A chemically etched D-band waveguide orthomode transducer for CMB measurements
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.
Authors
- A. Paiella (ORCID: https://orcid.org/0000-0002-8388-3480)
- E. Tommasi
- M. Gervasi (ORCID: https://orcid.org/0000-0003-3884-0905)
- Andrea Limonta (ORCID: https://orcid.org/0000-0002-7988-2178)
- F. Piacentini (ORCID: https://orcid.org/0000-0002-5444-9327)
- S. Masi (ORCID: https://orcid.org/0000-0001-5105-1439)
- N. Brancadori (ORCID: https://orcid.org/0000-0002-6621-2562)
- A. Coppolecchia (ORCID: https://orcid.org/0000-0003-4522-5214)
- Angela Volpe (ORCID: https://orcid.org/0000-0002-3021-8823)
- F. Pezzotta (ORCID: https://orcid.org/0000-0002-0140-1346)
- ANIELLO MENNELLA (ORCID: https://orcid.org/0000-0002-5343-6655)
- M. Zannoni (ORCID: https://orcid.org/0000-0002-4495-571X)
- Giorgio Pettinari (ORCID: https://orcid.org/0000-0003-0187-3770)
- P. de Bernardis (ORCID: https://orcid.org/0000-0001-6547-6446)
- Elenia Manzan (ORCID: https://orcid.org/0009-0006-4235-9988)
- C. Franceschet (ORCID: https://orcid.org/0000-0002-3528-5240)
- S. Mandelli (ORCID: https://orcid.org/0000-0001-6737-6422)
- L. Lamagna (ORCID: https://orcid.org/0000-0002-2978-1352)
- Marco Bersanelli (ORCID: https://orcid.org/0000-0002-7866-948X)
- Andrea Passerini (ORCID: https://orcid.org/0000-0001-9766-517X)
- F. Cavaliere (ORCID: https://orcid.org/0009-0005-8829-2048)
- D. Viganò
- F. Montonati
- E. Boria
Institutions
- University of Milan (IT)
- Agenzia Spaziale Italiana (IT)
- Istituto Nazionale di Fisica Nucleare, Sezione di Milano (IT)
- Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca (IT)
- Consorzio Roma Ricerche (IT)
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma I (IT)
- University of Milano-Bicocca (IT)
- Sapienza University of Rome (IT)
Publication Details
- Journal
- Experimental Astronomy
- Published
- 2026-10-17
- DOI
- https://doi.org/10.1007/s10686-026-10082-8
- Primary Topic
- Superconducting and THz Device Technology
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- Università degli Studi di Milano
- Agenzia Spaziale Italiana