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PICO: Probe of Inflation and Cosmic Origins

Hanany, Shaul and Bock, Jamie and Pearson, Tim and Doré, Olivier and O'Brient, Roger and Rocha, Graça (2019) PICO: Probe of Inflation and Cosmic Origins. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20190925-135806088

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Abstract

The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full-sky surveys of intensity and polarization with a final combined-map noise level of 0.87 μK arcmin for the required specifications, equivalent to 3300 Planck missions, and with our current best-estimate would have a noise level of 0.61 μK arcmin (6400 Planck missions). PICO will either determine the energy scale of inflation by detecting the tensor to scalar ratio at a level r = 5×10^(−4) (5σ), or will rule out with more than 5σ all inflation models for which the characteristic scale in the potential is the Planck scale. With LSST's data it could rule out all models of slow-roll inflation. PICO will detect the sum of neutrino masses at >4σ, constrain the effective number of light particle species with ΔN_(eff) < 0.06 (2σ), and elucidate processes affecting the evolution of cosmic structures by measuring the optical depth to reionization with errors limited by cosmic variance and by constraining the evolution of the amplitude of linear fluctuations σ_8(z) with sub-percent accuracy. Cross-correlating PICO's map of the thermal Sunyaev-Zeldovich effect with LSST's gold sample of galaxies will precisely trace the evolution of thermal pressure with z. PICO's maps of the Milky Way will be used to determine the make up of galactic dust and the role of magnetic fields in star formation efficiency. With 21 full sky legacy maps in intensity and polarization, which cannot be obtained in any other way, the mission will enrich many areas of astrophysics. PICO is the only single-platform instrument with the combination of sensitivity, angular resolution, frequency bands, and control of systematic effects that can deliver this compelling, timely, and broad science.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
https://arxiv.org/abs/1902.10541arXivDiscussion Paper
ORCID:
AuthorORCID
Bock, Jamie0000-0002-5710-5212
Pearson, Tim0000-0001-5213-6231
Doré, Olivier0000-0002-5009-7563
Rocha, Graça0000-0002-4150-8076
Additional Information:Report from a Probe-Scale Mission Study. This research was funded by a NASA grant NNX17AK52G to the University of Minnesota / Twin Cities, by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration, and by Lockheed Martin Corporation. Substantial contributions to the development of PICO were volunteered by scientists at many institutions world-wide. They are very gratefully acknowledged. The information presented about the PICO mission concept is pre-decisional and is provided for planning and discussion purposes only. The cost information contained in this document is of a budgetary and planning nature and is intended for informational purposes only. It does not constitute a commitment on the part of JPL and/or Caltech.
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
NASANNX17AK52G
NASA/JPL/CaltechUNSPECIFIED
Lockheed Martin CorporationUNSPECIFIED
Record Number:CaltechAUTHORS:20190925-135806088
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190925-135806088
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:98860
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Sep 2019 21:10
Last Modified:03 Oct 2019 21:45

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