The Standard Model of Cosmology: A Skeptic's Guide

Abstract

The status of the standard cosmological model, also known as "LCDM" is described. With some simple assumptions, this model fits a wide range of data, with just six (or seven) free parameters. One should be skeptical about this claim, since it implies that we now have an astonishingly good picture of the statistical properties of the large-scale Universe. However, the successes of the model cannot be denied, including more than 1000 sigma worth of detection of CMB anisotropy power. The model is older than most modern astrophysicists seem to appreciate, and has not fundamentally changed for more than a quarter of a century. Tensions and anomalies are often discussed, and while we should of course be open to the possibility of new physics, we should also be skeptical of the importance of 2-3 sigma differences between data sets until they become more significant. Still, today's SMC is surely not the full story and we should be looking for extensions or new ingredients to the model, guided throughout by a skeptical outlook.