Measurement of the 27 Al( p , α) 24 Mg fusion reaction at astrophysical energies via the Trojan Hors...
Measurement of the 27 Al( p , α) 24 Mg fusion reaction at astrophysical energies via the Trojan Horse Method
About this item
Full title
Author / Creator
La Cognata, M. , Palmerini, S. , Adsley, P. , Hammache, F. , Di Pietro, A. , Figuera, P. , Dell ’Agli, F. , Alba, R. , Cherubini, S. , Guardo, G.L. , Gulino, M. , Lamia, L. , Lattuada, D. , Maiolino, C. , Oliva, A. , Pizzone, R.G. , Prajapati, P. , Rapisarda, G.G. , Romano, S. , Santonocito, D. , Spartà, R. , Sergi, M.L. , Tumino, A. and Ventura, P.
Journal title
Language
English
Formats
More information
Scope and Contents
Contents
In astrophysics, the abundance of
26
Al is essential for understanding nucleosynthesis in the Milky Way and Galactic core-collapse supernovae rates. Detection methods involve γ-ray lines and comparing
26
Mg overabundance with the common Mg isotope in meteorites. Therefore, stable isotopes
27
Al and
24
Mg play a crucial role...
Alternative Titles
Full title
Measurement of the 27 Al( p , α) 24 Mg fusion reaction at astrophysical energies via the Trojan Horse Method
Authors, Artists and Contributors
Author / Creator
Palmerini, S.
Adsley, P.
Hammache, F.
Di Pietro, A.
Figuera, P.
Dell ’Agli, F.
Alba, R.
Cherubini, S.
Guardo, G.L.
Gulino, M.
Lamia, L.
Lattuada, D.
Maiolino, C.
Oliva, A.
Pizzone, R.G.
Prajapati, P.
Rapisarda, G.G.
Romano, S.
Santonocito, D.
Spartà, R.
Sergi, M.L.
Tumino, A.
Ventura, P.
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_crossref_primary_10_1051_epjconf_202430601010
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_crossref_primary_10_1051_epjconf_202430601010
Other Identifiers
ISSN
2100-014X
E-ISSN
2100-014X
DOI
10.1051/epjconf/202430601010
