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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10.1103/PhysRevC.55.R566

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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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