Improved limits on the tensor-to-scalar ratio using BICEP and Planck data

M. Tristram, A. J. Banday, K. M. Górski, R. Keskitalo, C. R. Lawrence, K. J. Andersen, R. B. Barreiro, J. Borrill, L. P. L. Colombo, H. K. Eriksen, R. Fernandez-Cobos, T. S. Kisner, E. Martínez-González, B. Partridge, D. Scott, T. L. Svalheim, and I. K. Wehus
Phys. Rev. D 105, 083524 – Published 26 April 2022

Abstract

We present constraints on the tensor-to-scalar ratio r using a combination of BICEP/Keck 2018 (BK18) and Planck PR4 data allowing us to fit for r consistently with the six parameters of the ΛCDM model. We discuss the sensitivity of constraints on r to uncertainties in the ΛCDM parameters as defined by the Planck data. In particular, we are able to derive a constraint on the reionization optical depth τ and thus propagate its uncertainty into the posterior distribution for r. While Planck sensitivity to r is slightly lower than the current ground-based measurements, the combination of Planck with BK18 and baryon-acoustic-oscillation data yields results consistent with r=0 and tightens the constraint to r<0.032 at 95% confidence.

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  • Received 15 December 2021
  • Accepted 1 April 2022

DOI:https://doi.org/10.1103/PhysRevD.105.083524

© 2022 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

M. Tristram1, A. J. Banday2, K. M. Górski3,4, R. Keskitalo5,6, C. R. Lawrence3, K. J. Andersen7, R. B. Barreiro8, J. Borrill5,9, L. P. L. Colombo10, H. K. Eriksen7, R. Fernandez-Cobos11, T. S. Kisner5,6, E. Martínez-González8, B. Partridge12, D. Scott13, T. L. Svalheim7, and I. K. Wehus7

  • 1Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
  • 2IRAP, Université de Toulouse, CNRS, CNES, UPS, (Toulouse), France
  • 3Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
  • 4Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
  • 5Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, California, USA
  • 6Department of Physics and Space Sciences Laboratory, University of California, Berkeley, California, USA
  • 7Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
  • 8Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avda. de los Castros s/n, Santander, Spain
  • 9Space Sciences Laboratory, University of California, Berkeley, California, USA
  • 10Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
  • 11Dpto. de Matemàticas, Estadística y Computación, Universidad de Cantabria, Avda. de los Castros s/n, E-39005 Santander, Spain
  • 12Haverford College Astronomy Department, 370 Lancaster Avenue, Haverford, Pennsylvania, USA
  • 13Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada

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Issue

Vol. 105, Iss. 8 — 15 April 2022

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