CERN Accelerating science

CERN Document Server 1,386 records found  1 - 10próximoend  jump to record: Search took 0.68 seconds. 
1.
Recent outreach activities of the EEE Project / Ripoli, C ; Abbrescia, M ; Avanzini, C ; Baldini, L ; Baldini Ferroli, R ; Batignani, G ; Battaglieri, M ; Boi, S ; Bossini, E ; Carnesecchi, F (CERN) et al.
The Extreme Energy Events Project is an educational and scientific initiative lead by the Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi (CREF) and the Istituto Nazionale di Fisica Nucleare (INFN), two research Institutions under the control of the Italian Ministero dell’Universit`a e Ricerca (MUR). The EEE Project studies cosmic rays by means of a series of detectors located inside Italian high schools or INFN/University laboratories. [...]
2025 - 7 p. - Published in : J. Phys. : Conf. Ser. 3053 (2025) 012042 Fulltext: PDF;
2.
High latitude observation of the Forbush decrease during the May 2024 solar storms with muon and neutron detectors on Svalbard / Riggi, F (Unlisted, IT ; INFN, Catania ; U. Catania (main)) ; Hertle, L (Unlisted, DE) ; Abbrescia, M (Bari U. ; INFN, Bari) ; Avanzini, C (U. Pisa (main) ; INFN, Pisa) ; Baldini, L (U. Pisa (main) ; INFN, Pisa) ; Baldini Ferroli, R (Frascati) ; Batignani, G (U. Pisa (main) ; INFN, Pisa ; Unlisted, IT) ; Battaglieri, M (INFN, Genoa) ; Boi, S (U. Cagliari (main) ; INFN, Cagliari) ; Boike, J (Unlisted, DE ; Humboldt U., Berlin (main)) et al.
During the series of intense solar flares and coronal mass ejections, that occurred in May 2024, a remarkable Forbush decrease in the cosmic ray flux was observed on the Earth. While this event was observed by particle detectors around the world, the archipelago of Svalbard was heavily exposed to it due to the weak geomagnetic shielding in the polar region. [...]
2025 - 15 p. - Published in : Adv. Space Res. 76 (2025) 1225-1239
3.
Properties of Cosmic Lithium Isotopes Measured by the Alpha Magnetic Spectrometer / AMS Collaboration
We present the first measurement of cosmic-ray fluxes of  Li6 and  Li7 isotopes in the rigidity range from 1.9 to 25 GV. The measurements are based on 9.7×105  Li6 and 1.04×106  Li7 nuclei collected by the Alpha Magnetic Spectrometer on the International Space Station from May 2011 to October 2023. [...]
2025 - 8 p. - Published in : Phys. Rev. Lett. 134 (2025) 201001 Fulltext: PDF;
4.
$\phi \to \eta \gamma$ / Basile, M. ; Dalpiaz, P. ; Frabetti, P.L. ; Massam, T. ; Navarria, F.L. ; Schneegans, M.A. ; Zichichi, A.
CERN-PRE-14301.
- 1971 - 6.
5.
Measurement of the muon flux in the tunnels of Doss Trento hill / Abbrescia, M (Bari U. ; INFN, Bari) ; Avanzini, C (INFN, Pisa ; Pisa U.) ; Baldini, L (Pisa U. ; INFN, Pisa) ; Ferroli, R Baldini (Frascati) ; Batignani, G (Pisa U. ; INFN, Pisa ; Enrico Fermi Ctr., Rome) ; Battaglieri, M (INFN, Genoa) ; Battiston, R (Trento U. ; TIFPA-INFN, Trento) ; Bimbi, S (Rome U.) ; Boi, S (INFN, Cagliari) ; Bossini, E (INFN, Pisa) et al.
In the context of astroparticle physics, nuclear astrophysics and quantum computing projects, it is important identifying underground laboratories where the cosmogenic background is suppressed. Located about 500 m far from the center of Trento (Italy) the Piedicastello tunnels are covered by 100 m limestone rock of the Doss Trento hill. [...]
2024 - 9 p. - Published in : Nucl. Instrum. Methods Phys. Res., A 1072 (2025) 170163 Fulltext: PDF;
6.
Antiprotons and Elementary Particles over a Solar Cycle: Results from the Alpha Magnetic Spectrometer / AMS Collaboration
We present results over an 11-year Solar cycle of cosmic antiprotons based on 1.1×106 events in the rigidity range from 1.00 to 41.9 GV. The p¯ fluxes exhibit distinct properties. [...]
2025 - 12 p. - Published in : Phys. Rev. Lett. 134 (2025) 051002 Fulltext: PDF;
7.
Solar Modulation of Cosmic Nuclei over a Solar Cycle: Results from the Alpha Magnetic Spectrometer / AMS Collaboration
We report the properties of precision time structures of cosmic nuclei He, Li, Be, B, C, N, and O fluxes over an 11-year solar cycle from May 2011 to November 2022 in the rigidity range from 1.92 to 60.3 GV. The nuclei fluxes show similar but not identical time variations with amplitudes decreasing with increasing rigidity. [...]
2025 - 8 p. - Published in : Phys. Rev. Lett. 134 (2025) 051001 Fulltext: PDF;
8.
Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experiment / DarkSide-20k Collaboration
DarkSide-20k is a novel liquid argon dark matter detector currently under construction at the Laboratori Nazionali del Gran Sasso (LNGS) of the Istituto Nazionale di Fisica Nucleare (INFN) that will push the sensitivity for Weakly Interacting Massive Particle (WIMP) detection into the neutrino fog. [...]
arXiv:2412.18867.
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Fulltext
9.
First results on new helium based eco-gas mixtures for the Extreme Energy Events Project / EEE Collaboration
The Extreme Energy Events (EEE) Project, a joint project of the Centro Fermi (Museo Storico della Fisica e Centro Studi e Ricerche "E.Fermi") and INFN, has a dual purpose: a scientific research program on cosmic rays at ground level and an intense outreach and educational program. The project consists in a network of about 60 tracking detectors, called telescopes, mostly hosted in Italian High Schools. [...]
arXiv:2408.01802.- 2024-11-11 - 12 p. - Published in : JINST 19 (2024) P11003 Fulltext: 2408.01802 - PDF; document - PDF;
10.
Properties of Cosmic Deuterons Measured by the Alpha Magnetic Spectrometer / AMS Collaboration
Precision measurements by the Alpha Magnetic Spectrometer (AMS) on the International Space Station of the deuteron (D) flux are presented. The measurements are based on 21×106 D nuclei in the rigidity range from 1.9 to 21 GV collected from May 2011 to April 2021. [...]
2024 - 8 p. - Published in : Phys. Rev. Lett. 132 (2024) 261001 Fulltext: PDF;

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