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

dc.contributor.author	Fujii T.
dc.contributor.author	Moynier F.
dc.contributor.author	Albarède F.
dc.date.accessioned	2024-11-17T03:30:19Z
dc.date.available	2024-11-17T03:30:19Z
dc.date.issued	2006
dc.identifier	https://www.elibrary.ru/item.asp?id=14072231
dc.identifier.citation	Earth and Planetary Science Letters, 2006, 247, 1-2, 1-9
dc.identifier.issn	0012-821X
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/46561
dc.description.abstract	Even 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.subject	FUN
dc.subject	ISOTOPE ANOMALIES
dc.subject	MASS-INDEPENDENT
dc.subject	NUCLEAR FIELD
dc.subject	NUCLEOSYNTHESIS
dc.title	NUCLEAR FIELD VS. NUCLEOSYNTHETIC EFFECTS AS CAUSE OF ISOTOPIC ANOMALIES IN THE EARLY SOLAR SYSTEM
dc.type	Статья
dc.identifier.doi	10.1016/j.epsl.2006.04.034

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