MétaCan
Menu
← Back to cohort
Record W4414281556 · doi:10.17918/00011165

Background, calibration, and validation simulations for SBC dark matter and reactor CEvNS experiments

2025· dissertation· en· W4414281556 on OpenAlexaboutno aff
Noah R. Lamb

Bibliographic record

Venuenot available
Typedissertation
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsnot available
Fundersnot available
KeywordsDark matterNeutrinoBubble chamberBubbleParticle (ecology)Weakly interacting massive particlesNeutrino detectorRecoilTracking (education)

Abstract

fetched live from OpenAlex

The Scintillating Bubble Chamber (SBC) Collaboration plans to use liquid noble bubble chambers in rare event searches such as nuclear recoils from dark matter and neutrino scattering. Bubble chambers are particle detectors that use liquid above its boiling point in a "superheated" state in order to detect particle interactions. When a particle deposits energy inside the detector, the liquid boils, and a bubble forms. Liquid noble bubble chambers have unique potential as a scalable, low-background, low-energy nuclear recoil detector. Dark matter refers to yet undetected matter that is predicted to comprise most of the mass in the universe based on astronomical observations. SBC has plans to operate reactor neutrino experiments in the future. With the goal of being sensitive to 100 eV nuclear recoils, there is considerable potential for discovery for these experiments. SBC is constructing two 10-kg liquid argon bubble chambers, one to be deployed at Fermi National Accelerator Lab (Fermilab) and the other to be deployed in the SNOLAB underground facility (an expansion of the Sudbury Neutrino Observatory). The Fermilab chamber is a full-scale prototype designed for tests and calibrations, including a novel gamma nucleus elastic scattering calibration. The calibration is required to infer a dark matter sensitivity of the detector. The chamber at SNOLAB will conduct a dark matter search deep-underground with low cosmic radiation. This thesis focuses on the gamma-ray backgrounds and calibration for the SBC experiment. This includes simulations of inner shell electron ionization and nuclear recoils from gamma-rays to understand the detection of environmental radiation and predict the rate at which this radiation is detected. These inner shell ionization simulations helped to confirm a mechanism for electronic recoil backgrounds previously observed in PICO chambers and has implications for future experiments. I developed a high statistics method for simulating nuclear recoils from gamma-rays to inform the shielding design of SBC and design a calibration plan. A simulated calibration is performed to determine the best calibration sources to use and predict the accuracy that can be achieved with a realistic calibration campaign. SBC has a target of 20% or lower uncertainty on the detector threshold for a near-term dark matter search and a target of 5% or lower uncertainty on the detector threshold for a reactor neutrino experiment. The results from the simulated calibration suggest both targets are achievable and estimate the systematic uncertainties required to meet those targets.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.003
metaresearch head score (Gemma)0.009
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.038
Threshold uncertainty score0.075

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.009
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0020.002
Open science0.0020.001
Research integrity0.0020.003
Insufficient payload (model declined to judge)0.0070.001

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 head0.018
GPT teacher head0.289
Teacher spread0.272 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
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
Published2025
Admission routes1
Has abstractyes

Explore more

Same topicDark Matter and Cosmic Phenomena→French-language works237,207→