English

Polarization-preserving wavefront rotator

Optics 2026-04-29 v1 Instrumentation and Methods for Astrophysics Quantum Physics

Abstract

A K-mirror rotates the wavefront of an incident optical field. However, the rotation always introduces polarization changes in the transmitted field. This is a serious concern for applications ranging from astronomical image derotation to orbital angular momentum spectrum characterization in photonic quantum technology. Recent efforts have shown that the polarization change can be minimized significantly, but these require either a very small base angle that limits the field of view, or mirrors with a customized refractive index. Making the transmitted polarization state completely independent of the rotation angle has remained an open problem. In this work, we show that placing half-wave plates before and after a K-mirror and rotating them synchronously at half the K-mirror rotation angle makes the polarization change in the transmitted field exactly independent of the rotation angle. This works for any wavefront rotator, any base angle, any mirror refractive index, and any input state of polarization. We experimentally demonstrate the approach using a K-mirror with a base angle of 3030^{\circ}, which gives the largest field of view among practical designs, and find a mean polarization error of ~1%, limited only by the retardance imperfection of commercially available half-wave plates. This has significant practical implications for applications that require precise wavefront rotation without polarization change.

Keywords

Cite

@article{arxiv.2604.25475,
  title  = {Polarization-preserving wavefront rotator},
  author = {Suman Karan and Aman Srivastava and Pratham Sachin Todkar and Anand K. Jha},
  journal= {arXiv preprint arXiv:2604.25475},
  year   = {2026}
}

Comments

Main text: 5 pages, 4 figures; Supplementary: 1pages; Comments welcome

R2 v1 2026-07-01T12:38:57.939Z