[Formula Presented] decay of [Formula Presented] and [Formula Presented] and implication for solar-neutrino detection

W. Liu; M. Hellström; R. Collatz; J. Benlliure; L. Chulkov; D. Cortina Gil; F. Farget; H. Grawe; Z. Hu; N. Iwasa; M. Pfützner; A. Piechaczek; R. Raabe; I. Reusen; E. Roeckl; G. Vancraeynest; A. Wöhr

doi:10.1103/PhysRevC.58.2677

[Formula Presented] decay of [Formula Presented] and [Formula Presented] and implication for solar-neutrino detection

W. Liu, M. Hellström, R. Collatz, J. Benlliure, L. Chulkov, D. Cortina Gil, F. Farget, H. Grawe, Z. Hu, N. Iwasa, M. Pfützner, A. Piechaczek, R. Raabe, I. Reusen, E. Roeckl, G. Vancraeynest, A. Wöhr

Research output: Contribution to journal › Article › peer-review

34 Citations (Scopus)

Abstract

The [Formula Presented] decay of [Formula Presented] and [Formula Presented] was studied by measuring the [Formula Presented]-delayed proton and [Formula Presented] emission. The half-lives for [Formula Presented] and [Formula Presented] were determined to be 54(2) and 82(3) ms, respectively. The experimental [Formula Presented]-decay strengths are compared with shell-model calculations and results from other measurements. The integrated Gamow-Teller strengths for [Formula Presented] and [Formula Presented] were found to be quenched, compared to the calculations, by factors of 0.79(3) and 0.93(3), respectively. Based on the experimental [Formula Presented]-decay strength, the neutrino absorption cross section and induced neutrino event rates for [Formula Presented] were determined to be [Formula Presented] and [Formula Presented] SNU, respectively.

Original language	English
Pages (from-to)	2677-2688
Number of pages	12
Journal	Physical Review C - Nuclear Physics
Volume	58
Issue number	5
DOIs	https://doi.org/10.1103/PhysRevC.58.2677
Publication status	Published - 1998
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1103/PhysRevC.58.2677

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Liu, W., Hellström, M., Collatz, R., Benlliure, J., Chulkov, L., Gil, D. C., Farget, F., Grawe, H., Hu, Z., Iwasa, N., Pfützner, M., Piechaczek, A., Raabe, R., Reusen, I., Roeckl, E., Vancraeynest, G., & Wöhr, A. (1998). [Formula Presented] decay of [Formula Presented] and [Formula Presented] and implication for solar-neutrino detection. Physical Review C - Nuclear Physics, 58(5), 2677-2688. https://doi.org/10.1103/PhysRevC.58.2677

Liu, W, Hellström, M, Collatz, R, Benlliure, J, Chulkov, L, Gil, DC, Farget, F, Grawe, H, Hu, Z, Iwasa, N, Pfützner, M, Piechaczek, A, Raabe, R, Reusen, I, Roeckl, E, Vancraeynest, G & Wöhr, A 1998, '[Formula Presented] decay of [Formula Presented] and [Formula Presented] and implication for solar-neutrino detection', Physical Review C - Nuclear Physics, vol. 58, no. 5, pp. 2677-2688. https://doi.org/10.1103/PhysRevC.58.2677

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title = "[Formula Presented] decay of [Formula Presented] and [Formula Presented] and implication for solar-neutrino detection",

abstract = "The [Formula Presented] decay of [Formula Presented] and [Formula Presented] was studied by measuring the [Formula Presented]-delayed proton and [Formula Presented] emission. The half-lives for [Formula Presented] and [Formula Presented] were determined to be 54(2) and 82(3) ms, respectively. The experimental [Formula Presented]-decay strengths are compared with shell-model calculations and results from other measurements. The integrated Gamow-Teller strengths for [Formula Presented] and [Formula Presented] were found to be quenched, compared to the calculations, by factors of 0.79(3) and 0.93(3), respectively. Based on the experimental [Formula Presented]-decay strength, the neutrino absorption cross section and induced neutrino event rates for [Formula Presented] were determined to be [Formula Presented] and [Formula Presented] SNU, respectively.",

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AU - Benlliure, J.

AU - Chulkov, L.

AU - Gil, D. Cortina

AU - Farget, F.

AU - Grawe, H.

AU - Hu, Z.

AU - Iwasa, N.

AU - Pfützner, M.

AU - Piechaczek, A.

AU - Raabe, R.

AU - Reusen, I.

AU - Roeckl, E.

AU - Vancraeynest, G.

AU - Wöhr, A.

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[Formula Presented] decay of [Formula Presented] and [Formula Presented] and implication for solar-neutrino detection

Abstract

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