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Dark Matter Axion Search with HAYSTAC Phase II 暗物质轴子搜索与 HAYSTAC 第二阶段
Pub Date : 2024-09-13 DOI: arxiv-2409.08998
HAYSTAC Collaboration, Xiran Bai, M. J. Jewell, J. M. Echevers, K. van Bibber, S. B. Cahn, A. Droster, Maryam H. Esmat, Sumita Ghosh, Eleanor Graham, H. Jackson, Claire Laffan, S. K. Lamoreaux, A. F. Leder, K. W. Lehnert, S. M. Lewis, R. H. Maruyama, R. D. Nath, N. M. Rapidis, E. P. Ruddy, M. Silva-Feaver, M. Simanovskaia, Sukhman Singh, D. H. Speller, Sabrina Zacarias, Yuqi Zhu
This Letter reports new results from the HAYSTAC experiment's search for darkmatter axions in our galactic halo. It represents the widest search to datethat utilizes squeezing to realize sub-quantum limited noise. The new resultscover 1.71 $mu$eV of newly scanned parameter space in the mass ranges17.28--18.44 $mu$eV and 18.71--19.46 $mu$eV. No statistically significantevidence of an axion signal was observed, excluding couplings $|g_gamma|geq$2.75$times$$|g_{gamma}^{text{KSVZ}}|$ and $|g_gamma|geq$2.96$times$$|g_{gamma}^{text{KSVZ}}|$ at the 90$%$ confidence level overthe respective region. By combining this data with previously published resultsusing HAYSTAC's squeezed state receiver, a total of 2.27 $mu$eV of parameterspace has now been scanned between 16.96--19.46 $mu$eV, excluding$|g_gamma|geq$ 2.86$times$$|g_{gamma}^{text{KSVZ}}|$ at the 90$%$confidence level. These results demonstrate the squeezed state receiver'sability to probe axion models over a significant mass range while achieving ascan rate enhancement relative to a quantum-limited experiment.
这封信报告了HAYSTAC实验搜索银河系光晕中暗物质轴子的新结果。这是迄今为止利用挤压实现亚量子有限噪声的最广泛搜索。新结果在质量范围17.28--18.44 和18.71--19.46 美元/mu$eV的新扫描参数空间中覆盖了1.71 美元/mu$eV。在90%置信度下,在相应区域内没有观测到轴子信号的统计意义上的证据,不包括耦合度$2.75$times$|g_{gamma}^{text{KSVZ}}|$和$2.96$times$|g_{gamma}^{text{KSVZ}}|$。通过将这些数据与之前发表的使用HAYSTAC挤压态接收器的结果相结合,现在已经在16.96--19.46 $mu$eV 之间扫描了总共2.27 $mu$eV 的参数空间,其中不包括在90%置信水平上2.86 $times$$|g_gamma}^{text{KSVZ}} 的参数。这些结果表明,挤压态接收器能够在相当大的质量范围内探测轴子模型,同时实现相对于量子限制实验的速率增强。
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引用次数: 0
Exploring code portability solutions for HEP with a particle tracking test code 利用粒子跟踪测试代码探索 HEP 的代码可移植性解决方案
Pub Date : 2024-09-13 DOI: arxiv-2409.09228
Hammad Ather, Sophie Berkman, Giuseppe Cerati, Matti Kortelainen, Ka Hei Martin Kwok, Steven Lantz, Seyong Lee, Boyana Norris, Michael Reid, Allison Reinsvold Hall, Daniel Riley, Alexei Strelchenko, Cong Wang
Traditionally, high energy physics (HEP) experiments have relied on x86 CPUsfor the majority of their significant computing needs. As the field looks aheadto the next generation of experiments such as DUNE and the High-Luminosity LHC,the computing demands are expected to increase dramatically. To cope with thisincrease, it will be necessary to take advantage of all available computingresources, including GPUs from different vendors. A broad landscape of codeportability tools -- including compiler pragma-based approaches, abstractionlibraries, and other tools -- allow the same source code to run efficiently onmultiple architectures. In this paper, we use a test code taken from a HEPtracking algorithm to compare the performance and experience of implementingdifferent portability solutions.
传统上,高能物理(HEP)实验的大部分重要计算需求都依赖于 x86 CPU。随着该领域对下一代实验(如 DUNE 和高亮度 LHC)的展望,预计计算需求将急剧增加。为了应对这一增长,有必要利用所有可用的计算资源,包括来自不同供应商的 GPU。代码可移植性工具的广泛应用--包括基于编译器语法的方法、抽象库和其他工具--允许相同的源代码在多种架构上高效运行。在本文中,我们使用 HEPtracking 算法的测试代码来比较不同可移植性解决方案的性能和实施经验。
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引用次数: 0
The precision measurement of the W boson mass and its impact on physics W 玻色子质量的精确测量及其对物理学的影响
Pub Date : 2024-09-12 DOI: arxiv-2409.08244
Ashutosh Vijay Kotwal
As a mediator of the weak nuclear force, the W boson influences manyproperties of fundamental particles and their interactions. Understanding the Wboson as accurately as possible, including knowing its mass, has been apriority in particle physics for decades. In the past few years, in asuccession of increasing-precision measurements by multiple experiments, asignificant tension between the measured and predicted mass has been documentedby the CDF Collaboration. Furthermore, smaller differences between differentmeasurements exist. Because the W boson mass provides a window on new physics,a comparison between different measurement techniques can inform the path tofurther investigations. This Perspective article overviews the role of the Wboson mass in the Standard Model of Particle Physics and its extensions,compares and contrasts its measurement techniques and discusses prospects andfuture directions.
作为弱核力的媒介,W玻色子影响着基本粒子及其相互作用的许多特性。几十年来,尽可能准确地了解 W 玻色子,包括知道它的质量,一直是粒子物理学的当务之急。在过去的几年里,随着多个实验的测量精度不断提高,CDF 协作组织已经记录了测量质量与预测质量之间的显著差距。此外,不同测量结果之间也存在较小的差异。由于 W 玻色子的质量提供了一个了解新物理的窗口,对不同测量技术进行比较可以为进一步的研究提供信息。这篇 "视角 "文章概述了 W 玻色子质量在粒子物理标准模型及其扩展中的作用,比较和对比了其测量技术,并讨论了前景和未来方向。
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引用次数: 0
Measurements of the $CP$-even fractions of $D^0toπ^{+}π^{-}π^{0}$ and $D^0to K^{+}K^{-}π^{0}$ at BESIII 在 BESIII 测量 $D^0toπ^{+}π^{-}π^{0}$ 和 $D^0to K^{+}K^{-}π^{0}$ 的 $CP$ 偶数分数
Pub Date : 2024-09-11 DOI: arxiv-2409.07197
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, Q. P. 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. 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Prasad, F. Z. Qi, H. Qi, H. R. Qi, M. Qi, T. Y. Qi, S. Qian, W. B. Qian, C. F. Qiao, X. K. Qiao, J. J. Qin, L. Q. Qin, L. Y. Qin, X. P. Qin, X. S. Qin, Z. H. Qin, J. F. Qiu, Z. H. Qu, C. F. Redmer, K. J. Ren, A. Rivetti, M. Rolo, G. Rong, Ch. Rosner, M. Q. Ruan, S. N. Ruan, N. Salone, A. Sarantsev, Y. Schelhaas, K. Schoenning, M. Scodeggio, K. Y. Shan, W. Shan, X. Y. Shan, Z. J. Shang, J. F. Shangguan, L. G. Shao, M. Shao, C. P. Shen, H. F. Shen, W. H. Shen, X. Y. Shen, B. A. Shi, H. Shi, H. C. Shi, J. L. Shi, J. Y. Shi, Q. Q. Shi, S. Y. Shi, X. Shi, J. J. Song, T. Z. Song, W. M. Song, Y. J. Song, Y. X. Song, S. Sosio, S. Spataro, F. Stieler, S. S Su, Y. J. Su, G. B. Sun, G. X. Sun, H. Sun, H. K. Sun, J. F. Sun, K. Sun, L. Sun, S. S. Sun, T. Sun, W. Y. Sun, Y. Sun, Y. J. Sun, Y. Z. Sun, Z. Q. Sun, Z. T. Sun, C. J. Tang, G. Y. Tang, J. Tang, M. Tang, Y. A. Tang, L. Y. Tao, Q. T. Tao, M. Tat, J. X. Teng, V. Thoren, W. H. Tian, Y. Tian, Z. F. Tian, I. Uman, Y. Wan, S. J. Wang, B. 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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
The $CP$-even fractions ($F_{+}$) of the decays $D^0topi^{+}pi^{-}pi^{0}$and $D^0to K^{+}K^{-}pi^{0}$ are measured with a quantum-correlated$psi(3770)to Dbar{D}$ data sample collected by the BESIII experimentcorresponding to an integrated luminosity of 7.93 $mathrm{fb}^{-1}$. Theresults are $F_{+}^{pi^{+}pi^{-}pi^{0}}=0.9406pm0.0036pm0.0021$ and$F_{+}^{K^{+}K^{-}pi^{0}}=0.631pm0.014pm0.011$, where the firstuncertainties are statistical and the second systematic. These measurements areconsistent with the previous determinations, and the uncertainties for$F_{+}^{pi^{+}pi^{-}pi^{0}}$ and $F_{+}^{K^{+}K^{-}pi^{0}}$ are reduced byfactors of 3.9 and 2.6, respectively. The reported results provide importantinputs for the precise measurement of the angle $gamma$ of theCabibbo-Kobayashi-Maskawa matrix and indirect $CP$ violation in charm mixing.
用 BESIII 实验收集的量子相关$psi(3770)to Dbar{D}$ 数据样本测量了 $D^0topi^{+}pi^{-}pi^{0}$ 和 $D^0to K^{+}K^{-}pi^{0}$ 衰变的 $CP$ 偶数分数($F_{+}$),对应于 7.93 $mathrm{fb}^{-1}$.结果是$F_{+}^{pi^{+}/pi^{-}/pi^{0}}=0.9406/pm0.0036/pm0.0021$和$F_{+}^{K^{+}K^{-}/pi^{0}}=0.631/pm0.014/pm0.011$,其中第一个不确定度是统计不确定度,第二个是系统不确定度。这些测量结果与之前的测定结果一致,而且 $F_{+}^{pi^{+}pi^{-}pi^{0}}$ 和 $F_{+}^{K^{+}K^{-}pi^{0}}$ 的不确定性分别降低了 3.9 和 2.6 倍。报告的结果为精确测量卡比波-小林-马斯喀瓦矩阵的角度$gamma$和间接测量粲混合中的$CP$违反提供了重要的输入。
{"title":"Measurements of the $CP$-even fractions of $D^0toπ^{+}π^{-}π^{0}$ and $D^0to K^{+}K^{-}π^{0}$ at BESIII","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, Q. P. 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, J. J. Lane, 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. Qi, M. Qi, T. Y. Qi, S. Qian, W. B. Qian, C. F. Qiao, X. K. Qiao, J. J. Qin, L. Q. Qin, L. Y. Qin, X. P. Qin, X. S. Qin, Z. H. Qin, J. F. Qiu, Z. H. Qu, C. F. Redmer, K. J. Ren, A. Rivetti, M. Rolo, G. Rong, Ch. Rosner, M. Q. Ruan, S. N. Ruan, N. Salone, A. Sarantsev, Y. Schelhaas, K. Schoenning, M. Scodeggio, K. Y. Shan, W. Shan, X. Y. Shan, Z. J. Shang, J. F. Shangguan, L. G. Shao, M. Shao, C. P. Shen, H. F. Shen, W. H. Shen, X. Y. Shen, B. A. Shi, H. Shi, H. C. Shi, J. L. Shi, J. Y. Shi, Q. Q. Shi, S. Y. Shi, X. Shi, J. J. Song, T. Z. Song, W. M. Song, Y. J. Song, Y. X. Song, S. Sosio, S. Spataro, F. Stieler, S. S Su, Y. J. Su, G. B. Sun, G. X. Sun, H. Sun, H. K. Sun, J. F. Sun, K. Sun, L. Sun, S. S. Sun, T. Sun, W. Y. Sun, Y. Sun, Y. J. Sun, Y. Z. Sun, Z. Q. Sun, Z. T. Sun, C. J. Tang, G. Y. Tang, J. Tang, M. Tang, Y. A. Tang, L. Y. Tao, Q. T. Tao, M. Tat, J. X. Teng, V. Thoren, W. H. Tian, Y. Tian, Z. F. Tian, I. Uman, Y. Wan, S. J. Wang, B. Wang, B. L. Wang, Bo Wang, D. Y. Wang, F. Wang, H. J. Wang, J. J. Wang, J. P. Wang, K. Wang, L. L. Wang, M. Wang, N. Y. Wang, S. Wang, S. Wang, T. Wang, T. J. Wang, W. Wang, W. Wang, W. P. Wang, X. Wang, X. F. Wang, X. J. Wang, X. L. Wang, X. N. Wang, Y. Wang, Y. D. Wang, Y. F. Wang, Y. L. Wang, Y. N. Wang, Y. Q. Wang, Yaqian Wang, Yi Wang, Z. Wang, Z. L. Wang, Z. Y. Wang, Ziyi Wang, D. H. Wei, F. Weidner, S. P. Wen, Y. R. Wen, U. Wiedner, G. Wilkinson, M. Wolke, L. Wollenberg, C. Wu, J. F. Wu, L. H. Wu, L. J. Wu, X. Wu, X. H. Wu, Y. Wu, Y. H. Wu, Y. J. Wu, Z. Wu, L. Xia, X. M. Xian, B. H. Xiang, T. Xiang, D. Xiao, G. Y. Xiao, S. Y. Xiao, Y. L. Xiao, Z. J. Xiao, C. Xie, X. H. Xie, Y. Xie, Y. G. Xie, Y. H. Xie, Z. P. Xie, T. Y. Xing, C. F. Xu, C. J. Xu, G. F. Xu, H. Y. Xu, M. Xu, Q. J. Xu, Q. N. Xu, W. Xu, W. L. Xu, X. P. Xu, Y. Xu, Y. C. Xu, Z. S. Xu, F. Yan, L. 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-2409.07197","DOIUrl":"https://doi.org/arxiv-2409.07197","url":null,"abstract":"The $CP$-even fractions ($F_{+}$) of the decays $D^0topi^{+}pi^{-}pi^{0}$\u0000and $D^0to K^{+}K^{-}pi^{0}$ are measured with a quantum-correlated\u0000$psi(3770)to Dbar{D}$ data sample collected by the BESIII experiment\u0000corresponding to an integrated luminosity of 7.93 $mathrm{fb}^{-1}$. The\u0000results are $F_{+}^{pi^{+}pi^{-}pi^{0}}=0.9406pm0.0036pm0.0021$ and\u0000$F_{+}^{K^{+}K^{-}pi^{0}}=0.631pm0.014pm0.011$, where the first\u0000uncertainties are statistical and the second systematic. These measurements are\u0000consistent with the previous determinations, and the uncertainties for\u0000$F_{+}^{pi^{+}pi^{-}pi^{0}}$ and $F_{+}^{K^{+}K^{-}pi^{0}}$ are reduced by\u0000factors of 3.9 and 2.6, respectively. The reported results provide important\u0000inputs for the precise measurement of the angle $gamma$ of the\u0000Cabibbo-Kobayashi-Maskawa matrix and indirect $CP$ violation in charm mixing.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201407","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
Initial performance of the Radar Echo Telescope for Cosmic Rays, RET-CR 宇宙射线雷达回波望远镜(RET-CR)的初步性能
Pub Date : 2024-09-11 DOI: arxiv-2409.07511
P. Allison, J. Beatty, D. Besson, A. Connolly, A. Cummings, C. Deaconu, S. De Kockere, K. D. de Vries, D. Frikken, C. Hast, E. Huesca Santiago, C. -Y. Kuo, A. Kyriacou, U. A. Latif, J. Loonen, I. Loudon, V. Lukic, C. McLennan, K. Mulrey, J. Nam, K. Nivedita, A. Nozdrina, E. Oberla, S. Prohira, J. P. Ralston, M. F. H. Seikh, R. S. Stanley, S. Toscano, D. Van den Broeck, N. van Eijndhoven, S. Wissel
The Radar Echo Telescope for Cosmic Rays (RET-CR), a pathfinder instrumentfor the radar echo method of ultrahigh energy (UHE) neutrino detection, wasinitially deployed near Summit Station, Greenland, in May 2023. After a 4 weekcommissioning period, 9 days of data were taken before the instrument wentoffline. In this article, we describe the instrument as it was deployed, andthe initial performance of the detector. We show that the technical aspects ofrunning a radar based particle cascade detector in the ice have beendemonstrated. Analysis of the 2023 data informed improvements that wereincorporated into the May-August 2024 deployment, which has just concluded attime of writing. Results from the 2024 run will be presented in forthcomingpublications.
宇宙射线雷达回波望远镜(RET-CR)是超高能(UHE)中微子探测雷达回波法的探路仪器,于 2023 年 5 月首次部署在格陵兰高峰站附近。经过 4 周的调试,仪器在下线前采集了 9 天的数据。在这篇文章中,我们介绍了仪器的部署情况以及探测器的初始性能。我们展示了在冰层中运行基于雷达的粒子级联探测器的技术方面。对 2023 年数据的分析为 2024 年 5 月至 8 月的部署提供了改进信息,在撰写本报告时,部署刚刚结束。2024 年的运行结果将在即将出版的刊物中介绍。
{"title":"Initial performance of the Radar Echo Telescope for Cosmic Rays, RET-CR","authors":"P. Allison, J. Beatty, D. Besson, A. Connolly, A. Cummings, C. Deaconu, S. De Kockere, K. D. de Vries, D. Frikken, C. Hast, E. Huesca Santiago, C. -Y. Kuo, A. Kyriacou, U. A. Latif, J. Loonen, I. Loudon, V. Lukic, C. McLennan, K. Mulrey, J. Nam, K. Nivedita, A. Nozdrina, E. Oberla, S. Prohira, J. P. Ralston, M. F. H. Seikh, R. S. Stanley, S. Toscano, D. Van den Broeck, N. van Eijndhoven, S. Wissel","doi":"arxiv-2409.07511","DOIUrl":"https://doi.org/arxiv-2409.07511","url":null,"abstract":"The Radar Echo Telescope for Cosmic Rays (RET-CR), a pathfinder instrument\u0000for the radar echo method of ultrahigh energy (UHE) neutrino detection, was\u0000initially deployed near Summit Station, Greenland, in May 2023. After a 4 week\u0000commissioning period, 9 days of data were taken before the instrument went\u0000offline. In this article, we describe the instrument as it was deployed, and\u0000the initial performance of the detector. We show that the technical aspects of\u0000running a radar based particle cascade detector in the ice have been\u0000demonstrated. Analysis of the 2023 data informed improvements that were\u0000incorporated into the May-August 2024 deployment, which has just concluded at\u0000time of writing. Results from the 2024 run will be presented in forthcoming\u0000publications.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201373","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 inclusive and differential cross sections of single top quark production in association with a W boson in proton-proton collisions at $sqrt{s}$ = 13.6 TeV 在 $sqrt{s}$ = 13.6 TeV 的质子-质子对撞中测量与 W 玻色子相关的单顶夸克产生的包容截面和差分截面
Pub Date : 2024-09-10 DOI: arxiv-2409.06444
CMS Collaboration
The first measurement of the inclusive and normalised differential crosssections of single top quark production in association with a W boson inproton-proton collisions at a centre-of-mass energy of 13.6 TeV is presented.The data were recorded with the CMS detector at the LHC in 2022, and correspondto an integrated luminosity of 34.7 fb$^{-1}$. The analysed events contain onemuon and one electron in the final state. For the inclusive measurement,multivariate discriminants exploiting the kinematic properties of the eventsare used to separate the signal from the dominant top quark-antiquarkproduction background. A cross section of 82.3 $pm$ 2.1 (stat)${}^{+9.9}_{-9.7}$ (syst) $pm$ 3.3 (lumi) pb is obtained, consistent with thepredictions of the standard model. A fiducial region is defined according tothe detector acceptance to perform the differential measurements. The resultingdifferential distributions are unfolded to particle level and show goodagreement with the predictions at next-to-leading order in perturbative quantumchromodynamics.
本文首次测量了在质量中心能量为13.6 TeV的质子-质子对撞中与W玻色子相关的单顶夸克产生的包容截面和归一化微分截面。这些数据是2022年在大型强子对撞机上用CMS探测器记录的,对应于34.7 fb$^{-1}$的综合光度。所分析的事件在终态中包含一个介子和一个电子。在包容性测量中,利用事件的运动学特性进行多元判别,将信号与主要的顶夸克-反夸克产生背景分离开来。得到的横截面为82.3 $pm$ 2.1 (stat)${}^{+9.9}_{-9.7}$ (syst) $pm$ 3.3 (lumi) pb,与标准模型的预测一致。在进行差分测量时,根据探测器的接受程度定义了一个靶区。所得到的差分分布被展开到粒子水平,并显示出与微扰量子色动力学的次先导阶预言非常吻合。
{"title":"Measurement of inclusive and differential cross sections of single top quark production in association with a W boson in proton-proton collisions at $sqrt{s}$ = 13.6 TeV","authors":"CMS Collaboration","doi":"arxiv-2409.06444","DOIUrl":"https://doi.org/arxiv-2409.06444","url":null,"abstract":"The first measurement of the inclusive and normalised differential cross\u0000sections of single top quark production in association with a W boson in\u0000proton-proton collisions at a centre-of-mass energy of 13.6 TeV is presented.\u0000The data were recorded with the CMS detector at the LHC in 2022, and correspond\u0000to an integrated luminosity of 34.7 fb$^{-1}$. The analysed events contain one\u0000muon and one electron in the final state. For the inclusive measurement,\u0000multivariate discriminants exploiting the kinematic properties of the events\u0000are used to separate the signal from the dominant top quark-antiquark\u0000production background. A cross section of 82.3 $pm$ 2.1 (stat)\u0000${}^{+9.9}_{-9.7}$ (syst) $pm$ 3.3 (lumi) pb is obtained, consistent with the\u0000predictions of the standard model. A fiducial region is defined according to\u0000the detector acceptance to perform the differential measurements. The resulting\u0000differential distributions are unfolded to particle level and show good\u0000agreement with the predictions at next-to-leading order in perturbative quantum\u0000chromodynamics.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201306","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
First determination of the spin-parity of $Ξ_{c}(3055)^{+,0}$ baryons 首次测定 $Ξ_{c}(3055)^{+,0}$ 重子的自旋奇偶性
Pub Date : 2024-09-09 DOI: arxiv-2409.05440
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. A. Behling, S. Belin, V. Bellee, K. Belous, I. Belov, I. Belyaev, G. Benane, G. Bencivenni, E. Ben-Haim, A. Berezhnoy, R. Bernet, S. Bernet Andres, A. Bertolin, C. Betancourt, F. Betti, J. Bex, Ia. Bezshyiko, J. Bhom, M. S. Bieker, N. V. Biesuz, P. Billoir, A. Biolchini, M. Birch, F. C. R. Bishop, A. Bitadze, A. Bizzeti, T. Blake, F. Blanc, J. E. Blank, S. Blusk, V. Bocharnikov, J. A. Boelhauve, O. Boente Garcia, T. Boettcher, A. Bohare, A. Boldyrev, C. S. Bolognani, R. Bolzonella, N. Bondar, A. Bordelius, F. Borgato, S. Borghi, M. Borsato, J. T. Borsuk, S. A. Bouchiba, M. Bovill, T. J. V. Bowcock, A. Boyer, C. Bozzi, A. Brea Rodriguez, N. Breer, J. Brodzicka, A. Brossa Gonzalo, J. Brown, D. Brundu, E. Buchanan, A. Buonaura, L. Buonincontri, A. T. Burke, C. Burr, A. Butkevich, J. S. Butter, J. Buytaert, W. Byczynski, S. Cadeddu, H. Cai, A. C. Caillet, R. Calabrese, S. Calderon Ramirez, L. Calefice, S. Cali, M. Calvi, M. Calvo Gomez, P. Camargo Magalhaes, J. I. Cambon Bouzas, P. 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The ${{Xi}_{b}^{0(-)}to{Xi}_{c}(3055)^{+(0)}(toD^{+(0)}{Lambda}){pi}^{-}}$ decay chains are observed, and the spin-parity of${Xi}_{c}(3055)^{+(0)}$ baryons is determined for the first time. Themeasurement is performed using proton-proton collision data at a center-of-massenergy of $sqrt{s}=13,text{TeV}$, corresponding to an integrated luminosityof $5.4,text{fb}^{-1}$, recorded by the~$text{LHCb}$ experiment between 2016and 2018. The spin-parity of the ${Xi}_{c}(3055)^{+(0)}$ baryons is determinedto be $3/2^{+}$ with a significance of more than $6.5sigma$ ($3.5sigma$)compared to all other tested hypotheses. The up-down asymmetries of the${{Xi}_{b}^{0(-)}to{Xi}_{c}(3055)^{+(0)}{pi}^{-}}$ transitions are measuredto be $-0.92pm0.10pm0.05$ ($-0.92pm0.16pm0.22$), consistent with maximalparity violation, where the first uncertainty is statistical and the second issystematic. These results support the hypothesis that the${Xi}_{c}(3055)^{+(0)}$ baryons correspond to the first $D$-wave$lambda$-mode excitation of the ${Xi}_{c}$ flavor triplet.
观测到了${Xi}_{b}^{0(-)}to{Xi}_{c}(3055)^{+(0)}(toD^{+(0)}{Lambda}){pi}^{-}}$衰变链,并首次确定了${Xi}_{c}(3055)^{+(0)}$重子的自旋奇偶性。测量是利用质子-质子碰撞数据进行的,其质心能量为$sqrt{s}=13text{TeV}$,对应于5.4text{fb}^{-1}$的综合光度,由~$text{LHCb}$实验在2016年至2018年期间记录。${Xi}_{c}(3055)^{+(0)}$重子的自旋奇偶性被确定为$3/2^{+}$,与所有其他测试过的假说相比,其显著性超过$6.5sigma$(3.5sigma$)。测量到${{Xi}_{b}^{0(-)}to{{Xi}_{c}(3055)^{+(0)}{pi}^{-}}$转换的上下不对称性为$-0.92/pm0.10/pm0.05$($-0.92/pm0.16/pm0.22$),这与违反最大不等式一致,其中第一个不确定性是统计不确定性,第二个不确定性是系统不确定性。这些结果支持这样的假设,即${Xi}_{c}(3055)^{+(0)}$重子对应于${Xi}_{c}$味道三重子的第一个$D$波$lambda$模式激发。
{"title":"First determination of the spin-parity of $Ξ_{c}(3055)^{+,0}$ baryons","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. Battista, A. Bay, A. Beck, M. Becker, F. Bedeschi, I. B. Bediaga, N. A. Behling, S. Belin, V. Bellee, K. Belous, I. Belov, I. Belyaev, G. Benane, G. Bencivenni, E. Ben-Haim, A. Berezhnoy, R. Bernet, S. Bernet Andres, A. Bertolin, C. Betancourt, F. Betti, J. Bex, Ia. Bezshyiko, J. Bhom, M. S. Bieker, N. V. Biesuz, P. Billoir, A. Biolchini, M. Birch, F. C. R. Bishop, A. Bitadze, A. Bizzeti, T. Blake, F. Blanc, J. E. Blank, S. Blusk, V. Bocharnikov, J. A. Boelhauve, O. Boente Garcia, T. Boettcher, A. Bohare, A. Boldyrev, C. S. Bolognani, R. Bolzonella, N. Bondar, A. Bordelius, F. Borgato, S. Borghi, M. Borsato, J. T. Borsuk, S. A. Bouchiba, M. Bovill, T. J. V. Bowcock, A. Boyer, C. Bozzi, A. Brea Rodriguez, N. Breer, J. Brodzicka, A. Brossa Gonzalo, J. Brown, D. Brundu, E. Buchanan, A. Buonaura, L. Buonincontri, A. T. Burke, C. Burr, A. Butkevich, J. S. Butter, J. Buytaert, W. Byczynski, S. Cadeddu, H. Cai, A. C. Caillet, R. Calabrese, S. Calderon Ramirez, L. Calefice, S. Cali, M. Calvi, M. Calvo Gomez, P. Camargo Magalhaes, J. I. Cambon Bouzas, P. Campana, D. H. Campora Perez, A. F. Campoverde Quezada, S. Capelli, L. Capriotti, R. Caravaca-Mora, A. Carbone, L. Carcedo Salgado, R. Cardinale, A. Cardini, P. Carniti, L. Carus, A. Casais Vidal, R. Caspary, G. Casse, J. Castro Godinez, M. Cattaneo, G. Cavallero, V. Cavallini, S. Celani, D. Cervenkov, S. Cesare, A. J. Chadwick, I. Chahrour, M. Charles, Ph. Charpentier, E. Chatzianagnostou, C. A. Chavez Barajas, M. Chefdeville, C. Chen, S. Chen, Z. Chen, A. Chernov, S. Chernyshenko, X. Chiotopoulos, V. Chobanova, S. Cholak, M. Chrzaszcz, A. Chubykin, V. Chulikov, P. Ciambrone, X. Cid Vidal, G. Ciezarek, P. Cifra, P. E. L. Clarke, M. Clemencic, H. V. Cliff, J. Closier, C. Cocha Toapaxi, V. Coco, J. Cogan, E. Cogneras, L. Cojocariu, P. Collins, T. Colombo, M. C. Colonna, A. Comerma-Montells, L. Congedo, A. Contu, N. Cooke, I. Corredoira, A. Correia, G. Corti, J. J. Cottee Meldrum, B. Couturier, D. C. Craik, M. Cruz Torres, E. Curras Rivera, R. Currie, C. L. Da Silva, S. Dadabaev, L. Dai, X. Dai, E. Dall'Occo, J. Dalseno, C. D'Ambrosio, J. Daniel, A. Danilina, P. d'Argent, A. Davidson, J. E. Davies, A. Davis, O. De Aguiar Francisco, C. De Angelis, F. De Benedetti, J. de Boer, K. De Bruyn, S. De Capua, M. De Cian, U. De Freitas Carneiro Da Graca, E. De Lucia, J. M. De Miranda, L. De Paula, M. De Serio, P. De Simone, F. De Vellis, J. A. de Vries, F. Debernardis, D. Decamp, V. Dedu, S. Dekkers, L. Del Buono, B. Delaney, H. -P. Dembinski, J. Deng, V. Denysenko, O. Deschamps, F. Dettori, B. Dey, P. Di Nezza, I. Diachkov, S. Didenko, S. Ding, L. Dittmann, V. Dobishuk, A. D. Docheva, C. Dong, A. M. Donohoe, F. Dordei, A. C. dos Reis, A. D. Dowling, W. Duan, P. Duda, M. W. Dudek, L. Dufour, V. Duk, P. Durante, M. M. Duras, J. M. Durham, O. D. Durmus, A. Dziurda, A. Dzyuba, S. Easo, E. Eckstein, U. Egede, A. Egorychev, V. Egorychev, S. Eisenhardt, E. Ejopu, L. Eklund, M. Elashri, J. Ellbracht, S. 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Tuci, N. Tuning, L. H. Uecker, A. Ukleja, D. J. Unverzagt, E. Ursov, A. Usachov, A. Ustyuzhanin, U. Uwer, V. Vagnoni, V. Valcarce Cadenas, 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, P. V. Vidrier Villalba, 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, F. Zenesini, 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-2409.05440","DOIUrl":"https://doi.org/arxiv-2409.05440","url":null,"abstract":"The ${{Xi}_{b}^{0(-)}to{Xi}_{c}(3055)^{+(0)}(to\u0000D^{+(0)}{Lambda}){pi}^{-}}$ decay chains are observed, and the spin-parity of\u0000${Xi}_{c}(3055)^{+(0)}$ baryons is determined for the first time. The\u0000measurement is performed using proton-proton collision data at a center-of-mass\u0000energy of $sqrt{s}=13,text{TeV}$, corresponding to an integrated luminosity\u0000of $5.4,text{fb}^{-1}$, recorded by the~$text{LHCb}$ experiment between 2016\u0000and 2018. The spin-parity of the ${Xi}_{c}(3055)^{+(0)}$ baryons is determined\u0000to be $3/2^{+}$ with a significance of more than $6.5sigma$ ($3.5sigma$)\u0000compared to all other tested hypotheses. The up-down asymmetries of the\u0000${{Xi}_{b}^{0(-)}to{Xi}_{c}(3055)^{+(0)}{pi}^{-}}$ transitions are measured\u0000to be $-0.92pm0.10pm0.05$ ($-0.92pm0.16pm0.22$), consistent with maximal\u0000parity violation, where the first uncertainty is statistical and the second is\u0000systematic. These results support the hypothesis that the\u0000${Xi}_{c}(3055)^{+(0)}$ baryons correspond to the first $D$-wave\u0000$lambda$-mode excitation of the ${Xi}_{c}$ flavor triplet.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-09-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201381","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
Important Results of Different Experiments in Searching for Dark Matter Using Germanium and Silicon Detectors: A Comprehensive Review for Detecting Weakly Interacting Massive Particles 使用锗和硅探测器搜索暗物质的不同实验的重要结果:探测弱相互作用大质量粒子的全面回顾
Pub Date : 2024-09-09 DOI: arxiv-2409.08900
M. Mirzakhani, S. Maludze
Dark matter plays a crucial role in our comprehension of the universe, butits mysterious nature poses challenges for direct detection. A primary obstaclein detecting dark matter is distinguishing genuine signals from the prevailingelectromagnetic background. Germanium and Silicon detectors have emerged aseffective instruments in the pursuit of dark matter detection. Their minimalradioactive backgrounds, substantial active volumes, and efficient rejectionmechanisms have significantly advanced our understanding of dark matter and itsscattering cross section limits. Numerous experiments employing these detectorshave yielded valuable insights into the properties of dark matter. Scientistshave investigated potential dark matter candidates like Weakly InteractingMassive Particles (WIMPs) and evaluated their probability of being dark matterparticles based on observed scattering cross sections. This review consolidatesthe findings from significant experiments, encompassing possible candidates andtheir likelihood of being dark matter particles. It also recognizes thelimitations of dark matter scattering cross section by assessing progress inthis field, detector technologies, experimental outcomes, and future prospects.
暗物质在我们理解宇宙的过程中起着至关重要的作用,但其神秘的性质给直接探测带来了挑战。探测暗物质的一个主要障碍是从普遍存在的电磁背景中区分出真正的信号。锗和硅探测器已成为探测暗物质的有效工具。它们具有最小的放射性背景、巨大的有效容积和高效的剔除机制,极大地推动了我们对暗物质及其散射截面极限的理解。利用这些探测器进行的大量实验为我们深入了解暗物质的特性提供了宝贵的资料。科学家们研究了潜在的暗物质候选粒子,如弱相互作用大质量粒子(WIMPs),并根据观测到的散射截面评估了它们成为暗物质粒子的概率。这篇综述综合了重要实验的发现,包括可能的候选粒子及其成为暗物质粒子的可能性。它还通过评估该领域的进展、探测器技术、实验结果和未来前景,认识到暗物质散射截面的局限性。
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引用次数: 0
Study of the decay $D^0rightarrow ρ(770)^-e^+ν_e$ 研究衰变 $D^0rightarrow ρ(770)^-e^+ν_e$
Pub Date : 2024-09-06 DOI: arxiv-2409.04276
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, J. J. Lane, 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. Qi, M. Qi, T. Y. Qi, S. Qian, W. B. Qian, C. F. Qiao, X. K. Qiao, J. J. Qin, L. Q. Qin, L. Y. Qin, X. P. Qin, X. S. Qin, Z. H. Qin, J. F. Qiu, Z. H. Qu, C. F. Redmer, K. J. Ren, A. Rivetti, M. Rolo, G. Rong, Ch. Rosner, M. Q. Ruan, S. N. Ruan, N. Salone, A. Sarantsev, Y. Schelhaas, K. Schoenning, M. Scodeggio, K. Y. Shan, W. Shan, X. Y. Shan, Z. J. Shang, J. F. Shangguan, L. G. Shao, M. Shao, C. P. Shen, H. F. Shen, W. H. Shen, X. Y. Shen, B. A. Shi, H. Shi, H. C. Shi, J. L. Shi, J. Y. Shi, Q. Q. Shi, S. Y. Shi, X. Shi, J. J. Song, T. Z. Song, W. M. Song, Y. J. Song, Y. X. Song, S. Sosio, S. Spataro, F. Stieler, S. S Su, Y. J. Su, G. B. Sun, G. X. Sun, H. Sun, H. K. Sun, J. F. Sun, K. Sun, L. Sun, S. S. Sun, T. Sun, W. Y. Sun, Y. Sun, Y. J. Sun, Y. Z. Sun, Z. Q. Sun, Z. T. Sun, C. J. Tang, G. Y. Tang, J. Tang, M. Tang, Y. A. Tang, L. Y. Tao, Q. T. Tao, M. Tat, J. X. Teng, V. Thoren, W. H. Tian, Y. Tian, Z. F. Tian, I. Uman, Y. Wan, S. J. Wang, B. Wang, B. L. Wang, Bo Wang, D. Y. Wang, F. Wang, H. J. Wang, J. J. Wang, J. P. Wang, K. Wang, L. L. Wang, M. Wang, N. Y. Wang, S. Wang, S. Wang, T. Wang, T. J. Wang, W. Wang, W. Wang, W. P. Wang, X. Wang, X. F. Wang, X. J. Wang, X. L. Wang, X. N. Wang, Y. Wang, Y. D. Wang, Y. F. Wang, Y. L. Wang, Y. N. Wang, Y. Q. Wang, Yaqian Wang, Yi Wang, Z. Wang, Z. L. Wang, Z. Y. Wang, Ziyi Wang, D. H. Wei, F. Weidner, S. P. Wen, Y. R. Wen, U. Wiedner, G. Wilkinson, M. Wolke, L. Wollenberg, C. Wu, J. F. Wu, L. H. Wu, L. J. Wu, X. Wu, X. H. Wu, Y. Wu, Y. H. Wu, Y. J. Wu, Z. Wu, L. Xia, X. M. Xian, B. H. Xiang, T. Xiang, D. Xiao, G. Y. Xiao, S. Y. Xiao, Y. L. Xiao, Z. J. Xiao, C. Xie, X. H. Xie, Y. Xie, Y. G. Xie, Y. H. Xie, Z. P. Xie, T. Y. Xing, C. F. Xu, C. J. Xu, G. F. Xu, H. Y. Xu, M. Xu, Q. J. Xu, Q. N. Xu, W. Xu, W. L. Xu, X. P. Xu, Y. Xu, Y. C. Xu, Z. S. Xu, F. Yan, L. Yan, W. B. Yan, W. C. Yan, X. Q. Yan, H. J. Yang, H. L. Yang, H. X. 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
We present a study of the semileptonic decay $D^0rightarrowpi^-pi^0e^{+}nu_{e}$ using an $e^+e^-$ annihilation data sample of$7.93~mathrm{fb}^{-1}$ collected at the center-of-mass energy of 3.773 GeVwith the BESIII detector. The branching fraction of $D^0torho(770)^-e^+nu_e$ is measured to be $(1.439 pm 0.033(rm stat.) pm0.027(rm syst.)) times10^{-3}$, which is a factor 1.6 more precise thanprevious measurements. By performing an amplitude analysis, we measure thehadronic form-factor ratios of $D^0to rho(770)^-e^+nu_e$ at $q^2=0$ assumingthe single-pole-dominance parametrization: $r_{V}=V(0)/A_1(0)=1.548pm0.079(rmstat.)pm0.041(rm syst.)$ and $r_{2}=A_2(0)/A_1(0)=0.823pm0.056(rmstat.)pm0.026(rm syst.)$.
我们利用BESIII探测器在3.773 GeV的质心能量下收集到的7.93~mathrm{fb}^{-1}$的$e^+e^-$湮灭数据样本,对半轻子衰变$D^0rightarrowpi^-pi^0e^{+}nu_{e}$进行了研究。测得的 $D^0torho(770)^-e^+nu_e$ 的分支分数为 $(1.439 pm 0.033(rm stat.) pm0.027(rm syst.))times10^{-3}$,这比之前的测量精确了 1.6 倍。通过振幅分析,我们测量了在$q^2=0$假设单极支配参数:$r_{V}=V(0)/A_1(0)=1时,$D^0to rho(770)^-e^+nu_e$的强子形式因子比。548pm0.079(rmstat.)pm0.041(rm syst.)$ 和 $r_{2}=A_2(0)/A_1(0)=0.823pm0.056(rmstat.)pm0.026(rm syst.)$ 。
{"title":"Study of the decay $D^0rightarrow ρ(770)^-e^+ν_e$","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. Jackson, S. Janchiv, J. H. Jeong, Q. Ji, Q. P. Ji, W. Ji, X. B. 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X. 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-2409.04276","DOIUrl":"https://doi.org/arxiv-2409.04276","url":null,"abstract":"We present a study of the semileptonic decay $D^0rightarrow\u0000pi^-pi^0e^{+}nu_{e}$ using an $e^+e^-$ annihilation data sample of\u0000$7.93~mathrm{fb}^{-1}$ collected at the center-of-mass energy of 3.773 GeV\u0000with the BESIII detector. The branching fraction of $D^0to\u0000rho(770)^-e^+nu_e$ is measured to be $(1.439 pm 0.033(rm stat.) pm\u00000.027(rm syst.)) times10^{-3}$, which is a factor 1.6 more precise than\u0000previous measurements. By performing an amplitude analysis, we measure the\u0000hadronic form-factor ratios of $D^0to rho(770)^-e^+nu_e$ at $q^2=0$ assuming\u0000the single-pole-dominance parametrization: $r_{V}=V(0)/A_1(0)=1.548pm0.079(rm\u0000stat.)pm0.041(rm syst.)$ and $r_{2}=A_2(0)/A_1(0)=0.823pm0.056(rm\u0000stat.)pm0.026(rm syst.)$.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201376","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
Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA 在 NOvA 中对有源中微子振荡的双基线搜索
Pub Date : 2024-09-06 DOI: arxiv-2409.04553
The NOvA Collaboration
We report a search for neutrino oscillations to sterile neutrinos under amodel with three active and one sterile neutrinos (3+1 model). This analysisuses the NOvA detectors exposed to the NuMI beam, running in neutrino mode. Thedata exposure, 13.6e20 protons on target, doubles that previously analyzed byNOvA, and the analysis is the first to use $nu_{mu}$ charged-currentinteractions in conjunction with neutral-current interactions. Neutrino samplesin the Near and Far detectors are fitted simultaneously, enabling the search tobe carried out over a $Delta m^2_{41}$ range extending 2 (3) orders ofmagnitude above (below) 1 eV$^2$. NOvA finds no evidence for active-to-sterileneutrino oscillations under the 3+1 model at 90% confidence level. New limitsare reported in multiple regions of parameter space, excluding some regionscurrently allowed by IceCube at 90% confidence level. We additionally set themost stringent limits for anomalous $nu_{tau}$ appearance for $Deltam^{2}_{41} le 3$ eV$^2$.
我们报告了在三个有源中微子和一个无源中微子的模型(3+1 模型)下对中微子振荡到无源中微子的搜索。这项分析使用了暴露于 NuMI 射束的 NOvA 探测器,并以中微子模式运行。目标上的数据暴露量为13.6e20个质子,比NOvA以前分析的数据暴露量增加了一倍,这次分析首次将$nu_{mu}$带电电流相互作用与中性电流相互作用结合起来使用。近探测器和远探测器中的中微子样本是同时拟合的,这使得搜索能够在 1 eV$^2$ 以上(以下)2(3)个量级的 $Delta m^2_{41}$ 范围内进行。NOVA发现,在90%的置信度下,在3+1模型下没有证据表明有源中微子振荡。在参数空间的多个区域都报告了新的极限,其中不包括冰立方目前在 90%置信度下允许的一些区域。我们还为 $Deltam^{2}_{41}$ 的反常 $nu_{tau}$ 出现设定了最严格的限值。le 3$ eV$^2$。
{"title":"Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA","authors":"The NOvA Collaboration","doi":"arxiv-2409.04553","DOIUrl":"https://doi.org/arxiv-2409.04553","url":null,"abstract":"We report a search for neutrino oscillations to sterile neutrinos under a\u0000model with three active and one sterile neutrinos (3+1 model). This analysis\u0000uses the NOvA detectors exposed to the NuMI beam, running in neutrino mode. The\u0000data exposure, 13.6e20 protons on target, doubles that previously analyzed by\u0000NOvA, and the analysis is the first to use $nu_{mu}$ charged-current\u0000interactions in conjunction with neutral-current interactions. Neutrino samples\u0000in the Near and Far detectors are fitted simultaneously, enabling the search to\u0000be carried out over a $Delta m^2_{41}$ range extending 2 (3) orders of\u0000magnitude above (below) 1 eV$^2$. NOvA finds no evidence for active-to-sterile\u0000neutrino oscillations under the 3+1 model at 90% confidence level. New limits\u0000are reported in multiple regions of parameter space, excluding some regions\u0000currently allowed by IceCube at 90% confidence level. We additionally set the\u0000most stringent limits for anomalous $nu_{tau}$ appearance for $Delta\u0000m^{2}_{41} le 3$ eV$^2$.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201375","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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