Pregled bibliografske jedinice broj: 1145535
Destruction of the cosmic γ-ray emitter 26Al in massive stars: Study of the key 26Al(n,α) reaction
Destruction of the cosmic γ-ray emitter 26Al in massive stars: Study of the key 26Al(n,α) reaction // Physical review. C, 104 (2021), L032803, 6 doi:10.1103/PhysRevC.104.L032803 (međunarodna recenzija, pismo, znanstveni)
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Naslov
Destruction of the cosmic γ-ray emitter 26Al in massive stars: Study of the key 26Al(n,α) reaction
Autori
Lederer-Woods, C. ; ... ; Bosnar, Damir ; ... ; Žugec, Petar
Kolaboracija
N_TOF Collaboration
Izvornik
Physical review. C (2469-9985) 104
(2021);
L032803, 6
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, pismo, znanstveni
Ključne riječi
26Al(n, α) reaction, n_TOF, neutron time of flight, stellar nucleosynthesis
Sažetak
Neutron destruction reactions of the cosmic γ-ray emitter 26Al are of importance to determine the amount of 26Al ejected into our galaxy by supernova explosions and for 26Al production in asymptotic giant branch stars. We performed a new measurement of the 26Al(n, α) reaction up to 160-keV neutron energy at the neutron time-of-flight facilities n_TOF at CERN and GELINA at EC-JRC. We provide strengths for ten resonances, six of them for the first time. We use our data to calculate astrophysical reactivities for stellar temperatures up to 0.7 GK. Our results resolve a discrepancy between the two previous direct measurements of this reaction, and indicate higher stellar destruction rates than the most recently recommended reactivity.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Prirodoslovno-matematički fakultet, Zagreb
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus