CERN Accelerating science

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1.
Dark fluxes from electromagnetic cascades / Blinov, Nikita (Victoria U. ; York U., Canada) ; Fox, Patrick J. (Fermilab) ; Kelly, Kevin J. (CERN ; Texas A-M) ; Machado, Pedro A.N. (Fermilab) ; Plestid, Ryan (Caltech)
We study dark sector production in electromagnetic (EM) cascades. This problem requires accurate simulations of Standard Model (SM) and dark sector processes, both of which impact angular and energy distributions of emitted particles that ultimately determine flux predictions in a downstream detector. [...]
arXiv:2401.06843; CALT-TH/2024-001; FERMILAB-PUB-24-0003-T; CERN-TH-2024-006; MI-HET-825.- 2024-07-03 - 35 p. - Published in : JHEP 2407 (2024) 022 Fulltext: f1fd16bf02fd37d8be6bc96add7b369a - PDF; 2401.06843 - PDF; Fulltext from Publisher: PDF; External links: GitHub; Fermilab Library Server
2.
Physics Opportunities at a Beam Dump Facility at PIP-II at Fermilab and Beyond / Aguilar-Arevalo, A.A. (Mexico U., ICN) ; Barrow, J.L. (Minnesota U.) ; Bhat, C. (Fermilab) ; Bogenschuetz, J. (Texas U., Arlington) ; Bonifazi, C. (ICAS, UNSAM, Buenos Aires ; Rio de Janeiro Federal U.) ; Bross, A. (Fermilab) ; Cervantes, B. (Mexico U., ICN) ; D'Olivo, J. (Mexico U., ICN) ; De Roeck, A. (CERN) ; Dutta, B. (Texas A-M) et al.
The Fermilab Proton-Improvement-Plan-II (PIP-II) is being implemented in order to support the precision neutrino oscillation measurements at the Deep Underground Neutrino Experiment, the U.S. [...]
arXiv:2311.09915 ; FERMILAB-FN-1242-AD-ND-PPD.
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Fermilab Library Server - Fulltext - Fulltext
3.
Broad Sterile Neutrinos & the Reactor/Gallium Tension / Banks, Hannah (Cambridge U., DAMTP ; CERN) ; Kelly, Kevin J. (Texas A-M) ; McCullough, Matthew (CERN) ; Zhou, Tao (Texas A-M)
Significant evidence exists for the apparent disappearance of electron-type neutrinos in radioactive source experiments. Yet, interpreted within the standard `3+1 sterile neutrino scenario', precision short-baseline measurements of electron antineutrinos from nuclear reactors strongly disagree with these results. [...]
arXiv:2311.06352; CERN-TH-2023-195; MI-HET-818.- 2024-04-17 - 8 p. - Published in : JHEP 2404 (2024) 096 Fulltext: document - PDF; 2311.06352 - PDF;
4.
BSM Physics Opportunities with LHC Neutrino Beams / Kelly, Kevin James (speaker) (Texas A&M University)
2023 - 15156. Conferences, Workshops & Schools; Forward Physics Facility Theory Workshop External links: Talk details; Event details In : Forward Physics Facility Theory Workshop
5.
Keeping it Simple: Simplified Frameworks for Long-Lived Particles at Neutrino Facilities / Batell, Brian (Pittsburgh U.) ; Huang, Wenjie (Pittsburgh U.) ; Kelly, Kevin J. (CERN ; TAMU, College Station)
Modern-day accelerator neutrino facilities are excellent venues for searches for new-physics particles. Many distinct new-physics models predict overlapping signatures and phenomenology in these experiments. [...]
arXiv:2304.11189.- 2023-08-17 - 23 p. - Published in : JHEP 2308 (2023) 092 Fulltext: 2304.11189 - PDF; document - PDF;
6.
There and back again: Solar cycle effects in future measurements of low-energy atmospheric neutrinos / Kelly, Kevin J. (CERN ; Texas A-M) ; Machado, Pedro A.N. (Fermilab) ; Mishra, Nityasa (Texas A-M) ; Strigari, Louis E. (Texas A-M) ; Zhuang, Yi (Texas A-M)
We study the impact of time-dependent solar cycles in the atmospheric neutrino rate at DUNE and Hyper-Kamiokande (HK), focusing in particular on the flux below 1 GeV. Including the effect of neutrino oscillations for the upward-going component that travels through the Earth, we find that across the solar cycle the amplitude of time variation is about $\pm5\%$ at DUNE, and $\pm 1\%$ at HK. [...]
arXiv:2304.04689; FERMILAB-PUB-23-143-T; CERN-TH-2023-056; MI-HEE-800.- 2023-12-13 - 6 p. - Published in : Phys. Rev. D
- Published in : Phys. Rev. D Fulltext: b46edf2ae642528252558acec376c35b - PDF; 2304.04689 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
7.
Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino Experiment / DUNE Collaboration
A primary goal of the upcoming Deep Underground Neutrino Experiment (DUNE) is to measure the $\mathcal{O}(10)$ MeV neutrinos produced by a Galactic core-collapse supernova if one should occur during the lifetime of the experiment. The liquid-argon-based detectors planned for DUNE are expected to be uniquely sensitive to the $\nu_e$ component of the supernova flux, enabling a wide variety of physics and astrophysics measurements. [...]
arXiv:2303.17007; FERMILAB-PUB-23-132-CSAID-LBNF-ND-T.- 2023-06-01 - 25 p. - Published in : Phys. Rev. D 107 (2023) 112012 Fulltext: FERMILAB-PUB-23-132-CSAID-LBNF-ND-T - PDF; 2303.17007 - PDF; Publication - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
8.
Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector / DUNE Collaboration
Measurements of electrons from $\nu_e$ interactions are crucial for the Deep Underground Neutrino Experiment (DUNE) neutrino oscillation program, as well as searches for physics beyond the standard model, supernova neutrino detection, and solar neutrino measurements. This article describes the selection and reconstruction of low-energy (Michel) electrons in the ProtoDUNE-SP detector. [...]
arXiv:2211.01166; FERMILAB-PUB-22-784; CERN-EP-DRAFT-MISC-2022-008.- 2023-05-01 - 19 p. - Published in : Phys. Rev. D 107 (2023) 092012 Fulltext: 2211.01166 - PDF; FERMILAB-PUB-22-784 - PDF; FERMILAB-PUB-22-784 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
9.
More Ingredients for an Altarelli Cocktail at MiniBooNE / Kelly, Kevin J. (CERN ; Texas A-M) ; Kopp, Joachim (CERN ; Mainz U., Inst. Phys. ; U. Mainz, PRISMA)
The MiniBooNE excess persists as a significant puzzle in particle physics. Given that the MiniBooNE detector cannot discriminate between electron-like signals and backgrounds due to photons, the goal of this work is to study photon backgrounds in MiniBooNE in depth. [...]
arXiv:2210.08021; CERN-TH-2022-151.- 2023-05-15 - 29 p. - Published in : JHEP 2305 (2023) 113 Fulltext: 2210.08021 - PDF; document - PDF;
10.
How Broad is a Neutrino? / Banks, Hannah (Cambridge U., DAMTP ; CERN) ; Kelly, Kevin J. (CERN ; Texas A-M) ; McCullough, Matthew (CERN)
Canonical neutrino oscillations arise due to the propagation of three mass eigenstates from production to detection. We aspire to capture, in one simple framework, a broad range of new physics effects on neutrino propagation beyond this canonical picture - this can be done by promoting the neutrino propagators to the general Källén-Lehmann form. [...]
arXiv:2209.11270; CERN-TH-2022-152.- 2023-02-14 - 27 p. - Published in : JHEP 02 (2023) 136 Fulltext: document - PDF; 2209.11270 - PDF;

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