Transverse Velocities with the Moving Lens Effect

Selim C. Hotinli, Joel Meyers, Neal Dalal, Andrew H. Jaffe, Matthew C. Johnson, James B. Mertens, Moritz Münchmeyer, Kendrick M. Smith, and Alexander van Engelen
Phys. Rev. Lett. 123, 061301 – Published 6 August 2019

Abstract

Gravitational potentials that change in time induce fluctuations in the observed cosmic microwave background (CMB) temperature. Cosmological structure moving transverse to our line of sight provides a specific example known as the moving lens effect. Here, we explore how the observed CMB temperature fluctuations, combined with the observed matter overdensity, can be used to infer the transverse velocity of cosmological structures on large scales. We show that near-future CMB surveys and galaxy surveys will have the statistical power to make a first detection of the moving lens effect, and we discuss applications for the reconstructed transverse velocity.

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  • Received 8 January 2019
  • Revised 29 May 2019

DOI:https://doi.org/10.1103/PhysRevLett.123.061301

© 2019 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Selim C. Hotinli1, Joel Meyers2, Neal Dalal3, Andrew H. Jaffe1, Matthew C. Johnson4,3, James B. Mertens4,3, Moritz Münchmeyer3, Kendrick M. Smith3, and Alexander van Engelen5

  • 1Astrophysics Group and Imperial Centre for Inference and Cosmology, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, United Kingdom
  • 2Department of Physics, Southern Methodist University, 3215 Daniel Avenue, Dallas, Texas 75275, USA
  • 3Perimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario N2L 2Y5, Canada
  • 4Department of Physics and Astronomy, York University, Toronto, Ontario M3J 1P3, Canada
  • 5Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 Saint George Street, Toronto, Ontario M5S 3H8, Canada

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Issue

Vol. 123, Iss. 6 — 9 August 2019

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