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Pregled bibliografske jedinice broj: 1047243

New Thermonuclear 10B(α, p)13C Rate and Its Astrophysical Implication in the νp-process


Zhang, L. Y.; He, J. J.; Wanajo, S.; Dell’Aquila, Daniele; Kubono, S.; Zhao, G.
New Thermonuclear 10B(α, p)13C Rate and Its Astrophysical Implication in the νp-process // The Astrophysical journal, 868 (2018), 1; 24, 11 doi:10.3847/1538-4357/aae479 (međunarodna recenzija, članak, ostalo)


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Naslov
New Thermonuclear 10B(α, p)13C Rate and Its Astrophysical Implication in the νp-process

Autori
Zhang, L. Y. ; He, J. J. ; Wanajo, S. ; Dell’Aquila, Daniele ; Kubono, S. ; Zhao, G.

Izvornik
The Astrophysical journal (0004-637X) 868 (2018), 1; 24, 11

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, ostalo

Ključne riječi
Nuclear Astrophysics

Sažetak
We have derived a new thermonuclear rate with an associated uncertainty for the 10B(α, p)13C reaction by evaluating the available experimental data for the first time. We provide this rate with a much smaller uncertainty than that estimated in the literature. Our rate differs significantly from the theoretical rates adopted in the current reaction rate libraries. Utilizing this new rate, we have investigated its astrophysical implications on the heavy-element (especially, p-nuclei) production in the νp- process in a stellar model of the neutrino-driven wind of type II core-collapse supernova. It shows that our rate with a much smaller uncertainty strongly constrains the nucleosynthetic results of the light p-nulcei with A ∼ 80-100. In addition, it shows that the difference between observed and predicted abundances for light p- nuclei is quite large, implying either that the present stellar model still needs modification or that additional astrophysical sources are required to account for the origin of some p- nuclei, such as 92Mo and 94Mo.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Profili:

Avatar Url Daniele Dell'Aquila (autor)

Poveznice na cjeloviti tekst rada:

doi iopscience.iop.org

Citiraj ovu publikaciju:

Zhang, L. Y.; He, J. J.; Wanajo, S.; Dell’Aquila, Daniele; Kubono, S.; Zhao, G.
New Thermonuclear 10B(α, p)13C Rate and Its Astrophysical Implication in the νp-process // The Astrophysical journal, 868 (2018), 1; 24, 11 doi:10.3847/1538-4357/aae479 (međunarodna recenzija, članak, ostalo)
Zhang, L., He, J., Wanajo, S., Dell’Aquila, D., Kubono, S. & Zhao, G. (2018) New Thermonuclear 10B(α, p)13C Rate and Its Astrophysical Implication in the νp-process. The Astrophysical journal, 868 (1), 24, 11 doi:10.3847/1538-4357/aae479.
@article{article, author = {Zhang, L. Y. and He, J. J. and Wanajo, S. and Dell’Aquila, Daniele and Kubono, S. and Zhao, G.}, year = {2018}, pages = {11}, DOI = {10.3847/1538-4357/aae479}, chapter = {24}, keywords = {Nuclear Astrophysics}, journal = {The Astrophysical journal}, doi = {10.3847/1538-4357/aae479}, volume = {868}, number = {1}, issn = {0004-637X}, title = {New Thermonuclear 10B(α, p)13C Rate and Its Astrophysical Implication in the νp-process}, keyword = {Nuclear Astrophysics}, chapternumber = {24} }
@article{article, author = {Zhang, L. Y. and He, J. J. and Wanajo, S. and Dell’Aquila, Daniele and Kubono, S. and Zhao, G.}, year = {2018}, pages = {11}, DOI = {10.3847/1538-4357/aae479}, chapter = {24}, keywords = {Nuclear Astrophysics}, journal = {The Astrophysical journal}, doi = {10.3847/1538-4357/aae479}, volume = {868}, number = {1}, issn = {0004-637X}, title = {New Thermonuclear 10B(α, p)13C Rate and Its Astrophysical Implication in the νp-process}, keyword = {Nuclear Astrophysics}, chapternumber = {24} }

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


Citati:





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