CONTRIBUTION OF NEUTRON-CAPTURE REACTIONS TO OBSERVED TUNGSTEN ISOTOPIC RATIOS

dc.contributor.authorMasarik J.
dc.date.accessioned2020-12-15T04:58:26Z
dc.date.available2020-12-15T04:58:26Z
dc.date.issued1997
dc.description.abstractTo study whether tungsten isotopic ratios observed in terrestrial samples relative to W ratios in an iron meteorite could be made by neutron-capture reactions in the iron meteorite, the fluxes of thermal and epithermal neutrons in a large iron meteoroid, Toluca, were calculated using Monte Carlo particle production and transport codes. Peak neutron-capture rates on W isotopes were calculated to occur at depths of 30-34 cm. The calculated changes in the 182W/183W due to neutrons are much less than those observed in terrestrial samples relative to iron meteorites, indicating a non-cosmogenic origin of the observed W isotopic ratios.
dc.identifierhttps://elibrary.ru/item.asp?id=268935
dc.identifier.citationEarth and Planetary Science Letters, 1997, , 1, 181-185
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/20813
dc.subjectTUNGSTEN
dc.subjectIRON METEORITES
dc.subjectISOTOPE RATIOS
dc.subjectNEUTRONS
dc.titleCONTRIBUTION OF NEUTRON-CAPTURE REACTIONS TO OBSERVED TUNGSTEN ISOTOPIC RATIOS
dc.typeСтатья

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