activity
20172025
most citedDynamical origin of non-thermal states in galactic filaments

13 citations · 40 across the 7 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20244 cited

Tidal mass loss in the Fornax dwarf spheroidal galaxy through N-body simulations with Gaia DR3-based orbits

Pierfrancesco Di Cintio, Giuliano Iorio, Francesco Calura +2

The Fornax dwarf spheroidal galaxy (dSph) represents a challenge for some globular cluster (GC) formation models, because an exceptionally high fraction of its stellar mass is lock…

astro-ph.GA20235 cited

Structure of the equivalent Newtonian systems in MOND N-body simulations. Density profiles and the core-cusp problem

Federico Re, Pierfrancesco Di Cintio

We investigate the core-cusp problem of the cold dark matter (CDM) scenario in the context of Modified Newtonian Dynamics (MOND) paradigm exploiting the concept of equivalen…

astro-ph.GA20237 cited

Dynamics of intermediate mass black holes in globular clusters. Wander radius and anisotropy profiles

Pierfrancesco Di Cintio, Mario Pasquato, Luca Barbieri +2

We recently introduced a new method for simulating collisional gravitational N-body systems with approximately linear time scaling with , based on the Multi-Particle Collision (…

cond-mat.stat-mech20219 cited

Kinetic and hydrodynamic regimes in multi-particle-collision dynamics of a one-dimensional fluid with thermal walls

Stefano Lepri, Guido Ciraolo, Pierfrancesco Di Cintio +2

We study the non-equilibrium steady-states of a one-dimensional () fluid in a finite space region of length . Particles interact among themselves by multi-particle collisi…

astro-ph.GA201713 cited

Dynamical origin of non-thermal states in galactic filaments

Pierfrancesco Di Cintio, Shamik Gupta, Lapo Casetti

Observations strongly suggest that filaments in galactic molecular clouds are in a non-thermal state. As a simple model of a filament we study a two-dimensional system of self-grav…