The past decades have witnessed the deployment of a new generation of cosmic ray (CR) observatories with unprecedented sensitivity and complexity, pushing towards ever-higher energies. To face the challenges of the multi-TeV domain, such instruments must be accompanied by equally powerful analysis techniques, able to exploit as much information as available. For example, the machine learning tool set may provide the needed techniques. We present a neural network optimised for the identification of multi-TeV electrons on DAMPE, a calorimetric spaceborne CR observatory with among other objectives the measurement of cosmic electrons up to 10 TeV. This constitutes a particularly challenging endeavour due to both the soft electron spectrum and the large proton background. The developed neural network significantly outperforms the more traditional cut-based approach, achieving a much lower proton contamination in the multi-TeV domain with a high signal efficiency, and retains its accuracy when transposed from Monte Carlo to real data.
{"title":"Neural networks for TeV cosmic electrons identification on the DAMPE experiment","authors":"D. Droz, A. Tykhonov, Xin Wu, M. Deliyergiyev","doi":"10.22323/1.398.0045","DOIUrl":"https://doi.org/10.22323/1.398.0045","url":null,"abstract":"The past decades have witnessed the deployment of a new generation of cosmic ray (CR) observatories with unprecedented sensitivity and complexity, pushing towards ever-higher energies. To face the challenges of the multi-TeV domain, such instruments must be accompanied by equally powerful analysis techniques, able to exploit as much information as available. For example, the machine learning tool set may provide the needed techniques. We present a neural network optimised for the identification of multi-TeV electrons on DAMPE, a calorimetric spaceborne CR observatory with among other objectives the measurement of cosmic electrons up to 10 TeV. This constitutes a particularly challenging endeavour due to both the soft electron spectrum and the large proton background. The developed neural network significantly outperforms the more traditional cut-based approach, achieving a much lower proton contamination in the multi-TeV domain with a high signal efficiency, and retains its accuracy when transposed from Monte Carlo to real data.","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"255 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"133931631","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}
{"title":"Measurement of the Drell-Yan transverse momentum dependence over a wide mass range at 13 TeV from CMS","authors":"Itana Bubanja","doi":"10.22323/1.398.0336","DOIUrl":"https://doi.org/10.22323/1.398.0336","url":null,"abstract":"","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"17 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"127614128","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}
Priyanka Giri, D. Bersanetti, M. Boldrini, J. Casanueva Diaz, M. Cifaldi, V. Fafone, M. Lorenzini, D. Lumaca, I. Nardecchia, M. Pinto, A. Rocchi, E. N. Tapia San Martín, M. Valentini, M. Mantovani
P. Giri, a,b,∗ D. Bersanetti, M. Boldrini, J. Casanueva Diaz, f M. Cifaldi, V. Fafone, M. Lorenzini, D. Lumaca, I. Nardecchia, M. Pinto, f A. Rocchi, C. Taranto, E. N. Tapia San Martín, M. Valentini, j ,k and M. Mantovani f Università di Pisa, I-56127 Pisa, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Genova, I-16146 Genova, Italy Università di Roma “La Sapienza”, I-00185 Roma, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Roma, I-00185 Roma, Italy f European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy Università degli Studi di Roma Tor Vergata,I-00133,Rome, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, I-00133 Roma, Italy Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy Istituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy E-mail: priyanka.giri@pi.infn.it
P ., a、b、∗转速,J . D . Bersanetti, M .德里尼Casanueva Diaz, f M . Cifaldi见Fafone, M . D .蜗牛,伦平托Nardecchia, M ., f。琼斯,C .塔兰托,E . Tapia圣·马丁M .解读f, J, k和M . Mantovani比萨大学I-56127比萨、意大利国家核物理研究所比萨节、I-56127比萨、热那亚的意大利国家核物理研究所,分庭,I-16146热那亚、意大利罗马大学的“智慧”,罗马I-00185意大利国家核物理研究所,罗马,I-00185罗马、意大利f节欧洲Gravitational天文台(EGO), I-56021农舍、比萨、意大利罗马universita degli Studi di Tor Vergata I-00133、罗马、意大利国家核物理研究所、罗马Tor Vergata节、I-00133罗马,意大利Nikhef,科学公园105、1098 /阿姆斯特丹,荷兰大学物理系,特伦托I-38123 Povo特伦托,意大利国家核物理研究所,特伦托基础物理与应用研究所，I-38123 Povo, Trento，意大利电子邮件:priyanka.giri@pi.infn.it
{"title":"Effects of cold aberrations on the longitudinal error signals and its compensation","authors":"Priyanka Giri, D. Bersanetti, M. Boldrini, J. Casanueva Diaz, M. Cifaldi, V. Fafone, M. Lorenzini, D. Lumaca, I. Nardecchia, M. Pinto, A. Rocchi, E. N. Tapia San Martín, M. Valentini, M. Mantovani","doi":"10.22323/1.398.0069","DOIUrl":"https://doi.org/10.22323/1.398.0069","url":null,"abstract":"P. Giri, a,b,∗ D. Bersanetti, M. Boldrini, J. Casanueva Diaz, f M. Cifaldi, V. Fafone, M. Lorenzini, D. Lumaca, I. Nardecchia, M. Pinto, f A. Rocchi, C. Taranto, E. N. Tapia San Martín, M. Valentini, j ,k and M. Mantovani f Università di Pisa, I-56127 Pisa, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Genova, I-16146 Genova, Italy Università di Roma “La Sapienza”, I-00185 Roma, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Roma, I-00185 Roma, Italy f European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy Università degli Studi di Roma Tor Vergata,I-00133,Rome, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, I-00133 Roma, Italy Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy Istituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy E-mail: priyanka.giri@pi.infn.it","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"70 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"124288229","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}
{"title":"Measurements of the R value at BESIII","authors":"M. Irshad","doi":"10.22323/1.398.0338","DOIUrl":"https://doi.org/10.22323/1.398.0338","url":null,"abstract":"","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"23 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"116455860","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}
Heavy-quark symmetry (HQS), despite being approximate, allows to relate dynamically many hadron systems. In the HQS-limit doubly-heavy baryons, whose dynamics is determined by a light quark situated in a color field of a static pair of heavy quarks, are similar to heavy mesons with a heavy antiquark. Non-local interpolation currents are introduced and corresponding matrix elements between the baryon and vacuum state are expressed in terms of light-cone distribution amplitudes. As well known, the first inverse moment of the leading twist -meson distribution amplitude (DA) is a very important hadronic parameter needed for an accurate theoretical description of -meson exclusive decays. It is quite natural that a similar moment of doubly-heavy baryons is of importance in exclusive doubly-heavy baryons’ decays. We obtain HQET sum rules for the first inverse moment based on the correlation functions containing nonlocal heavy-light operators of doubly-heavy baryons and their local interpolating currents.
{"title":"First inverse moment of the doubly-heavy baryon distribution amplitude from HQET sum rule","authors":"A. Shukhtina, Alexander Parkhomenko","doi":"10.22323/1.398.0349","DOIUrl":"https://doi.org/10.22323/1.398.0349","url":null,"abstract":"Heavy-quark symmetry (HQS), despite being approximate, allows to relate dynamically many hadron systems. In the HQS-limit doubly-heavy baryons, whose dynamics is determined by a light quark situated in a color field of a static pair of heavy quarks, are similar to heavy mesons with a heavy antiquark. Non-local interpolation currents are introduced and corresponding matrix elements between the baryon and vacuum state are expressed in terms of light-cone distribution amplitudes. As well known, the first inverse moment of the leading twist -meson distribution amplitude (DA) is a very important hadronic parameter needed for an accurate theoretical description of -meson exclusive decays. It is quite natural that a similar moment of doubly-heavy baryons is of importance in exclusive doubly-heavy baryons’ decays. We obtain HQET sum rules for the first inverse moment based on the correlation functions containing nonlocal heavy-light operators of doubly-heavy baryons and their local interpolating currents.","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"8 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"133073145","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 the context of the PanScales parton shower project, I describe two advances in the development of final-state parton showers with controlled logarithmic accuracy. The first (Ref. [1]) involves simple new algorithms to resolve the long-standing issue of incorrect subleading-colour contributions at leading logarithmic (LL) accuracy in dipoleand antenna-type final-state showers, and also enables the PanScales showers to obtain full-colour NLL accuracy for many observables. The second (Ref. [2]) concerns spin correlations, where we propose a spinor-product based implementation of the well-established Collins algorithm. We verify the logarithmic accuracy of the results with separate purely collinear calculations, using novel spin-sensitive jet observables that are of potential interest also for future experimental measurements.
{"title":"Subleading colour effects and spin correlations in the PanScales showers","authors":"Ludovic Scyboz","doi":"10.22323/1.398.0416","DOIUrl":"https://doi.org/10.22323/1.398.0416","url":null,"abstract":"In the context of the PanScales parton shower project, I describe two advances in the development of final-state parton showers with controlled logarithmic accuracy. The first (Ref. [1]) involves simple new algorithms to resolve the long-standing issue of incorrect subleading-colour contributions at leading logarithmic (LL) accuracy in dipoleand antenna-type final-state showers, and also enables the PanScales showers to obtain full-colour NLL accuracy for many observables. The second (Ref. [2]) concerns spin correlations, where we propose a spinor-product based implementation of the well-established Collins algorithm. We verify the logarithmic accuracy of the results with separate purely collinear calculations, using novel spin-sensitive jet observables that are of potential interest also for future experimental measurements.","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"27 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"116599647","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}
Neutrinos play a significant and sometimes even dominant role in all phases of the supernova explosion. The most important neutrino processes in a core-collapse supernova are beta-processes, which are responsible for the energy exchange between neutrinos and the matter and change a chemical composition of a medium. We investigate an influence of a magnetic field on betaprocesses under conditions of a supernova matter. For any magnetic field strength discussed in applications to astrophysical objects we obtain simple analytical expressions for reaction rates of beta-processes. In our analysis we use results of one-dimensional simulations of a supernova explosion performed with the PROMETHEUS-VERTEX code. We found that, the magnetic field with the strength B ∼ 1015 G suppresses the neutron production on several percents in comparison with the unmagnetized case. The obtained analytical expressions can be also applied for postmerger accretion discs.
{"title":"Magnetic-field influence on beta-processes in core-collapse supernova","authors":"A. Dobrynina, I. Ognev","doi":"10.22323/1.398.0048","DOIUrl":"https://doi.org/10.22323/1.398.0048","url":null,"abstract":"Neutrinos play a significant and sometimes even dominant role in all phases of the supernova explosion. The most important neutrino processes in a core-collapse supernova are beta-processes, which are responsible for the energy exchange between neutrinos and the matter and change a chemical composition of a medium. We investigate an influence of a magnetic field on betaprocesses under conditions of a supernova matter. For any magnetic field strength discussed in applications to astrophysical objects we obtain simple analytical expressions for reaction rates of beta-processes. In our analysis we use results of one-dimensional simulations of a supernova explosion performed with the PROMETHEUS-VERTEX code. We found that, the magnetic field with the strength B ∼ 1015 G suppresses the neutron production on several percents in comparison with the unmagnetized case. The obtained analytical expressions can be also applied for postmerger accretion discs.","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"31 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"131988366","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}
F. di Renzo, N. Arnaud, Theodoros Avgitas, R. De Rosa, I. Fiori, C. Giunchi, K. Janssens, S. Katsanevas, A. Longo, J. Marteau, Marco Olivieri, M. Tringali, F. Paoletti, P. Ruggi
Francesco Di Renzo,0,1,∗ Nicolas Arnaud, Theodoros Avgitas, Rosario De Rosa, Irene Fiori, Carlo Giunchi, 5 Kamiel Janssens, Stavros Katsanevas, Alessandro Longo, Jacques Marteau, Marco Olivieri, 9 Federico Paoletti, Paolo Ruggi and Maria Concetta Tringali Università di Pisa, I-56127 Pisa, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy Universite Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy Università di Napoli “Federico II”, I-80126 Napoli, Italy 5 Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Pisa, I-56125 Pisa, Italy Universiteit Antwerpen, Prinsstraat 13, 2000 Antwerpen, Belgium Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tre, I-00146 Roma, Italy Institut de Physique Nucléaire de Lyon, Lyon, France 9 Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Bologna, I-40128 Bologna, Italy E-mail: francesco.direnzo@df.unipi.it
弗朗切斯科·尼古拉·阿尔诺·伦佐,0.1,∗表示Avgitas罗萨里奥De Rosa,艾琳,花儿,Carlo灯芯草、5信息Janssens、斯塔夫亚历山德罗·Katsanevas Longo Olivieri马克雅克·b、9、费德里科·Paoletti,比萨大学保罗Ruggi and Maria概念Tringali I-56127比萨、意大利国家核物理研究所比萨节、I-56127比萨、意大利Universite Paris-Saclay, CNRS / IN2P3、IJCLab 91405奥赛、法国、欧洲Gravitational天文台(EGO), I-56021,农舍比萨、意大利那不勒斯大学“Federico II”5、I-80126那不勒斯,意大利国家地球物理和火山学研究所,比萨科、I-56125比萨、意大利大学Antwerpen特13研究所,2000年比利时安特卫普、核物理、节罗马三个、I-00146罗马,意大利Institut de体质Nucléaire de里昂,里昂、法国国家地球物理和火山学研究所9、意大利博洛尼亚节,I-40128博洛尼亚,电子邮件:弗朗切斯科·direnzo@df unipi。
{"title":"Study of the cosmic muon rate nearby the Advanced Virgo detector at the end of the O3 run","authors":"F. di Renzo, N. Arnaud, Theodoros Avgitas, R. De Rosa, I. Fiori, C. Giunchi, K. Janssens, S. Katsanevas, A. Longo, J. Marteau, Marco Olivieri, M. Tringali, F. Paoletti, P. Ruggi","doi":"10.22323/1.398.0059","DOIUrl":"https://doi.org/10.22323/1.398.0059","url":null,"abstract":"Francesco Di Renzo,0,1,∗ Nicolas Arnaud, Theodoros Avgitas, Rosario De Rosa, Irene Fiori, Carlo Giunchi, 5 Kamiel Janssens, Stavros Katsanevas, Alessandro Longo, Jacques Marteau, Marco Olivieri, 9 Federico Paoletti, Paolo Ruggi and Maria Concetta Tringali Università di Pisa, I-56127 Pisa, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy Universite Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy Università di Napoli “Federico II”, I-80126 Napoli, Italy 5 Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Pisa, I-56125 Pisa, Italy Universiteit Antwerpen, Prinsstraat 13, 2000 Antwerpen, Belgium Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tre, I-00146 Roma, Italy Institut de Physique Nucléaire de Lyon, Lyon, France 9 Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Bologna, I-40128 Bologna, Italy E-mail: francesco.direnzo@df.unipi.it","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"14 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"115740100","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}
The local nonequilibrium neutrino distribution function in a core-collapse supernova is considered and two variants of its analytical approximation are suggested. The proposed analytical approximations are verified using the results of a one-dimensional simulation of neutrino propagation, performed self-consistently with hydrodynamics in Prometheus-Vertex code. It was shown that the approximation, based on a Fermi-like distribution of neutrino spectrum, agrees with results of Prometheus-Vertex simulation only in the inner parts of the supernova. Whereas the approximation based on alpha-fit of neutrino energy distribution, also known as Gamma-distribution, is more general and has no restrictions for application in any part of the supernova. The obtained results could be applied for estimation of various neutrino effects in supernova conditions without their direct inclusion in the explosion simulation.
{"title":"Construction and verification of analytical approximation of nonequilibrium neutrino distribution function in core-collapse supernova","authors":"E. Koptyaeva, A. Dobrynina, I. Ognev","doi":"10.22323/1.398.0052","DOIUrl":"https://doi.org/10.22323/1.398.0052","url":null,"abstract":"The local nonequilibrium neutrino distribution function in a core-collapse supernova is considered and two variants of its analytical approximation are suggested. The proposed analytical approximations are verified using the results of a one-dimensional simulation of neutrino propagation, performed self-consistently with hydrodynamics in Prometheus-Vertex code. It was shown that the approximation, based on a Fermi-like distribution of neutrino spectrum, agrees with results of Prometheus-Vertex simulation only in the inner parts of the supernova. Whereas the approximation based on alpha-fit of neutrino energy distribution, also known as Gamma-distribution, is more general and has no restrictions for application in any part of the supernova. The obtained results could be applied for estimation of various neutrino effects in supernova conditions without their direct inclusion in the explosion simulation.","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"20 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"114816739","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}
{"title":"Search for contact interactions with inclusive jet production at the LHC at 13 TeV with CMS","authors":"Toni Maekelae, K. Lipka","doi":"10.22323/1.398.0337","DOIUrl":"https://doi.org/10.22323/1.398.0337","url":null,"abstract":"","PeriodicalId":218352,"journal":{"name":"Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)","volume":"27 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2022-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"128125983","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}
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