2026-05-06 06:06 |
FCC― 次世代円形衝突型加速器
/ OIDE, Katsunobu (CERN ; U. Geneva (main) ; KEK, Tsukuba)
FCC is a project for a next generation circular collider based at CERN, as the next step of LEP/LHC experiments.
It will have at least two stages : (i) measurements on electroweak (Z/W), Higgs, tt by e+e- collision (FCC-ee) and (ii)
energy frontier pp collision (FCC-hh) up to 100 TeV center of mass (CM) energy. Both will be performed by colliders
in the same tunnel with 90–100 km circumference built around the Geneva area across the Swiss-French border..
2022 - 4 p.
- Published in : Vacuum and Surface Science 65 (2022) 556-559
Fulltext: PDF;
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2026-05-06 06:06 |
The DREAMS Project: Disentangling the Impact of Halo-to-halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles
/ Garcia, Alex M (Virginia U. (main) ; Harvard U. (main) ; IAIFI, Cambridge) ; Rose, Jonah C (Princeton U. (main) ; New York U., CCPP) ; Torrey, Paul (Virginia U. (main) ; Harvard U. (main) ; IAIFI, Cambridge) ; Caputo, Andrea (CERN ; U. Rome La Sapienza (main) ; Weizmann Inst.) ; Lisanti, Mariangela (Princeton U. (main) ; New York U., CCPP) ; Pace, Andrew B (Virginia U. (main)) ; Liu, Hongwan (Boston U. (main)) ; Hussein, Abdelaziz (MIT, MKI) ; Liu, Haozhe (Virginia U. (main)) ; Villaescusa-Navarro, Francisco (New York U., CCPP) et al.
In this work, we utilize a new suite of Milky Way-mass halos from the DREAMS Project, simulated with Cold Dark Matter (CDM), to quantify the influence of baryon feedback and intrinsic halo-to-halo variance on dark matter density profiles. Our suite of 1024 halos varies over supernova and black hole feedback parameters from the IllustrisTNG model, as well as variations in two cosmological parameters. [...]
arXiv:2512.03132.-
2026 - 19 p.
- Published in : Astrophys. J. 1002 (2026) 8
Fulltext: 2512.03132 - PDF; document - PDF;
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2026-05-06 06:06 |
IV.2 - The history of JUAS, 1994–2024
/ Rey-Champagnolle, Marcelle (CERN) ; Méot, Françoit (Brookhaven Natl. Lab.) ; Rinolfi, Louis (ESI, Archamps) ; Jowett, John M (CERN ; Darmstadt, GSI) ; Holland, Bob ; Métral, Elias (CERN) ; Lebrun, Philippe (ESI, Archamps) ; Le Duff, Joël
The first official JUAS school was held in 1994: this chapter gives a brief history of the school overthe 30 years..
2024 - 27 p.
- Published in : CERN Yellow Rep. School Proc. 4 (2024) 2211
Fulltext: PDF; External link: Fulltext
In : Proceedings of the Joint Universities Accelerator School (JUAS): courses and exercises, Geneva, Switzerland, 27 Nov 2024, pp.2211 (CERN-2024-003)
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2026-05-06 06:06 |
Ultraviolet cross-luminescence in ternary chlorides of alkali and alkaline-earth metals
/ Vanecek, Vojtech (Prague, Inst. Phys. ; Prague, Tech. U.) ; Paterek, Juraj (Prague, Inst. Phys. ; Prague, Tech. U.) ; Kral, Robert (Prague, Tech. U.) ; Kucerkova, Romana (Prague, Tech. U.) ; Babin, Vladimir (Prague, Inst. Phys.) ; Rohlicek, Jan (Prague, Inst. Phys.) ; Cala, Roberto (CERN ; Milan Bicocca U. (main)) ; Kratochwil, Nicolaus (CERN ; U. Vienna (main)) ; Auffray, Etiennette (CERN) ; Nikl, Martin (Prague, Inst. Phys.)
After the discovery of a cross-luminescence (CL) in BaF2 in 1982, a large number of CL scintillators were investigated. However, no CL scintillator superior to BaF2 has been discovered, and the research of CL scintillators has subsided. [...]
arXiv:2409.10823.-
2021 - 10 p.
- Published in : Opt. Mater. 10 (2021) 12
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2026-05-06 06:06 |
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2026-05-06 06:06 |
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2026-05-05 06:11 |
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2026-05-05 06:11 |
Analysis of High-Energy Heavy-Ion SEE Results Through Standard-Energy Ion SEE Data
/ Sacristan Barbero, Mario (IES, Montpellier ; CERN) ; Slipukhin, Ivan (IES, Montpellier ; CERN) ; Söderström, Daniel (CERN) ; Emriskova, Natalia (CERN) ; Waets, Andreas (CERN) ; Bilko, Kacper (CERN) ; Prelipcean, Daniel (Unlisted, DE) ; Coronetti, Andrea (CERN ; Unlisted, DE) ; Kettunen, Heikki (Jyvaskyla U.) ; Sivertz, Michael (Brookhaven) et al.
This work presents the results of several single-
event effect (SEE) measurements (bit upsets, latch-up, and
burn-out) performed in two SEE testing facilities, European
Organization for Nuclear Research (CERN) and NASA Space
Radiation Laboratory (NSRL) (100–1000 MeV/n), using high-
energy heavy ions. The results are compared with those obtained
at other SEE facilities using standard-energy ions, Radiation
Effects Facility (RADEF), UCL, and GANIL (<50 MeV/n). [...]
2026 - 11 p.
- Published in : IEEE Trans. Nucl. Sci. 73 (2026) 1032-1042
Fulltext: PDF; External link: Fulltext
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2026-05-05 06:11 |
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2026-05-05 06:10 |
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