scholarly journals Distributed angular double-slit interference with pseudo-thermal light

2017 ◽  
Vol 110 (7) ◽  
pp. 071107 ◽  
Author(s):  
Lu Gao ◽  
Seyed Mohammad Hashemi Rafsanjani ◽  
Yiyu Zhou ◽  
Zhe Yang ◽  
Omar S. Magaña-Loaiza ◽  
...  
Keyword(s):  
2013 ◽  
Vol 30 (7) ◽  
pp. 1422 ◽  
Author(s):  
Xi-Hao Chen ◽  
Wen Chen ◽  
Shao-Ying Meng ◽  
Wei Wu ◽  
Ling-An Wu ◽  
...  

Author(s):  
Lu Gao ◽  
Jiapeng. Zhao ◽  
Omar S. Magaña-Loaiza ◽  
Seyed Mohammad Hashemi Rafsanjani ◽  
Mohammad Mirhosseini ◽  
...  
Keyword(s):  

2008 ◽  
Vol 281 (10) ◽  
pp. 2838-2841 ◽  
Author(s):  
Lu Gao ◽  
Jun Xiong ◽  
Lu-Fang Lin ◽  
Wei Wang ◽  
Su-Heng Zhang ◽  
...  
Keyword(s):  

2015 ◽  
Vol 9 (3) ◽  
pp. 2470-2475
Author(s):  
Bheku Khumalo

This paper seeks to discuss why information theory is so important. What is information, knowledge is interaction of human mind and information, but there is a difference between information theory and knowledge theory. Look into information and particle theory and see how information must have its roots in particle theory. This leads to the concept of spatial dimensions, information density, complexity, particle density, can there be particle complexity, and re-looking at the double slit experiment and quantum tunneling. Information functions/ relations are discussed.


2015 ◽  
Vol 10 (2) ◽  
pp. 2692-2695
Author(s):  
Bhekuzulu Khumalo

Heat has often been described as part of the energy transfer process. Information theory says everything is information. If everything is information then what type of information is heat, this question can be settled by the double slit experiment, but we must know what we are looking for. 


2020 ◽  
Vol 500 (2) ◽  
pp. 1884-1888
Author(s):  
Mohammed Sabil ◽  
A Habib ◽  
Z Benkhaldoun

ABSTRACT In this work, we aim to calibrate an interferential seeing monitor (ISM), which is a testing instument used at astronomical sites. Its method is based on the study of the diffraction pattern produced by a Young’s double-slit at the focus plane of a telescope. This method allows us to obtain the wave structure function by taking into account both phase and amplitude fluctuations of the light wavefront. A phase seeing εϕ was assigned to phase fluctuations and an amplitude seeing εχ was assigned to amplitude fluctuations (scintillation phenomenon), which allows us to obtain both phase and amplitude fluctuations. The feasibility of the ISM method was demonstrated by numerical simulations presented in a previous work. In this work, we have conducted a cross-calibration campaign of the ISM with a differential image motion monitor (DIMM) over 16 nights at the Oukaimeden and Atlas Golf Marrakech Observatories. The goal of this campaign was to study the reliability of this new method. In this paper, we present the calibration measurements and a comparison between the seeing measured by the ISM (εϕ, εχ) and that obtained by the DIMM (εdimm). These results show good agreement between the phase- eeing εϕ and εdimm.


2001 ◽  
Author(s):  
Arie N. de Jong ◽  
Hans Winkel ◽  
Rick I. Ghauharali

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