Marco Battaglieri
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The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
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Marco Battaglieri has a total of 666 co-authors. Here are the top co-authors by number of shared publications:
- Mauro Taiuti
Università di Genova, Via Dodecaneso 33, Genova, 16146 Italy
11 shared publications - Mikhail Osipenko
INFN Sezione di Genova 16146 Genova Italy
10 shared publications R. De Vita
Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Genova 16146, Italy
10 shared publications- Silvia Pisano
INFN, Laboratori Nazionali di Frascati
10 shared publications - Alexandre Deur
Thomas Jefferson National Accelerator Facility, Newport News, VA 23606, USA
8 shared publications B. McKinnon
University of Glasgow, Glasgow, United Kingdom
8 shared publications
Latest Publications
- Open Access
- 25 June 2026
- Published by Springer Nature in The European Physical Journal C
- Vol. 86 (6) , 700
Investigation of the diurnal variation of cosmic rays at large latitudes by the detectors of the Extreme Energy Events Project
The diurnal modulation in galactic cosmic ray flux observed on the Earth is a widely studied phenomenon. Most of the analyses of this effect have been undertaken with data obtained by neutron monitor stations distributed over the world. The effect may also be seen in muon detectors, although muons are affected in a different way than neutrons. Particularly interesting is a comparison between the data obtained from neutron stations and muon telescopes located in the same region. In this paper we report an investigation of the diurnal modulation of cosmic rays at large latitudes, based on the data collected by three scintillator telescopes of the EEE (Extreme Energy Events) Project, installed at Ny-Ålesund, in the Svalbard archipelago, at $$79^{\circ }$$ N, during the period 2019–2025. Amplitudes and phases of the observed diurnal maximum in the cosmic ray flux were extracted in various periods by a harmonic fit of the averaged daily trend. Muon results were also compared to data collected in the period 2003–2025 by the Barentsburg Neutron Monitor Station, located not far from our detectors. The data, integrated along periods of one year, with a moving average in six months steps, show evidence of a diurnal modulation, with amplitudes of (0.05−0.1) $$\%$$ , smaller, roughly by a factor 2, than for neutrons, and a phase generally close to 12–16 h local time. No sensible differences were observed in the anisotropy parameters between solar nights and days in the polar region. The possible contribution of a second harmonic in the observed diurnal trend was also investigated.- 25 June 2026
- Published by Springer Nature in The European Physical Journal C
- Vol. 86 (6) , 700
Open AccessInvestigation of the diurnal variation of cosmic rays at large latitudes by the detectors of the Extreme Energy Events Project
The diurnal modulation in galactic cosmic ray flux observed on the Earth is a widely studied phenomenon. Most of the analyses of this effect have been undertaken with data obtained by neutron monitor stations distributed over the world. The effect may also be seen in muon detectors, although muons are affected in a different way than neutrons. Particularly interesting is a comparison between the data obtained from neutron stations and muon telescopes located in the same region. In this paper we report an investigation of the diurnal modulation of cosmic rays at large latitudes, based on the data collected by three scintillator telescopes of the EEE (Extreme Energy Events) Project, installed at Ny-Ålesund, in the Svalbard archipelago, at $$79^{\circ }$$ N, during the period 2019–2025. Amplitudes and phases of the observed diurnal maximum in the cosmic ray flux were extracted in various periods by a harmonic fit of the averaged daily trend. Muon results were also compared to data collected in the period 2003–2025 by the Barentsburg Neutron Monitor Station, located not far from our detectors. The data, integrated along periods of one year, with a moving average in six months steps, show evidence of a diurnal modulation, with amplitudes of (0.05−0.1) $$\%$$ , smaller, roughly by a factor 2, than for neutrons, and a phase generally close to 12–16 h local time. No sensible differences were observed in the anisotropy parameters between solar nights and days in the polar region. The possible contribution of a second harmonic in the observed diurnal trend was also investigated. - Open Access
- 20 March 2026
- Published by Springer Nature in The European Physical Journal C
- Vol. 86 (3) , 289
Measurement of the cosmic-ray rate over the period 2019–2025 at very high latitude (78.9°N)
Since 2019, the Extreme Energy Events (EEE) Project has installed three muon detection stations at the Svalbard Islands ( $$78.9^{\circ } \hbox {N}$$ latitude), employing scintillator-based detectors. This initiative represents the first systematic effort to monitor cosmic-muons rates at high geomagnetic latitudes beyond the Arctic Circle, with the objective of improving our understanding of cosmic-ray propagation and modulation in polar regions. The present study analyses temporal variations in the muon detection rates over a six-year period (2019–2025), including the study of periodic modulations and underlying trends in the observed rates.- 20 March 2026
- Published by Springer Nature in The European Physical Journal C
- Vol. 86 (3) , 289
Open AccessMeasurement of the cosmic-ray rate over the period 2019–2025 at very high latitude (78.9°N)
Since 2019, the Extreme Energy Events (EEE) Project has installed three muon detection stations at the Svalbard Islands ( $$78.9^{\circ } \hbox {N}$$ latitude), employing scintillator-based detectors. This initiative represents the first systematic effort to monitor cosmic-muons rates at high geomagnetic latitudes beyond the Arctic Circle, with the objective of improving our understanding of cosmic-ray propagation and modulation in polar regions. The present study analyses temporal variations in the muon detection rates over a six-year period (2019–2025), including the study of periodic modulations and underlying trends in the observed rates. - Open Access
- 24 December 2025
- Published by Springer Nature in The European Physical Journal A
- Vol. 61 (12)
A Beamdump facility at Jefferson Lab
The potential of the intense secondary muon, neutrino, and (hypothetical) light dark matter beams at the Thomas Jefferson National Accelerator Facility (Jefferson Lab) is explored. These are produced in the high-power dumps with high-current electron beams. Light dark matter searches with the approved Beam Dump eXperiment (BDX) are driving the realization of a new underground vault behind Hall A that could be extended to a Beamdump Facility with little additional installations. High-energy muons created via the Bethe–Heitler process uniquely do not proceed through the more common pion production and decay channels. Several possible muon physics applications are highlighted. Neutrino detector technologies and experiments suitable for a beamdump facility are outlined.
- 24 December 2025
- Published by Springer Nature in The European Physical Journal A
- Vol. 61 (12)
Open AccessA Beamdump facility at Jefferson Lab
The potential of the intense secondary muon, neutrino, and (hypothetical) light dark matter beams at the Thomas Jefferson National Accelerator Facility (Jefferson Lab) is explored. These are produced in the high-power dumps with high-current electron beams. Light dark matter searches with the approved Beam Dump eXperiment (BDX) are driving the realization of a new underground vault behind Hall A that could be extended to a Beamdump Facility with little additional installations. High-energy muons created via the Bethe–Heitler process uniquely do not proceed through the more common pion production and decay channels. Several possible muon physics applications are highlighted. Neutrino detector technologies and experiments suitable for a beamdump facility are outlined.
- Open Access
- 7 October 2025
- Published by EDP Sciences in EPJ Web of Conferences
- Vol. 337, 01135
Real Time implementation of Artificial Intelligence compression algorithm for High-Speed Streaming Readout signals
The new generation of high-energy physics experiments plans to acquire data in streaming mode. With this approach, it is possible to access the information of the whole detector (organized in time slices) for optimal and lossless triggering of data acquisitions. With this approach, data rates, especially in large detectors, are often very high, and the network is likely to be the bottleneck for the entire Streaming Read Out system. The aim of this work is to study the implementation of a lossy compression algorithm based on Artificial Intelligence: an Autoencoder. With Machine Learning it is possible to achieve a high compression ratio and fast inference time with only a small degradation of the signals, almost negligible for the specific application. This work explores different configurations of the Autoencoder and the implementation on different hardware. Different Autoencoder configurations are explored to find the best trade-off between compression ratio and reconstruction loss, both for signals and energy spectrum. Different hardware implementations are also explored to find the best platform to achieve real-time performance for the specific application.
- 7 October 2025
- Published by EDP Sciences in EPJ Web of Conferences
- Vol. 337, 01135
Open AccessReal Time implementation of Artificial Intelligence compression algorithm for High-Speed Streaming Readout signals
The new generation of high-energy physics experiments plans to acquire data in streaming mode. With this approach, it is possible to access the information of the whole detector (organized in time slices) for optimal and lossless triggering of data acquisitions. With this approach, data rates, especially in large detectors, are often very high, and the network is likely to be the bottleneck for the entire Streaming Read Out system. The aim of this work is to study the implementation of a lossy compression algorithm based on Artificial Intelligence: an Autoencoder. With Machine Learning it is possible to achieve a high compression ratio and fast inference time with only a small degradation of the signals, almost negligible for the specific application. This work explores different configurations of the Autoencoder and the implementation on different hardware. Different Autoencoder configurations are explored to find the best trade-off between compression ratio and reconstruction loss, both for signals and energy spectrum. Different hardware implementations are also explored to find the best platform to achieve real-time performance for the specific application.
- 17 April 2025
- Published by Springer Nature
- p. 50-58
Artificial Intelligence Data Reduction Algorithm for Streaming Readout in High Energy Physics Experiment
- 17 April 2025
- Published by Springer Nature
- p. 50-58
Artificial Intelligence Data Reduction Algorithm for Streaming Readout in High Energy Physics Experiment
- Open Access
- 4 January 2024
- Published by MDPI AG in Instruments
- Vol. 8 (1) , 1
Secondary Beams at High-Intensity Electron Accelerator Facilities
The interaction of a high-current O(100 µA), medium energy O(10 GeV) electron beam with a thick target O(1m) produces an overwhelming shower of standard model particles in addition to hypothetical light dark matter particles. While most of the radiation (gamma, electron/positron) is contained in the thick target, deep penetrating particles (muons, neutrinos, and light dark matter particles) propagate over a long distance, producing high-intensity secondary beams. Using sophisticated Monte Carlo simulations based on FLUKA and GEANT4, we explored the characteristics of secondary muons and neutrinos and (hypothetical) dark scalar particles produced by the interaction of the Jefferson Lab 11 GeV intense electron beam with the experimental Hall-A beam dump. Considering the possible beam energy upgrade, this study was repeated for a 22 GeV CEBAF beam.
- 4 January 2024
- Published by MDPI AG in Instruments
- Vol. 8 (1) , 1
Open AccessSecondary Beams at High-Intensity Electron Accelerator Facilities
The interaction of a high-current O(100 µA), medium energy O(10 GeV) electron beam with a thick target O(1m) produces an overwhelming shower of standard model particles in addition to hypothetical light dark matter particles. While most of the radiation (gamma, electron/positron) is contained in the thick target, deep penetrating particles (muons, neutrinos, and light dark matter particles) propagate over a long distance, producing high-intensity secondary beams. Using sophisticated Monte Carlo simulations based on FLUKA and GEANT4, we explored the characteristics of secondary muons and neutrinos and (hypothetical) dark scalar particles produced by the interaction of the Jefferson Lab 11 GeV intense electron beam with the experimental Hall-A beam dump. Considering the possible beam energy upgrade, this study was repeated for a 22 GeV CEBAF beam.
- Open Access
- 21 November 2023
- Published by American Physical Society (APS) in Physical Review D
- Vol. 108 (9) , 094030
Toward a generative modeling analysis of CLAS exclusive photoproductionAI-supported algorithms, particularly generative models, have been successfully used in a variety of different contexts. This work employs a generative modeling approach to unfold detector effects specifically tailored for exclusive reactions that involve multiparticle final states. Our study demonstrates the preservation of correlations between kinematic variables in a multidimensional phase space. We perform a full closure test on two-pion photoproduction pseudodata generated with a realistic model in the kinematics of the Jefferson Lab CLAS g11 experiment. The overlap of different reaction mechanisms leading to the same final state associated with the CLAS detector’s nontrivial effects represents an ideal test case for AI-supported analysis. Uncertainty quantification performed via bootstrap provides an estimate of the systematic uncertainty associated with the procedure. The test demonstrates that GANs can reproduce highly correlated multidifferential cross sections even in the presence of detector-induced distortions in the training datasets, and provides a solid basis for applying the framework to real experimental data.
- 21 November 2023
- Published by American Physical Society (APS) in Physical Review D
- Vol. 108 (9) , 094030
Open AccessToward a generative modeling analysis of CLAS exclusive photoproductionAI-supported algorithms, particularly generative models, have been successfully used in a variety of different contexts. This work employs a generative modeling approach to unfold detector effects specifically tailored for exclusive reactions that involve multiparticle final states. Our study demonstrates the preservation of correlations between kinematic variables in a multidimensional phase space. We perform a full closure test on two-pion photoproduction pseudodata generated with a realistic model in the kinematics of the Jefferson Lab CLAS g11 experiment. The overlap of different reaction mechanisms leading to the same final state associated with the CLAS detector’s nontrivial effects represents an ideal test case for AI-supported analysis. Uncertainty quantification performed via bootstrap provides an estimate of the systematic uncertainty associated with the procedure. The test demonstrates that GANs can reproduce highly correlated multidifferential cross sections even in the presence of detector-induced distortions in the training datasets, and provides a solid basis for applying the framework to real experimental data.
- Open AccessToward a generative modeling analysis of CLAS exclusive $2π$ photoproduction
AI-supported algorithms, particularly generative models, have been successfully used in a variety of different contexts. In this work, we demonstrate for the first time that generative adversarial networks (GANs) can be used in high-energy experimental physics to unfold detector effects from multi-particle final states, while preserving correlations between kinematic variables in multidimensional phase space. We perform a full closure test on two-pion photoproduction pseudodata generated with a realistic model in the kinematics of the Jefferson Lab CLAS g11 experiment. The overlap of different reaction mechanisms leading to the same final state associated with the CLAS detector's nontrivial effects represents an ideal test case for AI-supported analysis. Uncertainty quantification performed via bootstrap provides an estimate of the systematic uncertainty associated with the procedure. The test demonstrates that GANs can reproduce highly correlated multidifferential cross sections even in the presence of detector-induced distortions in the training datasets, and provides a solid basis for applying the framework to real experimental data.
Open AccessToward a generative modeling analysis of CLAS exclusive $2π$ photoproductionAI-supported algorithms, particularly generative models, have been successfully used in a variety of different contexts. In this work, we demonstrate for the first time that generative adversarial networks (GANs) can be used in high-energy experimental physics to unfold detector effects from multi-particle final states, while preserving correlations between kinematic variables in multidimensional phase space. We perform a full closure test on two-pion photoproduction pseudodata generated with a realistic model in the kinematics of the Jefferson Lab CLAS g11 experiment. The overlap of different reaction mechanisms leading to the same final state associated with the CLAS detector's nontrivial effects represents an ideal test case for AI-supported analysis. Uncertainty quantification performed via bootstrap provides an estimate of the systematic uncertainty associated with the procedure. The test demonstrates that GANs can reproduce highly correlated multidifferential cross sections even in the presence of detector-induced distortions in the training datasets, and provides a solid basis for applying the framework to real experimental data.
- Open Access
Feebly Interacting Particles: FIPs 2022 workshop report
Particle physics today faces the challenge of explaining the mystery of dark matter, the origin of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent fine-tuning of the electro-weak scale, and many other aspects of fundamental physics. Perhaps the most striking frontier to emerge in the search for answers involves new physics at mass scales comparable to familiar matter, below the GeV-scale, or even radically below, down to sub-eV scales, and with very feeble interaction strength. New theoretical ideas to address dark matter and other fundamental questions predict such feebly interacting particles (FIPs) at these scales, and indeed, existing data provide numerous hints for such possibility. A vibrant experimental program to discover such physics is under way, guided by a systematic theoretical approach firmly grounded on the underlying principles of the Standard Model. This document represents the report of the FIPs 2022 workshop, held at CERN between the 17 and 21 October 2022 and aims to give an overview of these efforts, their motivations, and the decadal goals that animate the community involved in the search for FIPs.
Open AccessFeebly Interacting Particles: FIPs 2022 workshop report
Particle physics today faces the challenge of explaining the mystery of dark matter, the origin of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent fine-tuning of the electro-weak scale, and many other aspects of fundamental physics. Perhaps the most striking frontier to emerge in the search for answers involves new physics at mass scales comparable to familiar matter, below the GeV-scale, or even radically below, down to sub-eV scales, and with very feeble interaction strength. New theoretical ideas to address dark matter and other fundamental questions predict such feebly interacting particles (FIPs) at these scales, and indeed, existing data provide numerous hints for such possibility. A vibrant experimental program to discover such physics is under way, guided by a systematic theoretical approach firmly grounded on the underlying principles of the Standard Model. This document represents the report of the FIPs 2022 workshop, held at CERN between the 17 and 21 October 2022 and aims to give an overview of these efforts, their motivations, and the decadal goals that animate the community involved in the search for FIPs.
- Open Access
- 28 October 2022
- Published by American Physical Society (APS) in Physical Review D
- Vol. 106 (7) , 072011
Dark matter search with the BDX-MINI experiment
BDX-MINI is a beam dump experiment optimized to search for light dark matter produced in the interaction of the intense CEBAF 2.176 GeV electron beam with the Hall A beam dump at Jefferson Lab. The BDX-MINI detector consists of a electromagnetic calorimeter surrounded by a hermetic veto system for background rejection. The experiment accumulated EOT in six months of running. Simulations of fermionic and scalar dark matter interactions with electrons of the active volume of the BDX-MINI detector were used to estimate the expected signal. Data collected during the beam-off time allowed us to characterize the background dominated by cosmic rays. A blind data analysis based on a maximum-likelihood approach was used to optimize the experiment sensitivity. An upper limit on the production of light dark matter was set using the combined event samples collected during beam-on and beam-off configurations. In some kinematic regions of interest, this pilot experiment is sensitive to the parameter space covered by some of the most sensitive experiments to date, which demonstrates the discovery potential of the next generation beam dump experiment planned at intense electron beam facilities.- 28 October 2022
- Published by American Physical Society (APS) in Physical Review D
- Vol. 106 (7) , 072011
Open AccessDark matter search with the BDX-MINI experiment
BDX-MINI is a beam dump experiment optimized to search for light dark matter produced in the interaction of the intense CEBAF 2.176 GeV electron beam with the Hall A beam dump at Jefferson Lab. The BDX-MINI detector consists of a electromagnetic calorimeter surrounded by a hermetic veto system for background rejection. The experiment accumulated EOT in six months of running. Simulations of fermionic and scalar dark matter interactions with electrons of the active volume of the BDX-MINI detector were used to estimate the expected signal. Data collected during the beam-off time allowed us to characterize the background dominated by cosmic rays. A blind data analysis based on a maximum-likelihood approach was used to optimize the experiment sensitivity. An upper limit on the production of light dark matter was set using the combined event samples collected during beam-on and beam-off configurations. In some kinematic regions of interest, this pilot experiment is sensitive to the parameter space covered by some of the most sensitive experiments to date, which demonstrates the discovery potential of the next generation beam dump experiment planned at intense electron beam facilities.