The Al-27(p, alpha)Mg-24 reaction at astrophysical energies studied by means of the Trojan Horse Method applied to the H-2(Al-27, alpha Mg-24)n reaction
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F21%3A00545624" target="_blank" >RIV/61389005:_____/21:00545624 - isvavai.cz</a>
Výsledek na webu
<a href="https://doi.org/10.1140/epjp/s13360-021-01872-4" target="_blank" >https://doi.org/10.1140/epjp/s13360-021-01872-4</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1140/epjp/s13360-021-01872-4" target="_blank" >10.1140/epjp/s13360-021-01872-4</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
The Al-27(p, alpha)Mg-24 reaction at astrophysical energies studied by means of the Trojan Horse Method applied to the H-2(Al-27, alpha Mg-24)n reaction
Popis výsledku v původním jazyce
The Al-27(p, alpha)Mg-24 reaction, which drives the destruction of Al-27 and the production of Mg-24 in stellar hydrogen burning, has been investigated via the Trojan Horse Method (THM), by measuring the H-2(Al-27, alpha Mg-24)n three-body reaction. The experiment covered a broad energy range (E-c.m. <= 1.5 MeV), aiming to investigate those of interest for astrophysics. The results confirm the THM as a valuable technique for the experimental study of fusion reactions at very low energies and suggest the presence of a rich pattern of resonances in the energy region close to the Gamow window of stellar hydrogen burning (70-120 keV), with potential impact on astrophysics. To estimate such an impact a second run of the experiment is needed, since the background due the three-body reaction hampered to collect enough data to resolve the resonant structures and extract the reaction rate.
Název v anglickém jazyce
The Al-27(p, alpha)Mg-24 reaction at astrophysical energies studied by means of the Trojan Horse Method applied to the H-2(Al-27, alpha Mg-24)n reaction
Popis výsledku anglicky
The Al-27(p, alpha)Mg-24 reaction, which drives the destruction of Al-27 and the production of Mg-24 in stellar hydrogen burning, has been investigated via the Trojan Horse Method (THM), by measuring the H-2(Al-27, alpha Mg-24)n three-body reaction. The experiment covered a broad energy range (E-c.m. <= 1.5 MeV), aiming to investigate those of interest for astrophysics. The results confirm the THM as a valuable technique for the experimental study of fusion reactions at very low energies and suggest the presence of a rich pattern of resonances in the energy region close to the Gamow window of stellar hydrogen burning (70-120 keV), with potential impact on astrophysics. To estimate such an impact a second run of the experiment is needed, since the background due the three-body reaction hampered to collect enough data to resolve the resonant structures and extract the reaction rate.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
<a href="/cs/project/EF16_013%2F0001679" target="_blank" >EF16_013/0001679: SPIRAL2 - Systeme de Production d´Ions Radioactifs Accélérés en Ligne - účast České republiky - OP</a><br>
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2021
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
European Physical Journal Plus
ISSN
2190-5444
e-ISSN
2190-5444
Svazek periodika
136
Číslo periodika v rámci svazku
9
Stát vydavatele periodika
DE - Spolková republika Německo
Počet stran výsledku
12
Strana od-do
898
Kód UT WoS článku
000692396700005
EID výsledku v databázi Scopus
2-s2.0-85114030768