Toward a General Correlation Theorem

2005 ◽  
Vol 51 (9) ◽  
pp. 3297-3302 ◽  
Author(s):  
K.C. Gupta ◽  
P. Sarkar
Keyword(s):  
General Correlation ◽  
Correlation Theorem

scholarly journals Shear modulus and yield stress of foams: contribution of interfacial elasticity

Soft Matter ◽  
2021 ◽  
Vol 17 (14) ◽  
pp. 3937-3944
Author(s):  
Annika R. Völp ◽  
Norbert Willenbacher
Keyword(s):  
Elastic Modulus ◽  
Block Copolymer ◽  
Shear Modulus ◽  
Yield Stress ◽  
Protein Food ◽  
General Correlation

A general correlation of foam shear modulus G0 and yield stress τy with the interfacial elastic modulus of foaming solutions in shear and dilation E∞ was found for surfactant, block-copolymer, protein, food, and particle-stabilized foams.

Complex area correlation theorem for statistical pulses in coherent linear absorbers

2012 ◽  
Vol 37 (17) ◽  
pp. 3498 ◽  
Author(s):  
Laleh Mokhtarpour ◽  
Sergey A. Ponomarenko
Keyword(s):  
Correlation Theorem

Numerical Simulation of Gas/Solid Heat Transfer in Metallic Foams: A General Correlation for Different Porosities and Pore Sizes

2018 ◽  
Vol 127 (2) ◽  
pp. 481-506 ◽  
Author(s):  
Azade Jafarizade ◽  
Masoud Panjepour ◽  
Mahmood Meratian ◽  
Mohsen Davazdah Emami
Keyword(s):  
Heat Transfer ◽  
Numerical Simulation ◽  
Metallic Foams ◽  
General Correlation ◽  
Pore Sizes

scholarly journals Searching for a link between the magnetic nature and other observed properties of Herbig Ae/Be stars

2008 ◽  
Vol 4 (S259) ◽  
pp. 395-396 ◽  
Author(s):  
Swetlana Hubrig ◽  
C. Grady ◽  
M. Schöller ◽  
O. Schütz ◽  
B. Stelzer ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Field Survey ◽  
Accretion Rate ◽  
Be Stars ◽  
General Correlation ◽  
X Ray ◽  
Mass Accretion Rate ◽  
Debris Disk ◽  
Magnetic Nature

AbstractWe present the results of a new magnetic field survey of Herbig Ae/Be and A debris disk stars. They are used to determine whether magnetic field properties in these stars are correlated with the mass-accretion rate, disk inclinations, companion(s), Silicates, PAHs, or show a more general correlation with age and X-ray emission as expected for the decay of a remnant dynamo.

scholarly journals Do quasars evolve over cosmological time scales?

1986 ◽  
Vol 119 ◽  
pp. 439-445
Author(s):  
E.J. Wampler ◽  
D. Ponz
Keyword(s):  
Emission Line ◽  
Time Scales ◽  
Line Strength ◽  
Schmidt Telescope ◽  
Spectral Evolution ◽  
General Correlation ◽  
Cosmological Time ◽  
Systematic Biases ◽  
Evolution Laws ◽  
Lower Luminosity

Systematic biases that are redshift dependent can influence the optical discovery of quasars and the evolution laws derived from counts of quasars. New data and their interpretation for quasars brighter than MB = −24 in the Palomar Bright Quasar Survey (BQS) (Schmidt and Green, 1983) are consistent with no evolution. A comparison of BQS quasars with the brightest quasars from the CTIO Schmidt Telescope Survey (Osmer and Smith, 1980) shows that if qo is near zero, the co-moving density of bright quasars in a Friedmann cosmology is about 15 times higher for the CTIO survey quasars (mean z ≈ 2.8) than for the BQS quasars (mean z ≈ 1.8). In this case spectral evolution is also required since the CTIO quasars have stronger CIV λ1548 lines than the BQS quasars of similar luminosity. Alternatively, if qO is taken to be near 1, the CTIO survey quasars would then have lower luminosity than the BQS quasars and these data would be consistent with no evolution. Strong CIV λ1548 lines for the CTIO quasars would then fit the general correlation between absolute quasar luminosity and emission line strength (Wampler, Gaskell, Burke and Baldwin, 1984).

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