Emission of radiation by a resonance medium excited with a variable superluminal velocity

2017 ◽  
Vol 122 (5) ◽  
pp. 768-773 ◽  
Author(s):  
R. M. Arkhipov ◽  
A. V. Pakhomov
Keyword(s):  
Resonance Medium ◽  
Superluminal Velocity

Barrier Penetration and Superluminal Velocity

1993 ◽  
Vol 228 (1) ◽  
pp. 184-202 ◽  
Author(s):  
J.M. Deutch ◽  
F.E. Low
Keyword(s):  
Superluminal Velocity ◽  
Barrier Penetration

Vibrationally induced transparency in optically dense resonance medium

2002 ◽  
Author(s):  
Y. V. Radeonychev ◽  
M. D. Tokman ◽  
A. G. Litvak ◽  
Olga A. Kocharovskaya
Keyword(s):  
Resonance Medium ◽  
Induced Transparency

A Slower Superluminal Velocity for the Quasar 1156+295

1997 ◽  
Vol 485 (2) ◽  
pp. L61-L63 ◽  
Author(s):  
B. Glenn Piner ◽  
Kerry A. Kingham
Keyword(s):  
Superluminal Velocity

scholarly journals The Relativistic Beaming Model and Superluminal Motions

1997 ◽  
Vol 159 ◽  
pp. 74-75
Author(s):  
J. H. Fan ◽  
G.Z. Xie ◽  
Y.H. Zhang ◽  
Y.P. Qin
Keyword(s):  
Brightness Temperature ◽  
Flux Density ◽  
Statistical Correlation ◽  
X Ray ◽  
Superluminal Velocity ◽  
Relativistic Beaming ◽  
Doppler Factor

In this paper, we consider a compilation of 55 objects with known superluminal motions (SM), and whose flux density (X-ray, optical, radio), core dominance parameter (R), superluminal velocity, and radio Doppler factor (δR) are known. Our study shows that SM is consistent with the beaming model, and the relationis reasonable. The statistical correlation between superluminal velocity and redshift is a result of selection and the statistical correlation between R and brightness temperature (Tob) is actually a reflection of the correlations between δ, R, and Tob for objects with SM. Up to now, 59 objects have been reported to have SM, but for reasons discussed elsewhere (Vermeulen & Cohen 1994), only 55 are considered here.

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