A chemically etched D-band waveguide orthomode transducer for CMB measurements
Abstract
Abstract This study presents a prototype D-band waveguide orthomode transducer (OMT) fabricated using chemically etched brass platelets. This method offers a fast, cost-effective, and scalable approach for producing such devices above 100 GHz, making it well-suited for current and future Cosmic Microwave Background polarization experiments, where large focal planes with thousands of receivers are required to detect the faint primordial B -modes. Chemical etching has already demonstrated its effectiveness in manufacturing corrugated feedhorn arrays with state-of-the-art performance up to 150 GHz. Here, we evaluate its applicability to more complex structures, such as OMTs. We designed a single OMT prototype operating in the 130–170 GHz range, fabricated by chemically etching 0.15 mm-thick brass plates, which were then stacked, aligned, and mechanically clamped. Simulations based on metrological measurements of the OMT profile predict reflected power below −10 dB, cross-polarization better than −30 dB, and transmission around −0.5 dB in the 140−170 GHz band. Measurements yield transmisison around −1.5/−2 dB and cross-polarization $$<-$$ 20 dB. Further simulations show that the degradation in the transmission is related to defects and roughness along the etched profile ( $$\textrm{RMS}\simeq $$ 3 $$\mu $$ m), which is a typical and unavoidable effect of chemical etching. The discrepancy in cross-polarization, instead, could arise from a $$\sim $$ 1.5 $$^{\circ }$$ rotation of the polarization angle within the measurement chain. Our results show that chemical etching is a fast, low-cost, and scalable technique for producing waveguide OMTs with state-of-the-art performance in terms of reflected power and cross-polarization. However, at frequencies above 100 GHz our results show that the mechanical precision limitations of the chemical etching process degrade the transmission coefficient.
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Authors: Elenia Manzan, ANIELLO MENNELLA, F. Cavaliere, C. Franceschet, S. Mandelli, F. Montonati, M. Zannoni, P. de Bernardis, Marco Bersanelli, E. Boria, N. Brancadori, A. Coppolecchia, M. Gervasi, L. Lamagna, Andrea Limonta, S. Masi, A. Paiella, Andrea Passerini, F. Pezzotta, Giorgio Pettinari, F. Piacentini, E. Tommasi, D. Viganò, Angela Volpe
Institutions: Sapienza University of Rome, University of Milan, University of Milano-Bicocca, Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca, Istituto Nazionale di Fisica Nucleare, Sezione di Roma I, Istituto Nazionale di Fisica Nucleare, Sezione di Milano, Agenzia Spaziale Italiana, Consorzio Roma Ricerche