activity
20042020
most citedCrossing the Phantom Divide: Theoretical Implications and Observational Status

356 citations · 1.7k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.CO2020★ 24 cited

Hints for possible low redshift oscillation around the best fit CDM model in the expansion history of the Universe

L. Kazantzidis, H. Koo, S. Nesseris +2

We search for possible deviations from the expectations of the concordance CDM model in the expansion history of the Universe by analysing the Pantheon Type Ia Supernovae (SnIa)…

astro-ph.CO2017★ 228 cited

Tension and constraints on modified gravity parametrizations of from growth rate and Planck data

Savvas Nesseris, George Pantazis, Leandros Perivolaropoulos

We construct an updated and extended compilation of growth rate data consisting of 34 points and including corrections for model dependence. In order to maximize the independence o…

astro-ph.CO2016★ 82 cited

A Comparison of Thawing and Freezing Dark Energy Parametrizations

G. Pantazis, S. Nesseris, L. Perivolaropoulos

Dark energy equation of state parametrizations with two parameters and given monotonicity are generically either convex or concave functions. This makes them suitable for fi…

astro-ph.CO2013★ 117 cited

Observational constraints on viable f(R) parametrizations with geometrical and dynamical probes

Spyros Basilakos, Savvas Nesseris, Leandros Perivolaropoulos

We demonstrate that a wide range of viable f(R) parameterizations (including the Hu & Sawicki and the Starobinsky models) can be expressed as perturbations deviating from the LCDM…

astro-ph.CO2009★ 36 cited

Comparison of Recent SnIa datasets

J. C. Bueno Sanchez, S. Nesseris, L. Perivolaropoulos

We rank the six latest Type Ia supernova (SnIa) datasets (Constitution (C), Union (U), ESSENCE (Davis) (E), Gold06 (G), SNLS 1yr (S) and SDSS-II (D)) in the context of the Chevalie…

astro-ph2008★ 9 cited

Is the CMB shift parameter connected with the growth of cosmological perturbations?

S. Basilakos, S. Nesseris, L. Perivolaropoulos

We verify numerically that in the context of general relativity (GR), flat models which have the same and CMB shift parameter but different and also h…