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From the same journal

The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate

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The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate. / Chipps, K. A.; Bardayan, D. W.; Chae, K. Y.; Cizewski, J. A.; Kozub, R. L.; Liang, J. F.; Matei, C.; Moazen, B. H.; Nesaraja, C. D.; O'Malley, P. D.; Pain, S. D.; Peters, W. A.; Pittman, S. T.; Schmitt, K. T.; Smith, M. S.

In: Physical Review C, Vol. 82, No. 4, 045803, 25.10.2010, p. -.

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

Harvard

Chipps, KA, Bardayan, DW, Chae, KY, Cizewski, JA, Kozub, RL, Liang, JF, Matei, C, Moazen, BH, Nesaraja, CD, O'Malley, PD, Pain, SD, Peters, WA, Pittman, ST, Schmitt, KT & Smith, MS 2010, 'The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate', Physical Review C, vol. 82, no. 4, 045803, pp. -. https://doi.org/10.1103/PhysRevC.82.045803

APA

Chipps, K. A., Bardayan, D. W., Chae, K. Y., Cizewski, J. A., Kozub, R. L., Liang, J. F., Matei, C., Moazen, B. H., Nesaraja, C. D., O'Malley, P. D., Pain, S. D., Peters, W. A., Pittman, S. T., Schmitt, K. T., & Smith, M. S. (2010). The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate. Physical Review C, 82(4), -. [045803]. https://doi.org/10.1103/PhysRevC.82.045803

Vancouver

Chipps KA, Bardayan DW, Chae KY, Cizewski JA, Kozub RL, Liang JF et al. The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate. Physical Review C. 2010 Oct 25;82(4):-. 045803. https://doi.org/10.1103/PhysRevC.82.045803

Author

Chipps, K. A. ; Bardayan, D. W. ; Chae, K. Y. ; Cizewski, J. A. ; Kozub, R. L. ; Liang, J. F. ; Matei, C. ; Moazen, B. H. ; Nesaraja, C. D. ; O'Malley, P. D. ; Pain, S. D. ; Peters, W. A. ; Pittman, S. T. ; Schmitt, K. T. ; Smith, M. S. / The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate. In: Physical Review C. 2010 ; Vol. 82, No. 4. pp. -.

Bibtex - Download

@article{2eb1ddbb7db548f3b51c651bda297081,
title = "The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate",
abstract = "Several resonances in Al-25(p,gamma)Si-26 have been studied via the Si-28(p,t)Si-26 reaction. Triton energies and angular distributions were measured using a segmented annular detector array. An additional silicon detector array was used to simultaneously detect the coincident protons emitted from the decay of states in Si-26 above the proton threshold in order to determine branching ratios. A resonance at 5927 +/- 4 keV has been experimentally confirmed as the first l = 0 state above the proton threshold, with a proton branching ratio consistent with one.",
keywords = "AL-26",
author = "Chipps, {K. A.} and Bardayan, {D. W.} and Chae, {K. Y.} and Cizewski, {J. A.} and Kozub, {R. L.} and Liang, {J. F.} and C. Matei and Moazen, {B. H.} and Nesaraja, {C. D.} and O'Malley, {P. D.} and Pain, {S. D.} and Peters, {W. A.} and Pittman, {S. T.} and Schmitt, {K. T.} and Smith, {M. S.}",
year = "2010",
month = oct,
day = "25",
doi = "10.1103/PhysRevC.82.045803",
language = "English",
volume = "82",
pages = "--",
journal = "Physical Review C - Nuclear Physics",
issn = "0556-2813",
publisher = "American Physical Society",
number = "4",

}

RIS (suitable for import to EndNote) - Download

TY - JOUR

T1 - The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate

AU - Chipps, K. A.

AU - Bardayan, D. W.

AU - Chae, K. Y.

AU - Cizewski, J. A.

AU - Kozub, R. L.

AU - Liang, J. F.

AU - Matei, C.

AU - Moazen, B. H.

AU - Nesaraja, C. D.

AU - O'Malley, P. D.

AU - Pain, S. D.

AU - Peters, W. A.

AU - Pittman, S. T.

AU - Schmitt, K. T.

AU - Smith, M. S.

PY - 2010/10/25

Y1 - 2010/10/25

N2 - Several resonances in Al-25(p,gamma)Si-26 have been studied via the Si-28(p,t)Si-26 reaction. Triton energies and angular distributions were measured using a segmented annular detector array. An additional silicon detector array was used to simultaneously detect the coincident protons emitted from the decay of states in Si-26 above the proton threshold in order to determine branching ratios. A resonance at 5927 +/- 4 keV has been experimentally confirmed as the first l = 0 state above the proton threshold, with a proton branching ratio consistent with one.

AB - Several resonances in Al-25(p,gamma)Si-26 have been studied via the Si-28(p,t)Si-26 reaction. Triton energies and angular distributions were measured using a segmented annular detector array. An additional silicon detector array was used to simultaneously detect the coincident protons emitted from the decay of states in Si-26 above the proton threshold in order to determine branching ratios. A resonance at 5927 +/- 4 keV has been experimentally confirmed as the first l = 0 state above the proton threshold, with a proton branching ratio consistent with one.

KW - AL-26

UR - http://www.scopus.com/inward/record.url?scp=78649372402&partnerID=8YFLogxK

U2 - 10.1103/PhysRevC.82.045803

DO - 10.1103/PhysRevC.82.045803

M3 - Article

VL - 82

SP - -

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

SN - 0556-2813

IS - 4

M1 - 045803

ER -

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