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Record W2945089151 · doi:10.25911/5d5140d1b5181

Diamonds - Time capsules of volatiles and the key to dynamic Earth evolution

2018· dissertation· en· W2945089151 on OpenAlexfundno aff
Suzette Timmerman

Bibliographic record

VenueANU Open Research (Australian National University) · 2018
Typedissertation
Languageen
FieldEarth and Planetary Sciences
TopicMarine and environmental studies
Canadian institutionsnot available
FundersAustralian Research CouncilUniversity of AlbertaAustralian Government
KeywordsKey (lock)Earth (classical element)AstrobiologyEarth scienceGeologyComputer sciencePhysicsAstronomyComputer security

Abstract

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Noble gas analyses of basalts indicate that the present-day structure of the Earth comprises a slightly degassed lower mantle and highly degassed upper mantle. The extent and timing of mantle in and out-gassing and sources of volatiles are, however, not well-constrained and require quantification. The objective of this thesis is to address these questions through a study of the noble gas composition of diamonds as diamonds, being chemically inert, can preserve information on the fluid and mantle composition at the time of diamond formation. Specific objectives are to explore the potential of U-Th/He systematics for dating fibrous diamonds, the influence of volatile subduction on the heterogeneity in the sub-continental lithospheric mantle (SCLM), and how noble gas compositions have evolved over time in the SCLM. High-density fluid (HDF) inclusions with different major element compositions found in South African fibrous diamonds have different noble gas compositions that show these fluids originated from subducted sediments and oceanic crust and had either limited interaction with the SCLM (silicic-low Mg carbonatitic fluids) or significant interaction with the SCLM (saline fluids). A positive correlation between 3He/4He and d13C values in monocrystalline lithospheric diamonds from Argyle (Australia), together with low 40Ar/36Ar and He/Ne isotopic compositions, demonstrates a subduction influence caused by high U-Th/3He ratios and thus low 3He/4He ratios in subducted organic material. A noble gas depth profile based on N systematics of these diamonds shows fluid-rock interaction over scales of at least 15 kilometres above the accreted subducted material. Sub-lithospheric diamonds from Brazil, in contrast, show a negative correlation between 3He/4He and d13C values, but 3He/4He ratios are decoupled from trace elements and Pb-Sr isotope systematics that have characteristics of subducted material. This indicates that the subducted sediments have been deprived of U-Th-He and a high 3He/4He source, located in the deep mantle, is dominating the helium budget. Fibrous diamonds are generally assumed to have formed shortly before kimberlite eruption but there is currently no way to date these diamonds. The U-Th-Sm/He systematics of fibrous Congo and Jwaneng diamonds showed that in most cases U-Th/He ratios are sufficiently high to produce significant radiogenic 4He to provide age constraints and some fibrous diamonds are up to several 100 Myr older than the kimberlite eruption age. Previously dated monocrystalline diamonds (with multiple ages ranging from 0.07 to ~3.4 Ga) were analysed for trace elements and He-Ar isotopic compositions and showed similar trace element patterns for all diamonds but a correlation between the age and 4He-40Ar*-3He/4He values. After correcting for radiogenic ingrowth since diamond formation a large variation remains in 3He/4He values at ~1.0 Ga in eclogitic diamonds that can be explained by mixing between mantle and subducted components. Given the preservation of heterogeneities, it is difficult to develop a simple noble gas evolution curve for the SCLM. From examination of fibrous and monocrystalline diamonds from different formation depths, formation ages, and geographic locations this study showed the large influence of subduction at the base of the lithosphere and a more SCLM-like noble gas composition at shallower depths.

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How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.545
Threshold uncertainty score0.998

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.036
GPT teacher head0.286
Teacher spread0.250 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations0
Published2018
Admission routes1
Has abstractyes

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