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Reconstructing isotropic and anisotropic <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi mathvariant="script">Q</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> cosmologies

Fabrizio Esposito, Sante Carloni, Roberto Cianci, Stefano Vignolo

2022Physical review. D/Physical review. D.63 citationsDOIOpen Access PDF

Abstract

We present a reconstruction algorithm for cosmological models based on $f(\mathcal{Q})$ gravity. We specifically focus on Bianchi type I and Friedmann-Lema\^{\i}tre-Robertson-Walker spacetimes, obtaining exact solutions that might have application in a variety of scenarios such as spontaneous isotropization of Bianchi type I models, dark energy, and inflation, as well as pre-big bang cosmologies.

Topics & Concepts

Type (biology)PhysicsFocus (optics)Mathematical physicsAlgorithmComputer scienceBiologyEcologyOpticsCosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsGalaxies: Formation, Evolution, Phenomena
Reconstructing isotropic and anisotropic <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi mathvariant="script">Q</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> cosmologies | Litcius