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Liangjian Wen (高能所)12/09/2026, 09:00
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LOC12/09/2026, 09:10
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Igor Ostrovskiy12/09/2026, 09:20
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12/09/2026, 09:35
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Toshihiro Fujii (Osaka Metropolitan University)12/09/2026, 10:15
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Anna Obertacke (Stockholm University)12/09/2026, 10:45
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Alexander Antoshkin (Joint Institute for Nuclear Research)12/09/2026, 11:15
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Michele Doro (University of Padova)12/09/2026, 11:30
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Nikolaos Mavromatos (Nat. Tech. U. Athens and King's College London)12/09/2026, 13:10
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Oliver Gould (University of Nottingham)12/09/2026, 13:50
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Takeshi Kobayashi (SISSA)12/09/2026, 14:20
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Chen Zhang (Northeastern University (China))12/09/2026, 14:50
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Maximilian Bachmaier (Max-Planck-Institute for Physics)12/09/2026, 15:05
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Igor Ostrovskiy12/09/2026, 15:40
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maurizio spurio (University of Bologna and INFN)12/09/2026, 16:10
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Andrey Alexandrov (INFN-Napoli)12/09/2026, 16:40
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Yi Jia (高能所)13/09/2026, 09:00
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Shoushan Zhang (Institute of High Energy Physics)13/09/2026, 09:30
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Andrey Saveliev (Immanuel Kant Baltic Federal University)13/09/2026, 10:00
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Ala'a AL-Zetoun (Chinese Academy of Sciences), Peiwen Mi13/09/2026, 10:15
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Ye-Ling Zhou (Hangzhou Institute for Advanced Study)13/09/2026, 10:50
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Perri Daniele (University of Warsaw)13/09/2026, 11:20
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Krzysztof Szafrański (Faculty of Physics, University of Warsaw)13/09/2026, 11:50
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Emanuela Musumeci (University of Alabama)13/09/2026, 12:05
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Dan Zhu (Institute of Modern Physics, Huizhou)13/09/2026, 12:20
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Arttu Rajantie (Imperial College London)14/09/2026, 09:00
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Chitta Ranjan Das (The Bogoliubov Laboratory of Theoretical Physics, International intergovernmental scientific research organization Joint Institute for Nuclear Research, 6 Joliot-Curie St, Dubna, Moscow Region, Russia, 141980)14/09/2026, 09:30
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Jarah Evslin (Institute of Modern Physics, Lanzhou)14/09/2026, 10:00
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Kimyeong Lee (BIMSA)14/09/2026, 10:15Contributed talk - 12+3 min
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Qing Lin (University of Science and Technology of China)14/09/2026, 11:00
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Mesut Arslandok (Yale Univesity)14/09/2026, 11:30
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Valeri Saveliev (BFU)14/09/2026, 12:00Contributed talk - 12+3 min
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14/09/2026, 13:45
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14/09/2026, 14:10
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Michele Doro (University of Padova)Contributed talk - 12+3 min
Experimental limits on relativistic magnetic monopoles (MMs) are conventionally quoted as functions of detector velocity, leaving the astrophysically relevant quantity — MM mass — only loosely constrained, since the acceleration MMs undergo in cosmic magnetic fields has been treated as a free parameter. We close this gap by explicitly computing the MM velocity as a function of mass, combining...
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Jarah Evslin (Institute of Modern Physics, Lanzhou)Contributed talk - 12+3 min
We present a novel formalism for calculations involving quantum solitons which is much simpler than previous approaches. It has so far allowed the calculation of one and two-loop mass and tension corrections, quantum corrections to form factors, decay rates of excited states, binding energies of bound excitations and elastic and inelastic scattering amplitudes involving a soliton struck by...
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Krzysztof Szafrański (Faculty of Physics, University of Warsaw)Contributed talk - 12+3 min
Magnetic monopoles remain a compelling target in searches for physics beyond the Standard Model. In this talk, we discuss the cosmological consequences of a population of monopoles that is accelerated by galactic magnetic fields and, as a result, stops behaving like ordinary clustered cold dark matter.
We describe this process using a generic accelerating dark matter framework, in which a...
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Maximilian Bachmaier (Max-Planck-Institute for Physics)Contributed talk - 12+3 min
The standard model of particle physics is a good approximation for lower energy scales. In the early hot universe, however, it is assumed that there was a so-called grand unified theory, which unifies the three fundamental forces of particle physics: the electromagnetic, the weak, and the strong force. However, all attempts to unify these three forces lead to a possible overabundance of ‘t...
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Maximilian Bachmaier (Max-Planck-Institute for Physics)Contributed talk - 12+3 min
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Andrey SavelievContributed talk - 12+3 min
We present CRPropa 3.3, the latest release of the publicly available Monte Carlo framework for simulating the propagation of high-energy particles in astrophysical environments. This version introduces significant extensions that enables multi-messenger studies across a broad energy range, from GeV to ZeV. New features include explicit time tracking, time-dependent advection fields, and...
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IHEP canteen or pre-ordered takeout
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Michael Padgett (Vanderbilt University)Contributed talk - 12+3 min
A recent event in Ultra High Energy Cosmic Rays (UHECRs) known as the Amaterasu particle is the foundation of a possible glimpse into beyond the standard model physics. The particle was detected by the Telescope Array Project in 2021 and later identified in 2023 with an energy exceeding 240 EeV. There exists a limit that applies to protons as UHECRs known as the GZK limit. It is derived by...
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Takeshi Kobayashi (SISSA)
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Oliver Gould (University of Nottingham)
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Toshihiro Fujii (Osaka Metropolitan University)Contributed talk - 12+3 min
Clarifying origins and acceleration mechanisms of ultra-high-energy cosmic rays (UHECRs) has been the centennial endeavor, being one of the most intriguing mysteries in an interdisciplinary research among astroparticle physics, high-energy physics and nuclear physics. With an ability to select events by the rigidity (E/Z), arrival directions of UHECRs can be exploited to probe the most...
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Toshihiro Fujii (Osaka Metropolitan University)
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Prof. Chitta Ranjan Das (The Bogoliubov Laboratory of Theoretical Physics, International intergovernmental scientific research organization Joint Institute for Nuclear Research, 6 Joliot-Curie St, Dubna, Moscow Region, Russia, 141980)Contributed talk - 12+3 min
Strange quark matter (SQM) has long been proposed as a possible true ground state of QCD at high baryon density, motivating extensive research on exotic compact objects and unusual cosmic-ray signatures. Recent observations strengthen this interest: the remnant HESS J1731-347 hosts an exceptionally low-mass neutron star, $M = 0.77^{+0.20}_{-0.17}\,M_\odot$ and $R =...
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Chen Zhang (Northeastern University (China))Contributed talk - 12+3 min
Magnetic monopoles arise generically in unified theories and offer a natural explanation of charge quantization. Beyond collider searches and cosmic-ray experiments, their flux is constrained by Parker-type bounds requiring galactic magnetic fields to survive monopole energy extraction. We formulate a self-consistent Parker bound anchored in the lowest eigenmode of the galactic mean-field...
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Chen Zhang (Northeastern University (China))Contributed talk - 12+3 min
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Prof. Valeri SavelievContributed talk - 12+3 min
A new type of photodetector — the Silicon photomultiplier (SiPM), was developed using CMOS semiconductor technology. SiPM is an optical sensor that fully meets the requirements of modern applications. SiPM exhibits excellent performance, including single-photon response at room temperature (with an intrinsic multiplication gain of 10^6), high detection efficiency of 25-60%, and a fast response...
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Ala'a AL-Zetoun (Chinese Academy of Sciences)Contributed talk - 12+3 min
The origin and composition of ultra-high energy cosmic rays (UHECRs) remain unresolved, particularly for events exceeding the Greisen–Zatsepin–Kuzmin cutoff and and whose apparent arrival directions do not point to plausible sources.
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This work investigates the hypothesis that a fraction of such events could be associated with low-mass magnetic monopoles (MMs) predicted in several theoretical... -
Alexander Antoshkin (Joint Institute for Nuclear Research (RU))Contributed talk - 12+3 min
We report the search for a magnetic monopole using the 2743-day exposure cosmic-ray triggered data collected by the NOvA far detector, which is a 14kt high segmented liquid scintillator one. The small overburden of the far detector helps us to extend the search to the low mass region that has been unexplored previously where the NOvA experiment has the best sensitivity.
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Igor OstrovskiyContributed talk - 12+3 min
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Nikolaos Mavromatos (Nat. Tech. U. Athens and King's College London)
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