A Fresnel rhomb is a prism designed in 1817 by Augustin-Jean Fresnel for converting linearly polarized light into circularly polarized light. While the device performs the same function as a quarter wave plate, the rhomb does not depend on a material's birefringence. Rather, the relative phase shift between the s and p polarizations is a result of total internal reflection, two of which each contribute a nominal retardance of 45°. This achieves a wide spectral bandwidth, which is difficult using birefringent waveplates. The precision of the 90° phase shift is compromised only due to changes in the refractive index of the material due to dispersion; this change can be very small over a wide spectral range. The material (typically glass) is itself specifically not birefringent.
The dimensions of the rhomb (usually a parallelepiped) are such that light entering one of the small faces undergoes two internal reflections, as seen in the figure, before exiting through the other small face. The angle of each internal reflection is designed to produce a 45° (π/4 radians) phase delay between the two linearly polarized components of the light. Hence a linearly polarized beam at 45° becomes elliptically polarized after the first reflection, but emerges as circularly polarized after the second reflection. For other input polarizations, the net effect of the rhomb is identical to that of a quarter wave plate. Two Fresnel rhombs can be used in tandem (usually cemented to avoid reflections at their interface) in order to achieve the function of a halfwave plate. The latter arrangement, unlike a single Fresnel rhomb used as a quarter-wave retarder, has the additional feature that the exiting beam can be collinear with the original incident beam.