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Topological invariant quintessence

The issues of quintessence and cosmic acceleration can be discussed in the framework of $F(R, {\cal G})$ theories of gravity where $R$ is the Ricci curvature scalar and ${\cal G}$ is the Gauss-Bonnet topological invariant. It is possible to show that such an approach exhausts all the curvature content related to the Riemann tensor giving rise to a fully geometric approach to dark energy.

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AuthorshipTopic signalTopic signalTopic signalRelated contextWTopological invariant quintessencepreprint / 2014AMariafelicia De LaurentisResearcherTastro-ph.GA10150 worksTgr-qc10727 worksThep-th13268 works
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Topological invariant quintessence

preprint / 2014

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