prikaz prve stranice dokumenta Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis
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Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis
Physics Letters B, 790 (2019); 458-465. https://doi.org/10.1016/j.physletb.2019.01.045
(n_TOF Collaboration) Lederer-Woods, C.; ...; Bosnar, Damir; ...; Žugec, Petar

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Lederer Woods, C., Bosnar, D. i Žugec, P. (2019). Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis. Physics Letters B, 790., 458-465. doi: 10.1016/j.physletb.2019.01.045

Lederer Woods, C., et al. "Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis." Physics Letters B, vol. 790, 2019, str. 458-465. https://doi.org/10.1016/j.physletb.2019.01.045

Lederer Woods, C., Damir Bosnar i Petar Žugec. "Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis." Physics Letters B 790 (2019): 458-465. https://doi.org/10.1016/j.physletb.2019.01.045

Lederer Woods, C., Bosnar, D. i Žugec, P. (2019) 'Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis', Physics Letters B, 790, str. 458-465. doi: 10.1016/j.physletb.2019.01.045

Lederer Woods C, Bosnar D, Žugec P. Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis. Physics Letters B [Internet]. 2019. [pristupljeno 18.11.2024.];790:458-465. doi: 10.1016/j.physletb.2019.01.045

C. Lederer Woods, D. Bosnar i P. Žugec, "Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis", Physics Letters B, vol. 790, str. 458-465, 2019. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:229366. [Citirano: 18.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:229366
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Podaci o radu
Naslov (engleski)Measurement of 73Ge(n, γ) cross sections and implications for stellar nucleosynthesis
AutorC. Lederer-Woods
Autor
...
AutorDamir Bosnar
MBZ: 134936
Autor
...
AutorPetar Žugec
MBZ: 326085
Kolaboracijan_TOF Collaboration
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
73Ge(n, γ) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT=30 keV is 1.5 to 1.7 times higher than most theoretical predictions. The new cross sections result in a substantial decrease of 73Ge produced in stars, which would explain the low isotopic abundance of 73Ge in the solar system.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaPhysics Letters B
Brojčani podacivol. 790, str. 458-465
p-ISSN0370-2693
DOIhttps://doi.org/10.1016/j.physletb.2019.01.045
URN:NBNurn:nbn:hr:217:229366
Datum objave publikacije2019
URL dokumentahttps://www.sciencedirect.com/science/article/pii/S037026931930070X
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Imenovanje 4.0 međunarodna (CC BY 4.0)
Javna napomena© 2019 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3. Received 24 September 2018. Received in revised form 22 January 2019. Accepted 23 January 2019. Available online 30 January 2019. Published 10 March 2019.
Datum i vrijeme pohrane2020-08-26 18:35:25