activity
20012024
most citedDark energy and the structure of the Coma cluster of galaxies

53 citations · 109 across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2024★ 1 cited

Energy equipartition in Globular Clusters through the eyes of dynamical models

M. Teodori, O. Straniero, M. Merafina

Gravitational encounters drive globular clusters toward energy equipartition, mass segregation and evaporation altering structural, spatial and kinematic features. We determine the…

gr-qc2024★ 3 cited

Orbital precession and other properties of two-body motion in the presence of dark energy

Gennady S. Bisnovatyi-Kogan, Marco Merafina

We consider the Kepler two-body problem in the presence of a cosmological constant Lambda. Several dimensionless parameters characterizing the possible orbit typologies are used to…

astro-ph.GA2022

Generalization of the Fokker-Planck equation for stellar orbit diffusion in multi-mass star systems

Marco Merafina, Matteo Teodori

We improve the standard theory of collisional stellar systems by considering the presence of a continuous mass distribution. The calculus of the diffusion coefficients is generaliz…

astro-ph.GA2020★ 15 cited

On self-gravitating strange dark matter halos around galaxies

Marco Merafina, Francesco G. Saturni, Catalina Curceanu +2

A new family of nonrelativistic, Newtonian, non-quantum equilibrium configurations describing galactic halos is introduced, by considering strange quark matter conglomerates with m…

gr-qc2019★ 3 cited

Two body problem in presence of cosmological constant

G. S. Bisnovatyi-Kogan, M. Merafina

We consider the Kepler two-body problem in presence of the cosmological constant . Contrary to the classical case, where finite solutions exist for any angular momentum of the s…

astro-ph.GA2016

Massive black holes interactions during the assembly of heavy sub-structures in the centre of galaxy clusters

M. Donnari, M. Arca-Sedda, M. Merafina

We performed a series of direct N-body simulations with the aim to follow the dynamical evolution of a galaxy cluster (GC) () in different environ…