Streamer chamber study of the cross sections and multiplicities in nucleus-nucleus interactions at the incident momentum of 4.5 GeV/c per nucleon

Aksinenko, V. D.; Anikina, M.; Buttsev, V.S.; Chkaidze, L.V.; Glagoleva, N.S.; Golokhvastov, A. I.; Grachov, O.; Gudima, K. K.; Dementjev, E. A.; Kadikova, S. V.; Kaminski, Noam; Khorozov, S.A.; Кузнецова, Е. С.; Lukstiņš, J.; Matyushin, A.T.; Matyushin, V.T.; Mescherjakov, M. G.; Musulmanbekov, G.; Nurgozhin, N. N.; Okonov, E.O.; Ostanevich, T.G.; Peisert, A.; Skrzypczak, E.; Szwed, R.; Shevchenko, E. A.; Sidorin, S. S.; Khusainov, E. K.; Тонеев, В.Д.; Vardenga, G.; Volodin, V.D.; Zakrzewski, J.; Zuravleva, M. S.

doi:10.1016/0375-9474(80)90269-9

Cited by 54 publications

(6 citation statements)

References 8 publications

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“…Figure 1 displays the inelastic cross section for combinations of hydrogen and carbon nuclei as function of the total energy per nucleon of the projectile, E CR . Also shown in the figure are literature values for the inelastic cross section (Aksinenko et al, 1980;Antchev et al, 2013;Terashima et al, 2014;Aaboud et al, 2016a,b;Tanabashi et al, 2018;Antchev et al, 2019) that are generally in good agreement with the simulated cross section. Other species combinations show a qualitatively similar behavior.…”

Section: The Inelastic Cross Sectionsupporting

confidence: 76%

Production of secondary particles in heavy nuclei interactions in supernova remnants

Bhatt,

Sushch,

Pohl

et al. 2020

Preprint

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Depending on their type, supernova remnants may have ejecta material with high abundance of heavy elements such as carbon or oxygen. In addition, core-collapse supernovae explode in the wind material of their progenitor star that may also have a high abundance of heavy elements. Hadronic collisions in these enriched media spawn the production of gamma rays, neutrinos, and secondary electrons with spectra that cannot be scaled from those calculated for pp collisions, potentially leading to erroneous results. We used Monte-Carlo event generators to calculate the differential production rate of secondary particles such as gamma rays, neutrinos, and secondary electrons for H, He, C, and O nuclei as projectiles and as target material. The cross sections and the multiplicity spectra are separately computed for each of the 16 combinations of projectile and target. We describe characteristic effects of heavy nuclei in the shape and normalization of the spectra of secondary particles.

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Section: The Inelastic Cross Sectionsupporting

confidence: 76%

Production of secondary particles in heavy nuclei interactions in supernova remnants

Bhatt,

Sushch,

Pohl

et al. 2020

Preprint

View full text Add to dashboard Cite

show abstract

Section: The Inelastic Cross Sectionsupporting

confidence: 68%

Production of secondary particles in heavy nuclei interactions in supernova remnants

Bhatt

Sushch

Pohl

et al. 2020

Astroparticle Physics

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Depending on their type, supernova remnants may have ejecta material with high abundance of heavy elements such as carbon or oxygen. In addition, core-collapse supernovae explode in the wind material of their progenitor star that may also have a high abundance of heavy elements. Hadronic collisions in these enriched media spawn the production of gamma rays, neutrinos, and secondary electrons with spectra that cannot be scaled from those calculated for pp collisions, potentially leading to erroneous results. We used Monte-Carlo event generators to calculate the differential production rate of particles such as gamma rays, neutrinos, and secondary electrons for H, He, C, and O nuclei as projectiles and as target material. The cross sections and the multiplicity spectra are separately computed for each of the 16 combinations of projectile and target. We describe characteristic effects of heavy nuclei in the shape and normalization of the spectra of the various particles produced.

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“…Therefore, it is reasonable to believe that the results of Ref. [93] are not reliable. For this reason, it is not surprising that none of the models fits the Aksinenko data point for the 12 C + 28 Si system.…”

Section: Comparison Of the Parametrisations With The Experimental Dat...mentioning

confidence: 95%

Total nuclear reaction cross-section database for radiation protection in space and heavy-ion therapy applications

Luoni,

Horst,

Reidel

et al. 2021

Preprint

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Realistic nuclear reaction cross-section models are an essential ingredient to reliable heavy-ion transport codes. Such codes are used for risk evaluation of manned space exploration missions as well as for ion-beam therapy dose calculation and treatment planning. Therefore, a total nuclear reaction crosssection data collection has been generated within a GSI-ESA-NASA collaboration (https://www.gsi.de/fragmentation).It is comprehensive of the so far experimentally measured total nucleus-nucleus reaction cross sections. The Tripathi, Kox, Shen, Kox-Shen and Hybrid-Kurotama models are compared with the data. Details about the implementation of such models are given within the work. At the end, literature gaps are pointed out and considerations are given about which models fit the existing data best for the most important systems for radiation protection in space and heavy-ion therapy.

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Streamer chamber study of the cross sections and multiplicities in nucleus-nucleus interactions at the incident momentum of 4.5 GeV/c per nucleon

Cited by 54 publications

References 8 publications

Production of secondary particles in heavy nuclei interactions in supernova remnants

Production of secondary particles in heavy nuclei interactions in supernova remnants

Production of secondary particles in heavy nuclei interactions in supernova remnants

Total nuclear reaction cross-section database for radiation protection in space and heavy-ion therapy applications

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