RTS&amp;T Monte Carlo code (facilities and computation methods)

Blokhin, A. I.; Degtyarev, I.I.; Lokhovitskii, A.E.; Maslov, M. A.; Yazynin, I. A.

doi:10.1109/pac.1997.749611

Cited by 3 publications

(5 citation statements)

References 6 publications

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“…All types of reactions provided by ENDF-6 format are taken into account for the particle transport modeling. More details on the RTS&T code may be found in [5] and references therein.…”

Section: Monte Carlo Simulationmentioning

confidence: 99%

“…, where S(E) is the energy spectrum of particles emitted from a target, e f (E) is the sensitivity of the detector, dE/dt is the time derivative of the particle energy for r-distance detector, and k is a coefficient. The sensitivity of the detector to neutrons (and cosmic μ-mesons ( eμ ) was calculated by the RTS&T code [6], see Fig. 2.…”

Section: Facility Description and Operation Principlementioning

confidence: 99%

“…The space between the target and detector was filled with air too. More details on the RTS&T code may be found in [6] and references therein.…”

Section: Monte Carlo Simulationmentioning

confidence: 99%

See 2 more Smart Citations

CTOF measurements and Monte Carlo analyses of neutron spectra for the backward direction from a lead target irradiated with 200–1000 MeV protons

Azhgirey¹,

Belyakov-Bodin²,

Degtyarev³

et al. 2010

Nuclear Instruments and Methods in Physics Research Section B:

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A description of the IntraNuclear Cascade (INC), preequilibrium, evaporation, fission, coalescence, and Fermi breakup models used by the latest versions of our CEM03.03 and LAQGSM03.03 event generators is presented, with a focus on our most recent developments of these models. The recently developed "S" and "G" versions of our codes, that consider multifragmentation of nuclei formed after the preequilibrium stage of reactions when their excitation energy is above 2A MeV using the Statistical Multifragmentation Model (SMM) code by Botvina et al. ("S" stands for SMM) and the fission-like binary-decay model GEMINI by Charity ("G" stands for GEMINI), respectively, are briefly described as well. Examples of benchmarking our models against a large variety of experimental data on particle-particle, particle-nucleus, and nucleus-nucleus reactions are presented. Open questions on reaction mechanisms and future necessary work are outlined.

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“…All types of reactions provided by ENDF-6 format are taken into account for the particle transport modeling. More details on the RTS&T code may be found in [5] and references therein.…”

Section: Monte Carlo Simulationmentioning

confidence: 99%

Section: Facility Description and Operation Principlementioning

confidence: 99%

See 1 more Smart Citation

CTOF measurements and Monte Carlo analyses of neutron spectra for the backward direction from a lead target irradiated with 200–1000 MeV protons

Azhgirey¹,

Belyakov-Bodin²,

Degtyarev³

et al. 2010

Nuclear Instruments and Methods in Physics Research Section B:

Self Cite

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show abstract

“…, where S(E) is the energy spectrum of particles emitted from a target, e f (E) is the sensitivity of the detector, dE/dt is the time derivative of particle energy for r-distance detector, and k is a coefficient. The sensitivity e f (E) of detector to neutron (and cosmic µ-meson ( eµ ) was calculated by the RTS&T code [4] (see Fig. 2).…”

Section: Facility Description and Operation Principlementioning

confidence: 99%

CTOF measurements and Monte Carlo analyses of neutron spectra for the backward direction from an iron target irradiated with 400–1200MeV protons

Azhgirey

Belyakov-Bodin

Degtyarev

et al. 2009

Nuclear Instruments and Methods in Physics Research Section B:

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A calorimetric-time-of-flight (CTOF) technique was used for real-time, high-precision measurement of neutron spectrum at the angle of 175 o from the initial proton beam direction, which hits a face plane of a cylindrical iron target of 20 cm in diameter and 25 cm thick. A comparison was performed between the neutron spectra predicted by the MARS and the MCNPX code systems and measured by experiments for 0.4-, 0.6-, 0.8-, 1.0-, and 1.2-GeV protons.

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“…The sensitivity e f (E) of detector to neutron (and cosmic m-meson (e m ) was calculated by the RTS&T code [3] (see Fig. 2).…”

Section: Article In Pressmentioning

confidence: 99%

The CTOF measurements and Monte Carlo analyses of neutron spectra for backward direction from tungsten target irradiated by protons with energies from 200 to 1200MeV

Belyakov-Bodin

Katinov

Nozdrachev

et al. 2008

Nuclear Instruments and Methods in Physics Research Section A:

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RTS&T Monte Carlo code (facilities and computation methods)

Cited by 3 publications

References 6 publications

CTOF measurements and Monte Carlo analyses of neutron spectra for the backward direction from a lead target irradiated with 200–1000 MeV protons

CTOF measurements and Monte Carlo analyses of neutron spectra for the backward direction from a lead target irradiated with 200–1000 MeV protons

CTOF measurements and Monte Carlo analyses of neutron spectra for the backward direction from an iron target irradiated with 400–1200MeV protons

The CTOF measurements and Monte Carlo analyses of neutron spectra for backward direction from tungsten target irradiated by protons with energies from 200 to 1200MeV

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