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Record W4214968761 · doi:10.1093/ptep/ptac150

Probing cosmic inflation with the<i>LiteBIRD</i>cosmic microwave background polarization survey

2022· article· en· W4214968761 on OpenAlexaff
Erwan Allys, Kam Arnold, J. Aumont, R. Aurlien, S. Azzoni, C. Baccigalupi, A. J. Banday, R. Banerji, R. B. Barreiro, N. Bartolo, Inmaculada Bautista, D. Beck, S. Beckman, M. Bersanelli, F. Boulanger, M. Brilenkov, M. Bucher, E. Calabrese, P. Campeti, A. Carones, F. J. Casas, A. Catalano, V. Chan, K. Cheung, Y. Chinone, Susan E. Clark, F. Columbro, G. D’Alessandro, P. de Bernardis, T. de Haan, E. de la Hoz, M. De Petris, S. Della Torre, P. Diego-Palazuelos, M. Dobbs, Tadayasu Dotani, J. M. Duval, T. Elleflot, H. K. Eriksen, Josquin Errard, Thomas Essinger-Hileman, F. Finelli⋆, Raphael Flauger, C. Franceschet, U. Fuskeland, M. Galloway, K. Ganga, M. Gerbino, M. Gervasi, R. T. Génova-Santos, T. Ghigna, S. Giardiello, E. Gjerløw, J. Grain, F. Grupp, A. Gruppuso, J. E. Gudmundsson, N. W. Halverson, Peter Hargrave, Takashi Hasebe, M. Hasegawa, M. Hazumi, S. Henrot–Versillé, Brandon S. Hensley, L. T. Hergt, D. Herman, E. Hivon, Renée Hložek, Amber Hornsby, Yurika Hoshino, Johannes Hubmayr, Kiyotomo Ichiki, Teruhito Iida, Hiroaki Imada, H. Ishino, G. Jaehnig, N. Katayama, A. Kato, Brian Keating, T. S. Kisner, Yosuke Kobayashi, A. Kogut, Kazunori Kohri, Eiichiro Komatsu, Kunimoto Komatsu, K. Konishi, N. Krachmalnicoff, C. L. Kuo, L. Lamagna, M. Lattanzi, A. T. Lee, C. Leloup, F. Levrier, E. Linder, G. Luzzi, J. F. Macías–Pérez, T. Maciaszek, B. Maffei, D. Maino, S. Mandelli, E. Martínez-González, S. Masi, M. Massa, S. Matarrese, Frederick Matsuda, T. Matsumura, L. Mele, M. Migliaccio, Y. Minami, A. Moggi, J. Montgomery, L. Montier, G. Morgante, B. Mot, Y. Nagano, T. Nagasaki, Ryo Nagata, Ryo Nakano, Toshiya Namikawa, F. Nati, P. Natoli, S. Nerval, F. Noviello, Kimihide Odagiri, S. Oguri, Hiroyuki Ohsaki, L. Pagano, A. Paiella, D. Paoletti, A. Passerini, G. Patanchon, F. Piacentini, M. Piat, G. Pisano, G. Polenta, D. Poletti, T. Prouvé, Giuseppe Puglisi, D Rambaud, C Raum, S Realini, M. Reinecke, M. Remazeilles, A. Ritacco, G Roudil, J A Rubino-Martin, Michael Russell, Hiroshi Sakurai, Y. Sakurai, M Sasaki, D. Scott, Yutaro Sekímoto, K. Shinozaki, Maresuke Shiraishi, Peter Shirron, G. Signorelli, F. Spinella, S. L. Stever, R Stompor, S. Sugiyama, R. M. Sullivan, A. Suzuki, T L Svalheim, E Switzer, Ryota Takaku, Hiroyuki Takakura, Y Takase, A. Tartari, Y Terao, J Thermeau, H. Thommesen, K L Thompson, M. Tomasi, M Tominaga, M Tristram, M Tsuji, Masahiro Tsujimoto, L. Vacher, P. Vielva, N. Vittorio, W. Wang, K Watanuki, I.K. Wehus, J. Weller, B Westbrook, J. Wilms, B. Winter, Edward J. Wollack, Junji Yumoto, M. Zannoni

Bibliographic record

VenueProgress of Theoretical and Experimental Physics · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsUniversity of British ColumbiaMcGill University
FundersIstituto Nazionale di AstrofisicaCentre National de la Recherche ScientifiqueNuclear PhysicsAgenzia Spaziale ItalianaJapan Aerospace Exploration AgencyCentre National d’Etudes SpatialesJapan Society for the Promotion of ScienceMinistry of Education, Culture, Sports, Science and TechnologyInstituto Nazionale di Fisica NucleareIllinois State Academy of Science
KeywordsPhysicsCosmic microwave backgroundCosmic background radiationAstronomyPayload (computing)CosmologyCOSMIC cancer databaseObservational cosmologySpacecraftPolarization (electrochemistry)AstrophysicsAerospace engineeringDark energyOptics

Abstract

fetched live from OpenAlex

Abstract LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. The Japan Aerospace Exploration Agency (JAXA) selected LiteBIRD in May 2019 as a strategic large-class (L-class) mission, with an expected launch in the late 2020s using JAXA’s H3 rocket. LiteBIRD is planned to orbit the Sun–Earth Lagrangian point L2, where it will map the cosmic microwave background polarization over the entire sky for three years, with three telescopes in 15 frequency bands between 34 and 448 GHz, to achieve an unprecedented total sensitivity of $2.2\, \mu$K-arcmin, with a typical angular resolution of 0.5○ at 100 GHz. The primary scientific objective of LiteBIRD is to search for the signal from cosmic inflation, either making a discovery or ruling out well-motivated inflationary models. The measurements of LiteBIRD will also provide us with insight into the quantum nature of gravity and other new physics beyond the standard models of particle physics and cosmology. We provide an overview of the LiteBIRD project, including scientific objectives, mission and system requirements, operation concept, spacecraft and payload module design, expected scientific outcomes, potential design extensions, and synergies with other projects.

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)0.002
metaresearch head score (Gemma)0.001
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.002
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.002
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0020.001

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 head0.009
GPT teacher head0.255
Teacher spread0.246 · 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

Citations326
Published2022
Admission routes1
Has abstractyes

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