In this seminar I will present the first measurement of the total cross-section of the coherent ultra-peripheral photoproduction of the Υ meson in lead-lead collisions at 5.02 TeV. The data used in the analysis has been collected in 2018 by the CMS experiment at the CERN’s Large Hadron Collider. The considered channel is the muon decay of the Υ meson, Υ → μ+μ−. This process is sensitive to the nuclear Parton Distribution Functions for gluons.Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743; Passcode: HEP_UW)
join us at 10:15

dr hab. Marcin Chrząszcz (IFJ PAN)
The FCC-ee is a high-luminosity, high-precision e+e- circular collider. Two separate e+ and e- storage rings with very strong focusing, fed by a full size continuous injector, provide e+e- collision luminosities ranging from (per interaction point) 230 1034 /cm2 /s at the Z pole, 8 1034 /cm2 /s at the ZH production maximum (240 GeV) and 1.7 1034 /cm2 /s at the tt threshold and up to 365 GeV. Two to four interaction points are considered.The run plan of 15-20 years yields 5 10^12 Z bosons, 10^8 W pairs, 1.3 10^6 Higgs bosons and 10^6 top quark pairs. Thanks to the availability of transverse polarization, the energy calibration at 100 keV precision offers unprecedented precision for measurements of Z and W properties. The possibility of s-channel Higgs production at ECM=125 GeV is under study, giving unique access to the electron Yukawa coupling. These opportunities make the FCC-ee stand out among the other Higgs factory proposals.Especially at the Z run, considerable challenges await experimenters and theorists, for systematic uncertainties to match the extraordinary available statistical precision. Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743; Passcode: HEP_UW)
The FCC-ee is a high-luminosity, high-precision e+e- circular collider. Two separate e+ and e- storage rings with very strong focusing, fed by a full size continuous injector, provide e+e- collision luminosities ranging from (per interaction point) 230 1034 /cm2 /s at the Z pole, 8 1034 /cm2 /s at the ZH production maximum (240 GeV) and 1.7 1034 /cm2 /s at the tt threshold and up to 365 GeV. Two to four interaction points are considered.The run plan of 15-20 years yields 5 10^12 Z bosons, 10^8 W pairs, 1.3 10^6 Higgs bosons and 10^6 top quark pairs. Thanks to the availability of transverse polarization, the energy calibration at 100 keV precision offers unprecedented precision for measurements of Z and W properties. The possibility of s-channel Higgs production at ECM=125 GeV is under study, giving unique access to the electron Yukawa coupling. These opportunities make the FCC-ee stand out among the other Higgs factory proposals.Especially at the Z run, considerable challenges await experimenters and theorists, for systematic uncertainties to match the extraordinary available statistical precision. Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743; Passcode: HEP_UW) join us at 10:15

Prof. UAM dr hab. Krzysztof Cichy (UAM)
In this talk, we will present recent directions in lattice QCD computations of nucleon structure, in particular for spin-dependent observables. We will provide a brief non-technical introduction to lattice QCD in general and to lattice methods that give access to the relevant physical quantities. Then, we will review selected results for spin-dependent parton distribution functions (PDFs) and generalized parton distributions (GPDs), including both their moments and their x-dependence. Finally, we will show the nucleon spin decomposition from the lattice in terms of contributions from valence/sea quarks and gluons. Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743; Passcode: HEP_UW)
In this talk, we will present recent directions in lattice QCD computations of nucleon structure, in particular for spin-dependent observables. We will provide a brief non-technical introduction to lattice QCD in general and to lattice methods that give access to the relevant physical quantities. Then, we will review selected results for spin-dependent parton distribution functions (PDFs) and generalized parton distributions (GPDs), including both their moments and their x-dependence. Finally, we will show the nucleon spin decomposition from the lattice in terms of contributions from valence/sea quarks and gluons. Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743; Passcode: HEP_UW) join us at 10:15

dr hab. Lech Wiktor Piotrowski (IFD UW)
Even though the first UHECR was detected almost 60 years ago, the origin of these particles remains a mystery. For lower energies, their paths are twisted by the Galactic magnetic field, while for higher energies their fluxes are too low to give a statistically significant location on the sky. This is even though the largest observatories occupy hundreds to thousands of square kilometres.In this seminar, I will show two approaches to solving this problem. The first one is significantly increasing the volume of the atmosphere observed. This can be achieved either with covering tens of thousands of square kilometres with simple radio antennas, which is the aim of the Giant Radio Array for Neutrino Detection (GRAND) experiment. Alternatively, UHECR induced fluorescent tracks in the atmosphere can be observed from the orbit, which is the idea behind JEM-EUSO and Poemma experiments. The second approach is to detect ultra-high energy neutrinos, unaffected by Galactic magnetic fields, created by the UHECRs close to their origin. This is, again, the aim of both GRAND and Poemma experiments. Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743; Passcode: HEP_UW)
Even though the first UHECR was detected almost 60 years ago, the origin of these particles remains a mystery. For lower energies, their paths are twisted by the Galactic magnetic field, while for higher energies their fluxes are too low to give a statistically significant location on the sky. This is even though the largest observatories occupy hundreds to thousands of square kilometres.In this seminar, I will show two approaches to solving this problem. The first one is significantly increasing the volume of the atmosphere observed. This can be achieved either with covering tens of thousands of square kilometres with simple radio antennas, which is the aim of the Giant Radio Array for Neutrino Detection (GRAND) experiment. Alternatively, UHECR induced fluorescent tracks in the atmosphere can be observed from the orbit, which is the idea behind JEM-EUSO and Poemma experiments. The second approach is to detect ultra-high energy neutrinos, unaffected by Galactic magnetic fields, created by the UHECRs close to their origin. This is, again, the aim of both GRAND and Poemma experiments. Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743; Passcode: HEP_UW) join us at 10:15

prof. dr hab. Barbara Badełek (IFD UW)
The talk is a pedagogical introduction to main aspects of the contemporary view of the proton structure, viewed from a perspective of the Electron-Ion Collider, a frontier accelerator facility, planned in the US. Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743; Passcode: HEP_UW)
join us at 10:15

dr hab. Paweł Malecki (IFJ PAN)
High-energy neutrino astronomy is a fascinating new field of research, rapidly developing1over the recent years. It opens a new observation window on the most violent processes in the universe, fitting very well to the concept of multi-messenger astronomy. Constraining astrophysical neutrino fluxes can also help to understand the long-standing mystery of the origin of the ultra-high energy cosmic rays. Astronomical studies of high-energy neutrinos are carried out by large-scale next-generation neutrino telescopes located in different regions of the world, forming a global network of complementary detectors. The Baikal-GVD, being currently the largest neutrino telescope in the Northern Hemisphere and still growing up, is an important constituent of this network.This talk briefly reviews working principles, analysis methods and some selected results of the Baikal-GVD neutrino telescope. Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743, Passcode: HEP_UW)
join us at 10:15

Piotr Kalaczyński (NCBJ)
KM3NeT/ORCA: status & perspectives for \nu oscillation and mass ordering measurements
A next-generation neutrino telescope, the Kilometer Cube Neutrino Telescope (KM3NeT), is currently under deployment in the Mediterranean Sea. Its low energy configuration ORCA (Oscillations Research with Cosmics in the Abyss) is optimised for the detection of atmospheric neutrinos with energies above ∼1 GeV. The main research target of the ORCA detector is the measurement of the neutrino mass ordering and atmospheric neutrino oscillation parameters, while the detector is also sensitive to a wide variety of other physics topics, such as dark matter, non-standard interactions and sterile neutrinos. The presentation will provide an overview of the ORCA detector and introduce its research programme, alongside early analyses of data collected with the array in its current configuration. https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743, Passcode: HEP_UW)
join us at 10:15

dr hab. Michał Bluj (NCBJ)
Measurements with the H→ττ decay channel play an important role in probing Higgs boson properties. In this talk recent results obtained by the CMS experiment with the H→ττ channel will be discussed: a measurement of the Higgs boson production cross-section and a measurement of the CP structure of the Yukawa coupling between the Higgs boson and tau leptons. https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743, Passcode: HEP_UW)
Measurements with the H→ττ decay channel play an important role in probing Higgs boson properties. In this talk recent results obtained by the CMS experiment with the H→ττ channel will be discussed: a measurement of the Higgs boson production cross-section and a measurement of the CP structure of the Yukawa coupling between the Higgs boson and tau leptons. https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743, Passcode: HEP_UW) room B2.38, Pasteura 5 at 10:15

(IFD UW)
W dniu 20 listopada zapraszamy do udziału w otwartej sesji plenarnej ECFA, która poświęcona będzie tzw. fabrykom gamma. Plan spotkania: Session on gamma factories: 10:30 Physics context and opportunities at the HL-LHC Speaker: Mieczyslaw Krasny (Centre National de la Recherche Scientifique (FR)) 11:10 Technical aspects, R&D and Proof-of-Principle Speaker: Yann Dutheil (CERN) 11:35 Physics applications of gamma-factories Speaker: DMITRY BUDKER (Helmholtz Institute Mainz and UC Berkeley) Szczegóły spotkania ECFA, które rozpoczyna się w czwartek, 19 listopada o godz. 14:00 i zakończy w piątek, 20 listopada o godz. 17:00 dostępne są nastronie: https://indico.cern.ch/event/966397/. Spotkanie będzie transmitowane za pośrednictwem platformy zoom. Bezpośredni link do spotkania: https://cern.zoom.us/j/94044206208?pwd=M3Z4OVF0RVZFdWxqalhpNy9xT1hKQT09
We invite you to participate in the open sessions of Plenary ECFA, held on 19-20 November 2020. A dedicated session of Friday morning will be devoted to gamma factories. Session on gamma factories: 10:30 Physics context and opportunities at the HL-LHC Speaker: Mieczyslaw Krasny (Centre National de la Recherche Scientifique (FR)) 11:10 Technical aspects, R&D and Proof-of-Principle Speaker: Yann Dutheil (CERN) 11:35 Physics applications of gamma-factories Speaker: DMITRY BUDKER (Helmholtz Institute Mainz and UC Berkeley) Details of the Plenary ECFA open session can be found on: https://indico.cern.ch/event/966397/ Direct link to the zoom meeting: https://cern.zoom.us/j/94044206208?pwd=M3Z4OVF0RVZFdWxqalhpNy9xT1hKQT09 room B2.38, Pasteura 5 at 10:15

prof. dr hab. Krzysztof DOROBA (IFD UW)
Branching rations Br(τ→μμμ) have been studied in particular by BELLE, BABAR, LHCb, ATLAS and CMS. Obtained results should be compared with existing or future predictions on Charged Lepton Flavor Violation (CLFV) of different Standard Model extensions. In this talk methods used by above experiments for data collection and analysis will be described and experimental results presented with particular emphasis on the CMS experiment. Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 Meeting ID: 845 1609 6743, Passcode: HEP_UW
Branching rations Br(τ→μμμ) have been studied in particular by BELLE, BABAR, LHCb, ATLAS and CMS. Obtained results should be compared with existing or future predictions on Charged Lepton Flavor Violation (CLFV) of different Standard Model extensions. In this talk methods used by above experiments for data collection and analysis will be described and experimental results presented with particular emphasis on the CMS experiment. Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 Meeting ID: 845 1609 6743, Passcode: HEP_UW room B2.38, Pasteura 5 at 10:15

Prof. dr hab. Krzysztof Golec-Biernat (IFJ PAN)
The planned Electron Ion Collider offers new opportunities to study quark-gluon strukture of nuclons and nuclei through deep inelastic scattering processes. I will present some of them refering to the currente status of our knowledge of this structure. Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 Meeting ID: 845 1609 6743, Passcode: HEP_UW
The planned Electron Ion Collider offers new opportunities to study quark-gluon strukture of nuclons and nuclei through deep inelastic scattering processes. I will present some of them refering to the currente status of our knowledge of this structure. Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 Meeting ID: 845 1609 6743, Passcode: HEP_UW room B2.38, Pasteura 5 at 10:15

dr hab. Marcin Konecki, prof. UW (IFD UW)
The top quark is the heaviest object in the standard model (SM).It allows for the precise test of the SM and searches for a new physics.Thus the top quark measurements are important part of CMS physics program.In the presentation the selection of recent CMS top-quark measurements will be given:t-tbar production in association with charm, 3rd generation of CKM matrix elements, forward-backward asymmetry, top Yukawa coupling determination and a search for CP violation effects in top production. Spotkanie odbędzie się za pośrednictwem platformy zoom: Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 Meeting ID: 845 1609 6743 Passcode: HEP_UW
The top quark is the heaviest object in the standard model (SM).It allows for the precise test of the SM and searches for a new physics.Thus the top quark measurements are important part of CMS physics program.In the presentation the selection of recent CMS top-quark measurements will be given:t-tbar production in association with charm, 3rd generation of CKM matrix elements, forward-backward asymmetry, top Yukawa coupling determination and a search for CP violation effects in top production. Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 Meeting ID: 845 1609 6743 Passcode: HEP_UW join us at 10:15

dr hab. Katarzyna Grzelak (IFD UW)
The XXIX International Conference on Neutrino Physics and Astrophysics was originally scheduled to take place in Chicago but due to COVID-19 was entirely virtual.This year more than 3400 people participated from 22 June to 2 July in this biggest conference in the neutrino physics field.In the seminar the results shown at the conference will be presented. Spotkanie odbędzie się za pośrednictwem platformy zoom:Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743 , Passcode: HEP_UW)
The XXIX International Conference on Neutrino Physics and Astrophysics was originally scheduled to take place in Chicago but due to COVID-19 was entirely virtual.This year more than 3400 people participated from 22 June to 2 July in this biggest conference in the neutrino physics field.In the seminar the results shown at the conference will be presented. Join Zoom Meeting https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09 (Meeting ID: 845 1609 6743 , Passcode: HEP_UW) join us at 10:15

prof. dr hab. Jan Królikowski (IFD UW)
Spotkanie odbędzie się za pośrednictwem platformy zoom:https://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09Meeting ID: 845 1609 6743Passcode: HEP_UW
Join Zoom Meetinghttps://us02web.zoom.us/j/84516096743?pwd=a3BYQ24zY1ZjQTF4eFIwUnM2WlNaZz09Meeting ID: 845 1609 6743Passcode: HEP_UW