# Understanding CMB physics through the exploration of exotic cosmological models: a classroom study using CLASS

## TL;DR

This paper presents a classroom exercise using the CLASS code to compare $bc$CDM with exotic models, helping students understand the impact of cosmological parameters on CMB observations and the nature of the standard model.

## Contribution

It introduces an educational approach that uses computational modeling of CMB spectra to teach students about cosmological models and their underlying physics.

## Key findings

- Students grasp the influence of parameters on CMB spectra
- Comparison highlights differences between $bc$CDM and exotic models
- Exercise enhances understanding of complex CMB physics

## Abstract

Every cosmology lecturer these days is confronted with teaching the modern cosmological standard model $\Lambda$CDM, and there are many approaches to do this. However, the danger is imminent that it is presented to students as something set into stone, merely to be accepted as a fact based on the plenty of evidences we have. This is even more critical, given that the standard model of cosmology confronts us with entities not yet fully understood, namely a cosmological constant $\Lambda$ and cold dark matter. In this article, we report on an advanced cosmology course exercise, conducted in computer lab, which was conceived as a means to have students experience first-hand why the $\Lambda$CDM model has become so prevalent in the interpretation of modern cosmological data. To this end, we focused on the cosmic microwave background radiation (CMB) and calculated theoretical temperature and matter power spectra, using the modern Boltzmann code CLASS. By comparing and analyzing the outcome for $\Lambda$CDM, as well as for three other exotic cosmological models, the students were able to grasp the impact of cosmological parameters on CMB observables, and also to understand some of the complicated CMB physics in a direct way. Our chosen examples are not exhaustive and can be easily modified or expanded, so we express the hope that this article will serve as a valuable resource for interested students and lecturers.