Pregled bibliografske jedinice broj: 1036437
Fusion Hindrance and Pauli Blocking in 58Ni + 64Ni
Fusion Hindrance and Pauli Blocking in 58Ni + 64Ni // EPJ Web of Conferences / de Angelis, G. ; Corradi, L (ur.).
Venecija, Italija, 2019. 01062, 4 doi:10.1051/epjconf/201922301062 (predavanje, međunarodna recenzija, sažetak, znanstveni)
CROSBI ID: 1036437 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Fusion Hindrance and Pauli Blocking in 58Ni + 64Ni
Autori
Stefanini, Alberto M. ; Montagnoli, Giovanna ; Del Fabbro, Mirco ; Colucci, Giulia ; Čolović, Petra ; Corradi, Lorenzo ; Fioretto, Enrico ; Galtarossa, Franco ; Goasduff, Alain ; Grebosz, Jerzy ; Heine, Marcel ; Jaworski, Grzegorz ; Mazzocco, Marco ; Mijatović, Tea ; Szilner, Suzana ; Bajzek, Martin ; Brugnara, Daniele ; Siciliano, Marco ; Zanon, Irene
Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, znanstveni
Izvornik
EPJ Web of Conferences
/ De Angelis, G. ; Corradi, L - , 2019
ISBN
978-2-7598-9084-2
Skup
4th International Conference on Nuclear Structure and Dynamics (NSD 2019)
Mjesto i datum
Venecija, Italija, 12.05.2019. - 17.05.2019
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
heavy-ion reactions ; fusion reaction
Sažetak
58Ni +64Ni is the first case where the influence of positive Q-value transfer channels on sub-barrier fusion was evidenced, in a very well known experiment by Beckerman et al., by comparing with the two systems 58Ni + 58Ni and 64Ni+64Ni. Subsequent measurements on 64Ni + 64Ni showed that fusion hindrance is clearly present in this case. On the other hand, no indication of hindrance can be observed for 58Ni + 64Ni down to the measured level of 0.1 mb. In the present experiment the excitation function has been extended by two orders of magnitude downward. The cross sections for 58Ni + 64Ni continue decreasing very smoothly below the barrier, down to '1 µb. The logarithmic slope of the excitation function increases slowly, showing a tendency to saturate at the lowest energies. No maximum of the astrophysical S -factor is observed. Coupled-channels (CC) calculations using a Woods-Saxon potential and includinginelastic excitations only, underestimate the sub-barrier cross sections by a large amount. Good agreement is found by adding two-neutron transfer couplings to a schematical level. This behaviour is quite different from what already observed for 64Ni+ 64Ni (no positive Q-value transfer channels available), where a clear low-energy maximum of the S -factorappears, and whose excitation function is overestimated by a standard Woods-Saxon CC calculation. No hindrance effect is observed in 58Ni+ 64Ni in the measured energy range. This trend at deep sub-barrier energies reinforces the recent suggestion that the availability of several states following transfer with Q>0, effectively counterbalances the Pauli repulsion that, in general, is predicted to reduce tunneling probability inside the Coulomb barrier.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
HRZZ-IP-2018-01-1257 - Zemljovid atomskih jezgara - neutronski bogata strana (NeRiS-Land) (Szilner, Suzana, HRZZ - 2018-01) ( CroRIS)
Ustanove:
Institut "Ruđer Bošković", Zagreb
Poveznice na cjeloviti tekst rada:
Pristup cjelovitom tekstu rada doi doi.org www.epj-conferences.org fulir.irb.hrCitiraj ovu publikaciju:
Časopis indeksira:
- Scopus