Measurement of the νμN total cross section at 2–30 GeV in a skat neutrino experiment

Baranov, D.S.; Bugorsky, A.P.; Ivanilov, A.; Kochetkov, V.; Konyushko, V.I.; Korablev, V. M.; Коротков, В. А.; Kurbakov, V.I.; Kuznetsov, E.P.; Макеев, В. В.; Mjagkov, A.G.; Mukhin, A.I.; Nikitin, Yu. P.; Parshikura, S.N.; Polyarush, A. Yu.; Rjabov, Yu.G.; Самойлов, А. В.; Smirnov, Yu. I.; Sokolov, A.; Sviridov, Yu M.; Волков, А. А.; Volkov, G.G.

doi:10.1016/0370-2693(79)90536-7

Cited by 27 publications

(13 citation statements)

References 6 publications

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“…1c shows the spectrum of the beam neutrino evaluated using the total cross sections [7] of reactions νp → µ − X and νn → µ − X and taking into account the proton and neutron content of the target nuclei. As it is seen, the latter spectrum is consistent with the expected neutrino flux spectrum (at E ν > 1.5 GeV) on the bubble chamber SKAT [5].…”

Section: B) the Identification Of Exclusive Channelsupporting

confidence: 86%

“…2e. The curves in this figure are obtained by approximation of available experimental data for νp and νn interactions [4] (taking into account the proton and neutron contents of the target nuclei) convoluted with the expected neutrino flux spectrum on the bubble chamber SKAT [5]. The normalization of these curves is chosen to fit our data on the main exclusive channel (1).…”

Section: B) the Identification Of Exclusive Channelmentioning

confidence: 99%

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The characteristics of neutrino-nuclear reactions at E ν = 1–3 GeV

Agababyan

Ammosov²,

Atayan

et al. 2007

Phys. Atom. Nuclei

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For the first time, the characteristics of the charged current neutrinonuclear interactions are investigated at E ν = 1 -3 GeV using the data obtained with SKAT propane-freon bubble chamber irradiated in the neutrino beam at Serpukhov accelerator. The E ν -dependence of the mean multiplicities of different types of secondary particles and their multiplicity, momentum and angular distributions are measured.

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Section: B) the Identification Of Exclusive Channelsupporting

confidence: 86%

Section: B) the Identification Of Exclusive Channelmentioning

confidence: 99%

The characteristics of neutrino-nuclear reactions at E ν = 1–3 GeV

Agababyan

Ammosov²,

Atayan

et al. 2007

Phys. Atom. Nuclei

Self Cite

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“…The DIS term of the inelastic differential cross section is expressed in terms of the differential cross section predicted by the Bodek-Yang model appropriately modulated in the "resonancedominance" region W < W cut so that the RES/DIS mixture in this region agrees with inclusive cross section data [62,63,64,65,66,67,68,69,70,71] and exclusive 1-pion [72,73,74,75,76,77,78,79,80,69,81] and 2-pion [82,76] cross section data:…”

Section: Modeling the Transition Regionmentioning

confidence: 99%

“…Baryon 4-momentum distributions are determined from fits to experimental data [90,91]. The settings for PYTHIA parameters are taken as the non-default values tuned for the NUX [18] [62] (CCFRR), [63] (CDHSW), [64] (GGM-SPS), [65,66] (BEBC), [67] (ITEP), [68] (CRS, SKAT), [69] (ANL), [70] (BNL) and [71] (GGM-PS)…”

Section: Physics Model Tuningmentioning

confidence: 99%

The GENIE neutrino Monte Carlo generator

Andreopoulos

Bell

Bhattacharya

et al. 2010

Nuclear Instruments and Methods in Physics Research Section A:

955

939

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GENIE[1] is a new neutrino event generator for the experimental neutrino physics community. The goal of the project is to develop a 'canonical' neutrino interaction physics Monte Carlo whose validity extends to all nuclear targets and neutrino flavors from MeV to PeV energy scales. Currently, emphasis is on the few-GeV energy range, the challenging boundary between the non-perturbative and perturbative regimes, which is relevant for the current and near future long-baseline precision neutrino experiments using accelerator-made beams. The design of the package addresses many challenges unique to neutrino simulations and supports the full life-cycle of simulation and generator-related analysis tasks.GENIE is a large-scale software system, consisting of ∼120,000 lines of C++ code, featuring a modern object-oriented design and extensively validated physics content.

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“…1. Charged-current inclusive neutrino-nucleon cross section measurements [8][9][10][11][12][13][14][15][16][17][18][19][20][21][22][23][24][25]. The new results from this work, based on 6 years of IceCube HESE showers [26][27][28][29], are an average between cross sections for ν andν, assuming equal astrophysical fluxes of each.…”

mentioning

confidence: 99%

Extracting the Energy-Dependent Neutrino-Nucleon Cross Section above 10 TeV Using IceCube Showers

2019

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Neutrinos are key to probing the deep structure of matter and the high-energy Universe. Yet, until recently, their interactions had only been measured at laboratory energies up to about 350 GeV. An opportunity to measure their interactions at higher energies opened up with the detection of high-energy neutrinos in IceCube, partially of astrophysical origin. Scattering off matter inside the Earth affects the distribution of their arrival directions -from this, we extract the neutrino-nucleon cross section at energies from 18 TeV to 2 PeV, in four energy bins, in spite of uncertainties in the neutrino flux. Using six years of public IceCube High-Energy Starting Events, we explicitly show for the first time that the energy dependence of the cross section above 18 TeV agrees with the predicted softer-than-linear dependence, and reaffirm the absence of new physics that would make the cross section rise sharply, up to a center-of-mass energy √ s ≈ 1 TeV.

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Measurement of the νμN total cross section at 2–30 GeV in a skat neutrino experiment

Cited by 27 publications

References 6 publications

The characteristics of neutrino-nuclear reactions at E ν = 1–3 GeV

The characteristics of neutrino-nuclear reactions at E ν = 1–3 GeV

The GENIE neutrino Monte Carlo generator

Extracting the Energy-Dependent Neutrino-Nucleon Cross Section above 10 TeV Using IceCube Showers

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