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

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

45 Scopus citations

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

Access to Document

10.1103/PhysRevC.53.1950

Cite this

@article{718cf160b9f645d4956d4545784bcb25,

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",

pages = "1950--1954",

journal = "Physical Review C - Nuclear Physics",

issn = "0556-2813",

publisher = "American Physical Society",

number = "4",

}

TY - JOUR

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.

UR - https://www.scopus.com/pages/publications/4243311130

U2 - 10.1103/PhysRevC.53.1950

DO - 10.1103/PhysRevC.53.1950

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:4243311130

SN - 0556-2813

VL - 53

SP - 1950

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

Abstract

Access to Document

Other files and links

Fingerprint

Cite this