Primary Orbital Reconstruction with Selective Laser Melting (SLM) of Patient-Specific Implants (PSIs): An Overview of 96 Surgically Treated Patients

Contemporary advances in technology have allowed the transfer of knowledge from industrial laser melting systems to surgery; such an approach could increase the degree of accuracy in orbital restoration. The aim of this study was to examine the accuracy of selective laser melted PSIs (patient-specif...

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Bibliographic Details
Main Authors: Majeed Rana, Henriette L. Moellmann, Lara Schorn, Julian Lommen, Madiha Rana, Max Wilkat, Karsten Hufendiek
Format: Article
Language:English
Published: MDPI AG 2022-06-01
Series:Journal of Clinical Medicine
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Online Access:https://www.mdpi.com/2077-0383/11/12/3361
Description
Summary:Contemporary advances in technology have allowed the transfer of knowledge from industrial laser melting systems to surgery; such an approach could increase the degree of accuracy in orbital restoration. The aim of this study was to examine the accuracy of selective laser melted PSIs (patient-specific implants) and navigation in primary orbital reconstruction. Ninety-six patients with orbital fractures were included in this study. Planned vs. achieved orbital volumes (a) and angles (b) were compared to the unaffected side (<i>n</i> = 96). The analysis included the overlay of post-treatment on planned images (iPlan 3.0.5, Brainlab<sup>®</sup>, Feldkirchen, Germany). The mean difference in orbital volume between the digitally planned orbit and the postoperative orbit was 29.16 cm<sup>3</sup> (SD 3.54, presurgical) to 28.33 cm<sup>3</sup> (SD 3.64, postsurgical, t = 5.00, df = 95.00; <i>p</i> < 0.001), resulting in a mean volume difference (planned vs. postop) of less than 1 cm<sup>3</sup>. A 3D analysis of the color mapping showed minor deviations compared to the mirrored unaffected side. The results suggested that primary reconstruction in complex orbital wall fractures can be routinely achieved with a high degree of accuracy by using selective laser melted orbital PSIs.
ISSN:2077-0383