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

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

10 Scopus citations

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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10.1103/PhysRevC.73.015801

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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",

issn = "0556-2813",

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TY - JOUR

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.

UR - https://www.scopus.com/pages/publications/32644472803

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DO - 10.1103/PhysRevC.73.015801

M3 - Article

AN - SCOPUS:32644472803

SN - 0556-2813

VL - 73

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

IS - 1

M1 - 015801

ER -

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

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