MétaCan
Menu
← Back to cohort
Record W4320559935 · doi:10.1051/0004-6361/202346155

Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations

2023· article· en· W4320559935 on OpenAlexafffund
U. Fuskeland, J. Aumont, R. Aurlien, C. Baccigalupi, A. J. Banday, H.K. Eriksen, J. Errard, R. T. Génova-Santos, Takashi Hasebe, J. Hubmayr, Hiroaki Imada, N. Krachmalnicoff, L. Lamagna, G. Pisano, D. Poletti, M. Remazeilles, K. L. Thompson, L. Vacher, I. K. Wehus, S. Azzoni, M. Ballardini, R. B. Barreiro, N. Bartolo, A. Basyrov, D. Beck, M. Bersanelli, M. Bortolami, M. Brilenkov, E. Calabrese, A. Carones, F. J. Casas, K. Cheung, Jens Chluba, Susan E. Clark, L. Clermont, F. Columbro, A. Coppolecchia, G. D’Alessandro, P. de Bernardis, T. de Haan, E. de la Hoz, M. De Petris, S. Della Torre, P. Diego-Palazuelos, F. Finelli⋆, C. Franceschet, G. Galloni, M. Galloway, M. Gerbino, M. Gervasi, T. Ghigna, S. Giardiello, E. Gjerløw, A. Gruppuso, Peter Hargrave, M. Hattori, M. Hazumi, L. T. Hergt, D. Herman, D. Herranz, E. Hivon, D. Hoang, Kazunori Kohri, M. Lattanzi, A. T. Lee, C. Leloup, F. Levrier, A.I. Lonappan, G. Luzzi, B. Maffei, E. Martínez-González, S. Masi, S. Matarrese, T. Matsumura, M. Migliaccio, L. Montier, G. Morgante, B. Mot, L. Mousset, Ryo Nagata, Toshiya Namikawa, F. Nati, P. Natoli, S. Nerval, A. Novelli, L. Pagano, A Paiella, D. Paoletti, G. Pascual-Cisneros, G. Patanchon, Vincent Pelgrims, F. Piacentini, G. Piccirilli, G. Polenta, Giuseppe Puglisi, N. Raffuzzi, A. Ritacco, J. A. Rubiño-Martín, G. Savini, D. Scott, Y. Sekimoto, Maresuke Shiraishi, G. Signorelli, S. L. Stever, N. Stutzer, R. M. Sullivan, H. Takakura, L. Terenzi, H. Thommesen, M. Tristram, M. Tsuji, P. Vielva, J. Weller, Benjamin Westbrook, G. Weymann-Despres, Edward J. Wollack, M. Zannoni

Bibliographic record

VenueAstronomy and Astrophysics · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsUniversity of British Columbia
FundersNuclear PhysicsAgencia Estatal de InvestigaciónScience and Technology Facilities CouncilCanadian Space AgencyJapan Society for the Promotion of ScienceNorges ForskningsrådMinistry of Education, Culture, Sports, Science and TechnologyCentre National d’Etudes SpatialesCommissariat à l'Énergie Atomique et aux Énergies AlternativesIstituto Nazionale di AstrofisicaVetenskapsrådetSwedish National Space AgencyNational Aeronautics and Space AdministrationJapan Aerospace Exploration AgencyAbdus Salam International Centre for Theoretical PhysicsCentre National de la Recherche ScientifiqueRoyal SocietyNuclear Safety and Security CommissionDeutsche Forschungsgemeinschaft
KeywordsPhysicsCosmic microwave backgroundGravitational waveAmplitudeSpectral indexScalar (mathematics)Computational physicsRadio spectrumRange (aeronautics)Cutoff frequencyLow frequencyAstrophysicsPolarization (electrochemistry)OpticsSpectral lineQuantum mechanicsAstronomyGeometryMathematics

Abstract

fetched live from OpenAlex

LiteBIRD is a planned JAXA-led cosmic microwave background (CMB) B -mode satellite experiment aiming for launch in the late 2020s, with a primary goal of detecting the imprint of primordial inflationary gravitational waves. Its current baseline focal-plane configuration includes 15 frequency bands between 40 and 402 GHz, fulfilling the mission requirements to detect the amplitude of gravitational waves with the total uncertainty on the tensor-to-scalar ratio, δr , down to δr < 0.001. A key aspect of this performance is accurate astrophysical component separation, and the ability to remove polarized thermal dust emission is particularly important. In this paper we note that the CMB frequency spectrum falls off nearly exponentially above 300 GHz relative to the thermal dust spectral energy distribution, and a relatively minor high frequency extension can therefore result in even lower uncertainties and better model reconstructions. Specifically, we compared the baseline design with five extended configurations, while varying the underlying dust modeling, in each of which the High-Frequency Telescope (HFT) frequency range was shifted logarithmically toward higher frequencies, with an upper cutoff ranging between 400 and 600 GHz. In each case, we measured the tensor-to-scalar ratio r uncertainty and bias using both parametric and minimum-variance component-separation algorithms. When the thermal dust sky model includes a spatially varying spectral index and temperature, we find that the statistical uncertainty on r after foreground cleaning may be reduced by as much as 30–50% by extending the upper limit of the frequency range from 400 to 600 GHz, with most of the improvement already gained at 500 GHz. We also note that a broader frequency range leads to higher residuals when fitting an incorrect dust model, but also it is easier to discriminate between models through higher χ 2 sensitivity. Even in the case in which the fitting procedure does not correspond to the underlying dust model in the sky, and when the highest frequency data cannot be modeled with sufficient fidelity and must be excluded from the analysis, the uncertainty on r increases by only about 5% for a 500 GHz configuration compared to the baseline.

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)0.004
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.011
Threshold uncertainty score0.021

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.004
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0000.000
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0010.000

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 head0.012
GPT teacher head0.254
Teacher spread0.243 · 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 designSimulation or modeling
Domainnot available
GenreEmpirical

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

Citations19
Published2023
Admission routes2
Has abstractyes

Explore more

Same venueAstronomy and Astrophysics→Same topicCosmology and Gravitation Theories→French-language works237,207→