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Prompt atmospheric neutrinos in the quark-gluon string model
High Energy Physics - Phenomenology · Submitted 29 Dec 2018
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim A new estimate of the prompt atmospheric neutrino flux is obtained and compared with the limit of the IceCube experiment as well as with predictions of other charm production models.
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The abstract, sentence by sentence
We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles at energies beyond 1 TeV. Cross sections of the $D$-mesons and ${\Lambda}^{+}_{c}$ baryons production in pA and $\pi$A collisions are calculated in the phenomenological quark-gluon string model (QGSM) which is updated using of the recent measurements of cross sections of the charmed meson production in the LHC experiments. A new estimate of the prompt atmospheric neutrino flux is obtained and compared with the limit of the IceCube experiment as well as with predictions of other charm production models.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles at energies beyond 1 TeV. | contribution 0.98 | 0.95 | 0.19 | asserted 1.00 |
| s1 | Cross sections of the $D$-mesons and ${\Lambda}^{+}_{c}$ baryons production in pA and $\pi$A collisions are calculated in the phenomenological quark-gluon string model (QGSM) which is updated using of the recent measurements of cross sections of the charmed meson production in the LHC experiments. | method 0.98 | 0.93 | 0.04 | asserted 1.00 |
| s2 | A new estimate of the prompt atmospheric neutrino flux is obtained and compared with the limit of the IceCube experiment as well as with predictions of other charm production models. | result 0.93 | 0.93 | 0.57 | asserted 0.99 |
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The paper
Original abstract
We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles at energies beyond 1 TeV. Cross sections of the $D$-mesons and ${\Lambda}^{+}_{c}$ baryons production in pA and $\pi$A collisions are calculated in the phenomenological quark-gluon string model (QGSM) which is updated using of the recent measurements of cross sections of the charmed meson production in the LHC experiments. A new estimate of the prompt atmospheric neutrino flux is obtained and compared with the limit of the IceCube experiment as well as with predictions of other charm production models.
Human review
How the literature uses it
1 arXiv paper cite this in 8 sentences
Papers citing it · 3 sentences without a confident label
Uses its method or tool 1 paper
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The PN fluxes were calculated using all listed charm production models, but only three of them, QGSM [ref] , SIBYLL 2.3c [ref] , and BEJKRSS [ref] , are presented in Tables [ref]–[ref].
High-energy spectra of the atmospheric neutrinos: predictions and measurements · Results and discussion · 0.87
Uses its data or values 1 paper
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Here, we use the results of the prompt muon neutrino flux calculations at 1 TeV – 100 PeV performed with the updated QGSM [ref] .
High-energy spectra of the atmospheric neutrinos: predictions and measurements · Charm production models · 0.89
Compares with it 1 paper
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The “crossing energies” derived with QGSM [ref] , PROSA [ref] and GM-VFNS [ref] are almost coincident for KM (close to that for SIBYLL 2.3c [ref] ) and QGSJET-II-03 [ref] taken separately.
High-energy spectra of the atmospheric neutrinos: predictions and measurements · Results and discussion · 0.81
Cites it as background 1 paper
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Calculations of the PN flux are most uncertain due to wide spread predictions of the charm production models (see for example [ref] ).
High-energy spectra of the atmospheric neutrinos: predictions and measurements · Spectra of atmospheric neutrinos · 0.82
What it cites · 22 sentences without a confident label
Uses the method or tool of 3 papers
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The calculation is based on the hadronic cascade model [ref] and cross sections of $D$ meson and $Λ^+_c$ baryon production in $pA$- and $πA$-collisions which are computed with the updated QGSM.
Kaon Decay Form Factors and Atmospheric Neutrino Flavor Ratio at High Energies · Introduction · 0.99
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In the present work, the calculation of prompt neutrino fluxes is performed with the method [ref] for QGSM for parameterization of cosmic ray spectrum by Nikolsky, Stamenov, Ushev (NSU) [ref] , the toy model by Thunman, Ingelman, Gondolo (TIG) [ref] , and the recent model for cosmic ray spectrum by Hillas and Gaisser (H3a) [ref] .
Spectrum of cosmic-ray nucleons and the atmospheric muon charge ratio · Energy spectra of the prompt atmospheric neutrinos · 0.93
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In the present work, the calculation of prompt neutrino fluxes is performed with the method [ref] for QGSM for parameterization of cosmic ray spectrum by Nikolsky, Stamenov, Ushev (NSU) [ref] , the toy model by Thunman, Ingelman, Gondolo (TIG) [ref] , and the recent model for cosmic ray spectrum by Hillas and Gaisser (H3a) [ref] .
Charm Production and High Energy Atmospheric Muon and Neutrino Fluxes · Energy spectra of the prompt atmospheric neutrinos · 0.93
Uses data or values from 5 papers
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For the $D$ and $Λ^+_c$ particles, we use the values from Refs. [ref] : $a^D=7.0·10^-4$, $a_0^Λ̅_c=7·10^-4$, $a^Λ_c_1=0.12$ (for $α_ψ(0)=-2.2$) and $a^Λ_c_1=0.02$ (for $α_ψ(0)=0$).
Charmed sea contribution to the inclusive hadroproduction of the mesons with open charm in the Quark -- Gluon String Model · Production of charmed particles in QGSM · 0.99
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The recent data on the cross sections of charmed particle production, obtained in experiments at the LHC [ref] , allow the QGSM free parameters updating.
Measurement of $D^{*\pm}$, $D^\pm$ and $D_s^\pm$ meson production cross sections in $pp$ collisions at $\sqrt{s}=7$ TeV with the ATLAS detector · Introduction · 0.87
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The recent data on the cross sections of charmed particle production, obtained in experiments at the LHC [ref] , allow the QGSM free parameters updating.
D-meson production in p-Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV and in pp collisions at $\sqrt{s}=7$ TeV · Introduction · 0.87
Compares with 9 papers
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We compare our result with the constraint obtained in the IceCube experiment [ref] as well as with predictions of the color dipole model (ERS) [ref] , SIBYLL 2.3c [ref] , the NLO pQCD models, BEJKRSS [ref] and GRRST [ref] .
The hadronic interaction model Sibyll-2.3c and inclusive lepton fluxes · Introduction · 1.00
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We compare our result with the constraint obtained in the IceCube experiment [ref] as well as with predictions of the color dipole model (ERS) [ref] , SIBYLL 2.3c [ref] , the NLO pQCD models, BEJKRSS [ref] and GRRST [ref] .
Prompt neutrino fluxes from atmospheric charm · Introduction · 1.00
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We compare our result with the constraint obtained in the IceCube experiment [ref] as well as with predictions of the color dipole model (ERS) [ref] , SIBYLL 2.3c [ref] , the NLO pQCD models, BEJKRSS [ref] and GRRST [ref] .
Prompt atmospheric neutrino fluxes: perturbative QCD models and nuclear effects · Introduction · 1.00
Cites as background 6 papers
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At present time the operating neutrino telescopes focus on the detection of astrophysical high-energy neutrino fluxes: IceCube, a cubic kilometer detector at the South Pole [ref] , ANTARES [ref] located in the Mediterranean Sea, and underwater Baikal Gigaton Volume Detector (Baikal-GVD), a cubic kilometer-scale array, which is currently under construction in lake Baikal [ref] .
Measurement of the atmospheric $\nu_\mu$ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope · Introduction · 1.00
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At present time the operating neutrino telescopes focus on the detection of astrophysical high-energy neutrino fluxes: IceCube, a cubic kilometer detector at the South Pole [ref] , ANTARES [ref] located in the Mediterranean Sea, and underwater Baikal Gigaton Volume Detector (Baikal-GVD), a cubic kilometer-scale array, which is currently under construction in lake Baikal [ref] .
The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part II: Properties of the Atmospheric and Astrophysical Neutrino Flux · Introduction · 1.00
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At present time the operating neutrino telescopes focus on the detection of astrophysical high-energy neutrino fluxes: IceCube, a cubic kilometer detector at the South Pole [ref] , ANTARES [ref] located in the Mediterranean Sea, and underwater Baikal Gigaton Volume Detector (Baikal-GVD), a cubic kilometer-scale array, which is currently under construction in lake Baikal [ref] .
All-flavor search for a diffuse flux of cosmic neutrinos with 9 years of ANTARES data · Introduction · 1.00
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