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University of Cambridge

Prototyping Blue Phase Wavefront Correctors for Astronomical Adaptive Optics

Abstract

dc:description.abstract

Adaptive optics is a technique developed in the field of astronomy for the correction of aberrations introduced by the atmosphere when observing stars, planets and deep sky objects using telescopes based on Earth. This correction is usually applied with deformable mirrors, which have the benefit of being polarisation and wavelength insensitive, while also matching the submillisecond rate at which the turbulence changes. This work provides an alternative solution, by using blue phase liquid crystals as the correcting medium, which also comes with the same benefits of polarisation insensitivity and speed. By using correctors made with blue phases, the cost of manufacturing is reduced, requiring much less precision during fabrication. Techniques to apply this specifically to the field of astronomical adaptive optics are demonstrated, and a streamlined process is developed, in which prototypes of blue phase correctors are achieved. These meet an expected rise and fall time of trise = 130 μs and tfall = 125 μs, respectively. They achieve a phase modulation of 1.23 radians, corresponding to 0.39π, at an applied field of 7.73 V/μm, in a transmissive topology. For reflective devices, which are further compatible with existing adaptive optics systems, a tip/tilt mode is successfully applied with a root mean square of the wavefront of 76.05 radians across a 1 cm x 1 cm area at an applied field of 14.3 V/μm. This is a milestone achievement for blue phases in the first ever demonstration of them being used for astronomical adaptive optics. Moreover, these devices were built on a PCB substrate with no intermediary layer, furthermore forming the first demonstration of blue phases grown on PCB. All the steps and architectures described throughout the work are optimised to achieve a low-cost, approachable alternative suitable for prototyping blue phase devices for adaptive optics

Degree

thesis:*
Name dc:type.qualificationname
Doctor of Philosophy (PhD)
Level dc:type.qualificationlevel
Doctoral
Grantor dc:publisher.institution
University of Cambridge
Year dc:date.issued
2026

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Niculescu, Oana
Advisor dc:contributor.advisor
  • Wilkinson, Timothy

Subjects

dc:subject × 6

Rights

dc:rights
Language dc:language
eng

Identifiers

dc:identifier.*
DOI dc:identifier.doi
https://doi.org/10.17863/CAM.131859
OAI identifier oai:identifier
oai:www.repository.cam.ac.uk:1810/405728

Chain of custody

source
Harvested from
Cambridge University
Base URL
api.repository.cam.ac.uk/server/oai/request
Last updated
2026-07-24
Source record
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citation

Niculescu, Oana. Prototyping Blue Phase Wavefront Correctors for Astronomical Adaptive Optics. Doctoral thesis, University of Cambridge, 2026. https://doi.org/10.17863/CAM.131859