Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV

Y. Parpottas; M. W. Ahmed; M. A. Blackston; B. A. Perdue; R. M. Prior; A. Sabourov; M. C. Spraker; H. R. Weller

doi:10.1103/PhysRevC.74.015804

Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV

Y. Parpottas
, M. W. Ahmed
, M. A. Blackston
, B. A. Perdue
, R. M. Prior
, A. Sabourov
, M. C. Spraker
, H. R. Weller

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

4 Scopus citations

Abstract

The B11(d,n)C12 reaction was studied using deuteron beams of 120-160 keV to determine the absolute astrophysical S factors and cross sections for the n0 and n1 neutron groups. The slopes of the S factors are consistent with zero for both the n0 and n1 cases. The measured S factor for the sum of both neutron groups at c.m. energies below 135 keV is S=3180±480 keV b. A DWBA calculation is able to reproduce the ratio of the S factors found here to those obtained in a recent study of the Li7(d,n0,1)Be8 reaction.

Original language	English
Article number	015804
Journal	Physical Review C - Nuclear Physics
Volume	74
Issue number	1
DOIs	https://doi.org/10.1103/PhysRevC.74.015804
State	Published - 2006
Externally published	Yes

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10.1103/PhysRevC.74.015804

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title = "Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV",

abstract = "The B11(d,n)C12 reaction was studied using deuteron beams of 120-160 keV to determine the absolute astrophysical S factors and cross sections for the n0 and n1 neutron groups. The slopes of the S factors are consistent with zero for both the n0 and n1 cases. The measured S factor for the sum of both neutron groups at c.m. energies below 135 keV is S=3180±480 keV b. A DWBA calculation is able to reproduce the ratio of the S factors found here to those obtained in a recent study of the Li7(d,n0,1)Be8 reaction.",

author = "Y. Parpottas and Ahmed, \{M. W.\} and Blackston, \{M. A.\} and Perdue, \{B. A.\} and Prior, \{R. M.\} and A. Sabourov and Spraker, \{M. C.\} and Weller, \{H. R.\}",

year = "2006",

doi = "10.1103/PhysRevC.74.015804",

language = "English",

volume = "74",

journal = "Physical Review C - Nuclear Physics",

issn = "0556-2813",

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TY - JOUR

T1 - Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV

AU - Parpottas, Y.

AU - Ahmed, M. W.

AU - Blackston, M. A.

AU - Perdue, B. A.

AU - Prior, R. M.

AU - Sabourov, A.

AU - Spraker, M. C.

AU - Weller, H. R.

PY - 2006

Y1 - 2006

N2 - The B11(d,n)C12 reaction was studied using deuteron beams of 120-160 keV to determine the absolute astrophysical S factors and cross sections for the n0 and n1 neutron groups. The slopes of the S factors are consistent with zero for both the n0 and n1 cases. The measured S factor for the sum of both neutron groups at c.m. energies below 135 keV is S=3180±480 keV b. A DWBA calculation is able to reproduce the ratio of the S factors found here to those obtained in a recent study of the Li7(d,n0,1)Be8 reaction.

AB - The B11(d,n)C12 reaction was studied using deuteron beams of 120-160 keV to determine the absolute astrophysical S factors and cross sections for the n0 and n1 neutron groups. The slopes of the S factors are consistent with zero for both the n0 and n1 cases. The measured S factor for the sum of both neutron groups at c.m. energies below 135 keV is S=3180±480 keV b. A DWBA calculation is able to reproduce the ratio of the S factors found here to those obtained in a recent study of the Li7(d,n0,1)Be8 reaction.

UR - https://www.scopus.com/pages/publications/33746114864

U2 - 10.1103/PhysRevC.74.015804

DO - 10.1103/PhysRevC.74.015804

M3 - Article

AN - SCOPUS:33746114864

SN - 0556-2813

VL - 74

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

IS - 1

M1 - 015804

ER -

Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV

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