Proposal of new optic elements

G. ChadzitaskosDepartment of Physics, FNSPE, Czech Technical University in

Prague

Stará Lesná 2012

Overview

Two diffraction grating Parabolic strip telescope Objective for X ray microscopy CNOT on polarizated states of light Objective for X ray telescope

Two diffraction systém(Wikipedia)

.

Two diffraction system

The light from monochromatic light source 1 is divided into two channels 3, by a 1:1 beam splitter 2, and is brought into the two-diffraction gratings 5. Two-diffraction grating generally consists of a large number of equally spaced slits, which allows connection of one channel with odd slits and the other channel with even slits 4. Then spots 7 – interference maxima – appear on the screen 6.

Maxima

case 1 :

d

kk 2

sin

case 2:

d

kk

sin

2

0

sinsin

sinsin

sin

sinsin

)(

ba

ban

a

a

II

Intensities

2

0

sin2

sin

sin2

sin

sin

sinsin1

ba

ban

a

a

Ip

2

0

sinsin

sinsin

sin

sinsin)(

ba

ban

a

a

pII

Exploitation

• Measurement of coincident part of light• Measurement of cross sections of interaction

light and electrons (two slit experiment)

CNOT ON POLARIZATED STATES OF COHERENT LIGHT

Optical activity of molecules with magnetic dipole

(C.Denz,Electro-optic composite polymers, Munster)

Linear dependence on electric field

CEkT

npP

2

2

Exploitation

• Quantum optics

PARABOLIC STRIP TELESCOPEPrinciple

Rotation around y axis and Radon inverse transform

Used experimental plexiglass telescope objectives

Artifitial constelations

Image procesing

From camera RGB uint8 Select central part, make

matrices 600 x 600x 3 and rotate, single precision

12th root of real matrices Point multiplication of 0

and 90 degree matrices Point multiplication,

optimalization Uint8 and image

Images of artificial star constellation

Original images at 0, 45, 90, and 135 degree

After MATLAB calculation

Image procesing

Advantages \• good angular resolution• low expenses• simple technological development• simple exploitation of adaptive optics• possibility to install a net of large telescopes over the Earth• lower weight for use on satellites

Proposal: Over Earth net of telescopes (30 degrees)

• high mounting not necessary• low wind influence• low gravitational influence 

Objective for X ray microscopy

Fresnel zone plates, polycapillar optics, Goebel mirrors, biconcave refractive optics.

New: Spatial grating – Bragg’s and interference conditions

.

Example

12

1

22

0

sRRd

nE

FS

1

222

000

0 sRdR

nESF

sin2dn 22sin

sR

R

X ray telescope

Wolter Kirkpatrick-Baez

Lobster eye objective

New X-ray telescope

Bragg’s condition

22

2px

p

nd

)1(0 Tdd

1

2

1)()( 22

0min px

pd

nxTxT

222

0

222max

2min

2max

44

ndnd

xx

Děkuji za pozornost

Pro destičku germaniového monokrystalu a teploty mezi 250 a 1000 K je pro vlnovou délku 0.5 nm hodnota například pro xmin = 10 cm bude xmax = 10,8 cm.