$\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum

TL;DR

This paper introduces a data-driven approach using a variational autoencoder to parametrize CMB temperature spectra, capturing key features and revealing new degrees of freedom, including effects of early dark energy.

Contribution

It presents a novel latent space parametrization of CMB spectra that disentangles physical features and isolates EDE effects, enhancing model flexibility and interpretability.

Findings

Latent parameters accurately reconstruct spectra within Planck errors.

Discovered a latent parameter isolating EDE effects from ΛCDM.

Constraints on latent parameters align with previous cosmological results.

Abstract

Finding the best parametrization for cosmological models in the absence of first-principle theories is an open question. We propose a data-driven parametrization of cosmological models given by the disentangled 'latent' representation of a variational autoencoder (VAE) trained to compress cosmic microwave background (CMB) temperature power spectra. We consider a broad range of $\Lambda$CDM and beyond-$\Lambda$CDM cosmologies with an additional early dark energy (EDE) component. We show that these spectra can be compressed into 5 ($\Lambda$CDM) or 8 (EDE) independent latent parameters, as expected when using temperature power spectra alone, and which reconstruct spectra at an accuracy well within the Planck errors. These latent parameters have a physical interpretation in terms of well-known features of the CMB temperature spectrum: these include the position, height and even-odd modulation of the acoustic peaks, as well as the gravitational lensing effect. The VAE also discovers one latent parameter which entirely isolates the EDE effects from those related to $\Lambda$CDM parameters, thus revealing a previously unknown degree of freedom in the CMB temperature power spectrum. We further showcase how to place constraints on the latent parameters using Planck data as typically done for cosmological parameters, obtaining latent values consistent with previous $\Lambda$CDM and EDE cosmological constraints. Our work demonstrates the potential of a data-driven reformulation of current beyond-$\Lambda$CDM phenomenological models into the independent degrees of freedom to which the data observables are sensitive.