References quoted in the XUNDL dataset: 18O 2H(17O,A14C):XUNDL-17

4 references found.

Clicking on a keynumber will list datasets that reference the given article.

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2002WA05

Phys.Rev. C65, 034614 (2002)

J.Wagemans, C.Wagemans, G.Goeminne, O.Serot, M.Loiselet, M.Gaelens

The ¹⁷O(n, α)¹⁴C Reaction from Subthermal up to Approximately 350 keV Neutron Energy

NUCLEAR REACTIONS ¹⁷O(n, α), E < 350 keV; measured σ; deduced resonance features, astrophysical reaction rate.

doi: 10.1103/PhysRevC.65.034614

2013GU02

Phys.Rev. C 87, 012801 (2013)

M.Gulino, C.Spitaleri, X.D.Tang, G.L.Guardo, L.Lamia, S.Cherubini, B.Bucher, V.Burjan, M.Couder, P.Davies, R.deBoer, X.Fang, V.Z.Goldberg, Z.Hons, V.Kroha, L.Lamm, M.La Cognata, C.Li, C.Ma, J.Mrazek, A.M.Mukhamedzhanov, M.Notani, S.O'Brien, R.G.Pizzone, G.G.Rapisarda, D.Roberson, M.L.Sergi, W.Tan, I.J.Thompson, M.Wiescher

Suppression of the centrifugal barrier effects in the off-energy-shell neutron + ¹⁷O interaction

NUCLEAR REACTIONS ²H(¹⁷O, α¹⁴C), E=41, 43.5 MeV; measured α and ¹⁴C particle spectra, (¹⁴C)α-coin, angular distributions, yields using position-sensitive silicon detectors (PSD) at LNS, Catania, and at NSL, Notre Dame. CD₂ target; deduced momentum distributions, Q value. DWBA analysis. ¹⁷O(n, α)¹⁴C, E(cm)=0-350 keV; deduced yields, angular distributions, neutron from quasifree breakup of deuteron. ¹⁸O; deduced resonances, J, π, and excitation functions. Trojan Horse method (THM), and suppression of centrifugal barrier. Comparison with previous studies. Relevance to neutron-induced reactions in nuclear reactors, and nucleosynthesis in astrophysics.

doi: 10.1103/PhysRevC.87.012801

2014AV04

Phys.Rev. C 90, 024327 (2014)

M.L.Avila, G.V.Rogachev, V.Z.Goldberg, E.D.Johnson, K.W.Kemper, Yu.M.Tchuvil'sky, A.S.Volya

α-cluster structure of ¹⁸O

NUCLEAR REACTIONS ⁴He(¹⁴C, α), E=14.9 MeV; measured Eα, Iα, differential σ(E), partial α- and neutron-decay widths at FSU Superconducting linear accelerator facility. ¹⁸O; deduced levels, resonances, J, π, widths, reduced α widths. Multilevel, multichannel R-matrix analysis. Discussed rotational bands, and α-cluster structure with reference to those in ¹⁶O and ²⁰Ne. Comparison with cluster-nucleon configuration interaction model calculations, and with earlier experimental results.

doi: 10.1103/PhysRevC.90.024327

2017GU05

Phys.Rev. C 95, 025807 (2017)

G.L.Guardo, C.Spitaleri, L.Lamia, M.Gulino, M.La Cognata, X.Tang, R.deBoer, X.Fang, V.Goldberg, J.Mrazek, A.Mukhamedzhanov, M.Notani, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, M.Wiescher

Assessing the near threshold cross section of the ¹⁷O(n, α)¹⁴C reaction by means of the Trojan horse method

NUCLEAR REACTIONS ²H(¹⁷O, α¹⁴C), E=43.5 MeV; measured reaction products, particle spectra, (particle)(particle)-coin, angular distributions using two telescopes of ionization chambers (IC) and silicon position-sensitive detector (PSD) at LNS-Catania and NSL-Notre Dame accelerator facilities; deduced normalized reaction yields, experimental momentum distribution, quasifission (QF) cross sections and best fit from R-matrix analysis. ¹⁸O; deduced levels, resonances, J, π, and Trojan horse method (THM) analysis of Γ_n, Γ_α and total widths. ¹⁷O(n, α)¹⁴C, T₉=0.01-10; deduce astrophysical reaction rates by THM method.

doi: 10.1103/PhysRevC.95.025807