Search Results - "Giammarchi, M"
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1
Injection and capture of antiprotons in a Penning–Malmberg trap using a drift tube accelerator and degrader foil
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (01-08-2024)“…The Antiproton Decelerator (AD) at CERN provides antiproton bunches with a kinetic energy of 5.3 MeV. The Extra-Low ENergy Antiproton ring at CERN,…”
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First demonstration of antimatter wave interferometry
Published in Science advances (01-05-2019)“…Interference of matter waves is at the heart of quantum physics and has been observed for a wide range of particles from electrons to complex molecules. Here,…”
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3
Upgrade of ASACUSA’s antihydrogen detector
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (01-01-2023)“…The goal of the ASACUSA (Atomic Spectroscopy And Collisions Using Slow Antiprotons) CUSP experiment at CERN’s Antiproton Decelerator is to measure the ground…”
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Nanoseconds Timing System Based on IEEE 1588 FPGA Implementation
Published in IEEE transactions on nuclear science (01-07-2019)“…Clock synchronization procedures are mandatory in most physical experiments where event fragments are readout by spatially dislocated sensors and must be glued…”
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Efficient two-step Positronium laser excitation to Rydberg levels
Published in Nuclear instruments & methods in physics research. Section B, Beam interactions with materials and atoms (01-07-2011)“…Antihydrogen production by charge exchange reaction between Positronium atoms and antiprotons requires efficient excitation of Positronium atoms up to high- n…”
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6
Analysis of reactor burnup simulation uncertainties for antineutrino spectrum prediction
Published in European physical journal plus (29-10-2024)“…Nuclear reactors are a source of electron antineutrinos due to the presence of unstable fission products that undergo β - decay. They will be exploited by the…”
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Science and technology of Borexino: a real-time detector for low energy solar neutrinos
Published in Astroparticle physics (2002)“…Borexino, a real-time device for low energy neutrino spectroscopy is nearing completion of construction in the underground laboratories at Gran Sasso, Italy…”
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8
Thermal production of positronium in porous alumina
Published in The European physical journal. D, Atomic, molecular, and optical physics (01-05-2012)“…A porous anodic alumina sample with ordered channels was studied in order to characterise its efficiency as a positron-positronium converter at cryogenic…”
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9
The scintillator solvent procurement for the Borexino solar neutrino detector
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (21-08-2011)“…This paper describes the procurement and the production quality control system of Pseudocumene, the scintillator solvent of the solar neutrino detector…”
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10
Laser sources for efficient two-step Positronium excitation to Rydberg states
Published in Journal of molecular structure (03-05-2011)“…Antihydrogen production by charge exchange reaction between Positronium atoms and antiprotons benefits from an efficient excitation of Positronium atoms to…”
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New experimental limits on violations of the Pauli exclusion principle obtained with the Borexino Counting Test Facility
Published in The European physical journal. C, Particles and fields (01-11-2004)“…The Pauli exclusion principle (PEP) has been tested for nucleons (n,p) in \({}^{12}{\rm C}\) and \({}^{16}{\rm O}\) nuclei, using the results of background…”
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12
Precision measurement of the (7)Be solar neutrino interaction rate in Borexino
Published in Physical review letters (30-09-2011)“…The rate of neutrino-electron elastic scattering interactions from 862 keV (7)Be solar neutrinos in Borexino is determined to be…”
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13
Analysis of reactor burnup simulation uncertainties for antineutrino spectrum prediction
Published 30-10-2024“…Eur. Phys. J. Plus 139, 952 (2024) Nuclear reactors are a source of electron antineutrinos due to the presence of unstable fission products that undergo…”
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14
Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun
Published in Nature (London) (26-11-2020)“…For most of their existence, stars are fuelled by the fusion of hydrogen into helium. Fusion proceeds via two processes that are well understood theoretically:…”
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15
Final results of Borexino Phase-I on low-energy solar neutrino spectroscopy
Published in Physical review. D, Particles, fields, gravitation, and cosmology (25-06-2014)“…Borexino has been running since May 2007 at the Laboratori Nazionali del Gran Sasso laboratory in Italy with the primary goal of detecting solar neutrinos. The…”
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Improved Measurement of Solar Neutrinos from the Carbon-Nitrogen-Oxygen Cycle by Borexino and Its Implications for the Standard Solar Model
Published in Physical review letters (16-12-2022)“…We present an improved measurement of the carbon-nitrogen-oxygen (CNO) solar neutrino interaction rate at Earth obtained with the complete Borexino Phase-III…”
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Precision Measurement of the Be7 Solar Neutrino Interaction Rate in Borexino
Published in Physical review letters (30-09-2011)“…The rate of neutrino-electron elastic scattering interactions from 862 keV Be7 solar neutrinos in Borexino is determined to be…”
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18
Precision Measurement of the Be 7 Solar Neutrino Interaction Rate in Borexino
Published in Physical review letters (30-09-2011)Get full text
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19
A large-scale low-background liquid scintillation detector: the counting test facility at Gran Sasso
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (11-04-1998)“…A 4.8 m 3 unsegmented liquid scintillation detector at the underground Laboratori Nazionali del Gran Sasso has shown the feasibility of multi-ton…”
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First evidence of pep solar neutrinos by direct detection in Borexino
Published in Physical review letters (03-02-2012)“…We observed, for the first time, solar neutrinos in the 1.0-1.5 MeV energy range. We determined the rate of pep solar neutrino interactions in Borexino to be…”
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