2025-08-12 08:56 |
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2025-08-12 08:56 |
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2025-08-12 08:56 |
Convergence of the ppp correlation function within the hyperspherical adiabatic basis
/ Garrido, E (Madrid, Inst. Estructura Materia) ; Kievsky, A (INFN, Pisa) ; Del Grande, R (Prague, Tech. U.) ; Serksnyte, L (CERN) ; Viviani, M (INFN, Pisa) ; Marcucci, L E (INFN, Pisa ; Pisa U.)
The computation of the three-particle correlation function involving three hadrons started just recently after the first publications of ALICE measurements. Key elements to be considered are the correct description of the asymptotics, antisymmetrization issues and, in most cases, the treatment of the Coulomb interaction. [...]
arXiv:2505.22190.-
2025 - 6 p.
- Published in : Phys. Lett. B 868 (2025) 139731
Fulltext: 2505.22190 - PDF; publication - PDF;
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2025-08-12 08:56 |
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2025-08-12 08:56 |
A hadronic calorimeter based on resistive micropattern gaseous detectors
/ Generoso, Lisa (INFN, Bari) ; Alviggi, Maria Grazia (INFN, Naples) ; Bianco, Michele (CERN) ; Borysova, Maryna (Weizmann Inst.) ; Biglietti, Michela (Rome III U.) ; Buonsante, Marco (INFN, Bari) ; Camerlingo, Maria Teresa (INFN, Bari) ; Colaleo, Anna (INFN, Bari) ; Della Pietra, Massimo (INFN, Naples) ; Di Nardo, Roberto (Rome III U.) et al.
Experiments at future Higgs factories will require excellent energy resolution to discriminate hadronic decays of W/Z and H bosons effectively. To meet this target, calorimeters must feature fine-granularity readouts, essential for implementing the Particle Flow Algorithm (PFA). [...]
2025 - 4 p.
- Published in : Nucl. Instrum. Methods Phys. Res., A 1080 (2025) 170741
In : 17th Vienna Conference on Instrumentation (VCI2025), Vienna, Austria, 17 - 21 Feb 2025, pp.170741
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2025-08-12 08:56 |
Empowering a broad and diverse community in beam dynamics simulations with Xsuite
/ Łopaciuk, Szymon (CERN) ; De Maria, Riccardo (CERN) ; Iadarola, Giovanni (CERN) ; Van der Veken, Frederik Florentinus (CERN)
Xsuite is a Python toolkit for modelling and simulation of particle accelerators, which has been developed at CERN together with collaborators from other institutes over the past four years. The code has reached a mature development stage and has become the workhorse for several studies and applications, allowing the gradual replacement of legacy tools like Sixtrack, COMBI, PyHEADTAIL. [...]
2025 - 4 p.
- Published in : JACoW IPAC 25 (2025) 1667-1669
Fulltext: PDF;
In : International Particle Accelerator Conference (IPAC'25), Taipei, Taiwan, 1-6 June 2025, pp.1667-1669
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2025-08-12 08:55 |
The vertexing challenge at FCC-ee
/ Ilg, Armin (U. Zurich (main)) ; Macchiolo, Anna (U. Zurich (main)) ; Palla, Fabrizio (INFN, Pisa)
/FCC Collaboration
Following in the footsteps of the LHC, the Future Circular Collider (FCC) plans to be the next multi-generational collider project. In the first stage, FCC-ee will collide intense beams of electrons and positrons at centre of mass energies between 88 and 365 GeV, making it an electroweak, flavour, Higgs and top factory. [...]
arXiv:2502.04071.-
2025 - 7 p.
- Published in : JINST
Fulltext: 2502.04071 - PDF; document - PDF;
In : 11th International Workshop on Semiconductor Pixel Detectors for Particles and Imaging (PIXEL 2024), Strasbourg, France, 18 - 22 Nov 2024, pp.C06069
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2025-08-12 08:55 |
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2025-08-12 08:55 |
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
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2025-08-12 08:55 |
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