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Athanassopoulos, C.; Auerbach, L.; Burman, R. L.; Cohen, I.; Caldwell, D. O.; Dieterle, B.; Donahue, J. B.; Eisner, A. M.; Fazely, A. R.; Federspiel, F.J.; Garvey, G. T.; Gray, Mark Girard; Gunasingha, R. M.; Imlay, R.; Johnston, K.; Kim, H. J.; Louis, W. C.; Majkic, R.; Margulies, J.; McIlhany, K.; Metcalf, W.; Mills, G. B.; Reeder, R. A.; Sandberg, V. D.; Smith, D.; Stancu, I.; Strossman, W.; Tayloe, R.; VanDalen, G.; Vernon, W.; Wadia, N.; Waltz, James P.; Wang, Y. X.; White, D. H.; Works, D.; Xiao, Y. J.; Yellin, S.

doi:10.1103/physrevc.55.2078

Cited by 89 publications

(79 citation statements)

References 27 publications

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“…One of the most extensively studied neutrino-nucleus reactions is 12 C(ν e , e − ) 12 N. This reaction is particularly important because 12 C is used in liquid scintillator detectors, and data on the cross section are available from the LSND [5,6], and KARMEN [7,8,9] collaborations, as well as from LAMPF [10,11]. In order to illustrate the contributions of different multipole excitations, in Fig.…”

Section: Illustrative Calculations: Cross Sections For Neutrino Dmentioning

confidence: 99%

“…Data on neutrino-nucleus cross sections have been obtained by the LSND [5,6] and KARMEN [7,8,9] collaborations, and at LAMPF [10,11], but only for 12 C and 56 Fe target nuclei. New experimental programs are being planned which will provide essential data on the neutrino-nucleus reactions, and also help to improve the reliability of present cross-section calculations.…”

Section: Introductionmentioning

confidence: 99%

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Inclusive charged-current neutrino-nucleus reactions calculated with the relativistic quasiparticle random-phase approximation

et al. 2008

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Section: Illustrative Calculations: Cross Sections For Neutrino Dmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

Inclusive charged-current neutrino-nucleus reactions calculated with the relativistic quasiparticle random-phase approximation

et al. 2008

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“…12 C(ν e , e − ) 12 N and 12 C(ν, ν ′ ) 12 C * have also been performed at KARMEN [19], at LAMPF [20], and by LSND [21]. Table 2 compares the theoretical predictions to the measured data.…”

Section: Measurements Of Cross Sections Formentioning

confidence: 97%

Supernova neutrino detection in Borexino

Cadonati

Calaprice

Chen

2002

Astroparticle Physics

102

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We calculated the expected neutrino signal in Borexino from a typical Type II supernova at a distance of 10 kpc. A burst of around 110 events would appear in Borexino within a time interval of about 10 s. Most of these events would come from the reaction channelν e + p → e + + n, while about 30 events would be induced by the interaction of the supernova neutrino flux on 12 C in the liquid scintillator. Borexino can clearly distinguish between the neutral-current excitations 12 C(ν, ν ′ ) 12 C * (15.11 MeV) and the charged-current reactions 12 C(ν e , e − ) 12 N and 12 C(ν e , e + ) 12 B, via their distinctive event signatures. The ratio of the chargedcurrent to neutral-current neutrino event rates and their time profiles with respect to each other can provide a handle on supernova and non-standard neutrino physics (mass and flavor oscillations).

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“…Therefore this background was about half of the µ − DAR background, although with a poorly known energy spectrum. Note that the π + DIF background is at least five times larger as the π + /π − ratio at LSND is about 8 and 3.4% (5%) of π + (π − ) decay in flight [17], but the resulting ν µ only produce neutrons in those interactions with 12 C that lead to particular final state interactions. In ref.…”

Section: Jhep01(2016)004mentioning

confidence: 99%

Neutrino physics with accelerator driven subcritical reactors

Ciuffoli

Evslin

Zhao

2016

J. High Energ. Phys.

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Accelerator driven system (ADS) subcritical nuclear reactors are under development around the world. They will be intense sources of free, 30-55 MeV µ + decay at rest ν µ . These ADS reactor neutrinos can provide a robust test of the LSND anomaly and a precise measurement of the leptonic CP-violating phase δ, including sign(cos(δ)). The first phase of many ADS programs includes the construction of a low energy, high intensity proton or deuteron accelerator, which can yield competitive bounds on sterile neutrinos.

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Measurements of the reactions12C(νe,e−

Cited by 89 publications

References 27 publications

Inclusive charged-current neutrino-nucleus reactions calculated with the relativistic quasiparticle random-phase approximation

Inclusive charged-current neutrino-nucleus reactions calculated with the relativistic quasiparticle random-phase approximation

Supernova neutrino detection in Borexino

Neutrino physics with accelerator driven subcritical reactors

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