F. Terrasi
Ruhr University Bochum
Network
Latest external collaboration on country level. Dive into details by clicking on the dots.
Publication
Featured researches published by F. Terrasi.
European Physical Journal A | 2005
D. Schürmann; A. Di Leva; L. Gialanella; Detlef Rogalla; F. Strieder; N. De Cesare; A. D'Onofrio; G. Imbriani; R. Kunz; Carmine Lubritto; A. Ordine; V. Roca; C. Rolfs; M. Romano; F. Schümann; F. Terrasi; H. P. Trautvetter
Abstract.The total cross-section of 12C(α,γ)16O was measured for the first time by a direct and ungated detection of the 16O recoils. This measurement in inverse kinematics using the recoil mass separator ERNA in combination with a windowless He gas target allowed to collect data with high precision in the energy range E = 1.9 to 4.9 MeV. The data represent new information for the determination of the astrophysical S(E) factor.The total cross-section of 12C(α,γ)16O was measured for the first time by a direct and ungated detection of the 16O recoils. This measurement in inverse kinematics using the recoil mass separator ERNA in combination with a windowless He gas target allowed to collect data with high precision in the energy range E = 1.9 to 4.9 MeV. The data represent new information for the determination of the astrophysical S(E) factor.
arXiv: Nuclear Experiment | 2005
D. Schuermann; A. Di Leva; L. Gialanella; Detlef Rogalla; F. Strieder; N. De Cesare; A. D'Onofrio; G. Imbriani; R. Kunz; Carmine Lubritto; A. Ordine; V. Roca; C. Rolfs; M. Romano; F. Schuemann; F. Terrasi; H. P. Trautvetter
Abstract.The total cross-section of 12C(α,γ)16O was measured for the first time by a direct and ungated detection of the 16O recoils. This measurement in inverse kinematics using the recoil mass separator ERNA in combination with a windowless He gas target allowed to collect data with high precision in the energy range E = 1.9 to 4.9 MeV. The data represent new information for the determination of the astrophysical S(E) factor.The total cross-section of 12C(α,γ)16O was measured for the first time by a direct and ungated detection of the 16O recoils. This measurement in inverse kinematics using the recoil mass separator ERNA in combination with a windowless He gas target allowed to collect data with high precision in the energy range E = 1.9 to 4.9 MeV. The data represent new information for the determination of the astrophysical S(E) factor.
European Physical Journal A | 2009
A. Caciolli; L. Agostino; D. Bemmerer; R. Bonetti; C. Broggini; F. Confortola; P. Corvisiero; H. Costantini; Z. Elekes; A. Formicola; Zs. Fülöp; G. Gervino; A. Guglielmetti; C. Gustavino; Gy. Gyürky; G. Imbriani; M. Junker; M. Laubenstein; A. Lemut; B. Limata; M. Marta; C. Mazzocchi; R. Menegazzo; P. Prati; V. Roca; C. Rolfs; C. Rossi Alvarez; E. Somorjai; O. Straniero; F. Strieder
Ultra-sensitive in-beam
The Astrophysical Journal | 2013
O. Straniero; G. Imbriani; F. Strieder; D. Bemmerer; C. Broggini; A. Caciolli; P. Corvisiero; Herve Costantini; S. Cristallo; A. DiLeva; A. Formicola; Z. Elekes; Zs. Fülöp; G. Gervino; A. Guglielmetti; C. Gustavino; G. Gyürky; M. Junker; A. Lemut; B. Limata; M. Marta; C. Mazzocchi; R. Menegazzo; Luciano Piersanti; P. Prati; V. Roca; C. Rolfs; C. Rossi Alvarez; E. Somorjai; F. Terrasi
\gamma
European Physical Journal A | 2012
A. Caciolli; D. A. Scott; A. Di Leva; A. Formicola; M. Aliotta; M. Anders; A. Bellini; D. Bemmerer; C. Broggini; M. Campeggio; P. Corvisiero; R. Depalo; Z. Elekes; Zs. Fülöp; G. Gervino; A. Guglielmetti; C. Gustavino; Gy. Gyürky; G. Imbriani; M. Junker; M. Marta; R. Menegazzo; E. Napolitani; P. Prati; V. Rigato; V. Roca; C. Rolfs; C. Rossi Alvarez; E. Somorjai; C. Salvo
-ray spectroscopy studies for nuclear astrophysics are performed at the LUNA (Laboratory for Underground Nuclear Astrophysics) 400 kV accelerator, deep underground in Italy’s Gran Sasso laboratory. By virtue of a specially constructed passive shield, the laboratory
Physical Review C | 2008
M. Marta; A. Formicola; G. Gyürky; D. Bemmerer; C. Broggini; A. Caciolli; P. Corvisiero; H. Costantini; Z. Elekes; Z. S. Fulop; G. Gervino; A. Guglielmetti; C. Gustavino; G. Imbriani; M. Junker; R. Kunz; A. Lemut; B. Limata; C. Mazzocchi; R. Menegazzo; P. Prati; V. Roca; C. Rolfs; M. Romano; C. R. Alvarez; E. Somorjai; O. Straniero; F. Strieder; F. Terrasi; H. P. Trautvetter
\gamma
European Physical Journal A | 2000
L. Gialanella; F. Strieder; L. Campajola; A. D'Onofrio; U. Greife; G. Gyürky; G. Imbriani; G. Oliviero; A. Ordine; V. Roca; C. Rolfs; M. Romano; Detlef Rogalla; C. Sabbarese; E. Somorjai; F. Terrasi; H. P. Trautvetter
-ray background for
European Physical Journal A | 2016
A. Boeltzig; C. G. Bruno; F. Cavanna; S. Cristallo; Thomas Davinson; R. Depalo; R. J. deBoer; A. Di Leva; F. Ferraro; G. Imbriani; P. Marigo; F. Terrasi; M. Wiescher
\ensuremath E_{\gamma}
European Physical Journal A | 1993
G. de Angelis; S. Lunardi; D. Bazzacco; J. Rico; F. Terrasi; M. Piiparinen; A. Atac; J. Nyberg
< 3 MeV at LUNA has been reduced to levels comparable to those experienced in dedicated offline underground
European Physical Journal A | 1992
G. de Angelis; D. Bazzacco; S. Lunardi; M. A. Cardona; M. De Poli; Yi-Xiao Guo; D. Ackermann; S. E. Arnell; A. Atac; S. Beghini; L. Corradi; A. D'Onofrio; D. Foltescu; E. Ideguchi; A. E. Nilsson; S. Mitarai; G. Montagnoli; H. Moreno; D. R. Napoli; V. Roca; H. A. Roth; F. Scarlassara; G. Segato; C. Signorini; O. Skeppstedt; P. Spolaore; A. M. Stefanini; F. Terrasi
\gamma
