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Articles by A. Bykov
Optically Addressing Spin Relaxation Mechanism in 2D Hybrid Organic–Inorganic Perovskites via Charge Transfer States Formation
1 Introduction Spintronics device, which use the spin degree of freedom for data recording and storage, is the preferred choice for the next generation of low-power electronics [1-9]. Usually, it is necessary to have a large spin-orbit coupling (SOC) and a long spin polarization lifetime for the materials applied to spintronic applications [10, 11]. However, materials that meet both of these two requirements need completely different material properties.
A Possible Solution to the Mystery of the ANITA Anomalous Events
1 Introduction The Antarctic Impulsive Transient Antenna (ANITA) experiment, a balloon-borne radio observatory launched by NASA, was designed to detect ultrahigh-energy neutrinos through the Askaryan effect in ice [1, 2]. It flew at 30–39 km $\, \mathrm{km}$ altitudes above Antarctica, and detected radio pulses that are consistent with coherent emission from ultrahigh-energy cosmic-ray (UHECR) air showers.
First-Principles Approach for Predicting Chiral Helimagnetism
1 Introduction Chiral helimagnets with exotic topological spin textures hold great potential for developing next-generation spintronic technology.[1, 2] These chiral helical spin structures are stabilized by the competition between the symmetric exchange interaction and the antisymmetric Dzyaloshinskii–Moriya interaction (DMI), driven by the absence of inversion symmetry.[3-5] The former promotes a collinear spin arrangement, while the latter favors a perpendicular spin ordering.
Mixed Adsorption Mono- and Multilayers of ß-Lactoglobulin Fibrils and Sodium Polystyrene Sulfonate
All articles published by MDPI are made immediately available worldwide under an open access license. No special permission is required to reuse all or part of the article published by MDPI, including figures and tables. For articles published under an open access Creative Common CC BY license, any part of the article may be reused without permission provided that the original article is clearly cited. For more information, please refer to https://www.mdpi.com/openaccess.
Quasi-Linear Convective Systems and Derechos across Europe: Climatology, Accompanying Hazards, and Societal Impacts
Keywords: Europe; Convective storms/systems; Severe storms; Climatology; Societal impacts 1. Introduction A quasi-linear convective system (QLCS) is a type of mesoscale convective system (MCS; Houze 2004, 2018) that is characterized by a linear organization of convective cells. This type of storm is often responsible for large socioeconomic impacts related to its high potential of producing convective hazards, particularly damaging wind gusts (Ashley and Mote 2005; Smith et al.
A Historical Overview on the Science of Derechos: Part II: Parent Storm Structure, Environmental Conditions, and History of Numerical Forecasts
Keywords: Convective storms/systems; Mesoscale systems; Derecho; Forecasting; Numerical weather prediction/forecasting A review on derecho-supporting MCS structure and dynamics The understanding of the physical mechanisms responsible for derecho production, particularly progressive derechos, stems from earlier studies of the vertical convective circulations that characterize linear derecho-producing mesoscale convective system (DMCS) structures. Beyond the squall line studies of Hamilton et al.
A Historical Overview on the Science of Derechos: Part I: Identification, Climatology, and Societal Impacts
Keywords: Derecho; Severe storms; Forecasting; Mesoscale forecasting; Societal impacts Strong, damaging surface winds have long been known to accompany thunderstorm clusters and squall lines, the most organized of which are classified as mesoscale convective systems (MCSs) (Houze 2018).
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Detection of large-scale X-ray bubbles in the Milky Way halo
Abstract The halo of the Milky Way provides a laboratory to study the properties of the shocked hot gas that is predicted by models of galaxy formation. There is observational evidence of energy injection into the halo from past activity in the nucleus of the Milky Way1,2,3,4; however, the origin of this energy (star formation or supermassive-black-hole activity) is uncertain, and the causal connection between nuclear structures and large-scale features has not been established unequivocally.
An ocular glymphatic clearance system removes β-amyloid from the rodent eye
An eye-opening look at the glymphatic system Similar to the brain, they eye is a privileged organ and lacks the classic lymphatic vessels responsible for the circulation of fluids and removal of waste products from peripheral organs. A glymphatic system has been demonstrated to be responsible of drainage of molecules, including amyloid-β (Aβ), from the brain. Now, Wang et al.
Populating the periodic table: Nucleosynthesis of the elements
Abstract Elements heavier than helium are produced in the lives and deaths of stars. This Review discusses when and how the process of nucleosynthesis made elements. High-mass stars fuse elements much faster, fuse heavier nuclei, and die more catastrophically than low-mass stars. The explosions of high-mass stars as supernovae release elements into their surroundings. Supernovae can leave behind neutron stars, which may later merge to produce additional heavy elements.
Carba- closo -dodecaborates as Superchaotropic Anions
1 Introduction Ten years ago, inorganic boron cluster anions [1-4], along with polyoxometalates [5-7], have been found to serve as high-affinity binders to cyclodextrins (CDs), with affinities approaching the micromolar regime in water [1-3]. This supramolecular affinity was unexpected, because CDs have been previously recognized as selective binders for hydrophobic organic guest molecules—while the cluster ions carry multiple negative charges.
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