prikaz prve stranice dokumenta Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis
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Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis
Physical Review Letters, 110 (2013), 2; 022501. https://doi.org/10.1103/PhysRevLett.110.022501
(n_TOF Collaboration) Lederer, C.; ...; Bosnar, Damir; ...; Žugec, Petar

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Lederer, C., Bosnar, D. i Žugec, P. (2013). Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis. Physical Review Letters, 110. (2). doi: 10.1103/PhysRevLett.110.022501

Lederer, C., et al. "Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis." Physical Review Letters, vol. 110, br. 2, 2013. https://doi.org/10.1103/PhysRevLett.110.022501

Lederer, C., Damir Bosnar i Petar Žugec. "Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis." Physical Review Letters 110, br. 2 (2013). https://doi.org/10.1103/PhysRevLett.110.022501

Lederer, C., Bosnar, D. i Žugec, P. (2013) 'Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis', Physical Review Letters, 110(2). doi: 10.1103/PhysRevLett.110.022501

Lederer C, Bosnar D, Žugec P. Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis. Physical Review Letters [Internet]. 2013. [pristupljeno 23.12.2024.];110(2). doi: 10.1103/PhysRevLett.110.022501

C. Lederer, D. Bosnar i P. Žugec, "Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis", Physical Review Letters, vol. 110, br. 2, 2013. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:796028. [Citirano: 23.12.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:796028
Podaci o radu
Naslov (engleski)Neutron capture cross section of unstable 63Ni : implications for stellar nucleosynthesis
AutorC. Lederer
Autor
...
AutorDamir Bosnar
MBZ: 134936
Autor
...
AutorPetar Žugec
Kolaboracijan_TOF Collaboration
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
The 63Ni(n ; gamma) cross section has been measured for the rst time at the neutron time-of- flight facility n_TOF at CERN from thermal neutron energies up to 200 keV. In total 16 resonances couldbe identi ed and capture kernels be determined for 14 of these resonances. Maxwellian averaged cross sections were calculated for thermal energies from kT = 5 keV to 90 keV with uncertainties around 20%. Stellar model calculations for a 25 M star show that the new data have a significant effect on the s-process production of 63Cu, 64Ni, and 64Zn in massive stars.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaPhysical Review Letters
Brojčani podacivol. 110, br. 2, 022501
p-ISSN0031-9007
e-ISSN1079-7114
DOIhttps://doi.org/10.1103/PhysRevLett.110.022501
URN:NBNurn:nbn:hr:217:796028
Datum objave publikacije2013
ProjektŠifra: 119-1191005-1021
Naziv (hrvatski): QCD i jezgre; primjena nuklearnih metoda:materijali,medicina,okoliš
Voditelj: Damir Bosnar
Pravna nadležnost: Hrvatska
Financijer: MZOS
Linija financiranja: ZP
URL dokumentahttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.110.022501
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomenaCopyright (2013) by the American Physical Society. Received 8 October 2012; published 8 January 2013.
Datum i vrijeme pohrane2019-11-24 12:30:02