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 to study the energetic particle sources in our Galaxy, and the interstellar environment through which these particles propagate. Uncertainties on hadronic models, ion-nucleon cross sections in particular, are currently the limiting factor towards obtaining more accurate CR ion flux measurements with calorimetric space-based experiments. We present an energy-dependent measurement 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 data collected by the DAMPE space mission. The kinetic energy range per nucleon of the measurement points ranges from 18 GeV to 9 TeV for protons, and from 5 GeV/n to 3 TeV/n for helium-4 nuclei. Our results lead to a significant improvement of the CR flux normalisation. In the case of helium-4, these results correspond to the first cross section measurements on a heavy target material at energies above 10 GeV/n.
{"title":"Hadronic cross section measurements with the DAMPE space mission using 20GeV-10TeV cosmic-ray protons and $^4$He","authors":"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","doi":"arxiv-2408.17224","DOIUrl":"https://doi.org/arxiv-2408.17224","url":null,"abstract":"Precise direct cosmic-ray (CR) measurements provide an important probe to\u0000study the energetic particle sources in our Galaxy, and the interstellar\u0000environment through which these particles propagate. Uncertainties on hadronic\u0000models, ion-nucleon cross sections in particular, are currently the limiting\u0000factor towards obtaining more accurate CR ion flux measurements with\u0000calorimetric space-based experiments. We present an energy-dependent\u0000measurement of the inelastic cross section of protons and helium-4 nuclei\u0000(alpha particles) on a Bi$_4$Ge$_3$O$_{12}$ target, using 88 months of data\u0000collected by the DAMPE space mission. The kinetic energy range per nucleon of\u0000the measurement points ranges from 18 GeV to 9 TeV for protons, and from 5\u0000GeV/n to 3 TeV/n for helium-4 nuclei. Our results lead to a significant\u0000improvement of the CR flux normalisation. In the case of helium-4, these\u0000results correspond to the first cross section measurements on a heavy target\u0000material at energies above 10 GeV/n.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201408","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}
A search for dark matter (DM) particles produced in association with bottom quarks is presented. The analysis uses proton-proton collision data at a center-of-mass energy of $sqrt{s}$ = 13 TeV, corresponding to an integrated luminosity of 138 fb$^{-1}$. The search is performed in the final state with large missing transverse momentum and a pair of jets originating from bottom quarks. No significant excess of data is observed with respect to the standard model expectation. Results are interpreted in the context of a type-II two-Higgs-doublet model with an additional light pseudoscalar (2HDM+a). An upper limit is set on the mass of the lighter pseudoscalar, excluding masses up to 260 GeV at 95% confidence level. This is the first search at the LHC to probe DM produced in association with two nonresonant bottom quarks in the 2HDM+a model. Sensitivity to the parameter space with the ratio of the vacuum expectation values of the two Higgs doublets, $tanbeta$, greater than 15 is achieved, capitalizing on the enhancement of couplings between pseudoscalars and bottom quarks with high $tanbeta$.
{"title":"Search for dark matter produced in association with a pair of bottom quarks in proton-proton collisions at $sqrt{s}$ = 13 TeV","authors":"CMS Collaboration","doi":"arxiv-2408.17336","DOIUrl":"https://doi.org/arxiv-2408.17336","url":null,"abstract":"A search for dark matter (DM) particles produced in association with bottom\u0000quarks is presented. The analysis uses proton-proton collision data at a\u0000center-of-mass energy of $sqrt{s}$ = 13 TeV, corresponding to an integrated\u0000luminosity of 138 fb$^{-1}$. The search is performed in the final state with\u0000large missing transverse momentum and a pair of jets originating from bottom\u0000quarks. No significant excess of data is observed with respect to the standard\u0000model expectation. Results are interpreted in the context of a type-II\u0000two-Higgs-doublet model with an additional light pseudoscalar (2HDM+a). An\u0000upper limit is set on the mass of the lighter pseudoscalar, excluding masses up\u0000to 260 GeV at 95% confidence level. This is the first search at the LHC to\u0000probe DM produced in association with two nonresonant bottom quarks in the\u00002HDM+a model. Sensitivity to the parameter space with the ratio of the vacuum\u0000expectation values of the two Higgs doublets, $tanbeta$, greater than 15 is\u0000achieved, capitalizing on the enhancement of couplings between pseudoscalars\u0000and bottom quarks with high $tanbeta$.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201302","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}
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 under laser-driven shock compression up to 209(10) GPa via time-resolved in situ x-ray diffraction. At 122(3) GPa, a diffuse signal is observed indicating the presence of a non-crystalline phase. Structure factors have been extracted up to 182(6) GPa showing the presence of two well-defined peaks. A rapid change in the 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 temperatures along Fe$_2$O$_3$ Hugoniot are in agreement with SESAME 7440 and indicate relatively low temperatures, below 2000 K, up to 150 GPa. The non-crystalline diffuse scattering is thus consistent with the - as yet unreported - shock amorphization of Fe$_2$O$_3$ between 122(3) and 145(10) GPa, followed by an amorphous-to-liquid transition above 151(10) GPa. Upon release, a non-crystalline phase is observed alongside crystalline $alpha$-Fe$_2$O$_3$. The extracted structure factor and pair distribution function of this release phase resemble those reported for Fe$_2$O$_3$ melt at ambient pressure.
{"title":"Shock-driven amorphization and melt in Fe$_2$O$_3$","authors":"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","doi":"arxiv-2408.17204","DOIUrl":"https://doi.org/arxiv-2408.17204","url":null,"abstract":"We present measurements on Fe$_2$O$_3$ amorphization and melt under\u0000laser-driven shock compression up to 209(10) GPa via time-resolved in situ\u0000x-ray diffraction. At 122(3) GPa, a diffuse signal is observed indicating the\u0000presence of a non-crystalline phase. Structure factors have been extracted up\u0000to 182(6) GPa showing the presence of two well-defined peaks. A rapid change in\u0000the intensity ratio of the two peaks is identified between 145(10) and 151(10)\u0000GPa, indicative of a phase change. Present DFT+$U$ calculations of temperatures\u0000along Fe$_2$O$_3$ Hugoniot are in agreement with SESAME 7440 and indicate\u0000relatively low temperatures, below 2000 K, up to 150 GPa. The non-crystalline\u0000diffuse scattering is thus consistent with the - as yet unreported - shock\u0000amorphization of Fe$_2$O$_3$ between 122(3) and 145(10) GPa, followed by an\u0000amorphous-to-liquid transition above 151(10) GPa. Upon release, a\u0000non-crystalline phase is observed alongside crystalline $alpha$-Fe$_2$O$_3$.\u0000The extracted structure factor and pair distribution function of this release\u0000phase resemble those reported for Fe$_2$O$_3$ melt at ambient pressure.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201308","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}
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 in association with a top-quark pair ($tbar{t}H/A$), and with the $H/A$ decaying into a $tbar{t}$ pair. Events are selected requiring exactly one or two opposite-charge electrons or muons. Data-driven corrections are applied to improve the modelling of the $tbar{t}$+jets background in the regime with high jet and $b$-jet multiplicities. These include a novel multi-dimensional kinematic reweighting based on a neural network trained using data and simulations. An $H/A$-mass parameterised graph neural network is trained to optimise the signal-to-background discrimination. In combination with the previous search performed by the ATLAS Collaboration in the multilepton final state, the observed upper limits on the $tbar{t}H/A rightarrow tbar{t}tbar{t}$ production cross-section at 95% confidence level range between 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 are excluded for a mass of 400 GeV or 1000 GeV, respectively. The results are also used to constrain a model predicting the pair production of a colour-octet scalar, with the scalar decaying into a $tbar{t}$ pair.
{"title":"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","authors":"ATLAS Collaboration","doi":"arxiv-2408.17164","DOIUrl":"https://doi.org/arxiv-2408.17164","url":null,"abstract":"A search is presented for a heavy scalar ($H$) or pseudo-scalar ($A$)\u0000predicted by the two-Higgs-doublet models, where the $H/A$ is produced in\u0000association with a top-quark pair ($tbar{t}H/A$), and with the $H/A$ decaying\u0000into a $tbar{t}$ pair. Events are selected requiring exactly one or two\u0000opposite-charge electrons or muons. Data-driven corrections are applied to\u0000improve the modelling of the $tbar{t}$+jets background in the regime with high\u0000jet and $b$-jet multiplicities. These include a novel multi-dimensional\u0000kinematic reweighting based on a neural network trained using data and\u0000simulations. An $H/A$-mass parameterised graph neural network is trained to\u0000optimise the signal-to-background discrimination. In combination with the\u0000previous search performed by the ATLAS Collaboration in the multilepton final\u0000state, the observed upper limits on the $tbar{t}H/A rightarrow\u0000tbar{t}tbar{t}$ production cross-section at 95% confidence level range\u0000between 14 fb and 5.0 fb for an $H/A$ with mass between 400 GeV and 1000 GeV,\u0000respectively. Assuming that both the $H$ and $A$ contribute to the\u0000$tbar{t}tbar{t}$ cross-section, $tanbeta$ values below 1.7 or 0.7 are\u0000excluded for a mass of 400 GeV or 1000 GeV, respectively. The results are also\u0000used to constrain a model predicting the pair production of a colour-octet\u0000scalar, with the scalar decaying into a $tbar{t}$ pair.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2024-08-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142201405","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}
L. Gao, H. Zheng, X. N. Feng, L. B. Zhao, L. F. Wei
Haloscope is one of the typical installations to detect the electromagnetic responses (EMRs) of axion field in radio-frequency (rf) band. Given what the detection by the existing Haloscope-type detector (HTD) biased only by a high stationary magnetic field, is just the second axion-photon energy converted effect and thus the detectable signal is still significantly weak, here we propose a feasible approach to upgrade the existing HTD by additionally applying a transverse rf modulated magnetic field for generating the first-order axion-photon energy converted signal. Accordingly, we argue that the detection sensitivity of the upgrading HTD (UHTD) could be enhanced feasibly by a few orders of magnitude, compared with those achieved by the existing HTDs. The feasibility of the proposed UHTD is also discussed.
{"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}
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. 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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. The study exploits a sample of quantum-correlated $Dbar{D}$ mesons collected by the BESIII experiment in $e^+e^-$ collisions at a center-of-mass energy of 3.773~GeV, corresponding to an integrated luminosity of 2.93~fb$^{-1}$. Here, $D$ denotes a neutral charm meson in a superposition of flavor eigenstates. The reported results are valuable for measurements of the $C!P$-violating phase $gamma$ (also denoted $phi_3$) in $B^pm to DK^pm$, $D to pi^+pi^-pi^+pi^-$ decays, and the binning schemes are designed to provide good statistical sensitivity to this parameter. The expected uncertainty on $gamma$ arising from the precision of the strong-phase measurements, when applied 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 parameters are combined to give a value of $F_+^{4pi} = 0.746 pm 0.010 pm 0.004$ for the $C!P$-even fraction of $D^0 to pi^+pi^-pi^+pi^-$ decays, which is around 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. 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. 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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, X. D. 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. 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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}
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 observed with a significance greatly exceeding the discovery threshold, using proton-proton collision data collected by the LHCb experiment during 2016-2018 at a center-of-mass energy of 13 TeV, corresponding to an integrated luminosity of $5.4,text{fb}^{-1}$. The rate of this decay is measured relative to that of the $J/psi to mu^+mu^-$ mode. Using the QED model for the four-muon decay in the efficiency estimation, its branching fraction is determined to be begin{equation*} {mathcal{B}}(J/psi to mu^+mu^-mu^+mu^-) = (1.13pm0.10pm0.05pm0.01)times 10^{-6}, end{equation*} where the uncertainties are statistical, systematic and due to the uncertainty on the branching 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. Battista, A. Bay, A. Beck, M. Becker, F. Bedeschi, I. B. Bediaga, N. B. 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, 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, X. Chang, 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. 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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}
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 branching fraction for this decay has been measured for the first time, and is $left(1.347 pm 0.066_{mathrm stat.}pm0.054_{mathrm syst.}right)times 10^{-3}$. The decay asymmetry parameter, which characterizes the effect of parity violation in the decay, is determined to be $-0.741 pm 0.062_{mathrm stat.}pm 0.019_{mathrm syst.}$. The obtained results are consistent with the world average values within the uncertainties, offering valuable insights into the underlying mechanism governing the weak radiative hyperon decays. The charge conjugation parity ($CP$) symmetries of branching fraction and decay asymmetry parameter in the decay are also studied. No statistically significant violation of charge conjugation parity symmetry is observed.
{"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}
Understanding the origin of the proton spin is one of the most fundamental and challenging questions in QCD. Much progress has been made since the first surprising result by the EMC experiment in the late 1980s. However, the helicity distributions of strange quarks and anti-quarks inside the proton are still not well constrained by the experimental data. Measurement of the longitudinal double spin asymmetry $A_{LL}$ of the inclusive jets tagged with a $pi^{pm}/pi^-$ carrying high jet momentum fraction, $z$, in $p+p$ collisions can provide further constraints on the gluon helicity distribution in the proton. In addition, the $A_{LL}$ of $Lambda$, $overline{Lambda}$ and $K_S^0$ in the longitudinally polarized $p+p$ collisions may shed light on the strange quark and anti-quark helicity distributions. In this contribution, we report the preliminary results on the $A_{LL}$ measurements of inclusive jets tagged 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 integrated luminosity of about 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}
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 discovery ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion haloscope. Sub-Kelvin noise temperatures are reached with an ultra low-noise Josephson parametric amplifier cooled by a dilution refrigerator. This work excludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to 3.34 {mu}eV, assuming a standard halo model with a local energy density of 0.45 GeV/cc made up 100% of axions.
{"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}