NUCLEAR FIELD VS. NUCLEOSYNTHETIC EFFECTS AS CAUSE OF ISOTOPIC ANOMALIES IN THE EARLY SOLAR SYSTEM

dc.contributor.authorFujii T.
dc.contributor.authorMoynier F.
dc.contributor.authorAlbarède F.
dc.date.accessioned2024-11-17T03:30:19Z
dc.date.available2024-11-17T03:30:19Z
dc.date.issued2006
dc.description.abstractEven in the absence of nucleosynthesis, mass-independent isotope effect due to nuclear field can lead to a number of isotope anomalies found in refractory inclusions of chondrites. Isotope anomalies observed for Ba, Ca, Sr, Ti, and Cr in FUN inclusions may simply be explained by the nuclear field effects of these elements. A whole class of isotopic heterogeneities may therefore reflect evaporation/condensation processes in the solar nebula rather than nucleosynthetic effects. We speculate that the current estimates of the r-process component of the normal solar material may be affected by non-mass dependent fractionation effects. © 2006 Elsevier B.V. All rights reserved.
dc.identifierhttps://www.elibrary.ru/item.asp?id=14072231
dc.identifier.citationEarth and Planetary Science Letters, 2006, 247, 1-2, 1-9
dc.identifier.doi10.1016/j.epsl.2006.04.034
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/46561
dc.subjectFUN
dc.subjectISOTOPE ANOMALIES
dc.subjectMASS-INDEPENDENT
dc.subjectNUCLEAR FIELD
dc.subjectNUCLEOSYNTHESIS
dc.titleNUCLEAR FIELD VS. NUCLEOSYNTHETIC EFFECTS AS CAUSE OF ISOTOPIC ANOMALIES IN THE EARLY SOLAR SYSTEM
dc.typeСтатья

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