scholarly journals Electron rest mass and line spectrum of atoms in the photonic crystal medium

2013 ◽  
Vol 478 ◽  
pp. 012017 ◽  
Author(s):  
R Kh Gainutdinov ◽  
M A Khamadeev ◽  
M Kh Salakhov
2012 ◽  
Vol 85 (5) ◽  
Author(s):  
Renat Kh. Gainutdinov ◽  
Marat A. Khamadeev ◽  
Myakzyum Kh. Salakhov

2016 ◽  
Vol 714 ◽  
pp. 012009
Author(s):  
R Kh Gainutdinov ◽  
M A Khamadeev ◽  
O V Steryakov ◽  
K A Ziyatdinova ◽  
M Kh Salakhov

2015 ◽  
Vol 613 ◽  
pp. 012005 ◽  
Author(s):  
A A Akhmadeev ◽  
R Kh Gainutdinov ◽  
G Hermann ◽  
M A Khamadeev ◽  
O V Steryakov ◽  
...  

2015 ◽  
Vol 613 ◽  
pp. 012001
Author(s):  
R Kh Gainutdinov ◽  
M A Khamadeev ◽  
M R Mohebbifar ◽  
A S Petrova ◽  
K A Ziyatdinova ◽  
...  

1967 ◽  
Vol 28 ◽  
pp. 207-244
Author(s):  
R. P. Kraft

(Ed. note:Encouraged by the success of the more informal approach in Christy's presentation, we tried an even more extreme experiment in this session, I-D. In essence, Kraft held the floor continuously all morning, and for the hour and a half afternoon session, serving as a combined Summary-Introductory speaker and a marathon-moderator of a running discussion on the line spectrum of cepheids. There was almost continuous interruption of his presentation; and most points raised from the floor were followed through in detail, no matter how digressive to the main presentation. This approach turned out to be much too extreme. It is wearing on the speaker, and the other members of the symposium feel more like an audience and less like participants in a dissective discussion. Because Kraft presented a compendious collection of empirical information, and, based on it, an exceedingly novel series of suggestions on the cepheid problem, these defects were probably aggravated by the first and alleviated by the second. I am much indebted to Kraft for working with me on a preliminary editing, to try to delete the side-excursions and to retain coherence about the main points. As usual, however, all responsibility for defects in final editing is wholly my own.)


1967 ◽  
Vol 28 ◽  
pp. 177-206
Author(s):  
J. B. Oke ◽  
C. A. Whitney

Pecker:The topic to be considered today is the continuous spectrum of certain stars, whose variability we attribute to a pulsation of some part of their structure. Obviously, this continuous spectrum provides a test of the pulsation theory to the extent that the continuum is completely and accurately observed and that we can analyse it to infer the structure of the star producing it. The continuum is one of the two possible spectral observations; the other is the line spectrum. It is obvious that from studies of the continuum alone, we obtain no direct information on the velocity fields in the star. We obtain information only on the thermodynamic structure of the photospheric layers of these stars–the photospheric layers being defined as those from which the observed continuum directly arises. So the problems arising in a study of the continuum are of two general kinds: completeness of observation, and adequacy of diagnostic interpretation. I will make a few comments on these, then turn the meeting over to Oke and Whitney.


2018 ◽  
Vol 1 (1) ◽  
pp. 2-19
Author(s):  
Mahmood Sh. Majeed ◽  
Raid W. Daoud

A new method proposed in this paper to compute the fitness in Genetic Algorithms (GAs). In this new method the number of regions, which assigned for the population, divides the time. The fitness computation here differ from the previous methods, by compute it for each portion of the population as first pass, then the second pass begin to compute the fitness for population that lye in the portion which have bigger fitness value. The crossover and mutation and other GAs operator will do its work only for biggest fitness portion of the population. In this method, we can get a suitable and accurate group of proper solution for indexed profile of the photonic crystal fiber (PCF).


2018 ◽  
Vol 8 (3) ◽  
pp. 172-188
Author(s):  
M. Abdulmahdi ◽  
S. Sarsooh ◽  
M. Oleiwi
Keyword(s):  

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