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NSR database version of May 3, 2024.

Search: Author = M.Brandis

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2023AV04      Appl.Radiat.Isot. 199, 110891 (2023)

O.Aviv, S.Nissim, M.Brandis, Z.Yungrais, L.Weissman, A.Shor, E.Gilad

Evaluating the intensity of the 803-keV γ ray of ²¹⁰Po using a 4παβ(LS)-γ(HPGe) measurement system

RADIOACTIVITY ²¹⁰Po(α); measured decay products, Eα, Iα, Eγ, Iγ; deduced 803 keV γ-ray energy and intensity. Comparison with available data. 4παβ(LS)-γ(HPGe) system.

doi: 10.1016/j.apradiso.2023.110891
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Data from this article have been entered in the XUNDL database. For more information, click here.

2022NI09      Appl.Radiat.Isot. 188, 110367 (2022)

S.Nissim, O.Aviv, M.Brandis, L.Weissman, R.Sasson, Z.Yungrais, H.Datz, L.Arazi

Evaluating the intensity of the `prompt` 140.5 keV γ-ray of ⁹⁹Mo using 4παβ(LS)-γ(HPGe) measurement system

RADIOACTIVITY ⁹⁹Mo(β^-); measured decay products, Eβ, Iβ, Eγ, Iγ; deduced γ-ray energies and intensities. Comparison with available data.

doi: 10.1016/j.apradiso.2022.110367
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Data from this article have been entered in the XUNDL database. For more information, click here.

2018SH12      Phys.Rev. C 97, 034303 (2018)

A.Shor, L.Weissman, O.Aviv, Y.Eisen, M.Brandis, M.Paul, A.Plompen, M.Tessler, S.Vaintraub

Branching ratio to the 803 keV level in ²¹⁰Po α decay

RADIOACTIVITY ²¹⁰Po(α)[from ²¹⁰Bi(β^-) decay, ²¹⁰Bi from ²⁰⁹Bi(n, γ), E=thermal at Soreq nuclear reactor facility]; measured Eγ, Iγ, Eα, Iα, α-branching ratio to the 803-keV level in ²⁰⁶Pb. Comparison with previous experimental results from 1951 to 1999, and evaluated data in ENSDF and DDEP databases. Relevance to cross section for ²⁰⁹Bi(n, γ)²¹⁰Bi involved in termination of the astrophysical s process.

NUCLEAR REACTIONS ²⁰⁹Bi(n, γ), E=thermal; measured Eα, Iα from decay of ²¹⁰Po; deduced σ for thermal capture σ.

doi: 10.1103/PhysRevC.97.034303
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Data from this article have been entered in the XUNDL database. For more information, click here.

2017SH47      Phys.Rev. C 96, 055805 (2017)

A.Shor, M.Tessler, A.Plompen, A.Arenshtam, O.Aviv, D.Berkovits, M.Brandis, Y.Eisen, I.Eliyahu, G.Feinberg, M.Friedman, S.Halfon, M.Hult, B.Kaizer, D.Kijel, A.Krasa, A.Kreisel, T.Palchan, M.Paul, A.Perry, I.Silverman, S.Vaintraub, L.Weissman

Bismuth activation with quasi-Maxwellian neutrons at kT ∼ 30 keV

NUCLEAR REACTIONS ²⁰⁹Bi(n, γ), kT≈30 keV quasi-Maxwellian neutrons; measured Eβ from the decay of ²¹⁰Bi and Eα and Eγ, Iγ from the decay of ²⁰⁶Po using PIPS silicon detector for particles and HPGe detector for γ rays at the linear accelerator of Soreq Applied Research Accelerator facility (SARAF); deduced Maxwellian averaged (MACS) σ, and compared with previous experimental results, and with evaluated cross sections in the ENDF, JEFF and JENDL data libraries. Relevance to termination point of the s-process cycle of nucleosynthesis in stellar environments.

doi: 10.1103/PhysRevC.96.055805
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset31780.