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05/03/2023, 07:00
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05/03/2023, 08:00
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Luciano Abreu et al.05/03/2023, 08:20
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Prof. Hildeson Vieira (UFBA)05/03/2023, 08:40
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Dr SOKRATIS TRIFINOPOULOS (MIT)05/03/2023, 09:00
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Prof. Melina Silva de Lima (UFBA)05/03/2023, 09:20
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Dr André Luiz Moura Brito (UFBA)05/03/2023, 09:40
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Prof. Rodrigo Oliveira Magalhães (UFBA)05/03/2023, 10:00
Using effective Lagrangians, we study the interactions of the state $Z_c(3900)$ with light mesons. We determine the cross sections for the processes $Z_c \pi \rightarrow \bar{D}^{(*)} D^{(*)}$ and as well as the inverse processes. To understand the influence of the medium on the results, we determined the thermal average of the cross-sections.
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Ms Fernanda Rodrigues (UNICAMP)05/03/2023, 10:20
We propose a non-standard interaction (NSI) in neutrino production to alleviate the tension between the results of the experiments NOvA (NuMI Off-axis $\nu_e$ Appearance) and T2K (Tokai to Kamioka). The NSI is computed through quantum field theory (QFT) formalism and we get perturbative analytic formulas for oscillation probabilities.
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Leonardo Santoro De Oliveira (CBPF)05/03/2023, 10:40
In this study, we investigate CP violation in $D_{s} \rightarrow\pi^{-}\pi^{+}K^{+}$ channel using simulations of the Dalitz plot and a technique called Mirandizing.We demonstrate the effectiveness of this approach by visualizing the shape of the CP violation in the Dalitz plot. By analyzing the local population differences, we are able to identify regions where CP symmetry is broken. Our...
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Alberto Santoro (Universidade do Estado do Rio de Janeiro (BR))06/03/2023, 09:00
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Dr Michelangelo Mangano (CERN)06/03/2023, 09:30
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Dr Christophe Grojean (DESY)06/03/2023, 10:50
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Dr Luca Malgeri (CMS)06/03/2023, 11:50
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Dr Harvey Newman (CALTECH)06/03/2023, 14:00
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Dr Ugo Moschella (Italian Institute)06/03/2023, 14:50
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Dr Sokratis Trifinopoulos (MIT)06/03/2023, 15:40
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Dr Andre Frankenthal (CMS)06/03/2023, 16:00
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Dr Patricia Rebello Teles (CBPF)06/03/2023, 16:20
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Dr Gustavo Gil da Silveira (UFRGS/UERJ)06/03/2023, 16:40
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Dr Yifang Wang (Institute of High Energy Physics, CAS)07/03/2023, 09:00
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Dr Marisilvia Donadelli (ATLAS - CERN)07/03/2023, 10:20
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Dr Gregorio Bernardi07/03/2023, 11:20
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Dr Jonathan Zarling (Jefferson Lab)07/03/2023, 14:00
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Dr Sridhara Rao Dasu (University of Wisconsin)07/03/2023, 14:50
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Dr Nuno Leonardo (LIP)07/03/2023, 15:40
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Dr Carlos Alberto Gottardo (ATLAS)07/03/2023, 16:40
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Dr Markus Cristinziani (Universität Siegen)07/03/2023, 17:00
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Rafael Coelho Lopes De Sa (University of Massachusetts (US))07/03/2023, 17:20
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Dr Prolay Kumar Mal (CMS)07/03/2023, 17:40
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Carola Dobrigkeit Chinellato (Uncamp)08/03/2023, 09:00
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Dr Bruno Souza de Paula (LHCb - CERN)08/03/2023, 10:20
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Dr Marcel Demateau (Oak Ridge National Laboratory)08/03/2023, 11:20
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Dr Renata Zukanovich (USP)08/03/2023, 14:00
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Dr Gerardo Herrera (ALICE)08/03/2023, 15:40
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Dr Pasquale Di Nezza (Instituto Nazionale di Física Nucleare)08/03/2023, 16:40
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Dr Felipe Luan Souza De Almeida08/03/2023, 17:00
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Prof. Shuangshi Fang (Institute of High Energy Physics, CAS)09/03/2023, 09:00
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Dr Kai Schweda (ALICE)09/03/2023, 10:20
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Dr Harvey Newman (CALTECH)09/03/2023, 11:20
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09/03/2023, 12:20
Participants: Alberto Santoro, Luiz Mundim e Sandro Fonseca
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Dr Gabriella Pugliese (INFN - Bari - Italy)09/03/2023, 14:00
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Prof. Oscar Eboli (USP)09/03/2023, 14:50
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Dr Joel Butler (FNAL - CMS)09/03/2023, 15:40
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Lia Merminga09/03/2023, 16:30
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Jose W F Valle (IFIc-SPAIN)10/03/2023, 09:00
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Dr Tomasz Skwarnicki (Syracuse University)10/03/2023, 10:00
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Diego Machado (lhcb)10/03/2023, 11:00
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Dr Pasquale Di Nezza (Instituto Nacional di Fisica Nucleare)10/03/2023, 11:20
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Dr JoAnne Hewett (SLAC – National Accelerator Laboratory)10/03/2023, 14:00
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Dr Roman Roman (CNRS/IN2P3/IJCLab)10/03/2023, 15:00
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Dr Jiayi Chen (ATLAS)10/03/2023, 15:50
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10/03/2023, 16:10
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Dr Ettore Segreto (UNICAMP)
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Dr Boleslaw Wyslouch (M .I .T.)
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Dr Oscar Eboli (I.F. USP)
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Dr Siridhara Dasu (CMS)
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Dr Salvatore Buontempo (CMS)
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Dr Jose WD Valle (Universidad de Valencia)
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Mr Aljandro Manuel Marthias (Cinvestav -Mexico)
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Dr Deepak Kumar (Theoretical Physics Division, Physical Research Laboratory,)
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Mr LEONARDO Santoro de Oliveira (CBPF)
In DsPPK selection process we find structure in background , the Challenge is identify and eliminate this structure before start the analysis. We investigate this contamination comes from D0 charm decay, and for testing this hypotesis we will use simulations with RapidSim for testing and confirm our hipotesys.
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Dr Gustavo Castelo Branco (Universidade de Lisboa)
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