Southern Federal

Jul 29, 2024 | link.springer.com | Southern Federal

Correction to: Translational Stroke ResearchIn our recent publication, an error occurred in the recording of author names. The given names were inadvertently listed as family names, and the family names were listed as given names. The incorrect author names are listed below:Kalyuzhnaya Y.N., Logvinov A.K., Pashkevich S.G., Golubova N.V., Seryogina E.S., Potapova E.V., Dremin V.V., Dunaev A.V., Demyanenko S.V.To correct this error, we provide the correct presentation of the author names below:Y. N.

Mar 29, 2024 | link.aps.org | Anish Ghoshal |Maxim Yu. Khlopov |Southern Federal |Zygmunt Lalak

We investigate the production of nonthermal dark matter (DM), χ, during the postinflationary reheating era. For inflation, we consider two slow roll single field inflationary scenarios—generalized version of Hilltop (GH) inflation, and Coleman-Weinberg (CW) inflation.

Mar 26, 2024 | onlinelibrary.wiley.com | Southern Federal

2.1. Synthesis Dimeric complexes of copper(II), Cu1, are synthesized during the interaction of solutions of equimolecular quantities of alcohol and copper acetate hydrate in ethanol (yield 65–75%). A hot solution of 200 mg (1 mmol) copper acetate hydrate in 16 ml of ethanol was added to a 1 mmol hot solution of ligand precursor [312 mg of (5-ethoxy-1-methylbenzimidazol-2-yl)(4-methoxyphenyl)methanol in 10 ml of ethanol], and left at an elevated temperature for 16 h.

Mar 18, 2024 | academic.oup.com | Southern Federal

There is a number of unsolved problems in the theory of planet formation, e.g. the formation of kilometre-scale planetesimals from micron grains. In the context of giant planet formation, the subsequent stages may possibly involve the core accretion mechanism (Mizuno 1980; Bodenheimer & Pollack 1986; Pollack et al. 1996; Boley 2009; Helled et al. 2014). Recently, more attention is drawn to the mechanism of pebble accretion (Ormel & Klahr 2010; Lambrechts & Johansen 2012; Morbidelli et al.

Oct 5, 2023 | academic.oup.com | Southern Federal

Recent advancements in observations have led to the discovery of over 5000 exoplanets (the NASA Exoplanet Archive; Akeson et al. 2013). In particular, observations of giant planets have progressed in the past decade by combining multiple observation methods, such as radial velocity, transit, microlensing, and direct imaging, revealing the presence of giant planets in a variety of environments with orbital radii ranging from ∼10−2 to 103 au (e.g. Zhu & Dong 2021 for a review).