Matches in SemOpenAlex for { <https://semopenalex.org/work/W320121964> ?p ?o ?g. }
- W320121964 abstract "Due to their ubiquity in nature and chemical reactivity, aluminosilicate minerals play an important role in retarding actinide subsurface migration. However, very few studies have examined Pu interaction with clay minerals in sufficient detail to produce a credible mechanistic model of its behavior. In this work, Pu(IV) and Pu(V) interactions with silica, gibbsite (Aloxide), and Na-montmorillonite (smectite clay) were examined as a function of time and pH. Sorption of Pu(IV) and Pu(V) to gibbsite and silica increased with pH (4 to 10). The Pu(V) sorption edge shifted to lower pH values over time and approached that of Pu(IV). This behavior is apparently due to surface mediated reduction of Pu(V) to Pu(IV). Surface complexation constants describing Pu(IV)/Pu(V) sorption to aluminol and silanol groups were developed from the silica and gibbsite sorption experiments and applied to the montmorillonite dataset. The model provided an acceptable fit to the montmorillonite sorption data for Pu(V). In order to accurately predict Pu(IV) sorption to montmorillonite, the model required inclusion of ion exchange. The objective of this work is to measure the sorption of Pu(IV) and Pu(V) to silica, gibbsite, and smectite (montmorillonite). Aluminosilicate minerals are ubiquitous at the Nevada National Security Site and improving our understanding of Pu sorption to aluminosilicates (smectite clays in particular) is essential to the accurate prediction of Pu transport rates. These data will improve the mechanistic approach for modeling the hydrologic source term (HST) and provide sorption Kd parameters for use in CAU models. In both alluvium and tuff, aluminosilicates have been found to play a dominant role in the radionuclide retardation because their abundance is typically more than an order of magnitude greater than other potential sorbing minerals such as iron and manganese oxides (e.g. Vaniman et al., 1996). The sorption database used in recent HST models (Carle et al., 2006) and upscaled for use in CAU models (Stoller-Navarro, 2008) includes surface complexation constants for U, Am, Eu, Np and Pu (Zavarin and Bruton, 2004). Generally, between 15 to 30 datasets were used to develop the constants for each radionuclide. However, the constants that describe Pu sorption to aluminosilicates were developed using only 10 datasets, most of which did not specify the oxidation state of Pu in the experiment. Without knowledge or control of the Pu oxidation state, a high degree of uncertainty is introduced into the model. The existing Pu surface complexation model (e.g. Zavarin and Bruton, 2004) drastically underestimates Pu sorption and, thus, will overestimate Pu migration rates (Turner, 1995). Recent HST simulations at Cambric (Carle et al., 2006) suggest that the existing surface complexation model may underpredict Pu K{sub d}s by as much as 3 orders of magnitude. In order to improve HST and CAU-scale transport models (and, as a result, reduce the conservative nature Pu migration estimates), sorption experiments were performed over a range of solution conditions that brackets the groundwater chemistry of the Nevada National Security Site. The aluminosilicates examined were gibbsite, silica, and montmorillonite." @default.
- W320121964 created "2016-06-24" @default.
- W320121964 creator A5028978175 @default.
- W320121964 creator A5036263267 @default.
- W320121964 creator A5043297271 @default.
- W320121964 creator A5078310119 @default.
- W320121964 date "2008-10-28" @default.
- W320121964 modified "2023-09-26" @default.
- W320121964 title "Development of a Composite Non-Electrostatic Surface Complexation Model Describing Plutonium Sorption to Aluminosilicates" @default.
- W320121964 cites W1488082657 @default.
- W320121964 cites W1507059058 @default.
- W320121964 cites W1513419231 @default.
- W320121964 cites W1515550974 @default.
- W320121964 cites W1578943547 @default.
- W320121964 cites W1661611782 @default.
- W320121964 cites W1817568681 @default.
- W320121964 cites W1964224601 @default.
- W320121964 cites W1965952878 @default.
- W320121964 cites W1966158621 @default.
- W320121964 cites W1975247662 @default.
- W320121964 cites W2004453378 @default.
- W320121964 cites W2017798670 @default.
- W320121964 cites W2020515714 @default.
- W320121964 cites W2029358844 @default.
- W320121964 cites W2033835675 @default.
- W320121964 cites W2034782193 @default.
- W320121964 cites W2040757996 @default.
- W320121964 cites W2052654679 @default.
- W320121964 cites W2053710223 @default.
- W320121964 cites W2060942646 @default.
- W320121964 cites W2068255197 @default.
- W320121964 cites W2071458899 @default.
- W320121964 cites W2077853275 @default.
- W320121964 cites W2079106312 @default.
- W320121964 cites W2089299698 @default.
- W320121964 cites W2094568102 @default.
- W320121964 cites W2110440609 @default.
- W320121964 cites W2113768184 @default.
- W320121964 cites W2132252129 @default.
- W320121964 cites W2146202933 @default.
- W320121964 cites W2148508034 @default.
- W320121964 cites W2164066306 @default.
- W320121964 cites W2460123941 @default.
- W320121964 cites W2558253588 @default.
- W320121964 cites W2562139049 @default.
- W320121964 cites W2562479965 @default.
- W320121964 cites W2565299668 @default.
- W320121964 cites W2779765635 @default.
- W320121964 doi "https://doi.org/10.2172/1019063" @default.
- W320121964 hasPublicationYear "2008" @default.
- W320121964 type Work @default.
- W320121964 sameAs 320121964 @default.
- W320121964 citedByCount "3" @default.
- W320121964 countsByYear W3201219642014 @default.
- W320121964 countsByYear W3201219642016 @default.
- W320121964 countsByYear W3201219642019 @default.
- W320121964 crossrefType "report" @default.
- W320121964 hasAuthorship W320121964A5028978175 @default.
- W320121964 hasAuthorship W320121964A5036263267 @default.
- W320121964 hasAuthorship W320121964A5043297271 @default.
- W320121964 hasAuthorship W320121964A5078310119 @default.
- W320121964 hasBestOaLocation W3201219642 @default.
- W320121964 hasConcept C150394285 @default.
- W320121964 hasConcept C161790260 @default.
- W320121964 hasConcept C178790620 @default.
- W320121964 hasConcept C179104552 @default.
- W320121964 hasConcept C185592680 @default.
- W320121964 hasConcept C199289684 @default.
- W320121964 hasConcept C2777515222 @default.
- W320121964 hasConcept C2777581007 @default.
- W320121964 hasConcept C2777975867 @default.
- W320121964 hasConcept C2778973568 @default.
- W320121964 hasConcept C2779899878 @default.
- W320121964 hasConcept C2780367224 @default.
- W320121964 hasConcept C40212044 @default.
- W320121964 hasConcept C58445606 @default.
- W320121964 hasConcept C85704489 @default.
- W320121964 hasConceptScore W320121964C150394285 @default.
- W320121964 hasConceptScore W320121964C161790260 @default.
- W320121964 hasConceptScore W320121964C178790620 @default.
- W320121964 hasConceptScore W320121964C179104552 @default.
- W320121964 hasConceptScore W320121964C185592680 @default.
- W320121964 hasConceptScore W320121964C199289684 @default.
- W320121964 hasConceptScore W320121964C2777515222 @default.
- W320121964 hasConceptScore W320121964C2777581007 @default.
- W320121964 hasConceptScore W320121964C2777975867 @default.
- W320121964 hasConceptScore W320121964C2778973568 @default.
- W320121964 hasConceptScore W320121964C2779899878 @default.
- W320121964 hasConceptScore W320121964C2780367224 @default.
- W320121964 hasConceptScore W320121964C40212044 @default.
- W320121964 hasConceptScore W320121964C58445606 @default.
- W320121964 hasConceptScore W320121964C85704489 @default.
- W320121964 hasLocation W3201219641 @default.
- W320121964 hasLocation W3201219642 @default.
- W320121964 hasLocation W3201219643 @default.
- W320121964 hasOpenAccess W320121964 @default.
- W320121964 hasPrimaryLocation W3201219641 @default.
- W320121964 hasRelatedWork W1587853257 @default.
- W320121964 hasRelatedWork W2048866703 @default.
- W320121964 hasRelatedWork W2060564067 @default.