Constraining thawing dark energy using galaxy cluster number counts
We study the formation of galaxy clusters in the presence of thawing class of scalar field dark energy (DE). We consider cases where the scalar field has canonical as well as non-canonical kinetic terms in its action. We also consider various forms for the potential of the scalar field, e.g. linear,...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2013-06, Vol.432 (2), p.1513-1524 |
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