MétaCan
Menu
Back to cohort
Record W3156992276 · doi:10.1038/s42254-021-00303-8

Gravitational-wave physics and astronomy in the 2020s and 2030s

2021· review· en· W3156992276 on OpenAlexafffund
M. Bailes, B. K. Berger, P. R. Brady, M. Branchesi, K. Danzmann, M. Evans, Kelly Holley‐Bockelmann, B. R. Iyer, T. Kajita, S. Katsanevas, M. Krämer, A. Lazzarini, Luis Lehner, G. Losurdo, Harald Lück, D. E. McClelland, M. A. McLaughlin, M. Punturo, S. M. Ransom, Somak Raychaudhury, D. H. Reitze, S. Rowan, Y. Saito, G. H. Sanders, B. S. Sathyaprakash, B. F. Schutz, Alberto Sesana, H. Shinkai, X. Siemens, D. H. Shoemaker, James Ira Thorpe, J. F. J. van den Brand, S. Vitale

Bibliographic record

VenueNature Reviews Physics · 2021
Typereview
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsPerimeter Institute
FundersGreat Southern Development Commission, Government of Western AustraliaJapan Society for the Promotion of ScienceAustralian Research CouncilNatural Sciences and Engineering Research Council of CanadaInstitut Périmètre de physique théoriqueCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftScience and Technology Facilities CouncilMinistero dell’Istruzione, dell’Università e della RicercaKorea Institute of Science and Technology InformationMinistry of Education, Culture, Sports, Science and TechnologyNederlandse Organisatie voor Wetenschappelijk OnderzoekEuropean CommissionAcademia SinicaIstituto Nazionale di Fisica NucleareGovernment of CanadaDeutsche ForschungsgemeinschaftCanadian Institute for Advanced ResearchAssociated UniversitiesLeibniz-GemeinschaftNational Aeronautics and Space AdministrationNational Radio Astronomy ObservatoryUniversité de ParisAgenzia Spaziale ItalianaNational Science Foundation
KeywordsPhysicsGravitational-wave astronomyGravitational waveLIGOGeneral relativityAstronomyNeutron starGravitational-wave observatoryGravitational fieldAstrophysicsTheoretical physics

Abstract

fetched live from OpenAlex

The 100 years since the publication of Albert Einstein’s theory of general relativity saw significant development of the understanding of the theory, the identification of potential astrophysical sources of sufficiently strong gravitational waves and development of key technologies for gravitational-wave detectors. In 2015, the first gravitational-wave signals were detected by the two US Advanced LIGO instruments. In 2017, Advanced LIGO and the European Advanced Virgo detectors pinpointed a binary neutron star coalescence that was also seen across the electromagnetic spectrum. The field of gravitational-wave astronomy is just starting, and this Roadmap of future developments surveys the potential for growth in bandwidth and sensitivity of future gravitational-wave detectors, and discusses the science results anticipated to come from upcoming instruments. In the past few years, gravitational-wave observations provided stunning insights into some of the most cataclysmic events in the Universe, heralding a bright future for gravitational-wave physics and astronomy. This is a Roadmap for the field in the coming two decades.

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)0.001
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Review · Consensus signal: Review
Teacher disagreement score0.005
Threshold uncertainty score0.016

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0020.002
Science and technology studies0.0000.001
Scholarly communication0.0020.003
Open science0.0010.001
Research integrity0.0020.002
Insufficient payload (model declined to judge)0.0050.003

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 head0.054
GPT teacher head0.410
Teacher spread0.357 · 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 designNot applicable
Domainnot available
GenreReview

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

Citations276
Published2021
Admission routes2
Has abstractyes

Explore more

Same venueNature Reviews PhysicsSame topicPulsars and Gravitational Waves ResearchFrench-language works237,207