Results 101 to 110 of about 1,809,603 (303)

A Critical Review on the Evolution of Chitosan‐Based Injectable Hydrogels in Bone Regeneration

open access: yesAdvanced Materials Interfaces, EarlyView.
The graphical illustration depicts hydrogel formulation using chitosan and biocompatible cross‐linkers, major advantages, and incorporation of cells, osteoinductive factors, and therapeutic drugs. Following injection, pH‐responsive gelation enables controlled drug release, promotes cell recruitment and osteogenic differentiation, enhances extracellular
Shivani Santosh Sakhrani   +2 more
wiley   +1 more source

Massive discs in cosmological simulations

open access: yes, 2020
VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Massive disc galaxies too dominated by dark matter in cosmological hydrodynamical simulations.' (bibcode: 2020A&A...640A ...
Fraternali, Filippo; id_orcid   +9 more
core   +1 more source

Hydrodynamical simulations of the stream-core interaction in the slow merger of massive stars [PDF]

open access: yes, 2002
We present detailed simulations of the interaction of a stream emanating from a mass-losing secondary with the core of a massive supergiant in the slow merger of two stars inside a common envelope.
Ivanova, Natasha   +7 more
core   +1 more source

Information Transmission Strategies for Self‐Organized Robotic Aggregation

open access: yesAdvanced Robotics Research, EarlyView.
In this review, we discuss how information transmission influences the neighbor‐based self‐organized aggregation of swarm robots. We focus specifically on local interactions regarding information transfer and categorize previous studies based on the functions of the information exchanged.
Shu Leng   +5 more
wiley   +1 more source

3D Radiation-hydrodynamical Simulations of Shadows on Transition Disks

open access: yesThe Astrophysical Journal Letters
Shadows are often observed in transition disks, which can result from obscuring by materials closer to the star, such as a misaligned inner disk. While shadows leave apparent darkened emission as observational signatures, they have significant dynamical ...
Shangjia Zhang, Zhaohuan Zhu
doaj   +1 more source

Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review

open access: yesUniverse
Merging galaxy clusters represent one of the most powerful macroscopic laboratories in the Universe for searching for new physics within the dark sector.
Rogério Monteiro-Oliveira
doaj   +1 more source

Simulation of the hydrodynamic drag force on aggregates

open access: yesAdvanced Powder Technology, 2000
Abstract —A simulation model to predict the dynamic behavior of large aggregates in flows was developed, in which the effective particle surface exposed to the flow was evaluated and the reduction of fluid velocity due to neighboring particles was taken into account.
Iimura, K, Higashitani, K
openaire   +2 more sources

Piezoresistivity Enhancement by Graphite Flake Alignment in Thin Composite Films for Dielectric Elastomer Switches

open access: yesAdvanced Robotics Research, EarlyView.
This article presents dielectric elastomer switch (DES) materials, based on composite thin films. Alignment of graphite flakes due to their physical confinement within the thin films lead to much stronger piezoresistive responses than bulk composites, while their durability exceeds that of conventional liquid‐based DES materials.
Lingyu Liu   +3 more
wiley   +1 more source

The Limited Lifetime of Self-Gravitating Accretion Disks in Galactic Centers

open access: yesGalaxies
Globally self-gravitating accretion disks in active galactic nuclei (AGN) have been frequently discussed in the literature, but never observed. A few dozen megamasering accretion disks in AGN have been detected, which display a clear Keplerian rotation ...
Isaac Shlosman
doaj   +1 more source

Hydrodynamic simulations of clumps [PDF]

open access: yes, 2008
Clumps in hot star winds can originate from shock compression due to the line driven instability. One-dimensional hydrodynamic simulations reveal a radial wind structure consisting of highly compressed shells separated by voids, and colliding with fast clouds. Two-dimensional simulations are still largely missing, despite first attempts.
Feldmeier, Achim (Prof. Dr.)   +3 more
openaire  

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