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PICO: Probe of Inflation and Cosmic Origins

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arxiv 1908.07495 v1 pith:F7XVF4UJ submitted 2019-08-20 astro-ph.IM astro-ph.COastro-ph.GAhep-th

S. Hanany , M. Alvarez , E. Artis , P. Ashton , J. Aumont , R. Aurlien , R. Banerji , R. B. Barreiro
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J. G. Bartlett S. Basak N. Battaglia J. Bock K. K. Boddy M. Bonato J. Borrill F. Bouchet F. Boulanger B. Burkhart J. Chluba D. Chuss S. Clark J. Cooperrider B. P. Crill G. De Zotti J. Delabrouille E. Di Valentino J. Didier O. Dore H. K. Eriksen J. Errard T. Essinger-Hileman S. Feeney J. Filippini L. Fissel R. Flauger U. Fuskeland V. Gluscevic K. M. Gorski D. Green B. Hensley D. Herranz J. C. Hill E. Hivon R. Hlozek J. Hubmayr B. R. Johnson W. Jones T. Jones L. Knox A. Kogut M. Lopez-Caniego C. Lawrence A. Lazarian Z. Li M. Madhavacheril J. B. Melin J. Meyers C. Murray M. Negrello G. Novak R. O'Brient C. Paine T. Pearson L. Pogosian C. Pryke G. Puglisi M. Remazeilles G. Rocha M. Schmittfull D. Scott P. Shirron I. Stephens B. Sutin M. Tomasi A. Trangsrud A. van Engelen F. Vansyngel I. K. Wehus Q. Wen S. Xu K. Young A. Zonca
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classification astro-ph.IMastro-ph.COastro-ph.GAhep-th
keywords picocosmicinflationoriginsprobeachievablebandsconsisting
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The Probe of Inflation and Cosmic Origins (PICO) is a proposed probe-scale space mission consisting of an imaging polarimeter operating in frequency bands between 20 and 800 GHz. We describe the science achievable by PICO, which has sensitivity equivalent to more than 3300 Planck missions, the technical implementation, the schedule and cost.

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Cited by 2 Pith papers

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

  1. Detecting rotation from lensing in the CMB

    astro-ph.CO 2025-01 accept novelty 5.0 of 10

    If lensing field rotation also rotates CMB polarization, SPT-3G plus galaxy-survey templates should detect the effect at SNR~7, and CMB-S4 deep could detect it internally at 3.9σ.

  2. Gravitational Waves from Spectator Scalar Fields

    hep-ph 2025-06 conditional novelty 4.0 of 10

    Heavy spectator scalar fields with masses near the inflationary Hubble scale generate a gravitational wave background observable across pulsar timing arrays, LISA, and ground-based interferometers, with constraints re...

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