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論文

First accurate normalization of the $$beta$$-delayed $$alpha$$ decay of $$^{16}$$N and implications for the $$^{12}$$C($$alpha$$,$$gamma$$)$$^{16}$$O astrophysical reaction rate

Kirsebom, O. S.*; Tengblad, O.*; Andreyev, A. N.; 他41名*

Physical Review Letters, 121(14), p.142701_1 - 142701_6, 2018/10

https://doi.org/10.1103/PhysRevLett.121.142701
 被引用回数：7 パーセンタイル：50.74(Physics, Multidisciplinary)

The $$^{12}$$C($$alpha$$,$$gamma$$)$$^{16}$$O reaction plays a central role in astrophysics, but its cross section at energies relevant for astrophysical applications is only poorly constrained by laboratory data. The reduced $$alpha$$ width, $$gamma_{rm 11}$$, of the bound 1$$^{-}$$ level in $$^{16}$$O is particularly important to determine the cross section. The magnitude of $$gamma_{11}$$ is determined via sub-Coulomb $$alpha$$-transfer reactions or the $$beta$$-delayed $$alpha$$ decay of $$^{16}$$N, but the latter approach is presently hampered by the lack of sufficiently precise data on the $$beta$$-decay branching ratios. Here we report improved branching ratios for the bound 1$$^{-}$$ level ($$b_{beta,11}$$) and for $$beta$$-delayed $$alpha$$ emission ($$b_{beta alpha}$$). Our value for $$b_{beta alpha}$$ is 33 $$%$$ larger than previously held, leading to a substantial increase in $$gamma_{11}$$. Our revised value for $$gamma_{11}$$ is in good agreement with the value obtained in $$alpha$$-transfer studies and the weighted average of the two gives a robust and precise determination of $$gamma_{11}$$, which provides significantly improved constraints on the $$^{12}$$C($$alpha$$,$$gamma$$)$$^{16}$$O cross section in the energy range relevant to hydro static He burning.

論文

Beta-delayed proton emission from $$^{20}$$Mg

Lund, M. V.*; Andreyev, A. N.; Borge, M. J. G.*; Cederk$"a$ll, J.*; De Witte, H.*; Fraile, L. M.*; Fynbo, H. O. U.*; Greenlees, P. T.*; Harkness-Brennan, L. J.*; Howard, A. M.*; et al.

European Physical Journal A, 52(10), p.304_1 - 304_14, 2016/10

https://doi.org/10.1140/epja/i2016-16304-x
 被引用回数：17 パーセンタイル：75.78(Physics, Nuclear)

Beta-delayed proton emission from $$^{20}$$Mg has been measured at ISOLDE, CERN, with the ISOLDE Decay Station setup including both charged-particle and $$gamma$$-ray detection capabilities. A total of 27 delayed proton branches were measured including seven so far unobserved. An updated decay scheme, including three new resonances above the proton separation energy in $$^{20}$$Na and more precise resonance energies, is presented. Beta-decay feeding to two resonances above the Isobaric Analogue State in $$^{20}$$Na is observed. This may allow studies of the 4032.9(2.4) keV resonance in $$^{19}$$Ne through the beta decay of $$^{20}$$Mg, which is important for the astrophysically relevant reaction $$^{15}$$O($$alpha$$,$$gamma$$)$$^{19}$$Ne. Beta-delayed protons were used to obtain a more precise value for the half-life of $$^{20}$$Mg, 91.4(1.0) ms.

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