In this review we summarize, expand, and set in context recent developments on the thermodynamics of black holes in extended phase space, where the cosmological constant is interpreted as thermodynamic pressure and treated as a thermodynamic variable in its own right. We specifically consider the thermodynamics of higher-dimensional rotating asymptotically flat and AdS black holes…
Galaxies Template
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About the Galaxies format
Galaxies is a peer-reviewed journal published by MDPI, covering Astrophysics and Cosmic Phenomena, Stellar, planetary, and galactic studies, Galaxies: Formation, Evolution, Phenomena. Over its lifetime it has published 1,290 papers, which have received 13,251 citations.
| Publisher | MDPI |
|---|---|
| Reference style | Numbered (MDPI) Numbered — [1], [2] in the text 1. Smith, A.; Jones, B.; Lee, C. A Representative Article Title. Galaxies 2023, 12, 45–58.
Formats any DOI in Galaxies style. No sign-up. |
| Publishes research in | Astrophysics and Cosmic Phenomena Stellar, planetary, and galactic studies Galaxies: Formation, Evolution, Phenomena Gamma-ray bursts and supernovae Astronomy and Astrophysical Research |
| ISSN | 2075-4434 |
| Citation impact (2-yr) | 2.51 |
| h-index | 48 |
| i10-index | 368 |
| Article processing charge | $1,515 |
| Open access | Yes — indexed in DOAJ |
| Top institutions publishing here | Centre National de la Recherche Scientifique |
| Journal website | www.mdpi.com |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
Papers published in Galaxies per year
Citation impact of Galaxies by publication year
Citations each year’s papers have accumulated so far — the most recent years are still building up.
Most-cited papers in Galaxies
In this work, we review a plethora of modified theories of gravity with generalized curvature-matter couplings. The explicit nonminimal couplings, for instance, between an arbitrary function of the scalar curvature R and the Lagrangian density of matter, induces a non-vanishing covariant derivative of the energy-momentum tensor, implying non-geodesic motion and, consequently, leads to the appearance…
The ΛCDM model, or concordance cosmology, as it is often called, is a paradigm at its maturity. It is clearly able to describe the universe at large scale, even if some issues remain open, such as the cosmological constant problem, the small-scale problems in galaxy formation, or the unexplained anomalies in the CMB. ΛCDM clearly…
The difference from 4 to 6 σ in the Hubble constant (H0) between the values observed with the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (Cosmic Microwave Background obtained by the Planck data) still challenges the astrophysics and cosmology community. Previous analysis has shown that there is an evolution in the…
We explore the effective degrees of freedom in the early Universe, from before the electroweak scale at a few femtoseconds after the Big Bang until the last positrons disappeared a few minutes later. We look at the established concepts of effective degrees of freedom for energy density, pressure, and entropy density, and introduce effective degrees…