of the heavy quarkonia in the magnetized matter should have observable consequences on the production of these heavy flavour mesons resulting from ultra-relativistic peripheral heavy ion collision experiments, where the created magnetic field can be extremely large.
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引用次数: 0
A review on anisotropic flow in heavy-ion collisions 重离子碰撞中各向异性流动的研究进展
Pub Date : 2023-09-21 DOI: 10.1142/s0218301323410033
Vipul Bairathi, Kishora Nayak
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引用次数: 0
An improved microscopic core–quasiparticle coupling model for spectroscopy of odd-mass nuclei with octupole correlations 一种改进的八极相关奇质量原子核光谱的微观核-准粒子耦合模型
Pub Date : 2023-07-28 DOI: 10.1142/s0218301323400062
Xin Zhao, Zhipan Li, Dario Vretenar
The microscopic core–quasiparticle coupling model for odd-A nuclei with octupole correlations is extended to include the monopole, quadrupole and octupole couplings between the core and the odd nucleon, based on the framework of covariant density functional theory. The model is tested in a study of low-lying excitation spectra for the odd-A nucleus [Formula: see text]Ra. Theoretical results, e.g., the parity doublets, interband [Formula: see text] and intraband [Formula: see text], are in very good agreement with the available data. In particular, the description of signature splitting in the ground-state band has been improved. This method provides a very useful tool for a systematic study of low-energy spectra in odd-mass actinides with octupole correlations.
基于协变密度泛函理论的框架,将具有八极子关联的奇a核微观核-准粒子耦合模型扩展到包括核与奇核子之间的单极子、四极子和八极子耦合。该模型在奇a核的低洼激发谱研究中得到了验证[公式:见原文]。理论结果,如奇偶态、带间[公式:见文]和带内[公式:见文],与现有数据非常吻合。特别地,改进了基态波段信号分裂的描述。该方法为系统地研究具有八极相关的奇质量锕系元素的低能谱提供了一个非常有用的工具。
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引用次数: 0
Systematic study of two-proton radioactivity half-lives based on a modified Gamow-like model 基于改进的类gamow模型的双质子放射性半衰期的系统研究
Pub Date : 2021-08-19 DOI: 10.1142/S0218301321500749
Hong-Ming Liu, Y. Zou, Xiao Pan, B. He, Xiao-Hua Li
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引用次数: 1
Current status of different detector technology in the searches of 0νββ decay 不同探测器技术在寻找0νββ衰变中的现状
Pub Date : 2021-08-19 DOI: 10.1142/S0218301321300083
S. Karmakar, M. Singh
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引用次数: 0
Study of the enhancement factor and electron potential in the D (3He, p)4He reaction using deuterated metal targets TiD and ZrD 用氘化金属靶品TiD和ZrD研究D (3He, p)4He反应的增强因子和电子势
Pub Date : 2021-06-24 DOI: 10.1142/S0218301321500452
V. Bystritsky, D. Chumakov, G. Dudkin, M. Filipowicz, B. Nechaev, A. Nurkin, V. N. Padalko, F. Pen'kov, A. Philippov, Y. Tuleushev, V. A. Varlachev, E. Zhakanbaev
The study of thermonuclear reactions such as D(d, p)3H, D(d, n)3He, T(d, n)3He, 3He(d, p)4He, and D(3He, p)4He is of great interest in the field of astrophysics, as it affects the primordial nucleosynthesis, as well as issues of stellar dynamics. These reactions are also of interest in thermonuclear power engineering, in connection with the increased interest in the possibility of practical application of thermonuclear fusion. In this work, the analysis of the results obtained in the course of studying the reaction D(3He, p)4He was carried out. The results were obtained by us in previous works on deuterated metal targets ZrD and TiD with Miller indices [111] and [100]. There is a need to more precise study of the effects accompanying thermonuclear reactions at low astrophysical energies. The purpose of this work is to study the behavior of the screening potential [Formula: see text] and the reaction enhancement factor [Formula: see text], depending on the crystal structure of targets and the interaction energy. The studies were carried out on a Hall accelerator (Tomsk, TPU) in the energy range [Formula: see text]([Formula: see text][Formula: see text]keV in lab reference frame with a step of 2[Formula: see text]keV. Experiments have shown that in reactions using metal deuterated targets a similar effect as in reactions using gas targets was observed. Specifically, an electron screening effect was observed, which leads to an increase in the reaction cross-section with decreasing energy, and in case of metal target this effect becomes stronger.
D(D, p)3H, D(D, n)3He, T(D, n)3He, 3He(D, p)4He和D(3He, p)4He等热核反应的研究是天体物理学领域的重要研究方向,因为它们影响着原始核合成以及恒星动力学问题。这些反应在热核动力工程中也引起了人们的兴趣,因为人们对热核聚变实际应用的可能性越来越感兴趣。本文对D(3He, p)4He反应的研究结果进行了分析。我们在前人对米勒指数的氘化金属靶ZrD和TiD的研究中得到的结果[111]和[100]。有必要更精确地研究低天体物理能量下热核反应的效应。本工作的目的是研究筛选势[公式:见文]和反应增强因子[公式:见文]的行为,取决于目标的晶体结构和相互作用能。在能量范围[公式:见文]([公式:见文][公式:见文][公式:见文])的霍尔加速器(托木斯克,TPU)上进行研究,在实验室参考系中,步长为2[公式:见文]keV。实验表明,在使用金属氘化靶的反应中,观察到的效果与使用气体靶的反应相似。具体而言,观察到电子屏蔽效应,导致反应截面随着能量的降低而增加,并且在金属靶中这种效应更强。
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引用次数: 0
Microscopic study of shape evolution and some important ground state properties of 190–210Au isotopes 190-210Au同位素形态演化及一些重要基态性质的微观研究
Pub Date : 2021-05-27 DOI: 10.1142/S021830132150049X
Vikesh Kumar, Pankaj Kumar, V. Thakur, S. Thakur, S. K. Dhiman
In this paper, we have examined the nuclear structural properties of 190–210Au isotopes within the framework of the Hartree–Fock–Bogoliubov Model. For the theoretical calculations, we have used the UNEDF2 and SKP interactions. The studies include the shape evolution, quadrupole deformation parameter [Formula: see text], nuclear electric quadrupole moment Q(b), single-particle energy levels, the binding energy per nucleon, nuclear charge radius, neutron rms radius, proton rms radius and neutron skin thickness. To analyze the accuracy of our theoretical results, we have presented the comparative analysis with experimental data and finite-range droplet model calculations. The adequate resemblance with experimental data is supporting our studies. We observe the oblate-prolate shape coexistence for 190Au, 193Au and 195Au using the UNEDF2 interaction.
在本文中,我们在Hartree-Fock-Bogoliubov模型的框架内研究了190-210Au同位素的核结构性质。在理论计算中,我们使用了UNEDF2和SKP相互作用。研究内容包括形状演变、四极变形参数[公式:见文]、核电四极矩Q(b)、单粒子能级、每核子结合能、核电荷半径、中子均方根半径、质子均方根半径和中子蒙皮厚度。为了分析理论结果的准确性,我们与实验数据和有限范围液滴模型计算进行了对比分析。与实验数据的充分相似性支持了我们的研究。我们利用UNEDF2相互作用观察到190Au、193Au和195Au的扁长形共存。
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引用次数: 0
Fragmentation of carbon on elemental targets at 290AMeV 290AMeV时元素目标上的碳碎片
Pub Date : 2021-05-27 DOI: 10.1142/S0218301321500464
Hailong Duan, Jing-Ya Wu, T. Ma, Jun-Sheng Li, Hui-Ling Li, Ming-ming Xu, Ruizhu Yang, Dong-Hai Zhang, Zhi Zhang, Qi Wang, S. Kodaira
The total charge-changing cross-sections and the partial cross-sections for projectile fragments (PFs) production for the fragmentation of 12C on C, Al, Cu, Pb and CH2 targets at the highest energy of 290[Formula: see text]A[Formula: see text]MeV were studied. It was found that the total charge-changing reaction cross-sections and the partial reaction cross-sections of PFs production were independent of the beam energy, and increased with increase of mass of target for the same beam energy. The total charge-changing reaction cross-section was the same as the prediction of Bradt–Peters semi-empirical formula, PHITS and NUCFRG2 simulation models. The partial cross-section of PFs production increased with the increase of the mass of target, and it was the same as the prediction of NUCFRG2 models. The mean scattering angle of projectile particle was smaller than the average emission angle of PF, and the width of scattering angle distribution of projectile particle was smaller than that of emission angle distribution of PFs. The mean emission angle of PFs does not obviously depend on the target mass and beam energy in our studied beam energy regions.
研究了12C在最高能量为290 MeV的C、Al、Cu、Pb和CH2靶上破碎产生抛射破片的总变电荷截面和部分破片截面。结果表明,PFs的总变电荷反应截面和部分变电荷反应截面与束流能量无关,在相同束流能量下,随目标质量的增加而增大。总变电荷反应截面与Bradt-Peters半经验公式、PHITS和NUCFRG2模拟模型的预测结果一致。随着目标质量的增加,PFs生成的部分截面增大,这与NUCFRG2模型的预测结果一致。弹丸颗粒的平均散射角小于PF的平均发射角,弹丸颗粒的散射角分布宽度小于PF的发射角分布宽度。在我们所研究的束流能区,光子激光器的平均发射角与目标质量和束流能量没有明显的关系。
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引用次数: 1
Emission characteristics of target black fragments in 16O-Emulsion collisions at 3.7AGeV 3.7AGeV下16o -乳剂碰撞目标黑色碎片发射特性
Pub Date : 2021-05-17 DOI: 10.1142/S0218301321500427
S. Kamel, N. Abdallah, H. Yousef, E. El-Falaky
As a function of collision centrality, the multiplicity and angular distributions for the slowest target fragments (black particles) emitted in interactions of 16O ions with emulsion nuclei at 3.7[Formula: see text]A[Formula: see text]GeV were investigated. The multiplicity distribution is unaffected by the projectile’s energy or mass. At different impact parameters, the higher moments of multiplicity distributions of black particles were measured. The calculated values of the scaled variance (variance divided by the mean) show that the emission of slower target fragments at high energies is not a statistically independent process in all cases. At various projectile spectators, the angular distributions of the emitted black particles were investigated. The obtained data were compared to the statistical model’s predictions to describe the process responsible for producing secondary particles.
作为碰撞中心性的函数,研究了16O离子与乳化液核在3.7 GeV[公式:见文]a[公式:见文]GeV下发射的最慢目标碎片(黑色粒子)的多重度和角分布。多重分布不受弹丸能量或质量的影响。在不同的冲击参数下,测量了黑色颗粒多重分布的高矩。计算得到的标度方差(方差除以均值)表明,在所有情况下,较慢的高能量目标碎片的发射都不是一个统计独立的过程。在不同的抛射观众席上,研究了发射出的黑色粒子的角分布。将获得的数据与统计模型的预测进行比较,以描述产生二次粒子的过程。
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引用次数: 0
12C(20Ne, 16O)16O α-transfer reaction and astrophysical S-factors at 300keV 300keV下12C(20Ne, 16O)16O α-转移反应及天体物理s因子
Pub Date : 2021-05-01 DOI: 10.1142/S0218301321500397
A. Mondal, C. Basu, S. Adhikari, C. Bhattacharya, T. Rana, S. Kundu, S. Manna, R. Pandey, P. Roy, A. Sen, J. K. Meena, A. Saha, J. K. Sahoo, D. Basak, T. Bar, H. Pai, A. Bisoi, A. Mitra, P. Biswas
The [Formula: see text]C([Formula: see text]Ne, [Formula: see text]O)[Formula: see text]O reaction has been used for the first time to determine ANC of [Formula: see text]O levels. The [Formula: see text]C([Formula: see text]Ne, [Formula: see text]O)[Formula: see text]O [Formula: see text]-transfer angular distributions are measured at [Formula: see text][Formula: see text]MeV and used to determine the ANC of the ground, 6.05[Formula: see text]MeV ([Formula: see text]), 6.13[Formula: see text]MeV ([Formula: see text]), 6.92[Formula: see text]MeV ([Formula: see text]) and 7.12[Formula: see text]MeV ([Formula: see text]) states of [Formula: see text]O. The ANC values are [Formula: see text] [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text] and [Formula: see text] [Formula: see text]. Astrophysical S-factors at 300[Formula: see text]keV are extracted [Formula: see text]) keV b and [Formula: see text] keV b[Formula: see text] using these ANC values by R-matrix theory.
[公式:见文]C([公式:见文]Ne,[公式:见文]O)[公式:见文]O反应首次用于测定[公式:见文]O水平的ANC。[公式:见文]C([公式:见文]Ne,[公式:见文]O)[公式:见文]O[公式:见文]传递角分布在[公式:见文][公式:见文]MeV处测量,用于确定地面的ANC, 6.05[公式:见文]MeV([公式:见文]),6.13[公式:见文]MeV([公式:见文]),6.92[公式:见文]MeV([公式:见文])和7.12[公式:见文]MeV([公式:见文])[公式:见文]O的状态。ANC值为[公式:见文本][公式:见文本][公式:见文本][公式:见文本],[公式:见文本][公式:见文本],[公式:见文本][公式:见文本],[公式:见文本][公式:见文本],[公式:见文本][公式:见文本]和[公式:见文本][公式:见文本][公式:见文本][公式:见文本][公式:见文本][公式:见文本][公式:见文本][公式:见文本][公式:见文本][公式:见文本][公式:见文本][公式:见文本]。根据r矩阵理论,利用这些ANC值提取300[公式:见文]keV的天体物理s因子[公式:见文])keV b和[公式:见文]keV b[公式:见文]。
{"title":"12C(20Ne, 16O)16O α-transfer reaction and astrophysical S-factors at 300keV","authors":"A. Mondal, C. Basu, S. Adhikari, C. Bhattacharya, T. Rana, S. Kundu, S. Manna, R. Pandey, P. Roy, A. Sen, J. K. Meena, A. Saha, J. K. Sahoo, D. Basak, T. Bar, H. Pai, A. Bisoi, A. Mitra, P. Biswas","doi":"10.1142/S0218301321500397","DOIUrl":"https://doi.org/10.1142/S0218301321500397","url":null,"abstract":"The [Formula: see text]C([Formula: see text]Ne, [Formula: see text]O)[Formula: see text]O reaction has been used for the first time to determine ANC of [Formula: see text]O levels. The [Formula: see text]C([Formula: see text]Ne, [Formula: see text]O)[Formula: see text]O [Formula: see text]-transfer angular distributions are measured at [Formula: see text][Formula: see text]MeV and used to determine the ANC of the ground, 6.05[Formula: see text]MeV ([Formula: see text]), 6.13[Formula: see text]MeV ([Formula: see text]), 6.92[Formula: see text]MeV ([Formula: see text]) and 7.12[Formula: see text]MeV ([Formula: see text]) states of [Formula: see text]O. The ANC values are [Formula: see text] [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text] and [Formula: see text] [Formula: see text]. Astrophysical S-factors at 300[Formula: see text]keV are extracted [Formula: see text]) keV b and [Formula: see text] keV b[Formula: see text] using these ANC values by R-matrix theory.","PeriodicalId":14032,"journal":{"name":"International Journal of Modern Physics E-nuclear Physics","volume":"54 1","pages":"2150039"},"PeriodicalIF":0.0,"publicationDate":"2021-05-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"75759887","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
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International Journal of Modern Physics E-nuclear Physics
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