New Evidence for Electron-Electron Scattering in Noble Metals from Radio-Frequency-Size-Effect Measurements

1987 ◽  
Vol 26 (S3-1) ◽  
pp. 643 ◽  
Author(s):  
Rene Stubi ◽  
Pierre-Alain Probst ◽  
Robert Huguenin ◽  
Vitali Gasparov
1988 ◽  
Vol 18 (6) ◽  
pp. 1211-1224 ◽  
Author(s):  
R Stubi ◽  
P -A Probst ◽  
R Huguenin ◽  
V A Gasparov

1979 ◽  
Vol 19 (6) ◽  
pp. 2905-2911 ◽  
Author(s):  
J. C. Kimball ◽  
Louis W. Adams ◽  
R. G. Goodrich

1965 ◽  
pp. 823-826 ◽  
Author(s):  
D. M. Sparlin ◽  
D. S. Schreiber
Keyword(s):  

2020 ◽  
Vol 9 (3) ◽  
pp. 1-25
Author(s):  
Faisal Khan ◽  
Sharif Ullah Jan

This research study analyses the role of size effect in detecting the pricing of risk, various volatility dynamics, and economic exposure of firm returns on the Pakistani stock market by employing monthly data for the period from 1998 to 2018. Three generalized autoregressive conditional heteroskedasticity models were applied: GARCH(1,1) for capturing different volatility dynamics, GARCH-M for pricing of risk, and EGARCH for asymmetric and leverage effect. The findings of the study are as follows: Firstly, the authors untie that pricing of risk is subject to considerable variations with respect to firm size. Secondly, in the process of detecting whether the firm size matters in the case of asymmetry and leverage effect, they find that it is indeed the case. Thirdly, size effect plays a substantial role in determining various volatility dynamics. Finally, they uncover that economic factors affect stock returns differently based on firm size, signifying the role of size effect.


1989 ◽  
Vol 134 ◽  
pp. 245-250
Author(s):  
Jules P. Halpern ◽  
Kaiyou Chen

We have refined our calculation of the line profile of a relativistic, Keplerian disk by incorporating a variety of emissivity laws, as well as broadening due to turbulence or electron scattering. The significant improvement in the fit to the double-peaked Ha line profile of the elliptical radio galaxy Arp 102B provides the most convincing direct evidence for an accretion disk in any AGN. Arp 102B appears to be a low-luminosity analog of 3C 390.3, and several lines of evidence point to the existence of small, hot ion tori illuminating an outer thin disk in both of these galaxies. The rarity of these emission-line profiles might be understood if this particular combination of ion torus/thin disk occurs only for a narrow range of ṁ(= Ṁ/ṀEdd).


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