17 GHz photonic band gap cavity with improved input coupling
We present the theoretical design and cold test of a 17 GHz photonic band gap (PBG) cavity with improved coupling from an external rectangular waveguide. The PBG cavity is made of a triangular lattice of metal rods with a defect (missing rod) in the center. The TM_{010}-like defect mode was chosen a...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
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American Physical Society
2001-04-01
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| Series: | Physical Review Special Topics. Accelerators and Beams |
| Online Access: | http://doi.org/10.1103/PhysRevSTAB.4.042001 |
| _version_ | 1818281214025400320 |
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| author | M. A. Shapiro W. J. Brown I. Mastovsky J. R. Sirigiri R. J. Temkin |
| author_facet | M. A. Shapiro W. J. Brown I. Mastovsky J. R. Sirigiri R. J. Temkin |
| author_sort | M. A. Shapiro |
| collection | DOAJ |
| description | We present the theoretical design and cold test of a 17 GHz photonic band gap (PBG) cavity with improved coupling from an external rectangular waveguide. The PBG cavity is made of a triangular lattice of metal rods with a defect (missing rod) in the center. The TM_{010}-like defect mode was chosen as the operating mode. Experimental results are presented demonstrating that critical coupling into the cavity can be achieved by partial withdrawal or removal of some rods from the lattice, a result that agrees with simulations. A detailed design of the PBG accelerator structure is compared with a conventional (pillbox) cavity. One advantage of the PBG cavity is that its resonance frequency is much less perturbed by the input/output coupling structure than in a comparable pillbox cavity. The PBG structure is attractive for future accelerator applications. |
| first_indexed | 2024-12-13T00:01:33Z |
| format | Article |
| id | doaj.art-d46b9f182dc34e468a9c2a34aeb4863b |
| institution | Directory Open Access Journal |
| issn | 1098-4402 |
| language | English |
| last_indexed | 2024-12-13T00:01:33Z |
| publishDate | 2001-04-01 |
| publisher | American Physical Society |
| record_format | Article |
| series | Physical Review Special Topics. Accelerators and Beams |
| spelling | doaj.art-d46b9f182dc34e468a9c2a34aeb4863b2022-12-22T00:06:24ZengAmerican Physical SocietyPhysical Review Special Topics. Accelerators and Beams1098-44022001-04-014404200110.1103/PhysRevSTAB.4.04200117 GHz photonic band gap cavity with improved input couplingM. A. ShapiroW. J. BrownI. MastovskyJ. R. SirigiriR. J. TemkinWe present the theoretical design and cold test of a 17 GHz photonic band gap (PBG) cavity with improved coupling from an external rectangular waveguide. The PBG cavity is made of a triangular lattice of metal rods with a defect (missing rod) in the center. The TM_{010}-like defect mode was chosen as the operating mode. Experimental results are presented demonstrating that critical coupling into the cavity can be achieved by partial withdrawal or removal of some rods from the lattice, a result that agrees with simulations. A detailed design of the PBG accelerator structure is compared with a conventional (pillbox) cavity. One advantage of the PBG cavity is that its resonance frequency is much less perturbed by the input/output coupling structure than in a comparable pillbox cavity. The PBG structure is attractive for future accelerator applications.http://doi.org/10.1103/PhysRevSTAB.4.042001 |
| spellingShingle | M. A. Shapiro W. J. Brown I. Mastovsky J. R. Sirigiri R. J. Temkin 17 GHz photonic band gap cavity with improved input coupling Physical Review Special Topics. Accelerators and Beams |
| title | 17 GHz photonic band gap cavity with improved input coupling |
| title_full | 17 GHz photonic band gap cavity with improved input coupling |
| title_fullStr | 17 GHz photonic band gap cavity with improved input coupling |
| title_full_unstemmed | 17 GHz photonic band gap cavity with improved input coupling |
| title_short | 17 GHz photonic band gap cavity with improved input coupling |
| title_sort | 17 ghz photonic band gap cavity with improved input coupling |
| url | http://doi.org/10.1103/PhysRevSTAB.4.042001 |
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