scholarly journals Determination of boson spectrum from optical data in pseudogap phase of underdoped cuprates

2012 ◽  
Vol 86 (9) ◽  
Author(s):  
Jungseek Hwang ◽  
J. P. Carbotte
Keyword(s):  
Optical Data ◽  
Pseudogap Phase ◽  
Underdoped Cuprates

scholarly journals Steps toward Determination of the Size and Structure of the Broad‐Line Region in Active Galactic Nuclei. X. Variability of Fairall 9 from Optical Data

1997 ◽  
Vol 112 (2) ◽  
pp. 271-283 ◽  
Author(s):  
M. Santos‐Lleo ◽  
E. Chatzichristou ◽  
C. Mendes de Oliveira ◽  
C. Winge ◽  
D. Alloin ◽  
...  
Keyword(s):  
Active Galactic Nuclei ◽  
Galactic Nuclei ◽  
Optical Data ◽  
Broad Line ◽  
Broad Line Region ◽  
Line Region ◽  
Size And Structure

scholarly journals An approach to analysis of dynamic crack growth at bimaterial interface

2009 ◽  
Vol 36 (4) ◽  
pp. 299-327 ◽  
Author(s):  
R. Nikolic ◽  
Jelena Djokovic
Keyword(s):  
Asymptotic Analysis ◽  
Strain Field ◽  
Crack Tip ◽  
Optical Data ◽  
Bimaterial Interface ◽  
Dynamic Crack ◽  
New Approach ◽  
Shear Wave Speed ◽  
Propagating Crack

In this paper is presented the new approach to asymptotic analysis of the stress and strain fields around a crack tip that is propagating dynamically along a bimaterial interface. Through asymptotic analysis the problem is being reduced to solving the Riemann-Hilbert's problem, what yields the strain potential that is used for determination of the strain field around a crack tip. The considered field is that of a dynamically propagating crack with a speed that is between zero and shear wave speed of the less stiffer of the two materials, bound along the interface. Using the new approach in asymptotic analysis of the strain field around a tip of a dynamically propagating crack and possibilities offered by the Mathematica programming package, the results are obtained that are compared to both experimental and numerical results on the dynamic interfacial fracture known from the literature. This comparison showed that it is necessary to apply the complete expression obtained by asymptotic analysis of optical data and not only its first term as it was done in previous analyses.

Calculation of helical gear’s basic parameters using COP-data acquired by optical 3D digitizer

2011 ◽  
Vol 225 (12) ◽  
pp. 2953-2962 ◽  
Author(s):  
P Asgharifard-Sharabiani ◽  
A Hannaneh ◽  
M Nikkhah-Bahrami
Keyword(s):  
Gear Tooth ◽  
Control Process ◽  
Surface Fitting ◽  
Optical Data ◽  
Tooth Surface ◽  
Cylinder Surface ◽  
Quality Control Process ◽  
Basic Parameters ◽  
Cloud Of Points

Gears are industrial components with a precise geometry. Identification of their basic parameters plays an important role in their reverse design and quality control process. This article describes a new approach for the calculation of helical gear’s basic parameters using optical data acquired by 3D digitizer. This approach is implemented by acquiring cloud-of-points data (COP-data) from the bearing seats and gear tooth surface. Cylinder surface fitting through COP-data acquired from bearing seats is performed for the determination of gear axis of rotation. In a final step, involute helicoid surface fitting through COP-data acquired from gear tooth surface determines the helical gear’s primary features. Particle swarm optimization algorithm as an efficient method is applied to perform the surface fitting process in this article.

scholarly journals Correlation and orbit determination of space objects based on sparse optical data

2011 ◽  
Vol 417 (3) ◽  
pp. 2094-2103 ◽  
Author(s):  
A. Milani ◽  
G. Tommei ◽  
D. Farnocchia ◽  
A. Rossi ◽  
T. Schildknecht ◽  
...  
Keyword(s):  
Orbit Determination ◽  
Optical Data ◽  
Space Objects

scholarly journals ClG 0217+70: A massive merging galaxy cluster with a large radio halo and relics

2020 ◽  
Vol 642 ◽  
pp. L3
Author(s):  
X. Zhang ◽  
A. Simionescu ◽  
J. S. Kaastra ◽  
H. Akamatsu ◽  
D. N. Hoang ◽  
...  
Keyword(s):  
Surface Brightness ◽  
Galaxy Cluster ◽  
Precise Determination ◽  
Optical Data ◽  
Scaling Relations ◽  
Thermal Pressure ◽  
X Ray ◽  
Radio Halo ◽  
Physical Scale

We present an analysis of archival Chandra data of the merging galaxy cluster ClG 0217+70. The Fe XXV Heα X-ray emission line is clearly visible in the 25 ks observation, allowing a precise determination of the redshift of the cluster as z = 0.180 ± 0.006. We measure kT500 = 8.3  ±  0.4 keV and estimate M500 = (1.06 ± 0.11) × 1015 M⊙ based on existing scaling relations. Correcting both the radio and X-ray luminosities with the revised redshift reported here, which is much larger than previously inferred based on sparse optical data, this object is no longer an X-ray underluminous outlier in the LX − Pradio scaling relation. The new redshift also means that, in terms of physical scale, ClG 0217+70 hosts one of the largest radio halos and one of the largest radio relics known to date. Most of the relic candidates lie in projection beyond r200. The X-ray morphological parameters suggest that the intracluster medium is still dynamically disturbed. Two X-ray surface brightness discontinuities are confirmed in the northern and southern parts of the cluster, with density jumps of 1.40 ± 0.16 and 3.0 ± 0.6, respectively. We also find a 700 × 200 kpc X-ray faint channel in the western part of the cluster, which may correspond to compressed heated gas or increased non-thermal pressure due to turbulence or magnetic fields.

scholarly journals Magnetism and Superconductivity in the Pseudogap Phase of Underdoped Cuprates

2013 ◽  
Vol 449 ◽  
pp. 012006 ◽  
Author(s):  
A J A James ◽  
R M Konik ◽  
K Huang ◽  
W-Q Chen ◽  
T M Rice ◽  
...  
Keyword(s):  
Pseudogap Phase ◽  
Underdoped Cuprates
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