Determination of the Subthreshold State Contribution in [Formula presented], the Main Neutron-Source Reaction for the [Formula presented] Process

S. Kubono; K. Abe; S. Kato; T. Teranishi; M. Kurokawa; X. Liu; N. Imai; K. Kumagai; P. Strasser; M. H. Tanaka; Y. Fuchi; C. S. Lee; Y. K. Kwon; L. Lee; J. H. Ha; Y. K. Kim

doi:10.1103/PhysRevLett.90.062501

Determination of the Subthreshold State Contribution in [Formula presented], the Main Neutron-Source Reaction for the [Formula presented] Process

S. Kubono, K. Abe, S. Kato, T. Teranishi, M. Kurokawa, X. Liu, N. Imai, K. Kumagai, P. Strasser, M. H. Tanaka, Y. Fuchi, C. S. Lee, Y. K. Kwon, L. Lee, J. H. Ha, Y. K. Kim

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

Abstract

The reaction rate of the stellar reaction [Formula presented], which is currently considered to be the main neutron source for the slow ([Formula presented]) process at low energies, has been rederived using the direct [Formula presented]-transfer reaction [Formula presented] leading to the subthreshold state at 6.356 MeV in [Formula presented]. The contribution of the subthreshold state is found to be much smaller than the currently accepted predictions for the main neutron source of the [Formula presented] process, indicating less of a role of this reaction as the neutron source for the [Formula presented]-process scenario in low-mass stars at the asymptotic giant branch.

Original language	English
Pages (from-to)	4
Number of pages	1
Journal	Physical review letters
Volume	90
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevLett.90.062501
Publication status	Published - 2003
Externally published	Yes

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

Access to Document

10.1103/PhysRevLett.90.062501

Cite this

Kubono, S., Abe, K., Kato, S., Teranishi, T., Kurokawa, M., Liu, X., Imai, N., Kumagai, K., Strasser, P., Tanaka, M. H., Fuchi, Y., Lee, C. S., Kwon, Y. K., Lee, L., Ha, J. H., & Kim, Y. K. (2003). Determination of the Subthreshold State Contribution in [Formula presented], the Main Neutron-Source Reaction for the [Formula presented] Process. Physical review letters, 90(6), 4. https://doi.org/10.1103/PhysRevLett.90.062501

Kubono, S, Abe, K, Kato, S, Teranishi, T, Kurokawa, M, Liu, X, Imai, N, Kumagai, K, Strasser, P, Tanaka, MH, Fuchi, Y, Lee, CS, Kwon, YK, Lee, L, Ha, JH & Kim, YK 2003, 'Determination of the Subthreshold State Contribution in [Formula presented], the Main Neutron-Source Reaction for the [Formula presented] Process', Physical review letters, vol. 90, no. 6, pp. 4. https://doi.org/10.1103/PhysRevLett.90.062501

@article{8b0be3ce94b24e3d889ae072a02ded6e,

title = "Determination of the Subthreshold State Contribution in [Formula presented], the Main Neutron-Source Reaction for the [Formula presented] Process",

abstract = "The reaction rate of the stellar reaction [Formula presented], which is currently considered to be the main neutron source for the slow ([Formula presented]) process at low energies, has been rederived using the direct [Formula presented]-transfer reaction [Formula presented] leading to the subthreshold state at 6.356 MeV in [Formula presented]. The contribution of the subthreshold state is found to be much smaller than the currently accepted predictions for the main neutron source of the [Formula presented] process, indicating less of a role of this reaction as the neutron source for the [Formula presented]-process scenario in low-mass stars at the asymptotic giant branch.",

author = "S. Kubono and K. Abe and S. Kato and T. Teranishi and M. Kurokawa and X. Liu and N. Imai and K. Kumagai and P. Strasser and Tanaka, {M. H.} and Y. Fuchi and Lee, {C. S.} and Kwon, {Y. K.} and L. Lee and Ha, {J. H.} and Kim, {Y. K.}",

year = "2003",

doi = "10.1103/PhysRevLett.90.062501",

language = "English",

volume = "90",

pages = "4",

journal = "Physical review letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "6",

}

TY - JOUR

T1 - Determination of the Subthreshold State Contribution in [Formula presented], the Main Neutron-Source Reaction for the [Formula presented] Process

AU - Kubono, S.

AU - Abe, K.

AU - Kato, S.

AU - Teranishi, T.

AU - Kurokawa, M.

AU - Liu, X.

AU - Imai, N.

AU - Kumagai, K.

AU - Strasser, P.

AU - Tanaka, M. H.

AU - Fuchi, Y.

AU - Lee, C. S.

AU - Kwon, Y. K.

AU - Lee, L.

AU - Ha, J. H.

AU - Kim, Y. K.

PY - 2003

Y1 - 2003

N2 - The reaction rate of the stellar reaction [Formula presented], which is currently considered to be the main neutron source for the slow ([Formula presented]) process at low energies, has been rederived using the direct [Formula presented]-transfer reaction [Formula presented] leading to the subthreshold state at 6.356 MeV in [Formula presented]. The contribution of the subthreshold state is found to be much smaller than the currently accepted predictions for the main neutron source of the [Formula presented] process, indicating less of a role of this reaction as the neutron source for the [Formula presented]-process scenario in low-mass stars at the asymptotic giant branch.

AB - The reaction rate of the stellar reaction [Formula presented], which is currently considered to be the main neutron source for the slow ([Formula presented]) process at low energies, has been rederived using the direct [Formula presented]-transfer reaction [Formula presented] leading to the subthreshold state at 6.356 MeV in [Formula presented]. The contribution of the subthreshold state is found to be much smaller than the currently accepted predictions for the main neutron source of the [Formula presented] process, indicating less of a role of this reaction as the neutron source for the [Formula presented]-process scenario in low-mass stars at the asymptotic giant branch.

UR - http://www.scopus.com/inward/record.url?scp=85038312592&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85038312592&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.90.062501

DO - 10.1103/PhysRevLett.90.062501

M3 - Article

AN - SCOPUS:85038312592

SN - 0031-9007

VL - 90

SP - 4

JO - Physical review letters

JF - Physical review letters

IS - 6

ER -

Determination of the Subthreshold State Contribution in [Formula presented], the Main Neutron-Source Reaction for the [Formula presented] Process

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this