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

3 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

Access to Document

10.1103/PhysRevC.74.015804

Cite this

@article{afd6cf5233fb468a969e3c0bb5605f66,

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",

number = "1",

}

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 - http://www.scopus.com/inward/record.url?scp=33746114864&partnerID=8YFLogxK

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

Abstract

Access to Document

Other files and links

Fingerprint

Cite this