Nonlinear polarization response of a gaseous medium in the regime of atom stabilization in a strong radiation field

2013 ◽  
Vol 116 (3) ◽  
pp. 372-380 ◽  
Author(s):  
E. A. Volkova ◽  
A. M. Popov ◽  
O. V. Tikhonova
2021 ◽  
Vol 104 (5) ◽  
Author(s):  
Zhanjie Gao ◽  
Patrice Genevet ◽  
Guixin Li ◽  
Konstantin E. Dorfman

1998 ◽  
Vol 188 ◽  
pp. 413-414
Author(s):  
Y. Watanabe ◽  
J. Fukue

Accretion-disk corona (ADC) is required from observational as well as theoretical reasons. In almost all of traditional studies, however, a stationary corona has been assumed; i.e., the corona gas corotates with the underlying (Keplerian) accretion disk, and the radial motion is ignored. Recently, in the theory of accretion disks a radiative interaction between the gas and the external radiation field has attracted the attention of researchers. In particular the radiation drag between the gas and the external radiation field becomes important from the viewpoint of the angular-momentum removal. We thus examine the effect of radiation drag on the accretion-disk corona above/below the accretion disk (Watanabe, Fukue 1996a, b). We suppose that an accretion disk can be described by the standard disk, and that radiation fields are produced by the central luminous source and the accretion disk, itself. In general an accretion-disk corona under the influence of strong radiation fields dynamically infalls (advected) toward the center.


1973 ◽  
Vol 16 (1) ◽  
pp. 1-7
Author(s):  
I. M. Ternov ◽  
V. R. Khalilov ◽  
A. F. Zhuravlev ◽  
G. A. Chizhov

2002 ◽  
Vol 94 (3) ◽  
pp. 525-533
Author(s):  
E. A. Volkova ◽  
A. M. Popov ◽  
O. V. Tikhonova

1985 ◽  
Vol 63 (7) ◽  
pp. 907-932 ◽  
Author(s):  
F. Ehlotzky

By continuing previous work, several different scattering and absorption phenomena in the presence of a strong, coherent, electromagnetic background field are considered from a unifying point of view to elucidate the essential similarities of these processes, in particular, in the limit of low frequencies of the radiation field. The connection with corresponding classical processes is investigated. The limitations of the low-frequency approach are considered, and consequences are discussed with respect to the possible physical implications and conditions of experimental verification.


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