Results 81 to 90 of about 1,809,603 (303)
Guangqi: A 2D Radiation Hydrodynamic Code with Realistic Equations of State
We present Guangqi , a new 2D, finite-volume radiation hydrodynamics code designed for high-performance astrophysical simulations. The code simultaneously resolves the hydrodynamic equations for complex equations of state (EoS) and implicit radiation ...
Zhuo Chen, Xue-Ning Bai
doaj +1 more source
Metal‐free carbon catalysts enable the sustainable synthesis of hydrogen peroxide via two‐electron oxygen reduction; however, active site complexity continues to hinder reliable interpretation. This review critiques correlation‐based approaches and highlights the importance of orthogonal experimental designs, standardized catalyst passports ...
Dayu Zhu +3 more
wiley +1 more source
Intermediate-Mass & Supermassive Black Hole Feedback in Cosmological Hydrodynamical Simulations
Intermediate-Mass Black Holes (IMBHs: with mass between 100 to 10^6 Msun) historically comprise of an elusive population in the Universe compared to the widely observed Stellar-Mass and Supermassive Black Holes.
Barai, Paramita
core +1 more source
Inverse Design of Nanoparticulate Materials
Inverse design shifts nanomaterial development from empirical trial‐and‐error to predictive model‐driven strategies. It can rely on knowledge‐based, data‐based, or hybrid process and property functions. This perspective article provides a practical framework for applying inverse design based on instructive examples. It discusses which modeling approach
Nabi Etienne Traoré +5 more
wiley +1 more source
Hydrodynamical Simulations of Helium-ignited Binary White Dwarf Mergers
Type Ia supernovae (SNe Ia) are luminous astrophysical transients. SNe Ia serve as distance indicators for measuring the expansion rate of the Universe and play important roles in galactic nucleosynthesis.
Vrutant Mehta +4 more
doaj +1 more source
Bars in hydrodynamical cosmological simulations
International audienceWe study the properties of two bars formed in fully cosmological hydrodynamical simulations of the formation of Milky Way-mass galaxies. In one case, the bar formed in a system with disc, bulge and halo components, and is relatively
Athanassoula, E., Scannapieco, Cecilia
core +1 more source
1T‐to‐2H Phase Evolution During Epitaxial Growth of Transition Metal Dichalcogenides
During MOCVD growth of MoS2 and WSe2, a transient metallic 1T phase emerges in early, edge‐rich, chalcogen‐deficient domains and declines as the films ultimately coalesce as 2H material. Together, experiments and ReaxFF simulations link domain size, edge stoichiometry, and vacancies to this evolution.
Andrew R. Graves +8 more
wiley +1 more source
Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations
Cosmological hydrodynamical simulations are rich tools to understand the role and impact of galaxy environment and mergers, and gas dynamics and stellar kinematics in galaxy formation and evolution.
van de Sande, Jesse, None
core +1 more source
Three-dimensional simulations of a starburst wind [PDF]
In order to better understand the formation of a starburst-driven wind, we have performed a series of three-dimensional hydrodynamical simulations in an inhomogeneous interstellar medium.
Bicknell, Geoffrey +3 more
core +1 more source
The lanthanide/transition metal ion coordination nanoparticles, La‐Cu@Lap/IWR‐1, with optimized coordination, have been proven to achieve remarkable results in realizing comprehensive tumor cuproptosis through efficient cuproptosis activation and multidimensional resistance elimination, thereby synchronously realizing the synergistic antitumor effects ...
Junrong Wang +8 more
wiley +1 more source

