Whether you need a multi-prism beam expander, an extra cavity hybrid beam transformer, or a simple beam expander, our design and engineering team is ready to work with you to produce the exact optical component needed for your application. Please contact us today to place your custom order or schedule an initial consultation.

One application of beam expanders is in tunable laser resonates. Here an intracavity beam expander is used to increase the diameter of the laser beam to illuminate the width of a given diffraction grating. The beam divergence is reduced, and very narrow line widths can be emitted.

Laserbeam expander

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If a piece of glass or other transparent material takes on the appropriate shape, it is possible that parallel incident rays would either converge to a point or appear to be diverging from a point. A piece of glass that has such a shape is referred to as a lens.

As we begin to discuss the refraction of light rays and the formation of images by these two types of lenses, we will need to use a variety of terms. Many of these terms should be familiar to you because they have already been discussed during Unit 13. If you are uncertain of the meaning of the terms, spend some time reviewing them so that their meaning is firmly internalized in your mind. They will be essential as we proceed through Lesson 5. These terms describe the various parts of a lens and include such words as

There are a variety of types of lenses. Lenses differ from one another in terms of their shape and the materials from which they are made. Our focus will be upon lenses that are symmetrical across their horizontal axis - known as the principal axis. In this unit, we will categorize lenses as converging lenses and diverging lenses. A converging lens is a lens that converges rays of light that are traveling parallel to its principal axis. Converging lenses can be identified by their shape; they are relatively thick across their middle and thin at their upper and lower edges. A diverging lens is a lens that diverges rays of light that are traveling parallel to its principal axis. Diverging lenses can also be identified by their shape; they are relatively thin across their middle and thick at their upper and lower edges.

Multi-prism beam expanders are formed from two to five prisms arranged to form an optical system with the desired properties. These prism beam expanders can be described by ray transfer matrices, and the generalized mathematical description is known as multi-prism dispersion theory.

Reflectivebeam expander

A Galilean telescope consists of one lens with a negative focal length (the objective) and another with a positive focal length (the image lens). These two lenses are also placed so the distance between them is equal to the sum of their focal lengths. As one of the lenses is negative, the objective and lens will be close together, and there will be no internal foci. This makes Galilean beam expanders a good choice of high-power laser applications, as there is no problem with high power density within the system.

As we discuss the characteristics of images produced by converging and diverging lenses, these vocabulary terms will become increasingly important. Remember that this page is here and refer to it as often as needed.

Double Convex Lenses are made of BK7 or other materials, which are manufactured with an identical convex surface on both sides of the lens. Double Convex lenses ...

Keplerianvs Galileanbeam expander

Our beam expanders offer a versatile range of magnification, spanning from 1.5 times to 10 times, and we specialize in crafting tailored optics and coatings to meet the precise requirements of your specific applications.

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A double convex lens is symmetrical across both its horizontal and vertical axis. Each of the lens' two faces can be thought of as originally being part of a sphere. The fact that a double convex lens is thicker across its middle is an indicator that it will converge rays of light that travel parallel to its principal axis. A double convex lens is a converging lens. A double concave lens is also symmetrical across both its horizontal and vertical axis. The two faces of a double concave lens can be thought of as originally being part of a sphere. The fact that a double concave lens is thinner across its middle is an indicator that it will diverge rays of light that travel parallel to its principal axis. A double concave lens is a diverging lens. These two types of lenses - a double convex and a double concave lens will be the only types of lenses that will be discussed in this unit of The Physics Classroom Tutorial.

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Beam expanders increase the diameter of beams of collimated light and simultaneously decrease beam divergence. At Avantier we produce custom beam expanders for laser applications as well as remote sensing and interferometry.

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A lens is merely a carefully ground or molded piece of transparent material that refracts light rays in such as way as to form an image. Lenses can be thought of as a series of tiny refracting prisms, each of which refracts light to produce their own image. When these prisms act together, they produce a bright image focused at a point.

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A Keplerian telescope consists of two plano-convex convergent lenses placed so that the distance between the lenses is equal to the sum of their focal length.  These simple beam expanders have high expansion ratios. Because the two lenses have positive focal lengths the input beam will focus at a point between the two lenses, enabling spatial filtering. However, that same property makes Keplerian beam expanders problematic for high power laser applications, as the resulting energy density and heat at the focal point can deflect light and lead to wavefront errors.

Beam expanders that consist of two lenses are known as telescopic beam expanders. These transmissive beam expanders can be divided into two primary types: Keplerian beam expanders and Galilean beam expanders.

If a symmetrical lens were thought of as being a slice of a sphere, then there would be a line passing through the center of the sphere and attaching to the mirror in the exact center of the lens. This imaginary line is known as the principal axis. A lens also has an imaginary vertical axis that bisects the symmetrical lens into halves. As mentioned above, light rays incident towards either face of the lens and traveling parallel to the principal axis will either converge or diverge. If the light rays converge (as in a converging lens), then they will converge to a point. This point is known as the focal point of the converging lens. If the light rays diverge (as in a diverging lens), then the diverging rays can be traced backwards until they intersect at a point. This intersection point is known as the focal point of a diverging lens. The focal point is denoted by the letter F on the diagrams below. Note that each lens has two focal points - one on each side of the lens. Unlike mirrors, lenses can allow light to pass through either face, depending on where the incident rays are coming from. Subsequently, every lens has two possible focal points. The distance from the mirror to the focal point is known as the focal length (abbreviated by f). Technically, a lens does not have a center of curvature (at least not one that has any importance to our discussion). However a lens does have an imaginary point that we refer to as the 2F point. This is the point on the principal axis that is twice as far from the vertical axis as the focal point is.

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Beam expanders are used whenever the diameter of a collimated beam must be increased. They can also be used to change the focus spot size for a focusing lens, or to keep a beam collimated in optical systems that have a long beam path.

For both the Galilean and Keplerian configuration the output beam divergence can be calculated by the beam divergence of the input beam and the diameters of both output and input beams. In both cases, the ratio of input beam divergence to output beam divergence is equal to the ratio of output beam diameter to input beam diameter. This ratio is equal to the magnifying power of the beam expander system.

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