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2024-01-09 04:11 |
Femtoscopy analysis in small systems at NA61/SHINE
/ Porfy, Barnabas (Eotvos U., Dept. Atomic Phys. ; Wigner RCP, Budapest)
/NA61/SHINE Collaboration
Recent measurements of femtoscopic correlations at NA61/SHINE unravel that the shape of the particle emitting source is not Gaussian. The measurements are based on Lévy-stable symmetric sources, and we discuss the average pair transverse mass dependence of the source parameters. [...]
arXiv:2401.02553.-
2024 - 4 p.
- Published in : EPJ Web Conf.: 296 (2024) , pp. 06004
Fulltext: 2401.02553 - PDF; document - PDF;
In : 30th Conference on Ultra-Relativistic Nucleus-Nucleus Collisions (Quark Matter 2023), Houston, Texas, United States of America, 3 - 9 Sep 2023, pp.06004
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2023-10-12 07:34 |
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2023-10-07 06:44 |
NA61/SHINE online noise filtering using machine learning methods
/ Kawęcka, Anna (Warsaw U. of Tech. (main) ; Chalmers U. Tech.) ; Bryliński, Wojciech (Warsaw U. of Tech. (main)) ; Omana Kuttan, Manjunath (Frankfurt U., FIAS ; Frankfurt U.) ; Linnyk, Olena (Frankfurt U., FIAS ; Giessen U.) ; Pawlowski, Janik (Frankfurt U., FIAS ; Philipps U. Marburg) ; Schmidt, Katarzyna (Silesia U.) ; Słodkowski, Marcin (Warsaw U. of Tech. (main)) ; Wyszyński, Oskar (Jan Kochanowski U., Kielce (main)) ; Zieliński, Jakub (Warsaw U. of Tech. (main))
The NA61/SHINE is a high-energy physics experiment operating at the SPS accelerator at CERN. The physics program of the experiment was recently extended, requiring a significant upgrade of the detector setup. [...]
2023 - 5 p.
- Published in : J. Phys. : Conf. Ser. 2438 (2023) 012104
Fulltext: PDF;
In : 20th International Workshop on Advanced Computing and Analysis Techniques in Physics Research (ACAT 2021), Daejeon, Korea, 29 Nov - 3 Dec 2021, pp.012104
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2023-08-23 06:25 |
Pilot Study on the Measurement of the Production of Boron Isotopes in C+p Reactions at 13.5A GeV/c with NA61/SHINE
/ Amin, Neeraj (KIT, Karlsruhe, IAP)
/NA61/SHINE Collaboration
The current understanding of cosmic-ray propagation in the Galaxy is significantly hindered by the inadequate knowledge of nuclear fragmentation cross-sections, while the other key component, the secondary cosmic-ray fluxes are measured with high precision by space-based detectors. This situation can be redressed by utilizing NA61/SHINE, a fixed-target experimental facility at CERN. [...]
2023 - 10 p.
- Published in : PoS ICRC2023 (2023) 075
Fulltext: PDF;
In : 38th International Cosmic Ray Conference (ICRC 2023), Nagoya, Japan, 26 Jul - 3 Aug 2023, pp.075
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