activity
20192024
most citedTurnaround radius of galaxy clusters in N-body simulations

22 citations · 36 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2024

Searching for a signature of turnaround in galaxy clusters with convolutional neural networks

Nikolaos Triantafyllou, Giorgos Korkidis, Vasiliki Pavlidou +1

Galaxy clusters are important cosmological probes that have helped to establish the CDM paradigm as the standard model of cosmology. However, recent tensions between diff…

astro-ph.CO2024

Hubble Expansion Signature on Simulated Halo Density Profiles: A Path to Observing the Turnaround Radius

Giorgos Korkidis, Vasiliki Pavlidou

Density profiles are important tools in galaxy cluster research, offering insights into clusters dynamical states and their relationship with the broader Universe. While these prof…

astro-ph.CO2024★ 2 cited

Mass scaling relations for dark halos from an analytic universal outer density profile

Giorgos Korkidis, Vasiliki Pavlidou

The average matter density within the turnaround scale, which demarcates where galaxies shift from clustering around a structure to joining the expansion of the Universe, is an imp…

astro-ph.CO2023★ 3 cited

Turnaround density evolution encodes cosmology in simulations

Giorgos Korkidis, Vasiliki Pavlidou, Konstantinos Tassis

The mean matter density within the turnaround radius, which is the boundary that separates a nonexpanding structure from the Hubble flow, was recently proposed as a novel cosmologi…

astro-ph.CO2020★ 9 cited

Turnaround density as a probe of the cosmological constant

Vasiliki Pavlidou, Giorgos Korkidis, Theodore Tomaras +1

Spherical collapse predicts that a single value of the turnaround density (average matter density within the scale on which a structure detaches from the Hubble flow) characterizes…

astro-ph.CO2019★ 22 cited

Turnaround radius of galaxy clusters in N-body simulations

Giorgos Korkidis, Vasiliki Pavlidou, Konstantinos Tassis +3

We use N-body simulations to examine whether a characteristic turnaround radius, as predicted from the spherical collapse model in a Universe, can be meaningfully iden…