Monopole Fluctuation of the CMB and its Gauge Invariance

TL;DR

This paper develops a gauge-invariant theoretical framework for the CMB monopole fluctuation, resolving previous divergences and clarifying its status as a fundamental, observable cosmological parameter derived from the angle-averaged temperature.

Contribution

It introduces a gauge-invariant description of the CMB monopole fluctuation and computes its value within the ΛCDM model, addressing previous issues with divergences and gauge dependence.

Findings

Monopole power C_0 = 1.66×10^{-9} in ΛCDM model.

Gauge-invariance of higher multipoles confirmed.

Monopole fluctuation is a well-defined, model-dependent observable.

Abstract

The standard theoretical description $\Theta(\hat n)$ of the observed CMB temperature anisotropies is gauge-dependent. It is, however, well known that the gauge mode is limited to the monopole and the higher angular multipoles $\Theta_l$ ($l\geq1$) 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 $C_0=1.66\times10^{-9}$ in a $\Lambda$CDM model. While the gauge-dependence in the standard calculations originates from the ambiguity in defining the hypersurface for the background CMB temperature $\bar T$ 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.