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Pregled bibliografske jedinice broj: 1049103

The 10B(p, α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method

Puglia, Sebastiana Maria Regina; Spitaleri, Claudio; La Cognata, Marco; Lamia, Livio; Broggini, Carlo; Caciolli, Antonio; Carlin, Nelson; Cherubini, Silvio; Cvetinovic, Alexandra; D’Agata, Giuseppe et al.
The 10B(p, α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method // EPJ Web of Conferences 165, Nuclear Physics in Astrophysics VIII (NPA8 2017)
Catania, Italija, 2017. 01042, 4 doi:10.1051/epjconf/201716501042 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)

CROSBI ID: 1049103 Za ispravke kontaktirajte CROSBI podršku putem web obrasca

Naslov
The 10B(p, α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method

Autori
Puglia, Sebastiana Maria Regina ; Spitaleri, Claudio ; La Cognata, Marco ; Lamia, Livio ; Broggini, Carlo ; Caciolli, Antonio ; Carlin, Nelson ; Cherubini, Silvio ; Cvetinovic, Alexandra ; D’Agata, Giuseppe ; Dell’Aquila, Daniele ; Depalo, Rosanna ; Gulino, Marisa ; Guardo, Giovanni Luca ; Indelicato, Iolanda ; Lombardo, Ivano ; Menegazzo, Roberto ; Munhoz, Marcelo Gimenez ; Pizzone, Rosario Gianluca ; Rapisarda, Giuseppe Gabriele ; Rigato, Valentino ; Romano, Stefano ; Sergi, Maria Letizia ; Souza, Francisco ; Sparta, Roberta ; Tudisco, Salvo ; Tumino, Aurora

Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni

Izvornik
EPJ Web of Conferences 165, Nuclear Physics in Astrophysics VIII (NPA8 2017) / - , 2017

Skup
8th International Conference on Nuclear Physics in Astrophysics(NPA8 2017)

Mjesto i datum
Catania, Italija, 18.06.2017. - 23.06.2017

Vrsta sudjelovanja
Poster

Vrsta recenzije
Međunarodna recenzija

Ključne riječi
Nuclear astrophysics ; trojan horse method

Sažetak
The 10B(p, α)7Be reaction is the main responsible for the 10B destruction in stellar interior [1]. In such environments this p-capture process occurs at a Gamow energy of 10 keV and takes places mainly through a resonant state (Ex = 8.701 MeV) of the compound 11C nucleus. Thus a resonance right in the region of the Gamow peak is expected to significantly influence the behavior of the astrophysical S(E)-factor. The 10B(p, α)7Be reaction was studied via the Trojan Horse Method (THM) applied to the 2H(10B, α7Be)n in order to extract the astrophysical S(E)-factor in a wide energy range from 5 keV to 1.5 MeV.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA

Profili:

Avatar Url Daniele Dell'Aquila (autor)

Poveznice na cjeloviti tekst rada:

doi www.epj-conferences.org doi.org

Citiraj ovu publikaciju:

Puglia, Sebastiana Maria Regina; Spitaleri, Claudio; La Cognata, Marco; Lamia, Livio; Broggini, Carlo; Caciolli, Antonio; Carlin, Nelson; Cherubini, Silvio; Cvetinovic, Alexandra; D’Agata, Giuseppe et al.
The 10B(p, α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method // EPJ Web of Conferences 165, Nuclear Physics in Astrophysics VIII (NPA8 2017)
Catania, Italija, 2017. 01042, 4 doi:10.1051/epjconf/201716501042 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
Puglia, S., Spitaleri, C., La Cognata, M., Lamia, L., Broggini, C., Caciolli, A., Carlin, N., Cherubini, S., Cvetinovic, A. & D’Agata, G. (2017) The 10B(p, α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method. U: EPJ Web of Conferences 165, Nuclear Physics in Astrophysics VIII (NPA8 2017) doi:10.1051/epjconf/201716501042.
@article{article, author = {Puglia, Sebastiana Maria Regina and Spitaleri, Claudio and La Cognata, Marco and Lamia, Livio and Broggini, Carlo and Caciolli, Antonio and Carlin, Nelson and Cherubini, Silvio and Cvetinovic, Alexandra and D’Agata, Giuseppe and Dell’Aquila, Daniele and Depalo, Rosanna and Gulino, Marisa and Guardo, Giovanni Luca and Indelicato, Iolanda and Lombardo, Ivano and Menegazzo, Roberto and Munhoz, Marcelo Gimenez and Pizzone, Rosario Gianluca and Rapisarda, Giuseppe Gabriele and Rigato, Valentino and Romano, Stefano and Sergi, Maria Letizia and Souza, Francisco and Sparta, Roberta and Tudisco, Salvo and Tumino, Aurora}, year = {2017}, pages = {4}, DOI = {10.1051/epjconf/201716501042}, chapter = {01042}, keywords = {Nuclear astrophysics, trojan horse method}, doi = {10.1051/epjconf/201716501042}, title = {The 10B(p, α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method}, keyword = {Nuclear astrophysics, trojan horse method}, publisherplace = {Catania, Italija}, chapternumber = {01042} }
@article{article, author = {Puglia, Sebastiana Maria Regina and Spitaleri, Claudio and La Cognata, Marco and Lamia, Livio and Broggini, Carlo and Caciolli, Antonio and Carlin, Nelson and Cherubini, Silvio and Cvetinovic, Alexandra and D’Agata, Giuseppe and Dell’Aquila, Daniele and Depalo, Rosanna and Gulino, Marisa and Guardo, Giovanni Luca and Indelicato, Iolanda and Lombardo, Ivano and Menegazzo, Roberto and Munhoz, Marcelo Gimenez and Pizzone, Rosario Gianluca and Rapisarda, Giuseppe Gabriele and Rigato, Valentino and Romano, Stefano and Sergi, Maria Letizia and Souza, Francisco and Sparta, Roberta and Tudisco, Salvo and Tumino, Aurora}, year = {2017}, pages = {4}, DOI = {10.1051/epjconf/201716501042}, chapter = {01042}, keywords = {Nuclear astrophysics, trojan horse method}, doi = {10.1051/epjconf/201716501042}, title = {The 10B(p, α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method}, keyword = {Nuclear astrophysics, trojan horse method}, publisherplace = {Catania, Italija}, chapternumber = {01042} }

Časopis indeksira:


  • Web of Science Core Collection (WoSCC)
    • Conference Proceedings Citation Index - Science (CPCI-S)
  • Scopus

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