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Record W7038654622

Investigating helium-layer stripping in the interacting SN 2021efd

2024· other· en· W7038654622 on OpenAlexfundno aff

Bibliographic record

VenueUTUPub (University of Turku) · 2024
Typeother
Languageen
FieldAgricultural and Biological Sciences
TopicFossil Insects in Amber
Canadian institutionsnot available
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesAgencia Estatal de InvestigaciónStockholms UniversitetDeutsches Elektronen-SynchrotronScience and Technology Facilities CouncilQueen's UniversityTrinity College DublinQueen's University BelfastCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationNuclear Safety and Security CommissionSpace Telescope Science InstituteNational Science Foundation
KeywordsSupernovaEjectaStarsLuminosityStripping (fiber)Light curveCommon envelopeHelium
DOInot available

Abstract

fetched live from OpenAlex

Some stars meet their ends in supernovae (SN) explosions. Massive stars (>8M_sun) at the end of their stellar evolution suffer a core-collapse and explode as core-collapse supernovae (CCSNe). SNe have diverse observational properties and are divided into classes based on them. Much can be known about the star that exploded from the SN it produced.
\nStripped-envelope supernovae (SESNe) are explosions of massive stars that lost a part of the hydrogen envelope (Type IIb), the whole hydrogen envelope (Type Ib), or the hydrogen envelope and the helium layer (Type Ic). Evidence has accumulated to support a binary interaction as the stripping mechanism for the hydrogen envelope. The mechanism responsible for the helium-layer stripping for the progenitors of Type Ic SNe is still an open question.
\nIn this thesis, I performed an in-depth analysis of the spectroscopic and photometric data of the peculiar Type Ib SN 2021efd. The light curve of SN 2021efd has an excess at late phases compared to the level that is expected from the decay of Nickel-56. I analyzed the spectra of SN 2021efd and concluded that the excess luminosity was caused by interaction of the ejecta with hydrogen-poor circumstellar material. I derived the ejecta parameters and the progenitor star mass and concluded that they do not separate SN 2021efd from the general population of SESNe. I estimated the mass-loss rate of the progenitor star by comparing the interaction luminosity in SN 2021efd to numerical calculations. Based on the high mass-loss rate, I concluded that the mass-loss mechanism is not consistent with line-driven wind. Instead, I suggest that the mass loss could have happened in eruptions. Based on the high mass-loss rate, I concluded that the mass-loss mechanism is not consistent with line-driven wind. Instead, I suggest that the mass loss could have happened in eruptions.

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 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)0.000
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: Not applicable · Consensus signal: Not applicable
GenreCandidate signal: Other · Consensus signal: Other
Teacher disagreement score0.326
Threshold uncertainty score0.999

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0040.000

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 head0.034
GPT teacher head0.221
Teacher spread0.187 · 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 designNot applicable
Domainnot available
GenreOther

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
Published2024
Admission routes1
Has abstractyes

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