scholarly journals Wave and particle properties can be spatially separated in a quantum entity

2021 ◽  
Author(s):  
Jing-Ling Chen ◽  
Pratyusha Chowdhury ◽  
Aran Kumar Pati
Keyword(s):  
Particle Properties ◽  
Quantum Entity

scholarly journals Balancing particle properties for practical lithium-ion batteries

Particuology ◽  
2021 ◽  
Author(s):  
Jing Zhang ◽  
Jinshuo Qiao ◽  
Kening Sun ◽  
Zhenhua Wang
Keyword(s):  
Lithium Ion Batteries ◽  
Lithium Ion ◽  
Particle Properties

scholarly journals DESTINY: Database for the Effects of STellar encounters on dIsks and plaNetary sYstems

2019 ◽  
Vol 6 (1) ◽  
Author(s):  
Asmita Bhandare ◽  
Susanne Pfalzner
Keyword(s):  
Planetary System ◽  
Planetary Systems ◽  
Gravitational Effect ◽  
Parameter Study ◽  
Orbital Inclination ◽  
Particle Properties ◽  
Disk Size ◽  
Stellar Group ◽  
Cluster Environment ◽  
Parabolic Orbits

Abstract Most stars form as part of a stellar group. These young stars are mostly surrounded by a disk from which potentially a planetary system might form. Both, the disk and later on the planetary system, may be affected by the cluster environment due to close fly-bys. The here presented database can be used to determine the gravitational effect of such fly-bys on non-viscous disks and planetary systems. The database contains data for fly-by scenarios spanning mass ratios between the perturber and host star from 0.3 to 50.0, periastron distances from 30 au to 1000 au, orbital inclination from 0∘ to 180∘ and angle of periastron of 0∘, 45∘ and 90∘. Thus covering a wide parameter space relevant for fly-bys in stellar clusters. The data can either be downloaded to perform one’s own diagnostics like for e.g. determining disk size, disk mass, etc. after specific encounters, obtain parameter dependencies or the different particle properties can be visualized interactively. Currently the database is restricted to fly-bys on parabolic orbits, but it will be extended to hyperbolic orbits in the future. All of the data from this extensive parameter study is now publicly available as DESTINY.

Development of a new method to evaluate critical flux and system reliability based on particle properties in a membrane bioreactor

Chemosphere ◽  
2021 ◽  
pp. 130763
Author(s):  
Yongsun Jang ◽  
Han-Shin Kim ◽  
Jeong-Hoon Lee ◽  
So-Young Ham ◽  
Jeong-Hoon Park ◽  
...  
Keyword(s):  
System Reliability ◽  
Membrane Bioreactor ◽  
New Method ◽  
Critical Flux ◽  
Particle Properties

scholarly journals Designing enhanced spray dried particles for inhalation: A review of the impact of excipients and processing parameters on particle properties

2021 ◽  
Vol 384 ◽  
pp. 313-331
Author(s):  
Nasser Alhajj ◽  
Niall J. O'Reilly ◽  
Helen Cathcart
Keyword(s):  
Processing Parameters ◽  
Particle Properties ◽  
The Impact ◽  
Spray Dried

Particle properties of a nitric solution of cerium nitrate as a substitute of Pu-nitrate

1986 ◽  
Vol 17 (3) ◽  
pp. 592-596
Author(s):  
H.D. Seehars ◽  
D. Hochrainer ◽  
M. Spiekermann
Keyword(s):  
Cerium Nitrate ◽  
Particle Properties ◽  
Nitric Solution

Effect of particle properties on the energy-size reduction of coal in the ball-and-race mill

2018 ◽  
Vol 333 ◽  
pp. 404-409 ◽  
Author(s):  
Weining Xie ◽  
Yaqun He ◽  
Lili Qu ◽  
Xiaolu Sun ◽  
Xiangnan Zhu
Keyword(s):  
Size Reduction ◽  
Particle Properties

High-phase-angle observations of Neptune at 2650 and 7500 Å: Haze structure and particle properties

Icarus ◽  
1992 ◽  
Vol 99 (2) ◽  
pp. 302-317 ◽  
Author(s):  
Wayne R. Pryor ◽  
Robert A. West ◽  
Karen E. Simmons ◽  
Mona Delitsky
Keyword(s):  
Phase Angle ◽  
Particle Properties ◽  
High Phase

scholarly journals Ice Particle Properties Inferred from Aggregation Modelling

2020 ◽  
Author(s):  
Markus Konrad Karrer ◽  
Stefan Kneifel ◽  
Davide Ori ◽  
Christoph Siewert ◽  
Axel Seifert ◽  
...  
Keyword(s):  
Particle Properties

Proton Beam Abundance Variations and Their Relation to Alpha Particle Properties

2021 ◽  
Vol 923 (2) ◽  
pp. 170
Author(s):  
Tereza Ďurovcová ◽  
Jana Šafránková ◽  
Zdeněk Němeček
Keyword(s):  
Solar Wind ◽  
Proton Beam ◽  
Alpha Particle ◽  
Source Region ◽  
Radial Distance ◽  
Alpha Particles ◽  
Momentum Balance ◽  
Particle Interactions ◽  
Coulomb Collisions ◽  
Particle Properties

Abstract Less abundant but still dynamically important solar wind components are the proton beam and alpha particles, which usually contribute similarly to the total ion momentum. The main characteristics of alpha particles are determined by the solar wind source region, but the origin of the proton beam and its properties are still not fully explained. We use the plasma data measured in situ on the path from 0.3 to 1 au (Helios 1 and 2) and focus on the proton beam development with an increasing radial distance as well as on the connection between the proton beam and alpha particle properties. We found that the proton beam relative abundance increases with increasing distance from the Sun in the collisionally young streams. Among the mechanisms suggested for beam creation, we have identified the wave–particle interactions with obliquely propagating Alfvén modes being consistent with observations. As the solar wind streams get collisionally older, the proton beam decay gradually dominates and the beam abundance is reduced. In search for responsible mechanisms, we found that the content of alpha particles is correlated with the proton beam abundance, and this effect is more pronounced in the fast solar wind streams during the solar maximum. We suggest that Coulomb collisions are the main agent leading to merging of the proton beam and core. We are also showing that the variations of the proton beam abundance are correlated with a decrease of the alpha particle velocity in order to maintain the total momentum balance in the solar wind frame.

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