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NSR database version of April 11, 2024.

Search: Author = M.Chabot

Found 9 matches.

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2021AD06      Phys.Rev. C 103, 035804 (2021)

P.Adsley, F.Hammache, N.de Sereville, V.Alcindor, M.Assie, D.Beaumel, M.Chabot, M.Degerlier, C.Delafosse, T.Faestermann, F.Flavigny, S.P.Fox, R.Garg, A.Georgiadou, S.A.Gillespie, J.Guillot, V.Guimaraes, A.Gottardo, R.Hertenberger, J.Kiener, A.M.Laird, A.Lefebvre-Schuhl, I.Matea, A.Meyer, M.Mahgoub, L.Olivier, L.Perrot, J.Riley, I.Sivacek, I.Stefan, V.Tatischeff, H.-F.Wirth

Charged-particle branching ratios above the neutron threshold in ¹⁹F: Constraining ¹⁵N production in core-collapse supernovae

COMPILATION ¹⁹F; compiled data from the ENSDF database and from different nuclear reactions in literature for levels, J, π, Γ, Γ_p, and Γ_α.

NUCLEAR REACTIONS ¹⁹F(p, p'), E=16, 15 MeV; measured E(p), I(p), πα- and pp-coin using the Q3D magnetic spectrograph at Munich at E(p)=16 MeV, and Enge split-pole magnetic spectrometer, and double-sided silicon strip detector (DSSSD) detectors at Orsay at E(p)=15 MeV. ¹⁹F; deduced levels between 10.091 and 10.676 MeV in the region of astrophysical interest, width, branching ratios for proton and α decays from levels above the neutron binding energy in ¹⁹F. ¹⁵N, ¹⁸O; deduced energies of the emitted particles, matrices of experimental and simulated coincidence events from α and proton decays of neutron-unbound states in ¹⁹F. Relevance to ¹⁸F(n, α)¹⁵N and ¹⁸F(n, p)¹⁸O reaction rates for abundances of ¹⁵N and ¹⁸O in the helium-burning shell during core-collapse supernovae.

doi: 10.1103/PhysRevC.103.035804
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Data from this article have been entered in the XUNDL database. For more information, click here.

2015AS03      Eur.Phys.J. A 51, 11 (2015)

M.Assie, B.Le Crom, B.Genolini, M.Chabot, D.Mengoni, J.A.Duenas, S.Ancelin, D.Beaumel, Y.Blumenfeld, N.de Sereville, J.-J.Dormard, T.Faul, J.Guillot, A.Jallat, V.Le Ven, I.Martel, E.Rauly, D.Suzuki, A.-S.Torrento

Characterization of light particles (Z ≤ 2) discrimination performances by pulse shape analysis techniques with high-granularity silicon detector

doi: 10.1140/epja/i2015-15011-6
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2009AS07      Eur.Phys.J. A 42, 441 (2009)

M.Assie, J.A.Scarpaci, D.Lacroix, J.C.Angelique, D.Bazin, D.Beaumel, Y.Blumenfeld, W.N.Catford, M.Chabot, A.Chatterjee, M.Fallot, H.Iwasaki, F.Marechal, D.Mengoni, C.Monrozeau, J.Nyberg, C.Petrache, F.Skaza, T.Tuna

Neutron correlations in ⁶He viewed through nuclear break-up

NUCLEAR REACTIONS ²⁰⁸Pb(⁶He, X), E=20 MeV/nucleon; measured En, In, Ep, Ed, Et, Eα, αn-, nn-coin; deduced σ(θ), angular correlations. SPIRAL radioactive beam facility at GANIL. Comparison with GEANT4 simulation.

doi: 10.1140/epja/i2009-10787-4
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2008FI10      Phys.Rev. C 78, 044613 (2008)

C.Fitoussi, J.Duprat, V.Tatischeff, J.Kiener, F.Naulin, G.Raisbeck, M.Assuncao, C.Bourgeois, M.Chabot, A.Coc, C.Engrand, M.Gounelle, F.Hammache, A.Lefebvre, M.-G.Porquet, J.-A.Scarpaci, N.De Sereville, J.-P.Thibaud, F.Yiou

Measurement of the ²⁴Mg(³He, p)²⁶Al cross section: Implication for ²⁶Al production in the early solar system

NUCLEAR REACTIONS Mg(³He, p)²⁵Al/²⁶Al/²⁵Mg/²²Na/²³Na, E=3-36 MeV; measured Eγ, Iγ, γγ-coin, σ. ²⁶Al; deduced levels, J, π. Implications for production in early solar system.

doi: 10.1103/PhysRevC.78.044613
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1718.

2007BE47      Phys.Rev. C 76, 034607 (2007); Erratum Phys.Rev. C 80, 029902 (2009)

A.Belhout, J.Kiener, A.Coc, J.Duprat, C.Engrand, C.Fitoussi, M.Gounelle, A.Lefebvre-Schuhl, N.de Sereville, V.Tatischeff, J.-P.Thibaud, M.Chabot, F.Hammache, H.Benhabiles-Mezhoud

γ-ray production by proton and alpha-particle induced reactions on ¹²C, ¹⁶O, ²⁴Mg, and Fe

NUCLEAR REACTIONS ¹²C, ¹⁶O, ²⁴Mg, Fe(p, γ), e=5-25 meV; ¹²C, ¹⁶O, ²⁴Mg, Fe(α, γ), E=5-40 MeV; measured Eγ, Iγ, angular distributions, cross sections and excitation functions. Compared results to model calculations.

doi: 10.1103/PhysRevC.76.034607
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1631.

2007CH46      Nucl.Instrum.Methods Phys.Res. A577, 353 (2007)

M.Chabot, D.Gardes, M.Nectoux, G.Maynard, C.Deutsch

Energy loss of Cl^q+ (52 MeV) through dilute H2 target: Evidence of non-linear term and non-Coulombian potential contribution

doi: 10.1016/j.nima.2007.02.029
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2007LI62      Nucl.Phys. A795, 1 (2007)

V.Lima, J.A.Scarpaci, D.Lacroix, Y.Blumenfeld, C.Bourgeois, M.Chabot, Ph.Chomaz, P.Desesquelles, V.Duflot, J.Duprat, M.Fallot, N.Frascaria, S.Grevy, D.Guillemaud-Mueller, P.Roussel-Chomaz, H.Savajols, O.Sorlin

Nuclear break-up of ¹¹Be

NUCLEAR REACTIONS ⁴⁸Ti(¹¹Be, n), E=41 MeV/nucleon; measured En, In, Eγ, Iγ, σ(θ), (¹⁰Be)n-, γn-coin. ¹¹Be deduced spectroscopic factor, configurations.

doi: 10.1016/j.nuclphysa.2007.07.005
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0475.

2003TA13      Phys.Rev. C 68, 025804 (2003)

V.Tatischeff, J.Duprat, J.Kiener, M.Assuncao, A.Coc, C.Engrand, M.Gounelle, A.Lefebvre, M.-G.Porquet, N.de Sereville, J.P.Thibaud, C.Bourgeois, M.Chabot, F.Hammache, J.-A.Scarpaci

Cross sections relevant to γ-ray line emission on solar flares: ³He-induced reactions on ¹⁶O nuclei

NUCLEAR REACTIONS ¹⁶O(³He, n), (³He, p), E=3.7-36 MeV; measured Eγ, Iγ; deduced γ-ray production σ(E). Astrophysical implications discussed.

doi: 10.1103/PhysRevC.68.025804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO0757.

1992HO17      Phys.Rev. A46, 2572 (1992)

V.Horvat, G.Sampoll, K.Wohrer, M.Chabot, R.L.Watson

K-Shell Ionization of Intermediate-Z Elements by 30-MeV/amu H, N, Ne, and Ar Ions

NUCLEAR REACTIONS ²⁷Al, Ti, Fe, Cu, Ge, Zr, Mo, Pd, Sn(p, X), (N, X), (Ne, X), (Ar, X), E=30 MeV/nucleon; measured K (X-ray) production σ, double K-shell ionization I X-ray.

ATOMIC PHYSICS ²⁷Al, Ti, Fe, Cu, Ge, Zr, Mo, Pd, Sn(p, X), (N, X), (Ne, X), (Ar, X), E=30 MeV/nucleon; measured K (X-ray) production σ, double K-shell ionization I X-ray.

doi: 10.1103/PhysRevA.46.2572
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