Towards a comprehensive study of the $$^{14}$$N(p,$$\gamma $$)$$^{15}$$O astrophysical key reaction: Description of the experimental technique including novel target preparation

Abstract While the $$^{14}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>14</mml:mn> </mml:mmultiscripts> </mml:math> N(p, $$\gamma $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>γ</mml:mi> </mml:math> ) $$^{15}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>15</mml:mn> </mml:mmultiscripts> </mml:math> O reaction plays a key role in the hydrogen-burning processes in various stellar conditions, its reaction rate is not known with sufficient precision. Therefore, the first scientific project at the recently launched Bellotti Ion Beam Facility of the Laboratori Nazionali del Gran Sasso was the measurement of the $$^{14}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>14</mml:mn> </mml:mmultiscripts> </mml:math> N(p, $$\gamma $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>γ</mml:mi> </mml:math> ) $$^{15}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>15</mml:mn> </mml:mmultiscripts> </mml:math> O reaction cross section in the proton energy range between 250 and 1500 keV. In this paper, the experimental techniques are summarized with special emphasis on the description of solid state nitrogen target production and characterization. The first results of the reaction yield measured at 55 $$^\circ $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mo>∘</mml:mo> </mml:mmultiscripts> </mml:math> detection angle are also presented.

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Journal
The European Physical Journal A
Published
2025-08-15
DOI
https://doi.org/10.1140/epja/s10050-025-01658-7
Citations
1
Primary Topic
Advanced Chemical Physics Studies
Type
article
Field-Weighted Citation Impact
1.25

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article

Towards a comprehensive study of the $$^{14}$$N(p,$$\gamma $$)$$^{15}$$O astrophysical key reaction: Description of the experimental technique including novel target preparation

F. Ferraro, L. Csedreki, C. Gustavino, L. Schiavulli et al.
1 citations
The European Physical Journal A
Advanced Chemical Physics Studies
1.25
article

Towards a comprehensive study of the $$^{14}$$N(p,$$\gamma $$)$$^{15}$$O astrophysical key reaction: Description of the experimental technique including novel target preparation

F. Ferraro, L. Csedreki, C. Gustavino, L. Schiavulli, R. S. Sidhu, A. Boeltzig, P. Colombetti, D. Rapagnani, P. Corvisiero, R. Menegazzo, D. Piatti, S. Turkat, O. Straniero, C. Ananna, M. Junker, G. F. Ciani, D. Bemmerer, J. Marsh, Z. Elekes, Fausto Casaburo, G. Imbriani, T. Szücs, D. Robb, E. Masha, Andreas Best, A. Compagnucci, F. Cavanna, C. Broggini, A. Caciolli, S. Zavatarelli, Antonino Di Leva, Gy. Gyürky, J. Skowronski, Paola Marigo, A. Guglielmetti, A. Formicola, V. Paticchio, M. Aliotta, Matteo Campostrini, C. G. Bruno, Zsolt Fülöp, P. Prati, J. Cruz, R. Depalo, L. Barbieri, V. Rigato, F. Barile, T. Davinson, M. Lugaro
article en
1 citations

Abstract

Abstract While the $$^{14}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>14</mml:mn> </mml:mmultiscripts> </mml:math> N(p, $$\gamma $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>γ</mml:mi> </mml:math> ) $$^{15}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>15</mml:mn> </mml:mmultiscripts> </mml:math> O reaction plays a key role in the hydrogen-burning processes in various stellar conditions, its reaction rate is not known with sufficient precision. Therefore, the first scientific project at the recently launched Bellotti Ion Beam Facility of the Laboratori Nazionali del Gran Sasso was the measurement of the $$^{14}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>14</mml:mn> </mml:mmultiscripts> </mml:math> N(p, $$\gamma $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>γ</mml:mi> </mml:math> ) $$^{15}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>15</mml:mn> </mml:mmultiscripts> </mml:math> O reaction cross section in the proton energy range between 250 and 1500 keV. In this paper, the experimental techniques are summarized with special emphasis on the description of solid state nitrogen target production and characterization. The first results of the reaction yield measured at 55 $$^\circ $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mo>∘</mml:mo> </mml:mmultiscripts> </mml:math> detection angle are also presented.

The European Physical Journal AVol. 61(8)
Eötvös Loránd University (HU), University of Padua (IT), Istituto Nazionale di Fisica Nucleare (IT), HUN-REN Institute for Nuclear Research (HU), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso (IT), Helmholtz-Zentrum Dresden-Rossendorf (DE), Konkoly Observatory (HU), University of Surrey (GB), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Padova (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Bari (IT), Collurania Teramo Observatory (IT), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Genova (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Milano (IT), Gran Sasso Science Institute (IT), University of Turin (IT), University of Bari Aldo Moro (IT), University of Naples Federico II (IT), Universidade Nova de Lisboa (PT), University of Genoa (IT), University of Edinburgh (GB)
Alexander von Humboldt-Stiftung, Nemzeti Kutatási Fejlesztési és Innovációs Hivatal, Fundação para a Ciência e a Tecnologia
Openalex Percentile: Top 18%
Advanced Chemical Physics Studies
1.25
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