C
Carmen Angulo
Researcher at Université catholique de Louvain
Publications - 80
Citations - 5220
Carmen Angulo is an academic researcher from Université catholique de Louvain. The author has contributed to research in topics: Elastic scattering & Big Bang nucleosynthesis. The author has an hindex of 26, co-authored 80 publications receiving 4902 citations. Previous affiliations of Carmen Angulo include University of Münster & Ruhr University Bochum.
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Journal ArticleDOI
A compilation of charged-particle induced thermonuclear reaction rates
Carmen Angulo,Marcel Arnould,Marc Rayet,Pierre Descouvemont,Daniel Jean Baye,Ch. Leclercq-Willain,Alain Coc,S. Barhoumi,P. Aguer,C. Rolfs,R. Kunz,J. W. Hammer,A. Mayer,T. Paradellis,S. Kossionides,C. Chronidou,K. Spyrou,Scilla Degl'Innocenti,Giovanni Fiorentini,Barbara Ricci,Sandra Zavatarelli,Constança Providência,Helmut Wolters,J. Soares,C. Grama,Javad Rahighi,A. C. Shotter,M. Lamehi Rachti +27 more
TL;DR: In this paper, the corresponding Maxwellian-averaged thermonuclear reaction rates of relevance in astrophysical plasmas at temperatures in the range from 10(6) K to 10(10) K were calculated.
Journal ArticleDOI
Astrophysical S-factor of 14N(p,γ) 15O
A. Formicola,Gianluca Imbriani,H. Costantini,Carmen Angulo,Daniel Bemmerer,R. Bonetti,C. Broggini,P. Corvisiero,João Cruz,Pierre Descouvemont,Zs. Fülöp,G. Gervino,A. Guglielmetti,C. Gustavino,Gy. Gyürky,A. P. Jesus,M. Junker,A. Lemut,R. Menegazzo,Paolo Prati,Vincenzo Roca,C. Rolfs,Mario R. Romano,C. Rossi Alvarez,F. Schümann,E. Somorjai,Oscar Straniero,Frank Strieder,Filippo Terrasi,H. P. Trautvetter,Alberto Vomiero,Sandra Zavatarelli +31 more
TL;DR: In this article, a new measurement of the 14N(p,γ) 15O capture cross section at Ep=140 to 400 keV using the 400 kV LUNA accelerator facility at the Laboratori Nazionali del Gran Sasso (LNGS) was reported.
Journal ArticleDOI
Updated Big Bang nucleosynthesis confronted to WMAP observations and to the abundance of light elements
TL;DR: In this article, the authors improved Standard Big Bang Nucleosynthesis (SBBN) calculations taking into account new nuclear physics analyses (Descouvemont et al. 2003) using a Monte-Carlo technique, calculating the abundances of light nuclei versus the baryon to photon ratio.
Journal ArticleDOI
Compilation and R-matrix analysis of Big Bang nuclear reaction rates
TL;DR: In this paper, the authors used the R-matrix theory to fit low-energy data on nuclear reactions involved in Big Bang nucleosynthesis, and provided S factors and reaction rates in tabular and graphical formats.
Journal ArticleDOI
S-factor of 14N(p,γ)15O at astrophysical energies⋆
Gianluca Imbriani,H. Costantini,A. Formicola,Alberto Vomiero,Carmen Angulo,Daniel Bemmerer,R. Bonetti,Carlo Broggini,F. Confortola,P. Corvisiero,João Cruz,Pierre Descouvemont,Zs. Fülöp,G. Gervino,A. Guglielmetti,C. Gustavino,Gy. Gyürky,A. P. Jesus,M. Junker,J. N. Klug,A. Lemut,R. Menegazzo,P. Prati,Vincenzo Roca,C. Rolfs,Mario R. Romano,C. Rossi-Alvarez,F. Schümann,D. Schürmann,E. Somorjai,Oscar Straniero,Frank Strieder,Filippo Terrasi,H. P. Trautvetter +33 more
TL;DR: In this paper, the astrophysical S(E) factor of 14N(p,γ)15O has been measured for effective center-of-mass energies between Eeff = 119 and 367 keV at the LUNA facility using TiN solid targets and Ge detectors.