Total reaction cross section from the interaction of 4He ions with 28Si at 10–30 MeV

Baktybayev, M. K.; Duisebaev, A.; Duisebaev, B. A.; Ismailov, K. M.; Itkis, M. G.; Кадыржанов, К. К.; Kalpakchieva, R.; Kuznetsov, I. V.; Кутербеков, К. А.; Kukhtina, I. N.; Lukyanov, S. M.; Mukhamedzhan, A.; Penionzhkevich, Yu. É.; Sadykov, B. M.; Sobolev, Yu. G.; Ugryumov, V. Yu.

doi:10.1134/1.1611566

Phys. Atom. Nuclei

2003

DOI: 10.1134/1.1611566

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Total reaction cross section from the interaction of 4He ions with 28Si at 10–30 MeV

M. K. Baktybayev

A. Duisebaev

B. A. Duisebaev

et al.

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Cited by 6 publications

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“…Reaction cross section for α + 28 Si and6 Li + 208 Pb, as calculated by the NASA, Dostrovsky et al, GEM2, and B&P models. The yellow circles are experimental data[56][57][58][59][60].…”

mentioning

confidence: 99%

Total reaction cross sections in CEM and MCNP6 at intermediate energies

Kerby

Mashnik

2015

Nuclear Instruments and Methods in Physics Research Section B:

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Accurate total reaction cross section models are important to achieving reliable predictions from spallation and transport codes. The latest version of the Cascade Exciton Model (CEM) as incorporated in the code CEM03.03, and the Monte Carlo N-Particle transport code (MCNP6), both developed at Los Alamos National Laboratory (LANL), each use such cross sections. Having accurate total reaction cross section models in the intermediate energy region (∼50 MeV to ∼5 GeV) is very important for different applications, including analysis of space environments, use in medical physics, and accelerator design, to name just a few. The current inverse cross sections used in the preequilibrium and evaporation stages of CEM are based on the Dostrovsky et al. model, published in 1959. Better cross section models are available now. Implementing better cross section models in CEM and MCNP6 should yield improved predictions for particle spectra and total production cross sections, among other results. Our current results indicate this is, in fact, the case.

show abstract

“…Reaction cross section for α + 28 Si and6 Li + 208 Pb, as calculated by the NASA, Dostrovsky et al, GEM2, and B&P models. The yellow circles are experimental data[56][57][58][59][60].…”

mentioning

confidence: 99%

Total reaction cross sections in CEM and MCNP6 at intermediate energies

Kerby

Mashnik

2015

Nuclear Instruments and Methods in Physics Research Section B:

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Global α - nucleus optical model based on an Dirac Brueckner Hartree Fock approach

Zhang

et al. 2019

Nuclear Physics A

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Parametrization study for the estimation of light particles (p, d, 3He, α) induced total reaction cross sections of target mass greater than 9 within the energy range of 10–200 MeV

Büyükuslu

2019

Radiation Physics and Chemistry

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Total reaction cross section from the interaction of 4He ions with 28Si at 10–30 MeV

Cited by 6 publications

References 6 publications

Total reaction cross sections in CEM and MCNP6 at intermediate energies

Total reaction cross sections in CEM and MCNP6 at intermediate energies

Global α - nucleus optical model based on an Dirac Brueckner Hartree Fock approach

Parametrization study for the estimation of light particles (p, d, 3He, α) induced total reaction cross sections of target mass greater than 9 within the energy range of 10–200 MeV

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Total reaction cross section from the interaction of 4He ions with 28Si at 10–30 MeV

Cited by 6 publications

References 6 publications

Total reaction cross sections in CEM and MCNP6 at intermediate energies

Total reaction cross sections in CEM and MCNP6 at intermediate energies

Global α - nucleus optical model based on an Dirac Brueckner Hartree Fock approach

Parametrization study for the estimation of light particles (p, d, 3He, α) induced total reaction cross sections of target mass greater than 9 within the energy range of 10–200 MeV

Contact Info

Product

Resources

About

Parametrization study for the estimation of light particles (p, d, 3He, α) induced total reaction cross sections of target mass greater than 9 within the energy range of 10–200 MeV