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Hadronic cross section measurements with the DAMPE space mission using 20GeV-10TeV cosmic-ray protons and $^4$He 利用 20GeV-10TeV 宇宙射线质子和 $^4$He 的 DAMPE 空间飞行任务测量强子截面
Pub Date : 2024-08-30 DOI: arxiv-2408.17224
F. Alemanno, Q. An, P. Azzarello, F. C. T. Barbato, P. Bernardini, X. J. Bi, I. Cagnoli, M. S. Cai, E. Casilli, E. Catanzani, J. Chang, D. Y. Chen, J. L. Chen, Z. F. Chen, P. Coppin, M. Y. Cui, T. S. Cui, Y. X. Cui, H. T. Dai, A. De Benedittis, I. De Mitri, F. de Palma, A. Di Giovanni, Q. Ding, T. K. Dong, Z. X. Dong, G. Donvito, D. Droz, J. L. Duan, K. K. Duan, R. R. Fan, Y. Z. Fan, F. Fang, K. Fang, C. Q. Feng, L. Feng, J. M. Frieden, P. Fusco, M. Gao, F. Gargano, K. Gong, Y. Z. Gong, D. Y. Guo, J. H. Guo, S. X. Han, Y. M. Hu, G. S. Huang, X. Y. Huang, Y. Y. Huang, M. Ionica, L. Y. Jiang, Y. Z. Jiang, W. Jiang, J. Kong, A. Kotenko, D. Kyratzis, S. J. Lei, W. H. Li, W. L. Li, X. Li, X. Q. Li, Y. M. Liang, C. M. Liu, H. Liu, J. Liu, S. B. Liu, Y. Liu, F. Loparco, C. N. Luo, M. Ma, P. X. Ma, T. Ma, X. Y. Ma, G. Marsella, M. N. Mazziotta, D. Mo, X. Y. Niu, X. Pan, A. Parenti, W. X. Peng, X. Y. Peng, C. Perrina, E. Putti-Garcia, R. Qiao, J. N. Rao, A. Ruina, R. Sarkar, P. Savina, A. Serpolla, Z. Shangguan, W. H. Shen, Z. Q. Shen, Z. T. Shen, L. Silveri, J. X. Song, M. Stolpovskiy, H. Su, M. Su, H. R. Sun, Z. Y. Sun, A. Surdo, X. J. Teng, A. Tykhonov, J. Z. Wang, L. G. Wang, S. Wang, S. X. Wang, X. L. Wang, Y. Wang, Y. F. Wang, Y. Z. Wang, Z. M. Wang, D. M. Wei, J. J. Wei, Y. F. Wei, D. Wu, J. Wu, S. S. Wu, X. Wu, Z. Q. Xia, H. T. Xu, J. Xu, Z. H. Xu, Z. L. Xu, E. H. Xu, Z. Z. Xu, G. F. Xue, H. B. Yang, P. Yang, Y. Q. Yang, H. J. Yao, Y. H. Yu, G. W. Yuan, Q. Yuan, C. Yue, J. J. Zang, S. X. Zhang, W. Z. Zhang, Yan Zhang, Yi Zhang, Y. J. Zhang, Y. L. Zhang, Y. P. Zhang, Y. Q. Zhang, Z. Zhang, Z. Y. Zhang, C. Zhao, H. Y. Zhao, X. F. Zhao, C. Y. Zhou, Y. Zhu
Precise direct cosmic-ray (CR) measurements provide an important probe tostudy the energetic particle sources in our Galaxy, and the interstellarenvironment through which these particles propagate. Uncertainties on hadronicmodels, ion-nucleon cross sections in particular, are currently the limitingfactor towards obtaining more accurate CR ion flux measurements withcalorimetric space-based experiments. We present an energy-dependentmeasurement of the inelastic cross section of protons and helium-4 nuclei(alpha particles) on a Bi$_4$Ge$_3$O$_{12}$ target, using 88 months of datacollected by the DAMPE space mission. The kinetic energy range per nucleon ofthe measurement points ranges from 18 GeV to 9 TeV for protons, and from 5GeV/n to 3 TeV/n for helium-4 nuclei. Our results lead to a significantimprovement of the CR flux normalisation. In the case of helium-4, theseresults correspond to the first cross section measurements on a heavy targetmaterial at energies above 10 GeV/n.
精确的宇宙射线(CR)直接测量为研究银河系中的高能粒子源以及这些粒子传播的星际环境提供了一个重要的探针。强子模型,特别是离子-核子截面的不确定性,是目前利用空间比量实验获得更精确的宇宙射线离子通量测量的限制因素。我们利用 DAMPE 空间任务收集的 88 个月数据,介绍了对 Bi$_4$Ge$_3$O$_{12}$ 靶上质子和氦-4 核(α 粒子)非弹性截面的随能量变化的测量。测量点每个核子的动能范围为:质子从 18 GeV 到 9 TeV,氦-4 核子从 5 GeV/n 到 3 TeV/n。我们的结果大大改进了 CR 通量的归一化。就氦-4 核而言,这些结果相当于首次在能量高于 10 GeV/n 的重目标材料上进行的截面测量。
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引用次数: 0
Search for dark matter produced in association with a pair of bottom quarks in proton-proton collisions at $sqrt{s}$ = 13 TeV 在$sqrt{s}$ = 13 TeV质子-质子对撞中寻找与一对底夸克结合产生的暗物质
Pub Date : 2024-08-30 DOI: arxiv-2408.17336
CMS Collaboration
A search for dark matter (DM) particles produced in association with bottomquarks is presented. The analysis uses proton-proton collision data at acenter-of-mass energy of $sqrt{s}$ = 13 TeV, corresponding to an integratedluminosity of 138 fb$^{-1}$. The search is performed in the final state withlarge missing transverse momentum and a pair of jets originating from bottomquarks. No significant excess of data is observed with respect to the standardmodel expectation. Results are interpreted in the context of a type-IItwo-Higgs-doublet model with an additional light pseudoscalar (2HDM+a). Anupper limit is set on the mass of the lighter pseudoscalar, excluding masses upto 260 GeV at 95% confidence level. This is the first search at the LHC toprobe DM produced in association with two nonresonant bottom quarks in the2HDM+a model. Sensitivity to the parameter space with the ratio of the vacuumexpectation values of the two Higgs doublets, $tanbeta$, greater than 15 isachieved, capitalizing on the enhancement of couplings between pseudoscalarsand bottom quarks with high $tanbeta$.
本文介绍了对与底夸克一起产生的暗物质粒子的搜索。分析使用了质心能量为$sqrt{s}$ = 13 TeV的质子-质子对撞数据,对应于138 fb$^{-1}$的综合光度。搜索是在具有较大缺失横动量和一对源于底夸克的喷流的终态下进行的。与标准模型预期相比,没有观测到明显的数据过剩。结果是在一个带有额外轻伪标星(2HDM+a)的II型二希格斯双星模型背景下解释的。对轻伪镜星的质量设定了上限,在95%的置信度下排除了高达260 GeV的质量。这是在大型强子对撞机上首次搜索在2HDM+a模型中产生的与两个非共振底夸克相关的DM。利用伪高星和底夸克之间耦合的增强,实现了对两个希格斯双星真空期望值之比大于15的参数空间的敏感性。
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引用次数: 0
Shock-driven amorphization and melt in Fe$_2$O$_3$ 冲击驱动的 Fe$_2$O$_3$ 中的非晶化和熔体
Pub Date : 2024-08-30 DOI: arxiv-2408.17204
Céline Crépisson, Alexis Amouretti, Marion Harmand, Chrystèle Sanloup, Patrick Heighway, Sam Azadi, David McGonegle, Thomas Campbell, David Alexander Chin, Ethan Smith, Linda Hansen, Alessandro Forte, Thomas Gawne, Hae Ja Lee, Bob Nagler, YuanFeng Shi, Guillaume Fiquet, François Guyot, Mikako Makita, Alessandra Benuzzi-Mounaix, Tommaso Vinci, Kohei Miyanishi, Norimasa Ozaki, Tatiana Pikuz, Hirotaka Nakamura, Keiichi Sueda, Toshinori Yabuuchi, Makina Yabashi, Justin S. Wark, Danae N. Polsin, Sam M. Vinko
We present measurements on Fe$_2$O$_3$ amorphization and melt underlaser-driven shock compression up to 209(10) GPa via time-resolved in situx-ray diffraction. At 122(3) GPa, a diffuse signal is observed indicating thepresence of a non-crystalline phase. Structure factors have been extracted upto 182(6) GPa showing the presence of two well-defined peaks. A rapid change inthe intensity ratio of the two peaks is identified between 145(10) and 151(10)GPa, indicative of a phase change. Present DFT+$U$ calculations of temperaturesalong Fe$_2$O$_3$ Hugoniot are in agreement with SESAME 7440 and indicaterelatively low temperatures, below 2000 K, up to 150 GPa. The non-crystallinediffuse scattering is thus consistent with the - as yet unreported - shockamorphization of Fe$_2$O$_3$ between 122(3) and 145(10) GPa, followed by anamorphous-to-liquid transition above 151(10) GPa. Upon release, anon-crystalline phase is observed alongside crystalline $alpha$-Fe$_2$O$_3$.The extracted structure factor and pair distribution function of this releasephase resemble those reported for Fe$_2$O$_3$ melt at ambient pressure.
我们通过时间分辨坐标X射线衍射,展示了在激光驱动的冲击压缩下,高达209(10) GPa的Fe$_2$O$_3$非晶化和熔融的测量结果。在 122(3) GPa 时,观察到一个扩散信号,表明存在非晶相。提取的结构因子最高可达 182(6) GPa,显示存在两个定义明确的峰值。在 145(10) 和 151(10) GPa 之间,这两个峰的强度比发生了快速变化,表明发生了相变。目前对 Fe$_2$O$_3$ Hugoniot 沿线温度的 DFT+$U$ 计算与 SESAME 7440 一致,表明温度相对较低,低于 2000 K,最高可达 150 GPa。因此,非结晶漫散射与 Fe$_2$O$_3$ 在 122(3) 和 145(10) GPa 之间的休克变质(尚未报道)以及随后在 151(10) GPa 以上的非结晶到液体转变是一致的。释放时,在晶体$alpha$-Fe$_2$O$_3$旁边观察到了非晶相。这种释放相的提取结构因子和对分布函数与所报道的常压下 Fe$_2$O$_3$ 熔体的结构因子和对分布函数相似。
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引用次数: 0
Search for $tbar{t}H/A rightarrow tbar{t}tbar{t}$ production in proton-proton collisions at $sqrt{s}=13$ TeV with the ATLAS detector 用ATLAS探测器搜索质子-质子对撞在$sqrt{s}=13$ TeV下的$tbar{t}H/A rightarrow tbar{t}tbar{t}$ 产出
Pub Date : 2024-08-30 DOI: arxiv-2408.17164
ATLAS Collaboration
A search is presented for a heavy scalar ($H$) or pseudo-scalar ($A$)predicted by the two-Higgs-doublet models, where the $H/A$ is produced inassociation with a top-quark pair ($tbar{t}H/A$), and with the $H/A$ decayinginto a $tbar{t}$ pair. Events are selected requiring exactly one or twoopposite-charge electrons or muons. Data-driven corrections are applied toimprove the modelling of the $tbar{t}$+jets background in the regime with highjet and $b$-jet multiplicities. These include a novel multi-dimensionalkinematic reweighting based on a neural network trained using data andsimulations. An $H/A$-mass parameterised graph neural network is trained tooptimise the signal-to-background discrimination. In combination with theprevious search performed by the ATLAS Collaboration in the multilepton finalstate, the observed upper limits on the $tbar{t}H/A rightarrowtbar{t}tbar{t}$ production cross-section at 95% confidence level rangebetween 14 fb and 5.0 fb for an $H/A$ with mass between 400 GeV and 1000 GeV,respectively. Assuming that both the $H$ and $A$ contribute to the$tbar{t}tbar{t}$ cross-section, $tanbeta$ values below 1.7 or 0.7 areexcluded for a mass of 400 GeV or 1000 GeV, respectively. The results are alsoused to constrain a model predicting the pair production of a colour-octetscalar, with the scalar decaying into a $tbar{t}$ pair.
本文介绍了对双希格斯双重模型预测的重标量($H$)或伪标量($A$)的搜索,其中$H/A$是与顶夸克对($tbar{t}H/A$)结合产生的,而$H/A$则衰变为一个$tbar{t}$对。选择的事件需要正好有一个或两个复合电荷电子或μ介子。应用数据驱动的修正来改进高喷流和$b$喷流倍率制度下$tbar{t}$+ 射流背景的建模。这些修正包括一种新颖的多维动力学重权重,它基于一个利用数据和模拟训练出来的神经网络。训练了一个以 H/A$ 质量为参数的图神经网络,以优化信噪比辨别。结合ATLAS合作体先前在多轻子终态中进行的搜索,对于质量介于400 GeV和1000 GeV之间的$H/A$,在95%置信度下观测到的$tbar{t}H/A rightarrowtbar{t}tbar{t}$ 产生截面的上限分别为14 fb和5.0 fb。假设$H$和$A$都对$tbar{t}tbar{t}$截面有贡献,那么当质量分别为400 GeV或1000 GeV时,$tanbeta$值低于1.7或0.7就被排除在外了。这些结果还用来约束一个预测色八面体标量的成对产生的模型,即标量衰变为一个$tbar{t}$对。
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引用次数: 0
Upgrading the existing Haloscope-type detector for sensitive axion detection 升级现有的 Haloscope 型探测器,实现灵敏的轴离子探测
Pub Date : 2024-08-29 DOI: arxiv-2408.16229
L. Gao, H. Zheng, X. N. Feng, L. B. Zhao, L. F. Wei
Haloscope is one of the typical installations to detect the electromagneticresponses (EMRs) of axion field in radio-frequency (rf) band. Given what thedetection by the existing Haloscope-type detector (HTD) biased only by a highstationary magnetic field, is just the second axion-photon energy convertedeffect and thus the detectable signal is still significantly weak, here wepropose a feasible approach to upgrade the existing HTD by additionallyapplying a transverse rf modulated magnetic field for generating thefirst-order axion-photon energy converted signal. Accordingly, we argue thatthe detection sensitivity of the upgrading HTD (UHTD) could be enhancedfeasibly by a few orders of magnitude, compared with those achieved by theexisting HTDs. The feasibility of the proposed UHTD is also discussed.
光镜是在射频(rf)波段探测轴心场电磁响应(EMR)的典型装置之一。鉴于现有的光镜型探测器(HTD)仅在高静磁场的偏置下探测到的只是第二阶轴子-光子能量转换效应,因此可探测到的信号仍然很弱,我们在这里提出了一种可行的方法来升级现有的HTD,即额外应用横向射频调制磁场来产生第一阶轴子-光子能量转换信号。因此,我们认为升级版 HTD(UHTD)的探测灵敏度可以比现有 HTD 提高几个数量级。我们还讨论了所建议的 UHTD 的可行性。
{"title":"Upgrading the existing Haloscope-type detector for sensitive axion detection","authors":"L. Gao, H. Zheng, X. N. Feng, L. B. Zhao, L. F. Wei","doi":"arxiv-2408.16229","DOIUrl":"https://doi.org/arxiv-2408.16229","url":null,"abstract":"Haloscope is one of the typical installations to detect the electromagnetic\u0000responses (EMRs) of axion field in radio-frequency (rf) band. Given what the\u0000detection by the existing Haloscope-type detector (HTD) biased only by a high\u0000stationary magnetic field, is just the second axion-photon energy converted\u0000effect and thus the detectable signal is still significantly weak, here we\u0000propose a feasible approach to upgrade the existing HTD by additionally\u0000applying a transverse rf modulated magnetic field for generating the\u0000first-order axion-photon energy converted signal. Accordingly, we argue that\u0000the detection sensitivity of the upgrading HTD (UHTD) could be enhanced\u0000feasibly by a few orders of magnitude, compared with those achieved by the\u0000existing HTDs. The feasibility of the proposed UHTD is also discussed.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201435","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
Model-independent determination of the strong-phase difference between $D^0$ and $bar{D}^0 to π^+π^-π^+π^-$ decays 独立于模型确定 $D^0$ 和 $bar{D}^0 to π^+π^-π^+π^-$ 衰变的强相差
Pub Date : 2024-08-29 DOI: arxiv-2408.16279
BESIII Collaboration, M. Ablikim, M. N. Achasov, P. Adlarson, O. Afedulidis, X. C. Ai, R. Aliberti, A. Amoroso, Q. An, Y. Bai, O. Bakina, I. Balossino, Y. Ban, H. -R. Bao, V. Batozskaya, K. Begzsuren, N. Berger, M. Berlowski, M. Bertani, D. Bettoni, F. Bianchi, E. Bianco, A. Bortone, I. Boyko, R. A. Briere, A. Brueggemann, H. Cai, X. Cai, A. Calcaterra, G. F. Cao, N. Cao, S. A. Cetin, X. Y. Chai, J. F. Chang, G. R. Che, Y. Z. Che, G. Chelkov, C. Chen, C. H. Chen, Chao Chen, G. Chen, H. S. Chen, H. Y. Chen, M. L. Chen, S. J. Chen, S. L. Chen, S. M. Chen, T. Chen, X. R. Chen, X. T. Chen, Y. B. Chen, Y. Q. Chen, Z. J. Chen, Z. Y. Chen, S. K. Choi, G. Cibinetto, F. Cossio, J. J. Cui, H. L. Dai, J. P. Dai, A. Dbeyssi, R. E. de Boer, D. Dedovich, C. Q. Deng, Z. Y. Deng, A. Denig, I. Denysenko, M. Destefanis, F. De Mori, B. Ding, X. X. Ding, Y. Ding, Y. Ding, J. Dong, L. Y. Dong, M. Y. Dong, X. Dong, M. C. Du, S. X. Du, Y. Y. Duan, Z. H. Duan, P. Egorov, Y. H. Fan, J. Fang, J. Fang, S. S. Fang, W. X. Fang, Y. Fang, Y. Q. Fang, R. Farinelli, L. Fava, F. Feldbauer, G. Felici, C. Q. Feng, J. H. Feng, Y. T. Feng, M. Fritsch, C. D. Fu, J. L. Fu, Y. W. Fu, H. Gao, X. B. Gao, Y. N. Gao, Yang Gao, S. Garbolino, I. Garzia, L. Ge, P. T. Ge, Z. W. Ge, C. Geng, E. M. Gersabeck, A. Gilman, K. Goetzen, L. Gong, W. X. Gong, W. Gradl, S. Gramigna, M. Greco, M. H. Gu, Y. T. Gu, C. Y. Guan, A. Q. Guo, L. B. Guo, M. J. Guo, R. P. Guo, Y. P. Guo, A. Guskov, J. Gutierrez, K. L. Han, T. T. Han, F. Hanisch, X. Q. Hao, F. A. Harris, K. K. He, K. L. He, F. H. Heinsius, C. H. Heinz, Y. K. Heng, C. Herold, T. Holtmann, P. C. Hong, G. Y. Hou, X. T. Hou, Y. R. Hou, Z. L. Hou, B. Y. Hu, H. M. Hu, J. F. Hu, S. L. Hu, T. Hu, Y. Hu, G. S. Huang, K. X. Huang, L. Q. Huang, X. T. Huang, Y. P. Huang, Y. S. Huang, T. Hussain, F. Hölzken, N. Hüsken, N. in der Wiesche, J. Jackson, S. Janchiv, J. H. Jeong, Q. Ji, Q. P. Ji, W. Ji, X. B. Ji, X. L. Ji, Y. Y. Ji, X. Q. Jia, Z. K. Jia, D. Jiang, H. B. Jiang, P. C. Jiang, S. S. Jiang, T. J. Jiang, X. S. Jiang, Y. Jiang, J. B. Jiao, J. K. Jiao, Z. Jiao, S. Jin, Y. Jin, M. Q. Jing, X. M. Jing, T. Johansson, S. Kabana, N. Kalantar-Nayestanaki, X. L. Kang, X. S. Kang, M. Kavatsyuk, B. C. Ke, V. Khachatryan, A. Khoukaz, R. Kiuchi, O. B. Kolcu, B. Kopf, M. Kuessner, X. Kui, N. Kumar, A. Kupsc, W. Kühn, L. Lavezzi, T. T. Lei, Z. H. Lei, M. Lellmann, T. Lenz, C. Li, C. Li, C. H. Li, Cheng Li, D. M. Li, F. Li, G. Li, H. B. Li, H. J. Li, H. N. Li, Hui Li, J. R. Li, J. S. Li, K. Li, K. L. Li, L. J. Li, L. K. Li, Lei Li, M. H. Li, P. R. Li, Q. M. Li, Q. X. Li, R. Li, S. X. Li, T. Li, W. D. Li, W. G. Li, X. Li, X. H. Li, X. L. Li, X. Y. Li, X. Z. Li, Y. G. Li, Z. J. Li, Z. Y. Li, C. Liang, H. Liang, H. Liang, Y. F. Liang, Y. T. Liang, G. R. Liao, Y. P. Liao, J. Libby, A. Limphirat, C. C. Lin, D. X. Lin, T. Lin, B. J. Liu, B. X. Liu, C. Liu, C. X. Liu, F. Liu, F. H. Liu, Feng Liu, G. M. Liu, H. Liu, H. B. Liu, H. H. Liu, H. M. Liu, Huihui Liu, J. B. Liu, J. Y. Liu, K. Liu, K. Y. Liu, Ke Liu, L. Liu, L. C. Liu, Lu Liu, M. H. Liu, P. L. Liu, Q. Liu, S. B. Liu, T. Liu, W. K. Liu, W. M. Liu, X. Liu, X. Liu, Y. Liu, Y. Liu, Y. B. Liu, Z. A. Liu, Z. D. Liu, Z. Q. Liu, X. C. Lou, F. X. Lu, H. J. Lu, J. G. Lu, X. L. Lu, Y. Lu, Y. P. Lu, Z. H. Lu, C. L. Luo, J. R. Luo, M. X. Luo, T. Luo, X. L. Luo, X. R. Lyu, Y. F. Lyu, F. C. Ma, H. Ma, H. L. Ma, J. L. Ma, L. L. Ma, L. R. Ma, M. M. Ma, Q. M. Ma, R. Q. Ma, T. Ma, X. T. Ma, X. Y. Ma, Y. M. Ma, F. E. Maas, I. MacKay, M. Maggiora, S. Malde, Y. J. Mao, Z. P. Mao, S. Marcello, Z. X. Meng, J. G. Messchendorp, G. Mezzadri, H. Miao, T. J. Min, R. E. Mitchell, X. H. Mo, B. Moses, N. Yu. Muchnoi, J. Muskalla, Y. Nefedov, F. Nerling, L. S. Nie, I. B. Nikolaev, Z. Ning, S. Nisar, Q. L. Niu, W. D. Niu, Y. Niu, S. L. Olsen, S. L. Olsen, Q. Ouyang, S. Pacetti, X. Pan, Y. Pan, A. Pathak, Y. P. Pei, M. Pelizaeus, H. P. Peng, Y. Y. Peng, K. Peters, J. L. Ping, R. G. Ping, S. Plura, V. Prasad, F. Z. Qi, H. Qi, H. R. 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Measurements of the strong-phase difference between $D^0$ and$bar{D}^0topi^+pi^-pi^+pi^-$ are performed in bins of phase space. Thestudy exploits a sample of quantum-correlated $Dbar{D}$ mesons collected bythe BESIII experiment in $e^+e^-$ collisions at a center-of-mass energy of3.773~GeV, corresponding to an integrated luminosity of 2.93~fb$^{-1}$. Here,$D$ denotes a neutral charm meson in a superposition of flavor eigenstates. Thereported results are valuable for measurements of the $C!P$-violating phase$gamma$ (also denoted $phi_3$) in $B^pm to DK^pm$, $D topi^+pi^-pi^+pi^-$ decays, and the binning schemes are designed to providegood statistical sensitivity to this parameter. The expected uncertainty on$gamma$ arising from the precision of the strong-phase measurements, whenapplied to very large samples of $B$-meson decays, is around $1.5^circ$ or$2^circ$, depending on the binning scheme. The binned strong-phase parametersare combined to give a value of $F_+^{4pi} = 0.746 pm 0.010 pm 0.004$ forthe $C!P$-even fraction of $D^0 to pi^+pi^-pi^+pi^-$ decays, which isaround 30% more precise than the previous best measurement of this quantity.
对 $D^0$ 和$bar{D}^0topi^+pi^-pi^+pi^-$ 之间的强相差进行了相空间测量。研究利用了BESIII实验在质量中心能量为3.773~GeV的e^+e^-$对撞中收集的量子相关$Dbar{D}$介子样本,对应于2.93~fb$^{-1}$的综合光度。这里,$D$表示处于味道特征态叠加中的中性粲介子。报告的结果对于测量$B^pm to DK^pm$、$D topi^+pi^-pi^+pi^-$ 衰变中的$C!P$-违反相$gamma$(也表示为$phi_3$)很有价值,而且分选方案的设计为这一参数提供了良好的统计灵敏度。当应用于很大的$B$介子衰变样本时,由强相测量精度引起的$gamma$的预期不确定性约为$1.5^circ$或$2^circ$,这取决于分选方案。将分选的强相参数结合起来,可以得到$F_+^{4pi} = 0.746 pm 0.010 pm 0.004$的D^0 to pi^+pi^-pi^+pi^-$衰变的$C!P$偶数分数,这比之前对这一数量的最佳测量精确了约30%。
{"title":"Model-independent determination of the strong-phase difference between $D^0$ and $bar{D}^0 to π^+π^-π^+π^-$ decays","authors":"BESIII Collaboration, M. Ablikim, M. N. Achasov, P. Adlarson, O. Afedulidis, X. C. Ai, R. Aliberti, A. Amoroso, Q. An, Y. Bai, O. Bakina, I. Balossino, Y. Ban, H. -R. Bao, V. Batozskaya, K. Begzsuren, N. Berger, M. Berlowski, M. Bertani, D. Bettoni, F. Bianchi, E. Bianco, A. Bortone, I. Boyko, R. A. Briere, A. Brueggemann, H. Cai, X. Cai, A. Calcaterra, G. F. Cao, N. Cao, S. A. Cetin, X. Y. Chai, J. F. Chang, G. R. Che, Y. Z. Che, G. Chelkov, C. Chen, C. H. Chen, Chao Chen, G. Chen, H. S. Chen, H. Y. Chen, M. L. Chen, S. J. Chen, S. L. Chen, S. M. Chen, T. Chen, X. R. Chen, X. T. Chen, Y. B. Chen, Y. Q. Chen, Z. J. Chen, Z. Y. Chen, S. K. Choi, G. Cibinetto, F. Cossio, J. J. Cui, H. L. Dai, J. P. Dai, A. Dbeyssi, R. E. de Boer, D. Dedovich, C. Q. Deng, Z. Y. Deng, A. Denig, I. Denysenko, M. Destefanis, F. De Mori, B. Ding, X. X. Ding, Y. Ding, Y. Ding, J. Dong, L. Y. Dong, M. Y. Dong, X. Dong, M. C. Du, S. X. Du, Y. Y. Duan, Z. H. Duan, P. Egorov, Y. H. Fan, J. Fang, J. Fang, S. S. Fang, W. X. Fang, Y. Fang, Y. Q. Fang, R. Farinelli, L. Fava, F. Feldbauer, G. Felici, C. Q. Feng, J. H. Feng, Y. T. Feng, M. Fritsch, C. D. Fu, J. L. Fu, Y. W. Fu, H. Gao, X. B. Gao, Y. N. Gao, Yang Gao, S. Garbolino, I. Garzia, L. Ge, P. T. Ge, Z. W. Ge, C. Geng, E. M. Gersabeck, A. Gilman, K. Goetzen, L. Gong, W. X. Gong, W. Gradl, S. Gramigna, M. Greco, M. H. Gu, Y. T. Gu, C. Y. Guan, A. Q. Guo, L. B. Guo, M. J. Guo, R. P. Guo, Y. P. Guo, A. Guskov, J. Gutierrez, K. L. Han, T. T. Han, F. Hanisch, X. Q. Hao, F. A. Harris, K. K. He, K. L. He, F. H. Heinsius, C. H. Heinz, Y. K. Heng, C. Herold, T. Holtmann, P. C. Hong, G. Y. Hou, X. T. Hou, Y. R. Hou, Z. L. Hou, B. Y. Hu, H. M. Hu, J. F. Hu, S. L. Hu, T. Hu, Y. Hu, G. S. Huang, K. X. Huang, L. Q. Huang, X. T. Huang, Y. P. Huang, Y. S. Huang, T. Hussain, F. Hölzken, N. Hüsken, N. in der Wiesche, J. 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Yan, W. B. Yan, W. C. Yan, X. Q. Yan, H. J. Yang, H. L. Yang, H. X. Yang, J. H. Yang, T. Yang, Y. Yang, Y. F. Yang, Y. F. Yang, Y. X. Yang, Z. W. Yang, Z. P. Yao, M. Ye, M. H. Ye, J. H. Yin, Junhao Yin, Z. Y. You, B. X. Yu, C. X. Yu, G. Yu, J. S. Yu, M. C. Yu, T. Yu, X. D. Yu, Y. C. Yu, C. Z. Yuan, J. Yuan, J. Yuan, L. Yuan, S. C. Yuan, Y. Yuan, Z. Y. Yuan, C. X. Yue, A. A. Zafar, F. R. Zeng, S. H. Zeng, X. Zeng, Y. Zeng, Y. J. Zeng, Y. J. Zeng, X. Y. Zhai, Y. C. Zhai, Y. H. Zhan, A. Q. Zhang, B. L. Zhang, B. X. Zhang, D. H. Zhang, G. Y. Zhang, H. Zhang, H. Zhang, H. C. Zhang, H. H. Zhang, H. H. Zhang, H. Q. Zhang, H. R. Zhang, H. Y. Zhang, J. Zhang, J. Zhang, J. J. Zhang, J. L. Zhang, J. Q. Zhang, J. S. Zhang, J. W. Zhang, J. X. Zhang, J. Y. Zhang, J. Z. Zhang, Jianyu Zhang, L. M. Zhang, Lei Zhang, P. Zhang, Q. Y. Zhang, R. Y. Zhang, S. H. Zhang, Shulei Zhang, X. M. Zhang, X. Y Zhang, X. Y. Zhang, Y. Zhang, Y. Zhang, Y. T. Zhang, Y. H. Zhang, Y. M. Zhang, Yan Zhang, Z. D. Zhang, Z. H. Zhang, Z. L. Zhang, Z. Y. Zhang, Z. Y. Zhang, Z. Z. Zhang, G. Zhao, J. Y. Zhao, J. Z. Zhao, L. Zhao, Lei Zhao, M. G. Zhao, N. Zhao, R. P. Zhao, S. J. Zhao, Y. B. Zhao, Y. X. Zhao, Z. G. Zhao, A. Zhemchugov, B. Zheng, B. M. Zheng, J. P. Zheng, W. J. Zheng, Y. H. Zheng, B. Zhong, X. Zhong, H. Zhou, J. Y. Zhou, L. P. Zhou, S. Zhou, X. Zhou, X. K. Zhou, X. R. Zhou, X. Y. Zhou, Y. Z. Zhou, Z. C. Zhou, A. N. Zhu, J. Zhu, K. Zhu, K. J. Zhu, K. S. Zhu, L. Zhu, L. X. Zhu, S. H. Zhu, T. J. Zhu, W. D. Zhu, Y. C. Zhu, Z. A. Zhu, J. H. Zou, J. Zu","doi":"arxiv-2408.16279","DOIUrl":"https://doi.org/arxiv-2408.16279","url":null,"abstract":"Measurements of the strong-phase difference between $D^0$ and\u0000$bar{D}^0topi^+pi^-pi^+pi^-$ are performed in bins of phase space. The\u0000study exploits a sample of quantum-correlated $Dbar{D}$ mesons collected by\u0000the BESIII experiment in $e^+e^-$ collisions at a center-of-mass energy of\u00003.773~GeV, corresponding to an integrated luminosity of 2.93~fb$^{-1}$. Here,\u0000$D$ denotes a neutral charm meson in a superposition of flavor eigenstates. The\u0000reported results are valuable for measurements of the $C!P$-violating phase\u0000$gamma$ (also denoted $phi_3$) in $B^pm to DK^pm$, $D to\u0000pi^+pi^-pi^+pi^-$ decays, and the binning schemes are designed to provide\u0000good statistical sensitivity to this parameter. The expected uncertainty on\u0000$gamma$ arising from the precision of the strong-phase measurements, when\u0000applied to very large samples of $B$-meson decays, is around $1.5^circ$ or\u0000$2^circ$, depending on the binning scheme. The binned strong-phase parameters\u0000are combined to give a value of $F_+^{4pi} = 0.746 pm 0.010 pm 0.004$ for\u0000the $C!P$-even fraction of $D^0 to pi^+pi^-pi^+pi^-$ decays, which is\u0000around 30% more precise than the previous best measurement of this quantity.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201410","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
Study of the rare decay $J/ψto μ^+μ^-μ^+μ^-$ 稀有衰变 $J/ψto μ^+μ^-μ^+μ^-$ 的研究
Pub Date : 2024-08-29 DOI: arxiv-2408.16646
LHCb collaboration, R. Aaij, A. S. W. Abdelmotteleb, C. Abellan Beteta, F. Abudinén, T. Ackernley, A. A. Adefisoye, B. Adeva, M. Adinolfi, P. Adlarson, C. Agapopoulou, C. A. Aidala, Z. Ajaltouni, S. Akar, K. Akiba, P. Albicocco, J. Albrecht, F. Alessio, M. Alexander, Z. Aliouche, P. Alvarez Cartelle, R. Amalric, S. Amato, J. L. Amey, Y. Amhis, L. An, L. Anderlini, M. Andersson, A. Andreianov, P. Andreola, M. Andreotti, D. Andreou, A. Anelli, D. Ao, F. Archilli, M. Argenton, S. Arguedas Cuendis, A. Artamonov, M. Artuso, E. Aslanides, R. Ataíde Da Silva, M. Atzeni, B. Audurier, D. Bacher, I. Bachiller Perea, S. Bachmann, M. Bachmayer, J. J. Back, P. Baladron Rodriguez, V. Balagura, W. Baldini, L. Balzani, H. Bao, J. Baptista de Souza Leite, C. Barbero Pretel, M. Barbetti, I. R. Barbosa, R. J. Barlow, M. Barnyakov, S. Barsuk, W. Barter, M. Bartolini, J. Bartz, J. M. Basels, S. Bashir, G. Bassi, B. Batsukh, P. B. Battista, A. Bay, A. Beck, M. Becker, F. Bedeschi, I. B. Bediaga, N. B. 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The rare electromagnetic $J/psi to mu^+mu^-mu^+mu^-$ decay is observedwith a significance greatly exceeding the discovery threshold, usingproton-proton collision data collected by the LHCb experiment during 2016-2018at a center-of-mass energy of 13 TeV, corresponding to an integrated luminosityof $5.4,text{fb}^{-1}$. The rate of this decay is measured relative to thatof the $J/psi to mu^+mu^-$ mode. Using the QED model for the four-muondecay in the efficiency estimation, its branching fraction is determined to bebegin{equation*} {mathcal{B}}(J/psi to mu^+mu^-mu^+mu^-) =(1.13pm0.10pm0.05pm0.01)times 10^{-6}, end{equation*} where theuncertainties are statistical, systematic and due to the uncertainty on thebranching fraction of the $J/psi to mu^+mu^-$ decay.
利用LHCb实验在2016-2018年间收集的质心能量为13 TeV的质子-质子碰撞数据,观测到了罕见的电磁$J/psi to mu^+mu^-mu^+mu^-$ 衰变,其意义大大超过了发现阈值,对应的综合光度为5.4,text{fb}^{-1}$。这种衰变的速率是相对于$J/psi to mu^+mu^-$ 模式的速率测量的。在效率估算中使用四月衰变的 QED 模型,其分支分数被确定为:begin{equation*}.{mathcal{B}}(J/psitomu^+mu^-mu^+mu^-) =(1.13pm0.10pm0.05pm0.01)times 10^{-6}, end{equation*} 其中的不确定性是统计的、系统的,并且是由于 $J/psitomu^+mu^-$ 衰变的分支分数的不确定性造成的。
{"title":"Study of the rare decay $J/ψto μ^+μ^-μ^+μ^-$","authors":"LHCb collaboration, R. Aaij, A. S. W. Abdelmotteleb, C. Abellan Beteta, F. Abudinén, T. Ackernley, A. A. Adefisoye, B. Adeva, M. Adinolfi, P. Adlarson, C. Agapopoulou, C. A. Aidala, Z. Ajaltouni, S. Akar, K. Akiba, P. Albicocco, J. Albrecht, F. Alessio, M. Alexander, Z. Aliouche, P. Alvarez Cartelle, R. Amalric, S. Amato, J. L. Amey, Y. Amhis, L. An, L. Anderlini, M. Andersson, A. Andreianov, P. Andreola, M. Andreotti, D. Andreou, A. Anelli, D. Ao, F. Archilli, M. Argenton, S. Arguedas Cuendis, A. Artamonov, M. Artuso, E. Aslanides, R. Ataíde Da Silva, M. Atzeni, B. Audurier, D. Bacher, I. Bachiller Perea, S. Bachmann, M. Bachmayer, J. J. Back, P. Baladron Rodriguez, V. Balagura, W. Baldini, L. Balzani, H. Bao, J. Baptista de Souza Leite, C. Barbero Pretel, M. Barbetti, I. R. Barbosa, R. J. Barlow, M. Barnyakov, S. Barsuk, W. Barter, M. Bartolini, J. Bartz, J. M. Basels, S. Bashir, G. Bassi, B. Batsukh, P. B. 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Majewski, J. J. Malczewski, S. Malde, L. Malentacca, A. Malinin, T. Maltsev, G. Manca, G. Mancinelli, C. Mancuso, R. Manera Escalero, D. Manuzzi, D. Marangotto, J. F. Marchand, R. Marchevski, U. Marconi, S. Mariani, C. Marin Benito, J. Marks, A. M. Marshall, L. Martel, G. Martelli, G. Martellotti, L. Martinazzoli, M. Martinelli, D. Martinez Santos, F. Martinez Vidal, A. Massafferri, R. Matev, A. Mathad, V. Matiunin, C. Matteuzzi, K. R. Mattioli, A. Mauri, E. Maurice, J. Mauricio, P. Mayencourt, J. Mazorra de Cos, M. Mazurek, M. McCann, L. Mcconnell, T. H. McGrath, N. T. McHugh, A. McNab, R. McNulty, B. Meadows, G. Meier, D. Melnychuk, F. M. Meng, M. Merk, A. Merli, L. Meyer Garcia, D. Miao, H. Miao, M. Mikhasenko, D. A. Milanes, A. Minotti, E. Minucci, T. Miralles, B. Mitreska, D. S. Mitzel, A. Modak, R. A. Mohammed, R. D. Moise, S. Mokhnenko, T. Mombächer, M. Monk, S. Monteil, A. Morcillo Gomez, G. Morello, M. J. Morello, M. P. Morgenthaler, A. B. Morris, A. G. Morris, R. Mountain, H. Mu, Z. M. Mu, E. Muhammad, F. Muheim, M. Mulder, K. Müller, F. Muñoz-Rojas, R. Murta, P. Naik, T. Nakada, R. Nandakumar, T. Nanut, I. Nasteva, M. Needham, N. Neri, S. Neubert, N. Neufeld, P. Neustroev, J. Nicolini, D. Nicotra, E. M. Niel, N. Nikitin, P. Nogarolli, P. Nogga, N. S. Nolte, C. Normand, J. Novoa Fernandez, G. Nowak, C. Nunez, H. N. Nur, A. Oblakowska-Mucha, V. Obraztsov, T. Oeser, S. Okamura, A. Okhotnikov, O. Okhrimenko, R. Oldeman, F. Oliva, M. Olocco, C. J. G. Onderwater, R. H. O'Neil, D. Osthues, J. M. Otalora Goicochea, P. Owen, A. Oyanguren, O. Ozcelik, A. Padee, K. O. Padeken, B. Pagare, P. R. Pais, T. Pajero, A. Palano, M. Palutan, G. Panshin, L. Paolucci, A. Papanestis, M. Pappagallo, L. L. Pappalardo, C. Pappenheimer, C. Parkes, B. Passalacqua, G. Passaleva, D. Passaro, A. Pastore, M. Patel, J. Patoc, C. Patrignani, A. Paul, C. J. Pawley, A. Pellegrino, J. Peng, M. Pepe Altarelli, S. Perazzini, D. Pereima, H. Pereira Da Costa, A. Pereiro Castro, P. Perret, A. Perro, K. Petridis, A. Petrolini, J. P. Pfaller, H. Pham, L. Pica, M. Piccini, B. Pietrzyk, G. Pietrzyk, D. Pinci, F. Pisani, M. Pizzichemi, V. Placinta, M. Plo Casasus, T. Poeschl, F. Polci, M. Poli Lener, A. Poluektov, N. Polukhina, I. Polyakov, E. Polycarpo, S. Ponce, D. Popov, S. Poslavskii, K. Prasanth, C. Prouve, V. Pugatch, G. Punzi, S. Qasim, Q. Q. Qian, W. Qian, N. Qin, S. Qu, R. Quagliani, R. I. Rabadan Trejo, J. H. Rademacker, M. Rama, M. Ramírez García, V. Ramos De Oliveira, M. Ramos Pernas, M. S. Rangel, F. Ratnikov, G. Raven, M. Rebollo De Miguel, F. Redi, J. Reich, F. Reiss, Z. Ren, P. K. Resmi, R. Ribatti, G. R. Ricart, D. Riccardi, S. Ricciardi, K. Richardson, M. Richardson-Slipper, K. Rinnert, P. Robbe, G. Robertson, E. Rodrigues, E. Rodriguez Fernandez, J. A. Rodriguez Lopez, E. Rodriguez Rodriguez, J. Roensch, A. Rogachev, A. Rogovskiy, D. L. Rolf, P. Roloff, V. Romanovskiy, M. Romero Lamas, A. Romero Vidal, G. Romolini, F. Ronchetti, T. Rong, M. Rotondo, S. R. Roy, M. S. Rudolph, M. Ruiz Diaz, R. A. Ruiz Fernandez, J. Ruiz Vidal, A. Ryzhikov, J. Ryzka, J. J. Saavedra-Arias, J. J. Saborido Silva, R. Sadek, N. Sagidova, D. Sahoo, N. Sahoo, B. Saitta, M. Salomoni, C. Sanchez Gras, I. Sanderswood, R. Santacesaria, C. Santamarina Rios, M. Santimaria, L. Santoro, E. Santovetti, A. Saputi, D. Saranin, A. Sarnatskiy, G. Sarpis, M. Sarpis, C. Satriano, A. Satta, M. Saur, D. Savrina, H. Sazak, L. G. Scantlebury Smead, A. Scarabotto, S. Schael, S. Scherl, M. Schiller, H. Schindler, M. Schmelling, B. Schmidt, S. Schmitt, H. Schmitz, O. Schneider, A. Schopper, N. Schulte, S. Schulte, M. H. Schune, R. Schwemmer, G. Schwering, B. Sciascia, A. Sciuccati, S. Sellam, A. Semennikov, T. Senger, M. Senghi Soares, A. Sergi, N. Serra, L. Sestini, A. Seuthe, Y. Shang, D. M. Shangase, M. Shapkin, R. S. Sharma, I. Shchemerov, L. Shchutska, T. Shears, L. Shekhtman, Z. Shen, S. Sheng, V. Shevchenko, B. Shi, Q. Shi, Y. Shimizu, E. Shmanin, R. Shorkin, J. D. Shupperd, R. Silva Coutinho, G. Simi, S. Simone, N. Skidmore, T. Skwarnicki, M. W. Slater, J. C. Smallwood, E. Smith, K. Smith, M. Smith, A. Snoch, L. Soares Lavra, M. D. Sokoloff, F. J. P. Soler, A. Solomin, A. Solovev, I. Solovyev, R. Song, Y. Song, Y. Song, Y. S. Song, F. L. Souza De Almeida, B. Souza De Paula, E. Spadaro Norella, E. Spedicato, J. G. Speer, E. Spiridenkov, P. Spradlin, V. Sriskaran, F. Stagni, M. Stahl, S. Stahl, S. Stanislaus, E. N. Stein, O. Steinkamp, O. Stenyakin, H. Stevens, D. Strekalina, Y. Su, F. Suljik, J. Sun, L. Sun, Y. Sun, D. Sundfeld, W. Sutcliffe, P. N. Swallow, F. Swystun, A. Szabelski, T. Szumlak, Y. Tan, M. D. Tat, A. Terentev, F. Terzuoli, F. Teubert, E. Thomas, D. J. D. Thompson, H. Tilquin, V. Tisserand, S. T'Jampens, M. Tobin, L. Tomassetti, G. Tonani, X. Tong, D. Torres Machado, L. Toscano, D. Y. Tou, C. Trippl, G. Tuci, N. Tuning, L. H. Uecker, A. Ukleja, D. J. Unverzagt, E. Ursov, A. Usachov, A. Ustyuzhanin, U. Uwer, V. Vagnoni, G. Valenti, N. Valls Canudas, H. Van Hecke, E. van Herwijnen, C. B. Van Hulse, R. Van Laak, M. van Veghel, G. Vasquez, R. Vazquez Gomez, P. Vazquez Regueiro, C. Vázquez Sierra, S. Vecchi, J. J. Velthuis, M. Veltri, A. Venkateswaran, M. Vesterinen, D. Vico Benet, M. Vieites Diaz, X. Vilasis-Cardona, E. Vilella Figueras, A. Villa, P. Vincent, F. C. Volle, D. vom Bruch, N. Voropaev, K. Vos, G. Vouters, C. Vrahas, J. Wagner, J. Walsh, E. J. Walton, G. Wan, C. Wang, G. Wang, J. Wang, J. Wang, J. Wang, J. Wang, M. Wang, N. W. Wang, R. Wang, X. Wang, X. Wang, X. W. Wang, Y. Wang, Z. Wang, Z. Wang, Z. Wang, J. A. Ward, M. Waterlaat, N. K. Watson, D. Websdale, Y. Wei, J. Wendel, B. D. C. Westhenry, C. White, M. Whitehead, E. Whiter, A. R. Wiederhold, D. Wiedner, G. Wilkinson, M. K. Wilkinson, M. Williams, M. R. J. Williams, R. Williams, Z. Williams, F. F. Wilson, W. Wislicki, M. Witek, L. Witola, C. P. Wong, G. Wormser, S. A. Wotton, H. Wu, J. Wu, Y. Wu, Z. Wu, K. Wyllie, S. Xian, Z. Xiang, Y. Xie, A. Xu, J. Xu, L. Xu, L. Xu, M. Xu, Z. Xu, Z. Xu, Z. Xu, D. Yang, K. Yang, S. Yang, X. Yang, Y. Yang, Z. Yang, Z. Yang, V. Yeroshenko, H. Yeung, H. Yin, C. Y. Yu, J. Yu, X. Yuan, Y Yuan, E. Zaffaroni, M. Zavertyaev, M. Zdybal, C. Zeng, M. Zeng, C. Zhang, D. Zhang, J. Zhang, L. Zhang, S. Zhang, S. Zhang, Y. Zhang, Y. Z. Zhang, Y. Zhao, A. Zharkova, A. Zhelezov, S. Z. Zheng, X. Z. Zheng, Y. Zheng, T. Zhou, X. Zhou, Y. Zhou, V. Zhovkovska, L. Z. Zhu, X. Zhu, X. Zhu, V. Zhukov, J. Zhuo, Q. Zou, D. Zuliani, G. Zunica","doi":"arxiv-2408.16646","DOIUrl":"https://doi.org/arxiv-2408.16646","url":null,"abstract":"The rare electromagnetic $J/psi to mu^+mu^-mu^+mu^-$ decay is observed\u0000with a significance greatly exceeding the discovery threshold, using\u0000proton-proton collision data collected by the LHCb experiment during 2016-2018\u0000at a center-of-mass energy of 13 TeV, corresponding to an integrated luminosity\u0000of $5.4,text{fb}^{-1}$. The rate of this decay is measured relative to that\u0000of the $J/psi to mu^+mu^-$ mode. Using the QED model for the four-muon\u0000decay in the efficiency estimation, its branching fraction is determined to be\u0000begin{equation*} {mathcal{B}}(J/psi to mu^+mu^-mu^+mu^-) =\u0000(1.13pm0.10pm0.05pm0.01)times 10^{-6}, end{equation*} where the\u0000uncertainties are statistical, systematic and due to the uncertainty on the\u0000branching fraction of the $J/psi to mu^+mu^-$ decay.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201411","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
Measurement of the Decay $Ξ^{0}toΛγ$ with Entangled $Ξ^{0}barΞ^{0}$ Pairs 用纠缠的 $Ξ^{0}barΞ^{0}$ 对测量 $Ξ^{0}toΛγ$ 衰变
Pub Date : 2024-08-29 DOI: arxiv-2408.16654
BESIII Collaboration
In this Letter, a systematic study of the weak radiative hyperon decay$Xi^{0}toLambdagamma$ at an electron-positron collider using entangled$Xi^{0}bar{Xi}^{0}$ pair events is presented. The absolute branchingfraction for this decay has been measured for the first time, and is$left(1.347 pm 0.066_{mathrm stat.}pm0.054_{mathrm syst.}right)times10^{-3}$. The decay asymmetry parameter, which characterizes the effect ofparity violation in the decay, is determined to be $-0.741 pm 0.062_{mathrmstat.}pm 0.019_{mathrm syst.}$. The obtained results are consistent with theworld average values within the uncertainties, offering valuable insights intothe underlying mechanism governing the weak radiative hyperon decays. Thecharge conjugation parity ($CP$) symmetries of branching fraction and decayasymmetry parameter in the decay are also studied. No statistically significantviolation of charge conjugation parity symmetry is observed.
在这封信中,我们介绍了利用纠缠$Xi^{0}bar{Xi}^{0}$对事件在电子-正电子对撞机上对弱辐射超子衰变$Xi^{0}toLambdagamma$的系统研究。首次测量了这种衰变的绝对分支率,它是$left(1.347 pm 0.066_mathrm stat.}pm0.054_mathrm syst.}/right)(times10^{-3}$)。衰变不对称参数表征了在衰变中违反均衡性的影响,它被确定为 $-0.741 pm 0.062_{mathrmstat.}pm 0.019_{mathrm syst.}$。所得到的结果与世界平均值在不确定范围内是一致的,为了解弱辐射超子衰变的内在机制提供了宝贵的启示。此外,还研究了衰变中分支率和衰变不对称参数的电荷共轭奇偶性($CP$)对称性。在统计意义上没有观察到电荷共轭奇偶对称性的明显违反。
{"title":"Measurement of the Decay $Ξ^{0}toΛγ$ with Entangled $Ξ^{0}barΞ^{0}$ Pairs","authors":"BESIII Collaboration","doi":"arxiv-2408.16654","DOIUrl":"https://doi.org/arxiv-2408.16654","url":null,"abstract":"In this Letter, a systematic study of the weak radiative hyperon decay\u0000$Xi^{0}toLambdagamma$ at an electron-positron collider using entangled\u0000$Xi^{0}bar{Xi}^{0}$ pair events is presented. The absolute branching\u0000fraction for this decay has been measured for the first time, and is\u0000$left(1.347 pm 0.066_{mathrm stat.}pm0.054_{mathrm syst.}right)times\u000010^{-3}$. The decay asymmetry parameter, which characterizes the effect of\u0000parity violation in the decay, is determined to be $-0.741 pm 0.062_{mathrm\u0000stat.}pm 0.019_{mathrm syst.}$. The obtained results are consistent with the\u0000world average values within the uncertainties, offering valuable insights into\u0000the underlying mechanism governing the weak radiative hyperon decays. The\u0000charge conjugation parity ($CP$) symmetries of branching fraction and decay\u0000asymmetry parameter in the decay are also studied. No statistically significant\u0000violation of charge conjugation parity symmetry is observed.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201409","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
Longitudinal double spin asymmetry of $π^{pm}$-tagged jet, $Λ$, $overlineΛ$, and $K_S^0$ in polarized $p+p$ collisions at $sqrt{s}=200$ $rm{GeV}$ at STAR 在STAR的$sqrt{s}=200$rm{GeV}$极化的$p+p$对撞中,$π^{pm}$标记的射流、$Λ$、$overlineΛ$和$K_S^0$的纵向双自旋不对称现象
Pub Date : 2024-08-28 DOI: arxiv-2408.15479
Yi Yu
Understanding the origin of the proton spin is one of the most fundamentaland challenging questions in QCD. Much progress has been made since the firstsurprising result by the EMC experiment in the late 1980s. However, thehelicity distributions of strange quarks and anti-quarks inside the proton arestill not well constrained by the experimental data. Measurement of thelongitudinal double spin asymmetry $A_{LL}$ of the inclusive jets tagged with a$pi^{pm}/pi^-$ carrying high jet momentum fraction, $z$, in $p+p$ collisionscan provide further constraints on the gluon helicity distribution in theproton. In addition, the $A_{LL}$ of $Lambda$, $overline{Lambda}$ and$K_S^0$ in the longitudinally polarized $p+p$ collisions may shed light on thestrange quark and anti-quark helicity distributions. In this contribution, wereport the preliminary results on the $A_{LL}$ measurements of inclusive jetstagged with a high-$z$ $pi^{pm}$, and the $Lambda$, $overline{Lambda}$ and$K_S^0$. We utilize the longitudinally polarized $p+p$ collisions at$sqrt{s}=200$ $rm{GeV}$ collected by the STAR experiment with an integratedluminosity of about 52 $rm{pb^{-1}}$.
理解质子自旋的起源是 QCD 最基本和最具挑战性的问题之一。自 20 世纪 80 年代末 EMC 实验首次得出令人惊讶的结果以来,已经取得了很大进展。然而,质子内部奇异夸克和反夸克的异性分布仍然没有得到实验数据的很好约束。在p+p对撞中,测量携带高喷流动量分数$z$的包容喷流的纵向双自旋不对称性$A_{LL}$,可以进一步约束质子内的胶子螺旋分布。此外,在纵向极化的p+p$对撞中,$Lambda$、$overline{Lambda}$和$K_S^0$的$A_{LL}$可能会揭示奇异夸克和反夸克的螺旋度分布。在这篇论文中,我们报告了对具有高$z$ $pi^{pm}$、$Lambda$、$overline{Lambda}$和$K_S^0$的包容射流的$A_{LL}$测量的初步结果。我们利用STAR实验收集到的在$sqrt{s}=200$$rm{GeV}$条件下纵向偏振的$p+p$对撞,其综合光度约为52$rm{pb^{-1}}$。
{"title":"Longitudinal double spin asymmetry of $π^{pm}$-tagged jet, $Λ$, $overlineΛ$, and $K_S^0$ in polarized $p+p$ collisions at $sqrt{s}=200$ $rm{GeV}$ at STAR","authors":"Yi Yu","doi":"arxiv-2408.15479","DOIUrl":"https://doi.org/arxiv-2408.15479","url":null,"abstract":"Understanding the origin of the proton spin is one of the most fundamental\u0000and challenging questions in QCD. Much progress has been made since the first\u0000surprising result by the EMC experiment in the late 1980s. However, the\u0000helicity distributions of strange quarks and anti-quarks inside the proton are\u0000still not well constrained by the experimental data. Measurement of the\u0000longitudinal double spin asymmetry $A_{LL}$ of the inclusive jets tagged with a\u0000$pi^{pm}/pi^-$ carrying high jet momentum fraction, $z$, in $p+p$ collisions\u0000can provide further constraints on the gluon helicity distribution in the\u0000proton. In addition, the $A_{LL}$ of $Lambda$, $overline{Lambda}$ and\u0000$K_S^0$ in the longitudinally polarized $p+p$ collisions may shed light on the\u0000strange quark and anti-quark helicity distributions. In this contribution, we\u0000report the preliminary results on the $A_{LL}$ measurements of inclusive jets\u0000tagged with a high-$z$ $pi^{pm}$, and the $Lambda$, $overline{Lambda}$ and\u0000$K_S^0$. We utilize the longitudinally polarized $p+p$ collisions at\u0000$sqrt{s}=200$ $rm{GeV}$ collected by the STAR experiment with an integrated\u0000luminosity of about 52 $rm{pb^{-1}}$.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201429","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
Axion Dark Matter eXperiment around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability 利用Dine-Fischler-Srednicki-Zhitnitsky发现能力进行3.3微伏左右的轴子暗物质实验
Pub Date : 2024-08-27 DOI: arxiv-2408.15227
C. Bartram, C. Boutan, T. Braine, J. H. Buckley, T. J. Caligiure, G. Carosi, A. S. Chou, C. Cisneros, John Clarke, E. J. Daw, N. Du, L. D. Duffy, T. A. Dyson, C. Gaikwad, J. R. Gleason, C. Goodman, M. Goryachev, M. Guzzetti, C. Hanretty, E. Hartman, A. T. Hipp, J. Hoffman, M. Hollister, R. Khatiwada, S. Knirck, C. L. Kuo, E. Lentz, B. T. McAllister, C. Mostyn, K. Murch, N. S. Oblath, M. G. Perry, A. Quiskamp, N. Robertson, L. J Rosenberg, S. Ruppert, G. Rybka, I. Siddiqi, P. Sikivie, J. Sinnis, M. E. Solano, A. Sonnenschein, N. S. Sullivan, D. B. Tanner, M. S. Taubman, M. E. Tobar, M. O. Withers, N. Woollett, D. Zhang
We report the results of a QCD axion dark matter search with discoveryability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axionhaloscope. Sub-Kelvin noise temperatures are reached with an ultra low-noiseJosephson parametric amplifier cooled by a dilution refrigerator. This workexcludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to3.34 {mu}eV, assuming a standard halo model with a local energy density of0.45 GeV/cc made up 100% of axions.
我们报告了利用轴子显微镜对具有发现性的 Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) 轴子进行 QCD 轴子暗物质搜索的结果。通过稀释冰箱冷却的超低噪声约瑟夫森参量放大器达到了亚开尔文噪声温度。这项工作(在90%的置信度下)排除了质量在3.27到3.34 {mu}eV 之间的DFSZ轴子,假定一个局部能量密度为0.45 GeV/cc的标准晕模型100%由轴子构成。
{"title":"Axion Dark Matter eXperiment around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability","authors":"C. Bartram, C. Boutan, T. Braine, J. H. Buckley, T. J. Caligiure, G. Carosi, A. S. Chou, C. Cisneros, John Clarke, E. J. Daw, N. Du, L. D. Duffy, T. A. Dyson, C. Gaikwad, J. R. Gleason, C. Goodman, M. Goryachev, M. Guzzetti, C. Hanretty, E. Hartman, A. T. Hipp, J. Hoffman, M. Hollister, R. Khatiwada, S. Knirck, C. L. Kuo, E. Lentz, B. T. McAllister, C. Mostyn, K. Murch, N. S. Oblath, M. G. Perry, A. Quiskamp, N. Robertson, L. J Rosenberg, S. Ruppert, G. Rybka, I. Siddiqi, P. Sikivie, J. Sinnis, M. E. Solano, A. Sonnenschein, N. S. Sullivan, D. B. Tanner, M. S. Taubman, M. E. Tobar, M. O. Withers, N. Woollett, D. Zhang","doi":"arxiv-2408.15227","DOIUrl":"https://doi.org/arxiv-2408.15227","url":null,"abstract":"We report the results of a QCD axion dark matter search with discovery\u0000ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion\u0000haloscope. Sub-Kelvin noise temperatures are reached with an ultra low-noise\u0000Josephson parametric amplifier cooled by a dilution refrigerator. This work\u0000excludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to\u00003.34 {mu}eV, assuming a standard halo model with a local energy density of\u00000.45 GeV/cc made up 100% of axions.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201508","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
期刊
arXiv - PHYS - High Energy Physics - Experiment
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