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19932018
most citedOptical Mass Estimates of Galaxy Clusters

390 citations · 1.7k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.CO2018★ 11 cited

Strongly Coupled Dark Energy Cosmologies yielding large mass Primordial Black Holes

S. A. Bonometto, R. Mainini, M. Mezzetti

Large primordial Black Hole (PBH) formation is enhanced if strongly coupled scalar and spinor fields ( and ) are a stable cosmic component since the primeval radiative expans…

astro-ph.CO2017★ 15 cited

Strongly Coupled Dark Energy with Warm dark matter vs. LCDM

Silvio A. Bonometto, Marino Mezzetti, Roberto Mainini

Cosmologies including strongly Coupled (SC) Dark Energy (DE) and Warm dark matter (SCDEW) are based on a conformally invariant (CI) attractor solution modifying the early radiative…

astro-ph.CO2014

Strongly Coupled Cosmologies

S. A. Bonometto, M. Mezzetti, I. Musco +2

Models including an energy transfer from CDM to DE are widely considered in the literature, namely to allow DE a significant high-z density. Strongly Coupled cosmologies assume a m…

astro-ph.CO2014★ 4 cited

Sample variance in N--body simulations and impact on tomographic shear predictions

Luciano Casarini, Oliver Piattella, Silvio Bonometto +1

We study the effects of sample variance in N--body simulations, as a function of the size of the simulation box, namely in connection with predictions on tomographic shear spectra.…

astro-ph.CO2013★ 1 cited

Recovery of fluctuation spectrum evolution from tomographic shear spectra

Silvio A. Bonometto, Marino Mezzetti

Forthcoming large angle surveys are planned to obtain high precision tomographic shear data. In principle, they will allow us to recover the spectra of matter density fluctuation,…

astro-ph.CO2012★ 8 cited

Constraints on Dark Energy state equation with varying pivoting redshift

Dario Scovacricchi, Silvio A. Bonometto, Marino Mezzetti +1

We assume the DE state equations w(a) = w_0+w_a(a_p-a), and study the dependence of the constraints on w_0 and w_a coefficients on the pivoting redshift 1+z_p=1/a_p. Coefficients a…