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Paraxial properties of three-element zoom systems for laser beam expanders

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Abstract

Our work is focused on the problem of theoretical analysis of paraxial properties of the three-element zoom optical system for laser beam expanders. Equations that enable to calculate mutual axial distances between individual elements of the system based on the axial position of the beam waist of the input Gaussian beam and the desired magnification of the system are derived. Finally, the derived equations are applied on an example of calculation of paraxial parameters of the three-element zoom system for the laser beam expander.

© 2014 Optical Society of America

1. Introduction

Currently, lasers [1,2] are being widely used in many areas of science and technology. Since the laser beam has specific properties special optical systems for transformation of laser beams are required. Common optical systems used both in classical imaging optics and laser optics are beam expanders. In case of transformation of a homocentric light beam simple telescopic systems are being used for beam expansion. In case of a laser beam the input Gaussian beam has to be transformed into output Gaussian beam with different diameter and divergence. The design of the optical system of the expander is different since different formulas are valid for the transformation of a laser beam (Gaussian beam). Thus one has to consider the properties of the Gaussian beam during the design of such laser beam expander. Zoom optical systems are often required in practical applications. For the case of classical (homocentric) beams the problem of analysis and design of zoom systems is described thoroughly e.g. in Refs [312].

Our work is focused on the problem of theoretical analysis of paraxial properties of the three-element zoom optical system for laser beam expanders. The equations enabling the calculation of axial distances between individual elements based on the location of a beam waist of the input Gaussian beam and the desired magnification of the system are derived. Finally, an example of calculation of paraxial parameters of such a beam expander is given.

2. Basic parameters of a laser beam

Laser beam is not a homocentric light beam, it is a Gaussian beam. Different equations therefore hold for the transformation of such a beam trough the optical system with respect to classical equations that are valid for homocentric light beams [1,2,13]. In laser beams, which are very narrow, the field is concentrated along one of the axis of the chosen coordinate system (e.g. z axis). In the transverse direction the field fades relatively fast to zero whereas in the longitudinal direction it changes very slowly. Let us now restrict our analysis on the most simple case of circular Gaussian beam, which is however the most important in practice. Let u=u(x,y,z) is an arbitrary component of e.g. the electric field vector in orthogonal Cartesian coordinate system, then for circular Gaussian beam one obtains [1,2,13]

u=w0wexp(x2+y2w2)exp(ikz+iψikx2+y22R),
where
R(z)=z(1+z02/z2),w2(z)=w02(1+z2/z02),ψ(z)=arctan(z/z0),z0=kw02/2,
whereas 2w0 denotes the diameter of the beam waist (Fig. 1), k=2π/λ is the wave number and λ is the wavelength of light. R is vertex radius of curvature i.e. it is the radius of curvature for the points in the close proximity to z axis. The envelope of the Gaussian beam is the one-sheeted rotational hyperboloid [1,2,13].

 figure: Fig. 1

Fig. 1 Basic parameters of a Gaussian beam

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The divergence of the beam is then characterized by the divergence angle θ, which is the angle between the asymptote of the x cross section of the hyperboloid and the axis of the beam (z-axis) see Fig. 1. The following equation is valid for the Gaussian beam [1,2,13]

w0θ=λ/π.
Without the loss of generality we will further deal with the paraxial transformation of a Gaussian beam by the thin lens system. The equations derived for the thin lens system are valid for the thick lens system assuming we take all the values with respect to focal points of individual optical elements or to their principal planes [1,1316].

As it is known from the geometrical optics theory the thin lens (Fig. 1) transforms the incident spherical wavefront with radius R to output spherical wavefront with radius R' according to the relation [1,1316]

1/R1/R=1/f,
where f is the focal length of the lens. Using Eqs. (2) and (4) we obtain the following equations for the transformation of a Gaussian beam by the thin lens system of n lenses (i = 1, 2, 3,…, n) [1,2,13]
Gi=fi2qi2+z0i2=mi21+mi2(z0i/fi)2,qi=qiGi,z0i+1=z0iGi,Δi=fi+fi+1di,qi+1=qi+Δi,si=qifi,si=qi+fi,
where fi is the focal length of the i-th lens and di is the distance between the i-th and the i + 1-th lens, si and si are image and object axial distance and qi and qi are image and object axial distance of the Gaussian beam waist from focal points (q1=s1+f1, z01=πw012/λ), mi=fi/qi is the transverse magnification of the lens (optical system) and Δi is the distance between the object-space focal point of i + 1-th lens and the image-space focal point of the i-th lens. The transverse magnification mG of the whole system (magnification of the Gaussian beam waist after transformation of the beam by this system) is given by
mG2=(w0/w0)2=(θ/θ)2=i=1i=nGi.
As it can be seen from Eq. (5) function G(q) will have maximum for q = 0 and according to Eq. (6) the divergence θ of the Gaussian beam transformed by the optical system is then minimal.

3. Three-element zoom systems for laser beam expander

Figure 2 shows a principal scheme of the three-element zoom system for laser beam expander.

 figure: Fig. 2

Fig. 2 Three-element zoom systems for laser beam expander

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The system consists of three thin lens elements with different focal lengths separated by appropriate axial distances.

By using Eqs. (5) for the three-element optical system, we obtain for the parameter Δ2 after tedious calculation the following equation

a2Δ22+a1Δ2+a0=0,
where
a2=(Δ1z01)2+(Δ1q1f12)2,a1=2f22[Δ1z012+q1(Δ1q1f12)],a0=f22[(z01f2)2+(q1f2)2(f1f3/mG)2].
We required that q3=0 (G3has maximum) during the derivation of Eq. (7) in order to obtain minimal divergence of the transformed Gaussian beam. For the real solution of Eq. (7) it must hold that the discriminant D(Δ1)=a124a2a00. By using Eq. (8) we obtain for the parameter Δ1min the following equation
b2Δ1min2+b1Δ1min+b0=0,
where
b2=f32(z012+q12),b1=2q1(f1f3)2,b0=f12[(f1f3)2(z01f2mG)2].
Distance d1 then must satisfy the condition d1d1min, where d1min=f1+f2Δ1min. The axial separation d2 of the second and the third element of the system is then given by d2=f2+f3Δ2. The transverse magnification of the Gaussian beam waist mG of the three-element optical system for laser beam expander can be expressed as
mG2=(f3f1f2)2[1+(q1z01)2][(d1f1f2+q1f12z012+q12)2+z012f14(z012+q12)2].
Due to the fact that for common lasers used in practice [14] z01 is relatively large (see Eq. (2)) the Eq. (11) for magnification mG can be approximated by the formula
(mG2)aprox[f3(f1+f2)f1f2d1f3f1f2]2=[f3(f1+f2d1)f1f2]2=(f3f12)2,
where f12 is the focal length of the first two elements of the optical system. Equation (12) is very simple and it enables to determine the magnification mG with the accuracy that is satisfactory for practice. As it can be seen from Eq. (12) magnification mG is a linear function of distance d1 for chosen values of focal lengths f1, f2 and f3 of individual elements of given optical system. Further, one can see that Eq. (12) is equivalent to classical equation for telescopic systems for transformation of homocentric beams [3,1316].

During the calculation of the paraxial parameters of such optical system one can also use another procedure. Firstly, one can choose focal lengths f2 and f3 of the second and the third element of the three-element optical system, magnification mG=mGminand distance d1 = d1min. The value of the focal length f1min of the first element can then be calculated using the following equation

c2f1min4+c1f1min2+c0=0,
where
c2=f32,c1=2d1q1f32mG2z012f22,c0=d12f32(q12+z012).
By solving Eq. (13) we have
f1min=±mG2z012f222d1q1f32±mG2f22(mG2z012f224d1q1f32)4d12f342f32.
If we choose for simplicity e.g. f2=f1, then we obtain
e2f1min4+e1f1min2+e0=0,
where
e2=f32mG2z012,e1=2d1q1f32,e0=d12f32(q12+z012).
By solving of Eq. (16) one obtains
f1min=±d1q1f32+d1f3z01mG2(q12+z012)f32mG2z012f32.
By solving of Eq. (7) one can calculate the axial separation d2=f2+f3Δ2. Let us now assume that the absolute value of the quantity z01 is much greater than the magnitudes of other quantities in Eq. (18), which is always true in practical cases. Then the focal length f1min can be approximately calculated as (f2=f1)

f1min±d1f3/mG.

4. Example

Let us show the application of the above described analysis on an example of the three-element zoom systems for laser beam expander. If we choose f12=f3, then according to Eq. (19) it holds that d1mG. The focal lengths of individual elements of the zoom system are chosen to be: f1=10mm, f2=10mm, f3=100mm. The beam waist radius of the input laser beam entering the optical system is w01=0.5mm (z01=1241mm) and the axial distance of the beam waist from the first element of the system is s1=100mm. Wavelength of light is λ=632.8nm. By solving of Eq. (9) we obtain: d1min=f1+f2Δ1min=9.9677mm. Thus we will choose the mutual distance between the first two elements d1 in the range d110,50mm.

The results of calculation using Eqs. (7) and (5) are given in Table 1, where wi (i = 1,2,3) stands for transverse radii of the Gaussian beam on individual elements of the zoom system, w03 is the beam waist radius of the output beam emerging out from the optical system, s3 is the distance of the output beam waist from the last element of our optical system and θ3 is the divergence angle of the output Gaussian beam. The linear dimensions in Table 1 are given in millimeters.

Tables Icon

Table 1. – Example of three-element zoom system for laser beam expansion

5. Conclusion

In our work we performed a detailed theoretical analysis of paraxial properties of the three-element zoom optical system for laser beam expanders. Equations that enable to calculate the mutual distance between individual elements of the three-element zoom optical system for laser beam expander in dependence on the value of magnification mG of the optical system were derived. It was shown that the magnification of such a system is approximately a linear function of the mutual distance d1 between the first and the second element of the optical system. Example of the calculation of paraxial parameters of the three-element zoom optical system for laser beam expander was shown and the results of this calculation (for several values of magnification mG) were given in Table 1. The problem of influence of aberrations of optical system on the transformation of the Gaussian beam was not studied in our work. We focused on the calculation of the paraxial parameters of the zoom system for transformation of the Gaussian beam. Those interested in the influence of aberrations on the transformed beam can find detailed information e.g. in [17]. The choice of the shape and calculation of radii of curvature of individual elements of zoom optical systems is described in detail in ref [5], thus we did not deal with this problem here.

Acknowledgments

This work has been supported from the Czech Science Foundation by the grant 13-31765S.

References and links

1. B. E. A. Saleh and M. C. Teich, Fundamentals of Photonics, 2nd ed. (Wiley-Interscience, New York, 2007).

2. H. Kogelnik and T. Li, “Laser Beams and Resonators,” Appl. Opt. 5(10), 1550–1567 (1966). [CrossRef]   [PubMed]  

3. A. D. Clark, Zoom Lenses (Adam Hilger, London, 1973).

4. K. Yamaji, Progres in Optics, Vol.VI (North-Holland Publishing Co., Amsterdam 1967).

5. A. Miks, J. Novák, and P. Novák, “Method of zoom lens design,” Appl. Opt. 47(32), 6088–6098 (2008). [CrossRef]   [PubMed]  

6. T. Kryszczyński and J. Mikucki, “Structural optical design of the complex multi-group zoom systems by means of matrix optics,” Opt. Express 21(17), 19634–19647 (2013). [CrossRef]   [PubMed]  

7. G. Wooters and E. W. Silvertooth, “Optically Compensated Zoom Lens,” J. Opt. Soc. Am. 55(4), 347–351 (1965). [CrossRef]  

8. T. Kryszczyński, M. Leśniewski, and J. Mikucki, “Use of matrix optics to analyze the complex multi-group zoom systems,” Proc. SPIE 8697, 86970I (2012). [CrossRef]  

9. S. Pal and L. Hazra, “Ab initio synthesis of linearly compensated zoom lenses by evolutionary programming,” Appl. Opt. 50(10), 1434–1441 (2011). [CrossRef]   [PubMed]  

10. L. Hazra and S. Pal, “A novel approach for structural synthesis of zoom systems,” Proc. SPIE 7786, 778607 (2010). [CrossRef]  

11. S. Pal and L. Hazra, “Stabilization of pupils in a zoom lens with two independent movements,” Appl. Opt. 52(23), 5611–5618 (2013). [CrossRef]   [PubMed]  

12. S. Pal, “Aberration correction of zoom lenses using evolutionary programming,” Appl. Opt. 52(23), 5724–5732 (2013). [CrossRef]   [PubMed]  

13. A. Miks, Applied Optics (Czech Technical University Press, Prague, 2009).

14. http://www.edmundoptics.com

15. W. T. Welford, Aberrations of the Symmetrical Optical Systems, (Academic Press, London, 1974).

16. W. Smith, Modern optical engineering, 4th Ed., (McGraw-Hill, New York, 2007).

17. A. Miks and J. Novak, “Propagation of Gaussian beam in optical system with aberrations,” Optik: International Journal for Light and Electron Optics 114(10), 437–440 (2003). [CrossRef]  

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Figures (2)

Fig. 1
Fig. 1 Basic parameters of a Gaussian beam
Fig. 2
Fig. 2 Three-element zoom systems for laser beam expander

Tables (1)

Tables Icon

Table 1 – Example of three-element zoom system for laser beam expansion

Equations (19)

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u= w 0 w exp( x 2 + y 2 w 2 )exp( ikz+iψik x 2 + y 2 2R ),
R(z)=z(1+ z 0 2 / z 2 ), w 2 (z)= w 0 2 (1+ z 2 / z 0 2 ),ψ(z)=arctan(z/ z 0 ), z 0 =k w 0 2 /2,
w 0 θ=λ/π.
1/ R 1/R=1/ f ,
G i = f i 2 q i 2 + z 0i 2 = m i 2 1+ m i 2 ( z 0i / f i ) 2 , q i = q i G i , z 0i+1 = z 0i G i , Δ i = f i + f i+1 d i , q i+1 = q i + Δ i , s i = q i f i , s i = q i + f i ,
m G 2 = ( w 0 / w 0 ) 2 = (θ/ θ ) 2 = i=1 i=n G i .
a 2 Δ 2 2 + a 1 Δ 2 + a 0 =0,
a 2 = ( Δ 1 z 01 ) 2 + ( Δ 1 q 1 f 1 2 ) 2 , a 1 =2 f 2 2 [ Δ 1 z 01 2 + q 1 ( Δ 1 q 1 f 1 2 ) ], a 0 = f 2 2 [ ( z 01 f 2 ) 2 + ( q 1 f 2 ) 2 ( f 1 f 3 / m G ) 2 ].
b 2 Δ 1min 2 + b 1 Δ 1min + b 0 =0,
b 2 = f 3 2 ( z 01 2 + q 1 2 ), b 1 =2 q 1 ( f 1 f 3 ) 2 , b 0 = f 1 2 [ ( f 1 f 3 ) 2 ( z 01 f 2 m G ) 2 ].
m G 2 = ( f 3 f 1 f 2 ) 2 [ 1+ ( q 1 z 01 ) 2 ][ ( d 1 f 1 f 2 + q 1 f 1 2 z 01 2 + q 1 2 ) 2 + z 01 2 f 1 4 ( z 01 2 + q 1 2 ) 2 ].
( m G 2 ) aprox [ f 3 ( f 1 + f 2 ) f 1 f 2 d 1 f 3 f 1 f 2 ] 2 = [ f 3 ( f 1 + f 2 d 1 ) f 1 f 2 ] 2 = ( f 3 f 12 ) 2 ,
c 2 f 1min 4 + c 1 f 1min 2 + c 0 =0,
c 2 = f 3 2 , c 1 =2 d 1 q 1 f 3 2 m G 2 z 01 2 f 2 2 , c 0 = d 1 2 f 3 2 ( q 1 2 + z 01 2 ).
f 1min =± m G 2 z 01 2 f 2 2 2 d 1 q 1 f 3 2 ± m G 2 f 2 2 ( m G 2 z 01 2 f 2 2 4 d 1 q 1 f 3 2 )4 d 1 2 f 3 4 2 f 3 2 .
e 2 f 1min 4 + e 1 f 1min 2 + e 0 =0,
e 2 = f 3 2 m G 2 z 01 2 , e 1 =2 d 1 q 1 f 3 2 , e 0 = d 1 2 f 3 2 ( q 1 2 + z 01 2 ).
f 1min =± d 1 q 1 f 3 2 + d 1 f 3 z 01 m G 2 ( q 1 2 + z 01 2 ) f 3 2 m G 2 z 01 2 f 3 2 .
f 1min ± d 1 f 3 / m G .
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