Reaction 1 - 45

Baldini, A.; Flaminio, V.; Moorhead, W. G.; Morrison, David R.

doi:10.1007/10367917_18

Cited by 3 publications

(3 citation statements)

References 19 publications

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“…1.1 Figure 4: Total cross section of the reaction γ * p → X for ε ≥ 0.9 and different Q 2 . For Q 2 = 0 the data are from [42] (squares) and [43] (triangles). For finite Q 2 the data are from [22].…”

Section: Discussionmentioning

confidence: 99%

Electron and photon induced reactions on nuclei in the nucleon resonance region

2000

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We calculate total photon-nucleus and electron-nucleus cross sections γA → X, eA → e ′ X and several cross sections on pion and eta production in nuclei in the energy regime between the first and the third resonance region for photon virtualities Q 2 ≤ 1.0 GeV 2 within a semi-classical BUU transport model. In both cases we discuss the varying influence of several medium modifications on the cross sections for different values of Q 2 .

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Section: Discussionmentioning

confidence: 99%

Electron and photon induced reactions on nuclei in the nucleon resonance region

2000

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“…This result is confirmed by the experimental data from [53] (see also [74]) where a larger cross section for dn → d(pπ − ) than for pn → p(pπ − ) was measured (see table 2 and fig. 6 in [53], see also [57]).…”

Section: Appendix: Inelasticity In Composite Particle Scatteringmentioning

confidence: 99%

Flux of light antimatter nuclei near Earth, induced by cosmic rays in the Galaxy and in the atmosphere

et al. 2005

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The fluxes of light antinuclei A<=4 induced near earth by Cosmic Ray intera ctions with the interstellar matter in the Galaxy and with the Earth atmosphere, are calculated in a phenomenological framework. The hadronic production cross section for antinucleons is based on a recent parametrization of a wide set of accelerator data. The production of light nuclei is calculated using coalescence models. For the standard coalescence model, the coalescence radius is fitted to the available experimental data. The non annihilating inelastic scattering process for the antideuterons is discussed and taken into account for the first time via a more realistic procedure than used so far for antiprotons

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“…• Antinucleons: The p total reaction cross section was taken from [51], with the energy dependence from the data compilation of [52]. The same production cross section and total reaction cross section have been assumed for n production as for p .…”

Section: Total Reaction Cross Sectionsmentioning

confidence: 99%

Secondary antiproton flux induced by cosmic ray interactions with the atmosphere

2003

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The atmospheric secondary antiproton flux is studied for detection altitudes extending from sea level up to about 3 earth radii, by means of a 3-dimensional Monte-Carlo simulation, successfully applied previously on other satellite and balloon data. The calculated antiproton flux at mountain altitude is found in fair agreement with the recent BESS measurements. The flux obtained at balloon altitude is also in agreement with calculations performed in previous studies and used for the analysis of balloon data. The flux at sea level is found to be significant. The antineutron flux is also evaluated. The antiproton flux is prospectively explored up to around 2 10 4 km. The results are discussed in the context of the forthcoming measurements by large acceptance experiments.

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Reaction 1 - 45

Cited by 3 publications

References 19 publications

Electron and photon induced reactions on nuclei in the nucleon resonance region

Electron and photon induced reactions on nuclei in the nucleon resonance region

Flux of light antimatter nuclei near Earth, induced by cosmic rays in the Galaxy and in the atmosphere

Secondary antiproton flux induced by cosmic ray interactions with the atmosphere

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