Results 31 to 40 of about 6,087,560 (207)

Spontaneous emission of color centers at 4eV in hexagonal boron nitride under hydrostatic pressure [PDF]

open access: yesSuperlattices and Microstructures (2019), 2019
The light emission properties of color centers emitting in 3.3-4 eV region are investigated for hydrostatic pressures ranging up to 5GPa at liquid helium temperature. The light emission energy decreases with pressure less sensitively than the bandgap. This behavior at variance from the shift of the bandgap is typical of deep traps.
arxiv   +1 more source

In situ high-pressure spectroscopic studies using moissanite (4H-SiC) anvils

open access: yesAIP Advances, 2018
We examined the Raman scattering and IR absorption spectroscopy of 4H-SiC and its performance as an anvil material for high-pressure UV-visible absorption spectroscopic measurements.
Jinbo Zhang   +7 more
doaj   +1 more source

Quantitative Estimates of Environmental Effects on the Star Formation Rate of Disk Galaxies in Clusters of Galaxies [PDF]

open access: yes, 1998
A simple model is constructed to evaluate the change of star formation rate of a disk galaxy due to environmental effects in clusters of galaxies. Three effects, (1) tidal force from the potential well of the cluster, (2) increase of external pressure ...
Evrard A. E.   +6 more
core   +2 more sources

Complete pressure dependent phase diagrams for SrFe2As2 and BaFe2As2 [PDF]

open access: yesPRB 79, 224518 (2009), 2009
The temperature dependent electrical resistivity of single crystalline SrFe2As2 and BaFe2As2 has been measured in a liquid medium, modified Bridgman anvil cell for pressures in excess of 75 kbar. These data allow for the determination of the pressure dependence of the higher temperature, structural / antiferromagnetic phase transitions as well as the ...
arxiv   +1 more source

Effects of Diamond on Microstructure, Fracture Toughness, and Tribological Properties of TiO2-Diamond Composites

open access: yesNanomaterials, 2022
The reinforcements represented by graphene nanoplatelets, graphite, and carbon nanotubes have demonstrated the great potential of carbon materials as reinforcements to enhance the mechanical properties of TiO2.
Bing Liu   +11 more
doaj   +1 more source

Synthesis of quenchable amorphous diamond

open access: yesNature Communications, 2017
Diamond’s properties are dictated by its crystalline, fully tetrahedrally bonded structure. Here authors synthesize a bulk sp 3-bonded amorphous form of carbon under high pressure and temperature, show that it has bulk modulus comparable to crystalline ...
Zhidan Zeng   +10 more
doaj   +1 more source

Grain-boundary-rich polycrystalline monolayer WS2 film for attomolar-level Hg2+ sensors

open access: yesNature Communications, 2021
Here, the authors report the controlled growth of polycrystalline WS2 films with high density of grain boundaries to realize surface plasmon Hg2+ ion sensors exhibiting attomolar sensitivity and enhanced selectivity.
Lixuan Liu   +15 more
doaj   +1 more source

A new room-temperature equation of state of Bi up to 260 GPa [PDF]

open access: yes, 2023
At room temperature, bismuth undergoes several structural transitions with increasing pressure before taking on a body-centered cubic (bcc) phase at approximately 8 GPa. The bcc structure is stable to the highest measured pressure and its simplicity, along with its high compressibility and atomic number, make it an enticing choice as a pressure ...
arxiv   +1 more source

Stars creating a gravitational repulsion

open access: yes, 2018
In the framework of the Theory of General Relativity, models of stars with an unusual equation of state $\rho c^20$ where $\rho$ is the mass density and $P$ is the pressure, are constructed.
Bisnovatyi-Kogan, G. S.   +2 more
core   +1 more source

Effects of Ram-Pressure from Intracluster Medium on the Star Formation Rate of Disk Galaxies in Clusters of Galaxies [PDF]

open access: yes, 1998
Using a simple model of molecular cloud evolution, we have quantitatively estimated the change of star formation rate (SFR) of a disk galaxy falling radially into the potential well of a cluster of galaxies.
Kodama T.   +4 more
core   +3 more sources

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