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The LiteBIRD mission to explore cosmic inflation

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arxiv 2406.02724 v1 pith:FGDPV22M submitted 2024-06-04 astro-ph.IM astro-ph.COphysics.ins-det

T. Ghigna , A. Adler , K. Aizawa , H. Akamatsu , R. Akizawa , E. Allys , A. Anand , J. Aumont
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J. Austermann S. Azzoni C. Baccigalupi M. Ballardini A. J. Banday R. B. Barreiro N. Bartolo S. Basak A. Basyrov S. Beckman M. Bersanelli M. Bortolami F. Bouchet T. Brinckmann P. Campeti E. Carinos A. Carones F. J. Casas K. Cheung Y. Chinone L. Clermont F. Columbro A. Coppolecchia D. Curtis P. de Bernardis T. de Haan E. de la Hoz M. De Petris S. Della Torre G. Delle Monache E. Di Giorgi C. Dickinson P. Diego-Palazuelos J. J. Díaz García M. Dobbs T. Dotani G. D'Alessandro H. K. Eriksen J. Errard T. Essinger-Hileman N. Farias E. Ferreira C. Franceschet U. Fuskeland G. Galloni M. Galloway K. Ganga M. Gerbino M. Gervasi R. T. Génova-Santos S. Giardiello C. Gimeno-Amo E. Gjerl{o}w R. González González L. Grandsire A. Gruppuso N. W. Halverson P. Hargrave S. E. Harper M. Hazumi S. Henrot-Versillé L. T. Hergt D. Herranz E. Hivon R. A. Hlozek T. D. Hoang J. Hubmayr K. Ichiki K. Ikuma H. Ishino G. Jaehnig B. Jost K. Kohri K. Konishi L. Lamagna M. Lattanzi C. Leloup F. Levrier A. I. Lonappan G. Luzzi J. Macias-Perez B. Maffei E. Marchitelli E. Martínez-González S. Masi S. Matarrese T. Matsumura S. Micheli M. Migliaccio M. Monelli L. Montier G. Morgante L. Mousset Y. Nagano R. Nagata P. Natoli A. Novelli F. Noviello I. Obata A. Occhiuzzi K. Odagiri R. Omae L. Pagano A. Paiella D. Paoletti G. Pascual-Cisneros G. Patanchon V. Pavlidou F. Piacentini M. Piat G. Piccirilli M. Pinchera G. Pisano L. Porcelli N. Raffuzzi C. Raum M. Remazeilles A. Ritacco J. Rubino-Martin M. Ruiz-Granda Y. Sakurai G. Savini D. Scott Y. Sekimoto M. Shiraishi G. Signorelli S. L. Stever R. M. Sullivan A. Suzuki R. Takaku H. Takakura S. Takakura Y. Takase. A. Tartari K. Tassis K. L. Thompson M. Tomasi M. Tristram C. Tucker L. Vacher B. van Tent P. Vielva K. Watanuki I. K. Wehus B. Westbrook G. Weymann-Despres B. Winter E. J. Wollack A. Zacchei M. Zannoni Y. Zhou the LiteBIRD Collaboration
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classification astro-ph.IMastro-ph.COphysics.ins-det
keywords litebirdmissionwillcosmicscientificsystematicyearachieve
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abstract

LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan's fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the Sun-Earth Lagrangian point L2, this JAXA-led strategic L-class mission will conduct a comprehensive mapping of the CMB polarization across the entire sky. During its 3-year mission, LiteBIRD will employ three telescopes within 15 unique frequency bands (ranging from 34 through 448 GHz), targeting a sensitivity of 2.2\,$\mu$K-arcmin and a resolution of 0.5$^\circ$ at 100\,GHz. Its primary goal is to measure the tensor-to-scalar ratio $r$ with an uncertainty $\delta r = 0.001$, including systematic errors and margin. If $r \geq 0.01$, LiteBIRD expects to achieve a $>5\sigma$ detection in the $\ell=$2-10 and $\ell=$11-200 ranges separately, providing crucial insight into the early Universe. We describe LiteBIRD's scientific objectives, the application of systems engineering to mission requirements, the anticipated scientific impact, and the operations and scanning strategies vital to minimizing systematic effects. We will also highlight LiteBIRD's synergies with concurrent CMB projects.

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Confronting Mukhanov Parametrization of Inflationary Equation-of-State with ACT-DR6

    astro-ph.CO 2025-07 conditional novelty 4.0 of 10

    Mukhanov's equation-of-state model of inflation still fits ACT-DR6-era data, with alpha set by the scalar tilt and beta set by the tensor-to-scalar ratio.

  2. The fate of Quasi-Exponential inflation in the light of ACT-DR6

    astro-ph.CO 2025-06 conditional novelty 4.0 of 10

    A single-parameter quasi-exponential inflation model remains viable for the high spectral index preferred by ACT-DR6, and predicts r≥0.01, to be tested by upcoming CMB missions.

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