1/3 factor in the CMB Sachs-Wolfe effect

J. Hwang, T. Padmanabhan, O. Lahav, and H. Noh
Phys. Rev. D 65, 043005 – Published 23 January 2002
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Abstract

We point out that a pseudo Newtonian interpretation of the 1/3 factor in the Sachs-Wolfe effect, which relates the fluctuations in temperature and potential, δT/T=(1/3)δΦ, is not supported by the general relativistic analysis. Dividing the full gravitational effect into separate parts depends on the choice of time slicing (gauge) and there exist infinitely many different choices. More importantly, interpreting the parts as being due to the gravitational redshift and the time dilation is not justified in the rigorous relativistic perturbation theory. We suggest regarding the 1/3 factor as a general relativistic result that applies in a restricted situation of adiabatic perturbation in the K=0=Λ model with the last scattering occurring in the matter dominated era. For an isocurvature initial condition the corresponding result δT/T=2δΦ has a different numerical coefficient.

  • Received 17 July 2001

DOI:https://doi.org/10.1103/PhysRevD.65.043005

©2002 American Physical Society

Authors & Affiliations

J. Hwang1,2, T. Padmanabhan3, O. Lahav2, and H. Noh4,2

  • 1Department of Astronomy and Atmospheric Sciences, Kyungpook National University, Taegu, Korea
  • 2Institute of Astronomy, Madingley Road, Cambridge, United Kingdom
  • 3Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkind, Pune 411 007, India
  • 4Korea Astronomy Observatory, San 36-1, Whaam-dong, Yusung-gu, Daejon, Korea

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Issue

Vol. 65, Iss. 4 — 15 February 2002

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