MétaCan
Menu
Back to cohort
Record W3107450206 · doi:10.1007/s41114-021-00032-5

Challenges and opportunities of gravitational-wave searches at MHz to GHz frequencies

2021· article· en· W3107450206 on OpenAlexaff
N. Aggarwal, Odylio D. Aguiar, Andreas Bauswein, G. Cella, S. Clesse, Adrian Michael Cruise, Valerie Domcke, Daniel G. Figueroa, Andrew Geraci, Maxim Goryachev, H. Grote, Mark Hindmarsh, Francesco Muia, N. Mukund, D. J. Ottaway, Marco Peloso, Fernando Quevedo, Angelo Ricciardone, Jessica Steinlechner, Sebastian Steinlechner, Sichun Sun, Michael E. Tobar, Francisco Torrentí, Caner Ünal, Graham White

Bibliographic record

VenueLiving Reviews in Relativity · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsInstitute of Particle Physics
FundersOffice of Naval ResearchAustralian Research CouncilMinisterio de Ciencia e InnovaciónConselho Nacional de Desenvolvimento Científico e TecnológicoScience and Technology Facilities CouncilMinistero dell’Istruzione, dell’Università e della RicercaAbdus Salam International Centre for Theoretical PhysicsEuropean CommissionHeising-Simons FoundationNorthwestern UniversityFundação de Amparo à Pesquisa do Estado de São PauloDipartimenti di EccellenzaDeutsche ForschungsgemeinschaftJohn Templeton FoundationSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungW. M. Keck FoundationEngineering and Physical Sciences Research CouncilUK Research and InnovationNational Science Foundation
KeywordsLIGOGravitational wavePhysicsGravitational-wave astronomyUltra high frequencyGravitational-wave observatoryUniverseGravitationAstronomyTelecommunicationsComputer science

Abstract

fetched live from OpenAlex

Abstract The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges and gains expected in gravitational-wave searches at frequencies above the LIGO/Virgo band, with a particular focus on Ultra High-Frequency Gravitational Waves (UHF-GWs), covering the MHz to GHz range. The absence of known astrophysical sources in this frequency range provides a unique opportunity to discover physics beyond the Standard Model operating both in the early and late Universe, and we highlight some of the most promising gravitational sources. We review several detector concepts that have been proposed to take up this challenge, and compare their expected sensitivity with the signal strength predicted in various models. This report is the summary of the workshop “Challenges and opportunities of high-frequency gravitational wave detection” held at ICTP Trieste, Italy in October 2019, that set up the stage for the recently launched Ultra-High-Frequency Gravitational Wave (UHF-GW) initiative.

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)0.008
metaresearch head score (Gemma)0.006
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Review · Consensus signal: Review
Teacher disagreement score0.008
Threshold uncertainty score0.041

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0080.006
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.001
Science and technology studies0.0010.002
Scholarly communication0.0040.007
Open science0.0010.002
Research integrity0.0030.003
Insufficient payload (model declined to judge)0.0040.002

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 head0.196
GPT teacher head0.379
Teacher spread0.183 · 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 designTheoretical or conceptual
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

Citations353
Published2021
Admission routes1
Has abstractyes

Explore more

Same venueLiving Reviews in RelativitySame topicPulsars and Gravitational Waves ResearchFrench-language works237,207