Astrophysical S factor for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions

A. Sabourov; M. W. Ahmed; M. A. Blackston; A. S. Crowell; C. R. Howell; B. A. Perdue; K. Sabourov; A. Tonchev; H. R. Weller; R. M. Prior; M. C. Spraker

doi:10.1103/PhysRevC.73.015801

Astrophysical S factor for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions

A. Sabourov, M. W. Ahmed, M. A. Blackston, A. S. Crowell, C. R. Howell, B. A. Perdue, K. Sabourov, A. Tonchev, H. R. Weller, R. M. Prior, M. C. Spraker

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Abstract

The absolute astrophysical S factor and cross section for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions have been determined using deuteron beams with energies between 45 and 80 keV. The slope of the S factor is consistent with zero in the n0 case but is slightly negative in the n1 case. The S factor for the sum of both neutron groups at c.m. energies below 70 keV is S(E)=5400(±1500)-37(±21)E keV b, where E is the c.m. energy in keV.

Original language	English
Article number	015801
Journal	Physical Review C - Nuclear Physics
Volume	73
Issue number	1
DOIs	https://doi.org/10.1103/PhysRevC.73.015801
State	Published - Jan 2006
Externally published	Yes

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title = "Astrophysical S factor for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions",

abstract = "The absolute astrophysical S factor and cross section for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions have been determined using deuteron beams with energies between 45 and 80 keV. The slope of the S factor is consistent with zero in the n0 case but is slightly negative in the n1 case. The S factor for the sum of both neutron groups at c.m. energies below 70 keV is S(E)=5400(±1500)-37(±21)E keV b, where E is the c.m. energy in keV.",

author = "A. Sabourov and Ahmed, {M. W.} and Blackston, {M. A.} and Crowell, {A. S.} and Howell, {C. R.} and Perdue, {B. A.} and K. Sabourov and A. Tonchev and Weller, {H. R.} and Prior, {R. M.} and Spraker, {M. C.}",

year = "2006",

month = jan,

doi = "10.1103/PhysRevC.73.015801",

language = "English",

volume = "73",

journal = "Physical Review C - Nuclear Physics",

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T1 - Astrophysical S factor for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions

AU - Sabourov, A.

AU - Ahmed, M. W.

AU - Blackston, M. A.

AU - Crowell, A. S.

AU - Howell, C. R.

AU - Perdue, B. A.

AU - Sabourov, K.

AU - Tonchev, A.

AU - Weller, H. R.

AU - Prior, R. M.

AU - Spraker, M. C.

PY - 2006/1

Y1 - 2006/1

N2 - The absolute astrophysical S factor and cross section for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions have been determined using deuteron beams with energies between 45 and 80 keV. The slope of the S factor is consistent with zero in the n0 case but is slightly negative in the n1 case. The S factor for the sum of both neutron groups at c.m. energies below 70 keV is S(E)=5400(±1500)-37(±21)E keV b, where E is the c.m. energy in keV.

AB - The absolute astrophysical S factor and cross section for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions have been determined using deuteron beams with energies between 45 and 80 keV. The slope of the S factor is consistent with zero in the n0 case but is slightly negative in the n1 case. The S factor for the sum of both neutron groups at c.m. energies below 70 keV is S(E)=5400(±1500)-37(±21)E keV b, where E is the c.m. energy in keV.

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DO - 10.1103/PhysRevC.73.015801

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JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

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ER -

Astrophysical S factor for the Li7(d,n0)Be8 and Li7(d,n1)Be8 reactions

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