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Tensor tomography of the residual stress field in graded-index YAG’s single crystals

  • Alfred Puro EMAIL logo and Egor Marin
Published/Copyright: August 25, 2023

Abstract

This work presents an application of tensor field tomography for non-destructive reconstructions of axially symmetric residual stresses in a graded-index YAG single crystal for the case of beam deflection. The axis of the cylinder coincides with the crystallographic axis [001] of the single crystal and it has an axially symmetric refractive index distribution. The transformation of the polarization of light is measured in a plane orthogonal to the axis of the cylinder. Stresses are determined within the framework of the Maxwell piezo-optic law (linear dependence of the permittivity tensor on stresses) and small rotation of quasi principal stress axes. This paper generalizes the method of integrated photoelasticity for the case of ray deflection.

MSC 2020: 35R30; 35Q60; 92C55

A Inversion of the ray integral H 1

We write H 1 in polar coordinates

H 1 ( S ) = 2 π 44 s 1 σ r z sin ( ν ) R ( r ) d r R 2 ( r ) - S 2 ( s ) = 2 π 44 s 1 σ r z S ( s ) R ( r ) R ( r ) d r R 2 ( r ) - S 2 ( s ) = 2 π 44 S R ( 1 ) σ r z d r d R S d R R 2 - S 2 .

This is the Abel integral equation and its solution can be written as

σ r z [ R ( r ) ] = - 1 2 π 44 d R d r R ( r ) R ( 1 ) d d S H 1 ( S ) d S S 2 - R 2 ( r ) .

B Inversion of the ray integral H b

The properties of integrals of this type have been studied in detail earlier [10], although an explicit analytical solution was not given there. We implement the method used in [25] to inversion H b . We transform H b by using polar coordinates R ( r ) , φ

H 02 ( S ) = 0 l σ ( r ) cos ( 4 α + 2 ν ) 𝑑 l = 2 S R ( 1 ) σ [ r ( R ) ] L ( R ) cos [ 4 α ( R , S ) + 2 ν ] R d R R 2 - S 2 , L ( R ) = d r d R .

Bearing in mind that

ν = a sin ( s n ( s ) r n ( r ) ) = π 2 - arccos ( S R ) and cos [ 4 α ( R , S ) + 2 ν ] = - cos [ 4 α ( R , S ) - 2 arccos ( S R ) ] ,

we can write H b as

(B.1) H b ( S ) = - 2 S R ( 1 ) cos [ E ( R , S ) ] σ ( R ) L ( R ) R d R R 2 - S 2 ,

where

E ( R , S ) = 4 α ( R , S ) - 2 arccos ( S R ) = S R S [ 4 D ( K ) - 2 ] d K K K 2 - S 2 , arccos ( S R ) = S R S d K K K 2 - S 2 .

By using results of [25], we will show that the inversion of integral H b can be written as

(B.2) σ ( r ) n ( r ) = 1 π r { r [ R R 0 c h [ B ( S , R ) ] H 02 ( S ) S S 2 - R 2 𝑑 S ] + ( 4 r - 2 d l n [ R ( r ) ] d r ) R R 0 s h [ B ( S , R ) ] H 02 ( S ) 𝑑 S } ,

where

B ( S , R ) = R | S | S [ 4 D ( K ) - 2 ] d K K S 2 - K 2 .

We will not give all the proof; we will indicate only those changes that are directly related to this solution. At first, we insert (B.1) into to solution (B.2) and will have then the equation as in [25, equation (6)]. In our case, the integral G 1 (see [25, (equation (9)]) transforms to

G 1 = Re R K c h [ I ( S , R , K ) ] K 2 - S 2 S 2 - R 2 S 𝑑 S , I ( S , R , K ) = R K [ 4 D ( T ) - 2 ] d T T 1 - ( T S ) 2 = m = 0 a m S - m .

Here,

a 0 = R K [ 4 D ( T ) - 2 ] d T T = R K { 4 d l n [ t ( T ) ] d l n ( T ) T - 2 T } 𝑑 T = 4 r ( R ) k ( K ) d t t - 2 R K d T T = ln { [ k ( K ) r ( R ) ] 4 [ R K ] 2 } .

Thus, the integral G 1 is equal to

G 1 = π 4 [ ( k ( K ) r ( R ) ) 4 ( R K ) 2 + ( r ( R ) k ( K ) ) 4 ( K R ) 2 ] .

The integral G c 1 (see [25, equation (11)]) transforms to

G c 1 = 1 4 Re s h [ I ( S , R , K ) ] K 2 - S 2 𝑑 S = π 4 [ ( k ( K ) r ( R ) ) 4 ( R K ) 2 - ( r ( R ) k ( K ) ) 4 ( K R ) 2 ]

and (B.2) transforms to

σ ( r ) n ( r ) = - 2 π r { r [ R R 0 π 4 [ ( k ( K ) r ( R ) ) 4 ( R K ) 2 + ( r ( R ) k ( K ) ) 4 ( K R ) 2 ] σ ( K ) L ( K ) K d K ]
+ ( 4 r - 2 d l n [ R ( r ) ] d r ) R R 0 π 4 [ ( k ( K ) r ( R ) ) 4 ( R K ) 2 - ( r ( R ) k ( K ) ) 4 ( K R ) 2 ] σ ( K ) L ( K ) K d K } .

After differentiation, we obtain the identity. In the case of straight ray tomography ν = 0.5 π - α , the solution (B.2) coincides with Cormack’s inversion formula for the second angular harmonics of the Radon transform. Using elementary transformations, the reconstructing algorithm can be written in the more familiar form

σ ( r ) = d R ( r ) π d r { [ R R 0 c h [ B ( S , R ) ] S 2 - R 2 d d S H 02 𝑑 S ] + 4 R R 0 s h [ B ( S , R ) ] H 02 ( S ) S 2 - R 2 R S D ( K ) d K S 2 - K 2 𝑑 S } .

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Received: 2021-07-21
Revised: 2022-11-23
Accepted: 2022-12-02
Published Online: 2023-08-25
Published in Print: 2023-12-01

© 2023 Walter de Gruyter GmbH, Berlin/Boston

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