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Record W4388327516 · doi:10.1007/s41114-025-00056-1

Waveform modelling for the Laser Interferometer Space Antenna

2025· preprint· en· W4388327516 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.

fundA Canadian funder is recorded on the work.
no affNo Canadian affiliation: this work is invisible to an affiliation-only frame.
No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.

Bibliographic record

VenueLiving Reviews in Relativity · 2025
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersLos Alamos National LaboratoryOffice of Naval ResearchFundação para a Ciência e a TecnologiaJapan Society for the Promotion of ScienceNatural Sciences and Engineering Research Council of CanadaHorizon 2020 Framework ProgrammeNational Nuclear Security AdministrationEuropean Regional Development FundInstitut Périmètre de physique théoriqueAgencia Estatal de InvestigaciónCenter for Research and Development in Mathematics and ApplicationsMinistero degli Affari Esteri e della Cooperazione InternazionaleU.S. Department of EnergyJohn Templeton FoundationFondazione CariploNational Aeronautics and Space AdministrationUniversity College DublinDanmarks GrundforskningsfondNational Research FoundationHORIZON EUROPE Framework ProgrammeNuclear Safety and Security CommissionLeverhulme TrustDeutsche ForschungsgemeinschaftInnovation, Science and Economic Development CanadaGeneralitat ValencianaMinistry of Colleges and UniversitiesVillum FondenAkademie Věd České RepublikyNational Science FoundationUK Research and InnovationScience Foundation IrelandDartmouth CollegeNational Research CentreUniversity of Massachusetts DartmouthGovernment of CanadaDirecció General de Recerca, Generalitat de CatalunyaEuropean CommissionSherman Fairchild Foundation
KeywordsGravitational waveWaveformPhysicsInterferometryGravitational-wave observatoryDetectorAstronomySpace (punctuation)OpticsComputer science

Abstract

fetched live from OpenAlex

Abstract LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectacular variety of interesting new sources abound: from millions of ultra-compact binaries in our Galaxy, to mergers of massive black holes at cosmological distances; from the early inspirals of stellar-mass black holes that will ultimately venture into the ground-based detectors’ view to the death spiral of compact objects into massive black holes, and many sources in between. Central to realising LISA’s discovery potential are waveform models, the theoretical and phenomenological predictions of the pattern of gravitational waves that these sources emit. This White Paper is presented on behalf of the Waveform Working Group for the LISA Consortium. It provides a review of the current state of waveform models for LISA sources, and describes the significant challenges that must yet be overcome.

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)0.002
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: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Methods · Consensus signal: none
Teacher disagreement score0.903
Threshold uncertainty score0.808

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0020.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.001
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 head0.059
GPT teacher head0.377
Teacher spread0.317 · 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