Astrophysical reaction rate for the 18F(p,α)15O reaction

K. E. Rehm; M. Paul; A. D. Roberts; C. L. Jiang; D. J. Blumenthal; S. M. Fischer; J. Gehring; D. Henderson; J. Nickles; J. Nolen; R. C. Pardo; J. P. Schiffer; R. E. Segel

doi:10.1103/PhysRevC.53.1950

Astrophysical reaction rate for the ¹⁸F(p,α)¹⁵O reaction

K. E. Rehm^*, M. Paul, A. D. Roberts, C. L. Jiang, D. J. Blumenthal, S. M. Fischer, J. Gehring, D. Henderson, J. Nickles, J. Nolen, R. C. Pardo, J. P. Schiffer, R. E. Segel

^*Corresponding author for this work

Racah Institute of Physics

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Abstract

An excitation function for the ¹⁸F(p,α)¹⁵O reaction has been measured in the energy range E_c.m.=600-800 keV using a radioactive ¹⁸F beam. A resonant state with a spin value of 3/2⁺ has been found at an energy of 652 keV above threshold. This l_p=0 resonance is found to dominate the astrophysical reaction rate at temperatures T₉>0.5.

Original language	English
Pages (from-to)	1950-1954
Number of pages	5
Journal	Physical Review C - Nuclear Physics
Volume	53
Issue number	4
DOIs	https://doi.org/10.1103/PhysRevC.53.1950
State	Published - Apr 1996

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10.1103/PhysRevC.53.1950

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title = "Astrophysical reaction rate for the 18F(p,α)15O reaction",

abstract = "An excitation function for the 18F(p,α)15O reaction has been measured in the energy range Ec.m.=600-800 keV using a radioactive 18F beam. A resonant state with a spin value of 3/2+ has been found at an energy of 652 keV above threshold. This lp=0 resonance is found to dominate the astrophysical reaction rate at temperatures T9>0.5.",

author = "Rehm, \{K. E.\} and M. Paul and Roberts, \{A. D.\} and Jiang, \{C. L.\} and Blumenthal, \{D. J.\} and Fischer, \{S. M.\} and J. Gehring and D. Henderson and J. Nickles and J. Nolen and Pardo, \{R. C.\} and Schiffer, \{J. P.\} and Segel, \{R. E.\}",

year = "1996",

month = apr,

doi = "10.1103/PhysRevC.53.1950",

language = "אנגלית",

volume = "53",

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issn = "0556-2813",

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T1 - Astrophysical reaction rate for the 18F(p,α)15O reaction

AU - Rehm, K. E.

AU - Paul, M.

AU - Roberts, A. D.

AU - Jiang, C. L.

AU - Blumenthal, D. J.

AU - Fischer, S. M.

AU - Gehring, J.

AU - Henderson, D.

AU - Nickles, J.

AU - Nolen, J.

AU - Pardo, R. C.

AU - Schiffer, J. P.

AU - Segel, R. E.

PY - 1996/4

Y1 - 1996/4

N2 - An excitation function for the 18F(p,α)15O reaction has been measured in the energy range Ec.m.=600-800 keV using a radioactive 18F beam. A resonant state with a spin value of 3/2+ has been found at an energy of 652 keV above threshold. This lp=0 resonance is found to dominate the astrophysical reaction rate at temperatures T9>0.5.

AB - An excitation function for the 18F(p,α)15O reaction has been measured in the energy range Ec.m.=600-800 keV using a radioactive 18F beam. A resonant state with a spin value of 3/2+ has been found at an energy of 652 keV above threshold. This lp=0 resonance is found to dominate the astrophysical reaction rate at temperatures T9>0.5.

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DO - 10.1103/PhysRevC.53.1950

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SN - 0556-2813

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EP - 1954

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

IS - 4

ER -

Astrophysical reaction rate for the ¹⁸F(p,α)¹⁵O reaction

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