Monopole fluctuation of the CMB and its gauge invariance

Abstract

The standard theoretical description $\mathrm{\ensuremath{\Theta}}(\stackrel{^}{n})$ of the observed cosmic microwave background (CMB) temperature anisotropies is gauge dependent. It is, however, well known that the gauge mode is limited to the monopole and that the higher angular multipoles ${\mathrm{\ensuremath{\Theta}}}_{l}$ ($l\ensuremath{\ge}1$) are gauge invariant. Several attempts have been made in the past to properly define the monopole fluctuation, but the resulting values of the monopole power ${C}_{0}$ are infinite due to the infrared divergences. The infrared divergences arise from the contribution of the uniform gravitational potential to the monopole fluctuation, in violation of the equivalence principle. Here we present the gauge-invariant theoretical description of the observed CMB temperature anisotropies and compute the monopole power ${C}_{0}=1.66\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}9}$ in a $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$ model. While the gauge dependence in the standard calculations originates from the ambiguity in defining the hypersurface for the background CMB temperature $\overline{T}$ today, it is in fact well defined and one of the fundamental cosmological parameters. We argue that once the cosmological parameters are chosen, the monopole fluctuation can be unambiguously inferred from the angle average of the observed CMB temperature, making it a model-dependent ``observable.'' Adopting simple approximations for the anisotropy formation, we derive a gauge-invariant analytical expression for the observed CMB temperature anisotropies to study the CMB monopole fluctuation and the cancellation of the uniform gravitational potential contributions on large scales.