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Record W176350038

Physics of the double pulsar

2006· article· en· W176350038 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.

Bibliographic record

Venue36th COSPAR Scientific Assembly · 2006
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsUniversity of Toronto
Fundersnot available
KeywordsPulsarPhysicsMillisecond pulsarMagnetosphereBinary pulsarNeutron starAstrophysicsAstronomyX-ray pulsarPulsar planetPlasmaNuclear physics
DOInot available

Abstract

fetched live from OpenAlex

Pulsar J0737-3039 is the only currently known double neutron star system in which both components exhibit themselves as radio pulsars. A number of peculiar properties very compact orbit (with period 2.4 hours), almost edge-on orientation of the orbital plane with respect to our line of sight provide us with unprecedented opportunities of checking effects of general relativity and probing the physics of pulsar magnetospheres. This report will provide a brief overview of our current understanding of some of the unique phenomena that have been observed in the double pulsar system: accumulation of relativistic plasma in the magnetosphere of normal pulsar causes periodic eclipses of its millisecond companion. Powerful wind of the millisecond pulsar distorts the magnetosphere of its normal companion, which affects the spindown and emission properties of normal pulsar. Future observational and theoretical work on this system may turn it into a Rosetta Stone of pulsar physics.

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.

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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: Theoretical or conceptual
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.171
Threshold uncertainty score0.279

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 science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.016
GPT teacher head0.303
Teacher spread0.287 · 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