M. Pozzato

ORCID: 0000-0003-0279-5436
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About
Contact & Profiles
Research Areas
  • Neutrino Physics Research
  • Particle physics theoretical and experimental studies
  • Astrophysics and Cosmic Phenomena
  • Particle Detector Development and Performance
  • Dark Matter and Cosmic Phenomena
  • Radiation Detection and Scintillator Technologies
  • Earthquake Detection and Analysis
  • Ionosphere and magnetosphere dynamics
  • Particle accelerators and beam dynamics
  • High-Energy Particle Collisions Research
  • Atomic and Subatomic Physics Research
  • Particle Accelerators and Free-Electron Lasers
  • earthquake and tectonic studies
  • Solar and Space Plasma Dynamics
  • Quantum Chromodynamics and Particle Interactions
  • Nuclear Physics and Applications
  • Gamma-ray bursts and supernovae
  • Muon and positron interactions and applications
  • Geomagnetism and Paleomagnetism Studies
  • Radiation Therapy and Dosimetry
  • Astro and Planetary Science
  • Superconducting Materials and Applications
  • Advanced Frequency and Time Standards
  • Planetary Science and Exploration
  • Mass Spectrometry Techniques and Applications

Istituto Nazionale di Fisica Nucleare, Sezione di Bologna
2016-2025

University of Bologna
2014-2024

Institute of Space Science - INFLPR Subsidiary
2024

Istituto Nazionale di Fisica Nucleare, Sezione di Padova
2019-2024

Istituto Nazionale di Fisica Nucleare
2019-2024

Istituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And Applications
2016-2023

University of Trento
2021-2023

Fondazione Bruno Kessler
2023

Imperial College London
2021

King's College London
2018-2021

The OPERA experiment was designed to study ν_{μ}→ν_{τ} oscillations in the appearance mode CERN Gran Sasso Neutrino beam (CNGS). In this Letter, we report final analysis of full data sample collected between 2008 and 2012, corresponding 17.97×10^{19} protons on target. Selection criteria looser than previous analyses have produced ten ν_{τ} candidate events, thus reducing statistical uncertainty measurement oscillation parameters properties. A multivariate approach for event identification...

10.1103/physrevlett.120.211801 article EN cc-by Physical Review Letters 2018-05-22

This search for magnetic monopoles (MMs) and high electric charge objects (HECOs) with spins 0, 1/2, 1, uses the first time full MoEDAL detector, exposed to 6.46 fb^{-1} proton-proton collisions at 13 TeV. The results are interpreted in terms of Drell-Yan photon-fusion pair production. Mass limits on direct production MMs up 10 Dirac charges HECOs range 10e 400e, were achieved. placed MM HECO currently strongest world. is only LHC experiment capable being directly calibrated highly ionizing...

10.1103/physrevlett.134.071802 article EN cc-by Physical Review Letters 2025-02-20

The MoEDAL experiment at Point 8 of the LHC ring is seventh and newest experiment. It dedicated to search for highly-ionizing particle avatars physics beyond Standard Model, extending significantly discovery horizon LHC. A would have revolutionary implications our fundamental understanding Microcosm. an unconventional largely passive detector comprised largest array Nuclear Track Detector stacks ever deployed accelerator, surrounding intersection region on ring. Another novel feature use...

10.1142/s0217751x14300506 article EN International Journal of Modern Physics A 2014-09-05

MoEDAL is designed to identify new physics in the form of long-lived highly ionizing particles produced high-energy LHC collisions. Its arrays plastic nuclear-track detectors and aluminium trapping volumes provide two independent passive detection techniques. We present here results a first search for magnetic monopole production 13 TeV proton-proton collisions using technique, extending previous publication with 8 data during Run 1. A total 222 kg detector samples was exposed forward region...

10.1103/physrevlett.118.061801 article EN cc-by Physical Review Letters 2017-02-10

The MoEDAL experiment is designed to search for magnetic monopoles and other highly-ionising particles produced in high-energy collisions at the LHC. largely passive detector, deployed Interaction Point 8 on LHC ring, relies two dedicated direct detection techniques. first technique based stacks of nucleartrack detectors with surface area ~18m2, sensitive particle ionisation exceeding a high threshold. These are analysed offline by optical scanning microscopes. second trapping charged an...

10.1007/jhep08(2016)067 article EN cc-by Journal of High Energy Physics 2016-08-01

MoEDAL is designed to identify new physics in the form of stable or pseudostable highly ionizing particles produced high-energy Large Hadron Collider (LHC) collisions. Here we update our previous search for magnetic monopoles Run 2 using full trapping detector with almost four times more material and twice integrated luminosity. For first time at LHC, data were interpreted terms photon-fusion monopole direct production addition Drell-Yan-like mechanism. The detector, consisting 794 kg...

10.1103/physrevlett.123.021802 article EN cc-by Physical Review Letters 2019-07-09

We update our previous search for trapped magnetic monopoles in LHC Run 2 using nearly six times more integrated luminosity and including additional models the interpretation of data. The MoEDAL forward trapping detector, comprising 222 kg aluminium samples, was exposed to 2.11 fb−1 13 TeV proton–proton collisions near LHCb interaction point analysed by searching induced persistent currents after passage through a superconducting magnetometer. Magnetic charges equal Dirac charge or above are...

10.1016/j.physletb.2018.05.069 article EN cc-by Physics Letters B 2018-05-29

Abstract The China Seismo-Electromagnetic Satellite ( CSES ) aims to monitor electromagnetic, particle, and plasma perturbations in the iono-magnetosphere inner Van Allen radiation belts originated by electromagnetic sources external internal geomagnetic cavity, cosmic rays, solar events. In particular, objective of space mission is investigate lithosphere–atmosphere–ionosphere coupling mechanisms (including effects lightning, earthquakes, volcanoes, artificial emissions) that induce top...

10.3847/1538-4365/ab276c article EN The Astrophysical Journal Supplement Series 2019-07-01

Abstract High-energy, long gamma-ray bursts (GRBs) can be generated by the core collapse of massive stars at end their lives. When they happen in close-by universe exceptionally bright, as seen from Earth case recent, giant, long-lasting GRB221009A. GRB221009A was produced a collapsing star with redshift 0.152: this event observed many space experiments, which also detected an extraordinary afterglow. The large fluence prompt emission about 0.013 erg cm −2 illuminated geographical region...

10.3847/2041-8213/acc247 article EN cc-by The Astrophysical Journal Letters 2023-03-01

Abstract The Deep Underground Neutrino Experiment (DUNE) is a next generation experiment aimed to study neutrino oscillation. Its long-baseline configuration will exploit Near Detector (ND) and Far (FD) located at distance of ∼1300 km. FD consist four Liquid Argon Time Projection Chamber (LAr TPC) modules. A Photon Detection System (PDS) be used detect the scintillation light produced inside detector after interactions. PDS based on collectors coupled Silicon Photomultipliers (SiPMs)....

10.1088/1748-0221/19/01/t01007 article EN cc-by Journal of Instrumentation 2024-01-01

The OPERA experiment, designed to conclusively prove the existence of νμ→ντ oscillations in atmospheric sector, makes use a massive lead-nuclear emulsion target observe appearance ντ's CNGS νμ beam. location and analysis neutrino interactions quasi real-time required development fast computer-controlled microscopes able reconstruct particle tracks with sub-micron precision high efficiency at speed ∼20 cm2/h. This paper describes performance track reconstruction theEuropean Scanning System,...

10.1088/1748-0221/2/05/p05004 article EN Journal of Instrumentation 2007-05-21

The OPERA experiment, designed to perform the first observation of $$\nu _\mu \rightarrow \nu _\tau $$ oscillations in appearance mode through detection $$\tau leptons produced charged current interactions, has collected data from 2008 2012. In present paper, procedure developed detect particle decays, occurring over distances order $$1~\mathrm{mm}$$ neutrino interaction point, is described detail and applied search for charmed hadrons, showing similar decay topologies as lepton. analysed...

10.1140/epjc/s10052-014-2986-0 article EN cc-by The European Physical Journal C 2014-08-01

Abstract The High-energy Particle Detector (HEPD) on board the China Seismo-Electromagnetic Satellite (CSES-01)—launched 2018 February 2—is a light and compact payload suitable for measuring electrons (3–100 MeV), protons (30–250 nuclei (up to few hundreds of MeV). Sun-synchronous orbit large acceptance allow HEPD measure cosmic-ray particles near ±65° latitude limit fair amount time per day. In this work, three semiannual galactic hydrogen energy spectra between ∼40 250 MeV are presented,...

10.3847/1538-4357/abad3e article EN cc-by The Astrophysical Journal 2020-09-01

The MoEDAL trapping detector, consists of approximately 800 kg aluminium volumes. It was exposed during Run-2 the LHC program to 6.46 fb^-1 13 TeV proton-proton collisions at LHCb interaction point. Evidence for dyons (particles with electric and magnetic charge) captured in detector sought by passing volumes comprising through a SQUID magnetometer. presence trapped dyon would be signalled persistent current induced On basis Drell-Yan production model, we exclude charge ranging up 5 Dirac...

10.1103/physrevlett.126.071801 article EN cc-by Physical Review Letters 2021-02-19

Abstract In this work we present the High‐Energy Particle Detector (HEPD‐01) observations of proton fluxes from space during 28 October 2021 solar energetic particle event, which produced a ground‐level enhancement on Earth. The event was associated with major, long‐duration X1‐class flare and concomitant coronal mass ejection (CME) that erupted Active Region 12887. This is first direct measurement particles emitted current cycle, recorded by single instrument in energy range ∼50 MeV/n up to...

10.1029/2022sw003191 article EN cc-by Space Weather 2022-10-11

Abstract Time-dependent energy spectra of galactic cosmic rays (GCRs) carry crucial information regarding their origin and propagation throughout the interstellar environment. When observed at Earth, after traversing interplanetary medium, such are heavily affected by solar wind embedded magnetic field permeating inner sectors heliosphere. The activity Sun changes significantly over an 11 yr cycle—and so does effect on particles; this translates into a phenomenon called modulation. Moreover,...

10.3847/2041-8213/acbea7 article EN cc-by The Astrophysical Journal Letters 2023-03-01

The ENUBET project recently concluded the R&D for a site independent design of monitored neutrino beam high precision cross section measurements, in which flux is inferred from measurement charged leptons an instrumented decay tunnel. In this phase three fundamental results were obtained and will be discussed here: 1) beamline not requiring horn relying on static focusing elements allows to perform $\nu_e$ DUNE energy range with 1% statistical uncertainty employing $10^{20}$ 400 GeV protons...

10.48550/arxiv.2501.04531 preprint EN arXiv (Cornell University) 2025-01-08

The OPERA experiment, exposed to the CERN Gran Sasso $ν_μ$ beam, collected data from 2008 2012. Four oscillated $ν_τ$ Charged Current interaction candidates have been detected in appearance mode, which are consistent with $ν_μ\to ν_τ$ oscillations at atmospheric $Δm^2$ within "standard" three-neutrino framework. In this paper, results used derive limits on mixing parameters of a massive sterile neutrino.

10.1007/jhep06(2015)069 article EN cc-by Journal of High Energy Physics 2015-06-01
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