Reconstructing isotropic and anisotropic $f(\mathcal{Q})$ cosmologies

Understand

We present a reconstruction algorithm for cosmological models based on $f(\mathcal{Q})$ gravity.

• We specifically focus on obtaining exact Bianchi Type-I and Friedmann-Lema\^{\i}tre-Robertson-Walker solutions, finding solutions that might have application in a variety of scenarios such as spontaneous isotropization of Bianchi Type-I models, dark energy, inflation as well as pre-Big Bang cosmologies.