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Alan Barr (University of Oxford (GB)), Brian Thomas Batell, Felix Kling (DESY), Juan Salvador Tafoya Vargas (University of California Davis (US))05/03/2026, 09:00
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Urs Wiedemann (CERN)05/03/2026, 09:15
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Matthew Philip Mccullough (CERN)05/03/2026, 09:30
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Dr Umut Kose (ETH-Zurich)05/03/2026, 09:45
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Ryan Plestid (CERN)05/03/2026, 10:10
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Dr Tanguy Pierog05/03/2026, 10:35
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Julien Prosic05/03/2026, 11:30
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Tamara Alice Bud (CERN)05/03/2026, 12:00
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Arindam Das (Hokkaido University)05/03/2026, 14:30
We study two general $U(1)$ extensions of the Standard Model (SM) those generate tiny neutrino masses via the seesaw mechanism after general $U(1)$ breaking. These models predict a new neutral gauge boson ($Z'$) and right-handed neutrinos (RHNs), the latter introduced for anomaly cancellation and neutrino mass generation. In both scenarios, left- and right-handed fermions couple differently...
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Mattia Bellotti (Università di Cagliari)05/03/2026, 14:30
One of the main goals of physics is to understand the inner structure of matter. To achieve this result, studying the composition of protons and neutrons (nucleons) is essential. In nonperturbative QCD the internal structure of nucleons can be described in terms of parton distribution functions (PDF). PDFs can in turn be investigated using deep-inelastic-scattering processes...
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Wei Su (Sun Yat-sen University)05/03/2026, 14:50
In this talk I will show our recent study about the LLP searches af FASER. There are two kinds of modes, with the production from the usual mesons, and from the PP collision directly.
For the meson production mode, we study the prospect of detecting light CP-even and CP-odd scalars. We develop the general formalism for the scalar production and decay from mesons at LHC, given modified...
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Jelle Koorn (Nikhef National institute for subatomic physics (NL))05/03/2026, 14:50
The recent detection of TeV neutrinos at FASER has launched a new era of collider physics. Measuring the flavor, energy and rapidity of these neutrinos allows for an unprecedented extraction of the full energy-dependence of far-forward neutrino production in p-p collisions. Analogous to PDF extractions from collider data, we determine the energy distribution of the (anti) muon neutrino flux at...
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Ken Ohashi (Universitaet Bern (CH))05/03/2026, 15:10
The muon puzzle --- an excess of muons relative to simulation predictions in ultra-high-energy cosmic-ray air showers --- has been reported by many experiments.
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This suggests that forward particle production in hadronic interactions is not fully understood.
Some of the scenarios proposed to resolve this predict reduced production of forward neutral pions and enhanced production of forward... -
Herbi Dreiner05/03/2026, 15:10
We have investigated single photon signatures of a light long-lived neutralino in supersymmetric models with broken R-parity. We consider the sensitivities at the detectors: ANUBIS, CODEXb, FACET, FASER, MAPP, MATHUSLA.
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Matteo Borrello (University of Florence, INFN of Florence)05/03/2026, 15:30
The origin of neutrino masses suggests the existence of a sterile neutrino sector, which may be either too heavy or too weakly coupled to the Standard Model (SM) to be detected in the near future. The inverse seesaw mechanism provides a testable framework where the coupling between the sterile sector and the SM is large enough to allow direct experimental probes. In this context, it is crucial...
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Diego Lopez Gutierrez (Washington University in St Louis)05/03/2026, 15:30
We present the first detailed study of Standard Model neutrino tridents involving tau leptons at the near detectors of accelerator neutrino facilities. The rates of these processes were previously thought to be negligible, even at future facilities. Our full $2\to4$
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calculation, including both coherent and incoherent scatterings, reveals that the DUNE near detector could observe a... -
Daniel La Rocco05/03/2026, 16:00
Heavy Neutral Leptons (HNLs) are a well-motivated extension of the Standard Model which may provide explanations for observed neutrino masses, dark matter, and baryogengesis via leptogenesis. In the event that a HNL signal is actually detected, much work will be dedicated to identifying the underlying nature of the observed signal excess. In this talk, we will use Monte-Carlo simulations of...
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Gabriel Rabelo-Soares05/03/2026, 16:00
The electromagnetic production of a dilepton pair in the muon - ion scattering, usually denoted as muon trident process, is investigated considering the feasibility of studying processes induced by muons at LHC using FASER$\nu$ and FASER$\nu$2 detectors. The total and differential cross - sections are estimated taking into account of the Bethe-Heitler and bremsstrahlung channels, and...
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Dr Toni Makela (University of California, Irvine)05/03/2026, 16:20
Most existing and proposed high energy neutrino experiments have excellent muon charge identification capabilities, enabling the distinction of $\nu_\mu$ and $\bar \nu_\mu$ charged current interactions. In contrast, distinguishing electrons and positrons from $\nu_e$ and $\bar \nu_e$ interactions is typically impossible, as they quickly interact within dense detector materials and do not reach...
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Misa Toman05/03/2026, 16:20
We investigate the spin correlations between production and decay in the process where dark photons $A'$ are produced in pseudoscalar meson decays, for example, $\pi^0, \eta \to \gamma A'$, and then decay to fermion pairs, $A' \to f \bar{f}$. This process is the focus of many experimental searches, but spin correlations are typically ignored. We derive analytic results that allow us to...
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Peiran Li (University of Minnesota)05/03/2026, 16:40
We study the sensitivity of the FORMOSA experiment at the LHC Forward Physics Facility to millicharged particles (mCPs), focusing on a previously unexplored production mechanism associated with the forward neutron flux. Existing studies mainly consider mCP production from forward mesons directly produced in pp collisions.
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We point out that pp collisions also generate an intense flux of... -
Isabella Coronado05/03/2026, 16:40
Measurements of neutrino fluxes at the Forward Physics Facility can be used to study predictions of hadronic interaction models. These advancements are critical for astroparticle physics, linking forward scattering processes to extensive air showers and improving our understanding of cosmic-ray interactions. This work investigates simulated neutrino fluxes at the FPF, focusing in particular on...
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Yu-Dai Tsai (University of California, Irvine)05/03/2026, 17:00
We demonstrate that the searches for dark sector particles can provide probes of reheating scenarios, focusing on the cosmic millicharge background produced in the early universe. We discuss two types of millicharge particles (mCPs): either with, or without, an accompanying dark photon. These two types of mCPs have distinct theoretical motivations and cosmological signatures. We discuss...
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Kemuel Cullimore (University of Utah)05/03/2026, 17:00
Our goal is to constrict hadronic interaction models in the far-forward region. To do this, we produce simulations of the muon fluxes produced from the decay of different hadrons using BDSIM with different event generators. We will present studies of the energy spectra and x-y position of the muon flux at FASER for different parent particles to constrain various hadronic interaction models.
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Prof. Subir Sarkar (University of Oxford)06/03/2026, 09:00
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Juan Salvador Tafoya Vargas (University of California Davis (US))06/03/2026, 09:30
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Jacob Henry Steenis (University of California Davis (US)), Jacob Steenis06/03/2026, 10:00
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Kohei Chinone (Chiba University (JP))06/03/2026, 11:00
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Josh McFayden (University of Sussex)06/03/2026, 11:20
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Elena Firu (Institute of Space Science subsidiary of INFLPR (RO))06/03/2026, 11:50
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Matteo Vicenzi (Brookhaven National Laboratory (US))06/03/2026, 14:00
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Peter Krack, Peter Krack (Nikhef National institute for subatomic physics (NL)), Peter Krack06/03/2026, 14:30
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Zahra Tabrizi (University of Pittsburgh (US))06/03/2026, 15:00
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06/03/2026, 16:00
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Jonathan Lee Feng (University of California Irvine (US))06/03/2026, 16:45
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