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The evolution of the virial overdensity $\Delta_{\rm vir}$ for $\Lambda$CDM and seven dynamical dark-energy models is investigated in the extended spherical collapse model (SCM).
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2011
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2003
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R. E. Smith, J. A. Peacock, A. Jenkins, S. D. M. White, C. S. Frenk, F. R. Pearce et al., Stable clustering, the halo model and non-linear cosmological power spectra , MNRAS 341
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P. S. Corasaniti and E. J. Copeland, Model independent approach to the dark energy equation of state , Phys. Rev. D 67
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2003
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R. C. Batista and F. Pace, Structure formation in inhomogeneous Early Dark Energy models , JCAP 6
2013
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R. C. Batista and V. Marra, Clustering dark energy and halo abundances , JCAP 11
2017
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2017
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R. Reischke, F. Pace, S. Meyer and B. M. Schäfer, Shear and vorticity in the spherical collapse of dark matter haloes , MNRAS 473
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