Astrophysical S-factor of the 12N(p,γ)13O reaction in Relation to population III star evolution

A. Banu; T. Al.-Abdullah; V. Burjan; F. Carstoiu; C. Fu; C. A. Gagliardi; M. McCleskey; G. Tabacaru; L. Trache; R. E. Tribble; Y. Zhai

doi:10.1063/1.2905579

Astrophysical S-factor of the ¹²N(p,γ)¹³O reaction in Relation to population III star evolution

A. Banu^*
, T. Al.-Abdullah
, V. Burjan
, F. Carstoiu
, C. Fu
, C. A. Gagliardi
, M. McCleskey
, G. Tabacaru
, L. Trache
, R. E. Tribble
, Y. Zhai

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

The reaction cross section for the direct radiative proton capture on the the drip line nucleus ¹²N - ¹²N(p,γ)¹³O - was studied at the Cyclotron Institute/Texas A&M University using the indirect asymptotic normalization coefficient method. This reaction is important in the hot pp chain nuclear burning processes in hydrogen-rich massive objects (Population III stars). The astrophysical S-factor of the direct proton capture was determined at zero energy yielding a value of S^DC _1-12=0.31(5)keVb. Interference between direct and resonant capture leads to a further enhancement of a factor of two.

Original language	English
Title of host publication	First Stars III
Publisher	American Institute of Physics Inc.
Pages	347-349
Number of pages	3
ISBN (Print)	9780735405097
DOIs	https://doi.org/10.1063/1.2905579
State	Published - 2008
Externally published	Yes

Publication series

Name	AIP Conference Proceedings
Volume	990
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Keywords

ANC
DWBA
Population III stars
Radiative proton capture

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1063/1.2905579

Cite this

Banu, A., Al.-Abdullah, T., Burjan, V., Carstoiu, F., Fu, C., Gagliardi, C. A., McCleskey, M., Tabacaru, G., Trache, L., Tribble, R. E., & Zhai, Y. (2008). Astrophysical S-factor of the ¹²N(p,γ)¹³O reaction in Relation to population III star evolution. In First Stars III (pp. 347-349). (AIP Conference Proceedings; Vol. 990). American Institute of Physics Inc.. https://doi.org/10.1063/1.2905579

@inproceedings{4b3660e8fe764dd1a04c648ab3ae3d1c,

title = "Astrophysical S-factor of the 12N(p,γ)13O reaction in Relation to population III star evolution",

abstract = "The reaction cross section for the direct radiative proton capture on the the drip line nucleus 12N - 12N(p,γ)13O - was studied at the Cyclotron Institute/Texas A\&M University using the indirect asymptotic normalization coefficient method. This reaction is important in the hot pp chain nuclear burning processes in hydrogen-rich massive objects (Population III stars). The astrophysical S-factor of the direct proton capture was determined at zero energy yielding a value of SDC 1-12=0.31(5)keVb. Interference between direct and resonant capture leads to a further enhancement of a factor of two.",

keywords = "ANC, DWBA, Population III stars, Radiative proton capture",

author = "A. Banu and T. Al.-Abdullah and V. Burjan and F. Carstoiu and C. Fu and Gagliardi, \{C. A.\} and M. McCleskey and G. Tabacaru and L. Trache and Tribble, \{R. E.\} and Y. Zhai",

year = "2008",

doi = "10.1063/1.2905579",

language = "English",

isbn = "9780735405097",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics Inc.",

pages = "347--349",

booktitle = "First Stars III",

}

Banu, A, Al.-Abdullah, T, Burjan, V, Carstoiu, F, Fu, C, Gagliardi, CA, McCleskey, M, Tabacaru, G, Trache, L, Tribble, RE & Zhai, Y 2008, Astrophysical S-factor of the ¹²N(p,γ)¹³O reaction in Relation to population III star evolution. in First Stars III. AIP Conference Proceedings, vol. 990, American Institute of Physics Inc., pp. 347-349. https://doi.org/10.1063/1.2905579

TY - GEN

T1 - Astrophysical S-factor of the 12N(p,γ)13O reaction in Relation to population III star evolution

AU - Banu, A.

AU - Al.-Abdullah, T.

AU - Burjan, V.

AU - Carstoiu, F.

AU - Fu, C.

AU - Gagliardi, C. A.

AU - McCleskey, M.

AU - Tabacaru, G.

AU - Trache, L.

AU - Tribble, R. E.

AU - Zhai, Y.

PY - 2008

Y1 - 2008

N2 - The reaction cross section for the direct radiative proton capture on the the drip line nucleus 12N - 12N(p,γ)13O - was studied at the Cyclotron Institute/Texas A&M University using the indirect asymptotic normalization coefficient method. This reaction is important in the hot pp chain nuclear burning processes in hydrogen-rich massive objects (Population III stars). The astrophysical S-factor of the direct proton capture was determined at zero energy yielding a value of SDC 1-12=0.31(5)keVb. Interference between direct and resonant capture leads to a further enhancement of a factor of two.

AB - The reaction cross section for the direct radiative proton capture on the the drip line nucleus 12N - 12N(p,γ)13O - was studied at the Cyclotron Institute/Texas A&M University using the indirect asymptotic normalization coefficient method. This reaction is important in the hot pp chain nuclear burning processes in hydrogen-rich massive objects (Population III stars). The astrophysical S-factor of the direct proton capture was determined at zero energy yielding a value of SDC 1-12=0.31(5)keVb. Interference between direct and resonant capture leads to a further enhancement of a factor of two.

KW - ANC

KW - DWBA

KW - Population III stars

KW - Radiative proton capture

UR - https://www.scopus.com/pages/publications/42449163823

U2 - 10.1063/1.2905579

DO - 10.1063/1.2905579

M3 - Conference contribution

AN - SCOPUS:42449163823

SN - 9780735405097

T3 - AIP Conference Proceedings

SP - 347

EP - 349

BT - First Stars III

PB - American Institute of Physics Inc.

ER -