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George Alestas

Researcher at University of Ioannina

Publications -  15
Citations -  634

George Alestas is an academic researcher from University of Ioannina. The author has contributed to research in topics: Redshift & Dark energy. The author has an hindex of 5, co-authored 10 publications receiving 128 citations.

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Journal ArticleDOI

Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Elcio Abdalla, +202 more
TL;DR: In this paper , the authors focus on the 5.0σ tension between the Planck CMB estimate of the Hubble constant H0 and the SH0ES collaboration measurements and discuss the importance of trying to fit a full array of data with a single model.
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H 0 tension, phantom dark energy, and cosmological parameter degeneracies

TL;DR: In this article, the best fit value of the CMB power spectrum is degenerate with a constant equation-of-state parameter $w, in accordance with the approximate effective linear equation ${H}_{0}+30.47=0$.
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A $w$ phantom transition at $z_t<0.1$ as a resolution of the Hubble tension

TL;DR: In this article, the authors proposed a model called the Late $w$ Phantom Transition (LwPT) model which avoids the discontinuity of the Pantheon Hubble diagram and thus does not require a step in the Hubble diagram.
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Late-time approaches to the Hubble tension deforming H(z), worsen the growth tension

TL;DR: In this paper, the authors show that the growth tension between dynamical probe data and CMB constraints is worse than the corresponding tension of the standard Planck18/$\Lambda$CDM model.
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Late-transition versus smooth <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>H</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>z</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> -deformation models for the resolution of the Hubble crisis

TL;DR: In this paper , the authors compare the quality of fit to cosmological data of this class of models, with the corresponding quality of fitting of the cosmologically constant model ($\Lambda$CDM) and some of the best smooth $H(z)$ deformation models.