NSR Query Results


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NSR database version of May 10, 2024.

Search: Author = T.Stanev

Found 6 matches.

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2006GA51      Nucl.Phys. A777, 98 (2006)

T.K.Gaisser, T.Stanev

High-energy cosmic rays

doi: 10.1016/j.nuclphysa.2005.01.024
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2000BL17      Phys.Rev. D62, 077501 (2000)

M.M.Block, F.Halzen, T.Stanev

Extending the Frontiers: Reconciling accelerator and cosmic ray p-p cross sections

NUCLEAR REACTIONS 1H(p, X), E(cm) < 30 TeV; analyzed total σ; deduced parameters. Accelerator and cosmic ray data considered.

doi: 10.1103/PhysRevD.62.077501
Citations: PlumX Metrics


2000EN01      Phys.Lett. 472B, 113 (2000)

R.Engel, T.K.Gaisser, T.Stanev

Pion Production in Proton Collisions with Light Nuclei: Implications for Atmospheric Neutrinos

NUCLEAR REACTIONS Be(p, π+X), (p, π-X), E ≈ 20 GeV; C(p, π-X), E=4.2, 10 GeV; analyzed pion production spectra; deduced implications for neutrino oscillation measurements.

doi: 10.1016/S0370-2693(99)01418-5
Citations: PlumX Metrics


1999BL21      Phys.Rev.Lett. 83, 4926 (1999)

M.M.Block, F.Halzen, T.Stanev

Predicting Proton-Air Cross Sections at √ s ∼ 30 TeV using Accelerator and Cosmic Ray Data

NUCLEAR REACTIONS 1H(p, X), (p-bar, X), E(cm) ≈ 2-2000 GeV; analyzed σ; deduced high-energy proton-air cross sections for cosmic ray measurements.

doi: 10.1103/PhysRevLett.83.4926
Citations: PlumX Metrics


1998EN07      Phys.Rev. D58, 014019 (1998)

R.Engel, T.K.Gaisser, P.Lipari, T.Stanev

Proton-Proton Cross Section at √ s ∼ 30 TeV

NUCLEAR REACTIONS 1H(p, X), E(cm) ≈ 30 TeV; analyzed air-shower cosmic-ray data; deduced σ constraints features. Extrapolation from accelerator data discussed.

doi: 10.1103/PhysRevD.58.014019
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1997FR24      Phys.Rev. D56, 3135 (1997)

G.M.Frichter, T.K.Gaisser, T.Stanev

Inelasticity in p-Nucleus Collisions and Its Application to High Energy Cosmic-Ray Cascades

NUCLEAR REACTIONS 1H, Be, C, 27Al, Cu, Ag, W, Pb, U(p, p'X), E=high; analyzed σ vs transverse momentum; deduced stopping power related features. Implications for high-energy cosmic ray studies discussed.

doi: 10.1103/PhysRevD.56.3135
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