Exploring the [Formula Presented] gateway to the formation of heavy elements in hot stars

K. E. Rehm; C. L. Jiang; M. Paul; D. Blumenthal; L. A. Daniel; C. N. Davids; P. Decrock; S. M. Fischer; D. Henderson; C. Lister; J. Nickles; J. Nolen; R. C. Pardo; J. P. Schiffer; D. Seweryniak; R. E. Segel

doi:10.1103/PhysRevC.55.R566

Exploring the [Formula Presented] gateway to the formation of heavy elements in hot stars

K. E. Rehm, C. L. Jiang, M. Paul, D. Blumenthal, L. A. Daniel, C. N. Davids, P. Decrock, S. M. Fischer, D. Henderson, C. Lister, J. Nickles, J. Nolen, R. C. Pardo, J. P. Schiffer, D. Seweryniak, R. E. Segel

Racah Institute of Physics

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

27 Scopus citations

Abstract

An upper limit to the production of [Formula Presented] through the [Formula Presented] reaction at the recently discovered [Formula Presented]-wave resonance has been determined. The limit implies that in a hot stellar environment [Formula Presented] this reaction is not a significant gateway from the hot CNO cycle towards the production of heavier elements in stars.

Original language	English
Pages (from-to)	R566-R569
Journal	Physical Review C - Nuclear Physics
Volume	55
Issue number	2
DOIs	https://doi.org/10.1103/PhysRevC.55.R566
State	Published - 1997

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Rehm, K. E., Jiang, C. L., Paul, M., Blumenthal, D., Daniel, L. A., Davids, C. N., Decrock, P., Fischer, S. M., Henderson, D., Lister, C., Nickles, J., Nolen, J., Pardo, R. C., Schiffer, J. P., Seweryniak, D., & Segel, R. E. (1997). Exploring the [Formula Presented] gateway to the formation of heavy elements in hot stars. Physical Review C - Nuclear Physics, 55(2), R566-R569. https://doi.org/10.1103/PhysRevC.55.R566

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abstract = "An upper limit to the production of [Formula Presented] through the [Formula Presented] reaction at the recently discovered [Formula Presented]-wave resonance has been determined. The limit implies that in a hot stellar environment [Formula Presented] this reaction is not a significant gateway from the hot CNO cycle towards the production of heavier elements in stars.",

author = "Rehm, \{K. E.\} and Jiang, \{C. L.\} and M. Paul and D. Blumenthal and Daniel, \{L. A.\} and Davids, \{C. N.\} and P. Decrock and Fischer, \{S. M.\} and D. Henderson and C. Lister and J. Nickles and J. Nolen and Pardo, \{R. C.\} and Schiffer, \{J. P.\} and D. Seweryniak and Segel, \{R. E.\}",

year = "1997",

doi = "10.1103/PhysRevC.55.R566",

language = "אנגלית",

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Rehm, KE, Jiang, CL, Paul, M, Blumenthal, D, Daniel, LA, Davids, CN, Decrock, P, Fischer, SM, Henderson, D, Lister, C, Nickles, J, Nolen, J, Pardo, RC, Schiffer, JP, Seweryniak, D & Segel, RE 1997, 'Exploring the [Formula Presented] gateway to the formation of heavy elements in hot stars', Physical Review C - Nuclear Physics, vol. 55, no. 2, pp. R566-R569. https://doi.org/10.1103/PhysRevC.55.R566

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T1 - Exploring the [Formula Presented] gateway to the formation of heavy elements in hot stars

AU - Rehm, K. E.

AU - Jiang, C. L.

AU - Paul, M.

AU - Blumenthal, D.

AU - Daniel, L. A.

AU - Davids, C. N.

AU - Decrock, P.

AU - Fischer, S. M.

AU - Henderson, D.

AU - Lister, C.

AU - Nickles, J.

AU - Nolen, J.

AU - Pardo, R. C.

AU - Schiffer, J. P.

AU - Seweryniak, D.

AU - Segel, R. E.

PY - 1997

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AB - An upper limit to the production of [Formula Presented] through the [Formula Presented] reaction at the recently discovered [Formula Presented]-wave resonance has been determined. The limit implies that in a hot stellar environment [Formula Presented] this reaction is not a significant gateway from the hot CNO cycle towards the production of heavier elements in stars.

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Exploring the [Formula Presented] gateway to the formation of heavy elements in hot stars

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