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Record W3081572918 · doi:10.3847/1538-4357/ac1596

CMB-S4: Forecasting Constraints on Primordial Gravitational Waves

2022· article· en· W3081572918 on OpenAlexafffund
Kevork N. Abazajian, Graeme E. Addison, Peter Adshead, Zeeshan Ahmed, D. S. Akerib, Aamir Ali, S. W. Allen, David Alonso, Marcelo A. Alvarez, Mustafa A. Amin, A. J. Anderson, Kam Arnold, Peter Ashton, C. Baccigalupi, Debbie Bard, D. Barkats, Darcy Barron, P. S. Barry, James G. Bartlett, R. Basu Thakur, Nicholas Battaglia, Rachel Bean, C. Bebek, A. N. Bender, B. A. Benson, F. Bianchini, C. A. Bischoff, L. E. Bleem, James J. Bock, S. Bocquet, Kimberly K. Boddy, J. Richard Bond, Julian Borrill, F. R. Bouchet, T. Brinckmann, Sean Bryan, V. Buza, K. Byrum, Carlos Hervias Caimapo, Erminia Calabrese, Victoria Calafut, Robert R. Caldwell, J. E. Carlstrom, Julien Carron, T. Cecil, A. Challinor, C. L. Chang, Y. Chinone, Hsiao-Mei Sherry Cho, Asantha Cooray, Will Coulton, T. M. Crawford, A. T. Crites, A. Cukierman, Francis-Yan Cyr-Racine, T. de Haan, Jacques Delabrouille, Mark J. Devlin, Eleonora Di Valentino, M. Dierickx, M. Dobbs, Shannon M. Duff, Cora Dvorkin, Joseph R. Eimer, T. Elleflot, Josquin Errard, Thomas Essinger-Hileman, Giulio Fabbian, Chang Qing Feng, Simone Ferraro, J. P. Filippini, Raphael Flauger, B. Flaugher, Aurélien A. Fraisse, Andrei Frolov, Nicholas Galitzki, Patricio A. Gallardo, S. Galli, K. Ganga, M. Gerbino, Vera Gluscevic, N. Goeckner-Wald, Daniel Green, Daniel Grin, Evan Grohs, R. Gualtieri, Jon E. Gudmundsson, Ian Gullett, N. Gupta, Salman Habib, M. Halpern, N. W. Halverson, Shaul Hanany, Kathleen Harrington, M. Hasegawa, Matthew Hasselfield, M. Hazumi, Katrin Heitmann, Shawn Henderson, Brandon S. Hensley, Charles A. Hill, J. Colin Hill, Renée Hložek, Shuay-Pwu Patty Ho, D. Hoang, G. P. Holder, W. L. Holzapfel, J. C. Hood, Johannes Hubmayr, K. M. Huffenberger, H. Hui, K. D. Irwin, O. Jeong, Bradley R. Johnson, W. C. Jones, J. Kang, K. S. Karkare, N. Katayama, Reijo Keskitalo, Theodore Kisner, Lloyd Knox, Brian J. Koopman, Arthur Kosowsky, J. M. Kovac, Ely D. Kovetz, Steve Kuhlmann, Chao‐Lin Kuo, A. Kusaka, A. Lähteenmäki, Charles R. Lawrence, Adrian T. Lee, Antony Lewis, Dale Li, Eric V. Linder, Marilena Loverde, A. E. Lowitz, Phil M. Lubin, Mathew S. Madhavacheril, A. Mantz, Gabriela A. Marques, Frederick Matsuda, P. Mauskopf, Heather McCarrick, Jeffrey McMahon, P. Daniel Meerburg, Jean-Baptiste Melin, F. Menanteau, Joel Meyers, M. Millea, J. J. Mohr, Lorenzo Moncelsi, M. E. Monzani, Tony Mroczkowski, Suvodip Mukherjee, Johanna M. Nagy, Toshiya Namikawa, F. Nati, T. Natoli, Laura Newburgh, Michael D. Niemack, H. Nishino, B. Nord, V. Novosad, Roger O’Brient, S. Padin, S. Palladino, Bruce Partridge, Don Petravick, E. Pierpaoli, Levon Pogosian, Karthik Prabhu, C. Pryke, Giuseppe Puglisi, B. Racine, A. Rahlin, Mayuri Sathyanarayana Rao, Marco Raveri, C. L. Reichardt, M. Remazeilles, G. Rocha, Natalie A. Roe, Anirban Roy, J. E. Ruhl, Maria Salatino, B. R. Saliwanchik, Emmanuel Schaan, A. Schillaci, Benjamin L. Schmitt, Marcel Schmittfull, D. Scott, Neelima Sehgal, Sarah Shandera, Blake D. Sherwin, E. Shirokoff, Sara M. Simon, Anže Slosar, David N. Spergel, T. St. Germaine, Suzanne T. Staggs, A. A. Stark, Glenn D. Starkman, R. Stompor, Chris Stoughton, Aritoki Suzuki, O. Tajima, G. P. Teply, K. Thompson, B. Thorne, Peter Timbie, M. Tomasi, M. Tristram, Gregory S. Tucker, Caterina Umiltà, Alexander van Engelen, Eve M. Vavagiakis, J. D. Vieira, A. G. Vieregg, Kasey Wagoner, Benjamin Wallisch, Gensheng Wang, Scott Watson, Benjamin Westbrook, N. Whitehorn, Edward J. Wollack, W. L. K. Wu, Zhilei Xu, Huan Yang, Siavash Yasini, V. Yefremenko, K. W. Yoon, E. Young, Cyndia Yu, A. Zonca

Bibliographic record

VenueThe Astrophysical Journal · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsPerimeter InstituteSimon Fraser UniversityUniversity of British ColumbiaMcGill UniversityCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersLawrence Berkeley National LaboratorySLAC National Accelerator LaboratoryFermilabScience and Technology Facilities CouncilOffice of ScienceNuclear Safety and Security CommissionAgence Nationale de la RechercheNederlandse Organisatie voor Wetenschappelijk OnderzoekArgonne National LaboratoryU.S. Department of EnergyEuropean CommissionNational Energy Research Scientific Computing CenterCanadian Institute for Advanced ResearchBasic Energy SciencesNatural Sciences and Engineering Research Council of CanadaAlfred P. Sloan FoundationNational Aeronautics and Space AdministrationSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungHarvard UniversityNational Science Foundation
KeywordsCosmic microwave backgroundGravitational wavePhysicsGravitational lensGravitationAstrophysicsSkyPolarization (electrochemistry)AstronomyRedshiftOpticsGalaxy

Abstract

fetched live from OpenAlex

Abstract CMB-S4—the next-generation ground-based cosmic microwave background (CMB) experiment—is set to significantly advance the sensitivity of CMB measurements and enhance our understanding of the origin and evolution of the universe. Among the science cases pursued with CMB-S4, the quest for detecting primordial gravitational waves is a central driver of the experimental design. This work details the development of a forecasting framework that includes a power-spectrum-based semianalytic projection tool, targeted explicitly toward optimizing constraints on the tensor-to-scalar ratio, r , in the presence of Galactic foregrounds and gravitational lensing of the CMB. This framework is unique in its direct use of information from the achieved performance of current Stage 2–3 CMB experiments to robustly forecast the science reach of upcoming CMB-polarization endeavors. The methodology allows for rapid iteration over experimental configurations and offers a flexible way to optimize the design of future experiments, given a desired scientific goal. To form a closed-loop process, we couple this semianalytic tool with map-based validation studies, which allow for the injection of additional complexity and verification of our forecasts with several independent analysis methods. We document multiple rounds of forecasts for CMB-S4 using this process and the resulting establishment of the current reference design of the primordial gravitational-wave component of the Stage-4 experiment, optimized to achieve our science goals of detecting primordial gravitational waves for r > 0.003 at greater than 5 σ , or in the absence of a detection, of reaching an upper limit of r < 0.001 at 95% CL.

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 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)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesScience and technology studies, Insufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: Theoretical or conceptual
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.074
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0020.000

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 head0.016
GPT teacher head0.250
Teacher spread0.234 · 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 teacher head, not a consensus.

Study designTheoretical or conceptual
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

Citations261
Published2022
Admission routes2
Has abstractyes

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