Conveners
Plenary Session
- Yuji Yamazaki (Kobe University (JP))
- Norbert Neumeister (Purdue University (US))
Plenary Session
- Michal Marcisovsky (Czech Academy of Sciences (CZ))
- Livia Ludhova
Plenary Session
- Analisa Gabriela Mariazzi
- Revaz Shanidze
Plenary Session
- Xiaoyan Shen (University of Science and Technology of China (CN))
- Michal Zamkovsky (CERN)
Plenary Session
- Michal Kreps (University of Warwick (GB))
- Roy Briere
- Caroline Rodenbeck
Plenary Session
- Achim Stahl (Rheinisch Westfaelische Tech. Hoch. (DE))
Plenary Session
- Livia Ludhova
Plenary Session
- Sonia Kabana (Instituto De Alta Investigación, Universidad de Tarapacá (CL))
- Thomas Muller (KIT - Karlsruhe Institute of Technology (DE))
Plenary Session
- Bernd Stelzer (SFU/TRIUMF)
- Su Dong
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Marco Pieri (Univ. of California San Diego (US))10/10/2023, 11:00High Energy Particle PhysicsOral presentation
The status of the LHC Run 3 and the results from ATLAS and CMS based on the data collected during 13.6 TeV pp runs at the LHC are presented.
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Kajari Mazumdar (Tata Inst. of Fundamental Research (IN))10/10/2023, 11:30High Energy Particle PhysicsOral presentation
Properties of the standard model Higgs boson
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Bernd Stelzer (SFU/TRIUMF)10/10/2023, 12:00High Energy Particle PhysicsOral presentation
Rare processes and search for new phenomena through Higgs bosons
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Michal Dubovsky (Comenius University (SK))10/10/2023, 12:30High Energy Particle PhysicsOral presentation
Top quark production, properties and rare processes
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Dr Ralph Massarczyk (Los Alamos National Laboratory)10/10/2023, 14:30High Energy Particle PhysicsOral presentation
With the discovery of neutrino oscillations and demonstrating that neutrinos have a mass, the Standard Model of particle physics is to be insufficient to describe it. It is too small to be explained with the Standard Model, hence other mass creating mechanisms must exist. In some of these models the neutrino is its own anti-particle. The practical only way to prove this Majorana nature of the...
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David Vanegas Forero (Universidad de Medellín)10/10/2023, 15:00High Energy Particle PhysicsOral presentation
Neutrino oscillations are the leading mechanism that successfully explain the neutrino flavor transitions observed at dedicated detectors from several sources of neutrinos like the Sun, from cosmic rays interacting with the Earth atmosphere, and neutrinos from artificial sources such as the ones produced in reactor and accelerator-based experiments. This wealth of data is well described by...
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Federico Ferraro (Istituto Nazionale di Fisica Nucleare (INFN) - Laboratori Nazionali del Gran Sasso)10/10/2023, 16:00Astroparticle PhysicsOral presentation
Nuclear fusion reactions within stars generate the energy and forge the elements observed throughout the Universe. These reactions transform primordial hydrogen and helium remnants from the Big Bang into a diverse array of elements. Nuclear astrophysics provides unique insights into the nuclear processes involved in astrophysical environments and responsible for the nucleosynthesis of the...
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Diego Ravignani10/10/2023, 16:30High Energy Particle PhysicsOral presentation
Highlights from the cosmic rays observed with the Pierre Auger Observatory
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Dr Mario A Acero (Universidad del Atlantico)10/10/2023, 17:00High Energy Particle PhysicsOral presentation
Research on neutrino physics in currently advancing at an impressive pace thanks to the great efforts on different fronts, including high energy physics, cosmology and astrophysics. In particular, the study of neutrino oscillations and interactions with matter concentrates important attention from the community, manifest from the remarkable experiments that have collected data and measured the...
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Yangheng Zheng (University of Chinese Academy of Sciences (CN))11/10/2023, 09:00High Energy Particle PhysicsOral presentation
I will present the recent experimental results on Charm hadron decays.
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Beijiang Liu11/10/2023, 09:30High Energy Particle PhysicsOral presentation
Hadron spectroscopy is essential in improving our understanding of the nonperturbative regime of QCD and to reveal the mechanism of color con?nement. Recent experimental results in light hadron sector and heavy hadron sector from LHC experiments, BESIII, Belle II and GlueX will be presented.
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Dr Roberto Mussa (INFN Torino)11/10/2023, 10:00High Energy Particle PhysicsOral presentation
Since the discovery of X(3872), Belle has been pioneering the exploration
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of tetraquarks, QCD bound states beyond standard mesons and baryons. More
than a decade after the end of data taking, the Belle datasets are still
producing results in hadron spectroscopy, and have provided the
motivations for the first energy scan above the energy of the $\Upsilon(4S)$ peak, between 10.65 GeV and... -
Jake Bennett11/10/2023, 11:00High Energy Particle PhysicsOral presentation
B CKM physics
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Michal Zamkovsky (CERN)11/10/2023, 11:30High Energy Particle PhysicsOral presentation
Overview of kaon physics
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Sergey Martynenko11/10/2023, 12:00High Energy Particle PhysicsOral presentation
The MicroBooNE experiment employs an 85-ton active mass liquid argon time projection chamber to detect neutrinos from both the on-axis Booster Neutrino Beam (BNB) and off-axis Neutrinos at the Main Injector (NuMI) beam. One of the main goals of MicroBooNE is to investigate MiniBooNE low energy excess/anomaly. In this talk, we will present the recent results from MicroBooNE’s low energy excess...
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Juan Pedro Ochoa Ricoux11/10/2023, 12:30High Energy Particle PhysicsOral presentation
Neutrinos can teach us volumes about the fundamental makeup of our world as well as about the sources that produce them. The extremely intense and well-understood electron antineutrino flux emitted by the beta-decays of fission products in nuclear reactors is an excellent resource to study these elusive particles. This talk will describe the considerable progress achieved recently in the field...
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Andrew Miller12/10/2023, 09:00GravityOral presentation
The third observing run of advanced LIGO, Virgo and KAGRA brought unprecedented sensitivity towards a variety of quasi-monochromatic, persistent gravitational-wave signals. Continuous waves allow us to probe not just the canonical asymmetrically rotating neutron stars, but also different forms of dark matter, thus showing the wide-ranging astrophysical implications of using a relatively simple...
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Prof. Segev BenZvi (University of Rochester)12/10/2023, 09:30CosmologyOral presentation
The Dark Energy Spectroscopic Instrument (DESI) is a fiber-fed, robotically-actuated galaxy redshift survey that has been in operation at Kitt Peak National Observatory near Tucson, Arizona, USA since mid-2021. DESI, which observes the growth of structure from the nearby universe out to a redshift of 3, is currently producing the largest catalog of gravity redshifts ever assembled. With an...
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Piera Sapienza (Laboratori Nazionali del Sud (IT))12/10/2023, 10:00Astroparticle PhysicsOral presentation
The discovery, in 2013, of a diffuse astrophysical neutrino flux by IceCube marked the beginning of neutrino astronomy. Since then, great efforts have been devoted to the search for cosmic neutrino sources. Although any neutrino source has been unambiguously identified, the neutrino high energy event candidate IC170922 triggered a multiwavelenght observation campaign providing a hint for...
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Caroline Rodenbeck13/10/2023, 09:00Astroparticle PhysicsOral presentation
Direct neutrino mass measurements
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Xuefeng Ding (Istitute of High Energy Physics, Chinese Academy of Sciences)13/10/2023, 09:30High Energy Particle PhysicsOral presentation
Over the past half-decade, the realm of solar neutrino physics has been illuminated with groundbreaking discoveries. These encompass the meticulous 3% measurements of $^7$Be solar neutrinos, the pioneering detection of CNO solar neutrinos, and the debut measurements of solar core C+N relative abundances utilizing solar neutrinos.
The upcoming contributions from experiments like JUNO,...
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Irina Nasteva (Federal University of Rio de Janeiro (BR))13/10/2023, 10:00Astroparticle PhysicsOral presentation
Coherent elastic neutrino-nucleus scattering
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Jonathan R. Ellis (University of London (GB))13/10/2023, 11:00High Energy Particle PhysicsOral presentation
Searching for New Physics at the LHC using Effective Field Theory
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Norbert Neumeister (Purdue University (US))13/10/2023, 11:30High Energy Particle PhysicsOral presentation
Experiments at the Large Hadron Collider (LHC) search for new physics beyond the standard model that could explain some of the shortcomings of the standard model. A selection of results for searches for new physics beyond the standard model using data recorded by the ATLAS, CMS and LHCb experiments are presented. The results are based on proton-proton collision data collected during Run 2 of the LHC.
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Sooraj Krishnan Radhakrishnan13/10/2023, 12:00Heavy Ion CollisionsOral presentation
Recent experimental results on heavy-ion collisions at RHIC and LHC
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Boris Kopeliovich13/10/2023, 12:30High Energy Particle PhysicsOral presentation
The anomalous excess of soft photons radiated in inelastic hadronic collisions, has been a challenge over four decades. The problem is rooted in comparison with an incorrect model for radiative corrections, which is based on an illegitimate extension of the Low theorem to radiative multi-particle production processes $2\to n+\gamma$. It turns out to contradict the unitarity relation and the...
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Takanori Kono (Ochanomizu University (JP))13/10/2023, 14:30High Energy Particle PhysicsOral presentation
Electroweak measurements from high statistics LHC data
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Samuel Louis Bein (Hamburg University (DE))13/10/2023, 15:00High Energy Particle PhysicsOral presentation
Searches for signatures with heavy stable neutral particles at the LHC
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