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| DOI | 10.1016/J.NIMA.2025.170224 | ||||
| Año | 2025 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
We present the results of an extensive evaluation of strip and pixel AC-LGAD sensors tested with a 120 GeV proton beam, focusing on the influence of design parameters on the sensor temporal and spatial resolutions. Results show that reducing the thickness of pixel sensors significantly enhances their time resolution, with 20 mu m-thick sensors achieving around 20 ps. Uniform performance is attainable with optimized n+ sheet resistance, making these sensors ideal for future timing detectors. Conversely, 20-mu m-thick strip sensors exhibit higher jitter than similar pixel sensors, negatively impacting time resolution, despite reduced Landau fluctuations with respect to the 50-mu m-thick versions. Additionally, it is observed that a low resistivity in strip sensors limits signal size and time resolution, whereas higher resistivity improves performance. This study highlights the importance of tuning the n+ sheet resistance and suggests that further improvements should target specific applications like the Electron-Ion Collider or other future collider experiments. In addition, the detailed performance of four AC-LGADs sensor designs is reported as examples of possible candidates for specific detector applications. These advancements position AC-LGADs as promising candidates for future 4D tracking systems, pending the development of specialized readout electronics.
| Revista | ISSN |
|---|---|
| Nuclear Instruments & Methods In Physics Research Section A Accelerators Spectrometers Detectors And Associated Equipment | 0168-9002 |
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Dutta, I. | - |
Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos |
| 2 | MADRID-ZAMBRANO, CRISTIAN | Hombre |
Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos |
| 3 | Heller, Ryan | Hombre |
Lawrence Berkeley Natl Lab - Estados Unidos
Lawrence Berkeley National Laboratory - Estados Unidos |
| 4 | Wang, R. | Hombre |
UNIV ILLINOIS - Estados Unidos
University of Illinois at Chicago - Estados Unidos |
| 5 | Shekar, Danush | - |
UNIV ILLINOIS - Estados Unidos
University of Illinois at Chicago - Estados Unidos |
| 6 | Martín, Claudio San | - |
Universidad Técnica Federico Santa María - Chile
Centro Científico Tecnológico de Valparaíso - Chile |
| 6 | San Martin, Claudio | - |
Universidad Técnica Federico Santa María - Chile
Centro Científico Tecnológico de Valparaíso - Chile |
| 7 | Barria, Matias | - |
Universidad Técnica Federico Santa María - Chile
Centro Científico Tecnológico de Valparaíso - Chile |
| 8 | Apresyan, A. | Hombre |
Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos |
| 9 | Ye, Z. | - |
Lawrence Berkeley Natl Lab - Estados Unidos
UNIV ILLINOIS - Estados Unidos Lawrence Berkeley National Laboratory - Estados Unidos University of Illinois at Chicago - Estados Unidos |
| 10 | BROOKS, WILLIAM KING | Hombre |
Universidad Técnica Federico Santa María - Chile
Instituto Milenio de Física Subatómica en la Frontera de Altas Energías - Chile Centro Científico Tecnológico de Valparaíso - Chile |
| 11 | Chen, Wei | - |
Lawrence Berkeley Natl Lab - Estados Unidos
Lawrence Berkeley National Laboratory - Estados Unidos |
| 12 | Wiedenmann, W. | Mujer |
Brookhaven Natl Lab - Estados Unidos
Brookhaven National Laboratory - Estados Unidos |
| 13 | Giacomini, Gabriele | - |
Brookhaven Natl Lab - Estados Unidos
Brookhaven National Laboratory - Estados Unidos |
| 14 | Tricoli, A. | Hombre |
Lawrence Berkeley Natl Lab - Estados Unidos
Lawrence Berkeley National Laboratory - Estados Unidos |
| 15 | Hayrapetyan, A. | - |
A Alikhanyan Natl Sci Lab - Armenia
Yerevan Physics Institute - Armenia |
| 16 | Lee, Hakseong | - |
Kyungpook Natl Univ - Corea del Sur
Kyungpook National University (KNU) - Corea del Sur |
| 17 | Koseyan, Ohannes Kamer | - |
UNIV IOWA - Estados Unidos
University of Iowa - Estados Unidos |
| 18 | Los, Sergey | - |
Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos |
| 19 | Nakamura, K. | Hombre |
High Energy Accelerator Res Org - Japón
High Energy Accelerator Organization - Japón |
| 20 | Kita, Sayuka | - |
UNIV TSUKUBA - Japón
University of Tsukuba - Japón |
| 21 | Imamura, Tomoka | - |
UNIV TSUKUBA - Japón
University of Tsukuba - Japón |
| 22 | PENA-OJEDA, CAMILA ISIDORA | Mujer |
Fermilab Natl Accelerator Lab - Estados Unidos
Fermi National Accelerator Laboratory - Estados Unidos |
| 23 | Xie, S. | - |
Fermilab Natl Accelerator Lab - Estados Unidos
CALTECH - Estados Unidos Fermi National Accelerator Laboratory - Estados Unidos California Institute of Technology - Estados Unidos |
| Fuente |
|---|
| U.S. Department of Energy |
| Brookhaven National Laboratory |
| Office of Science |
| Fermilab |
| U.S. Department of Energy (DOE) |
| Fermi Research Alliance, LLC (FRA) |
| Fermi Research Alliance, LLC |
| High Energy Physics |
| ANID PIA/APOYO |
| Agencia Nacional de Investigación y Desarrollo |
| University of Illinois at Chicago |
| Millennium Science Foundation |
| Science Committee of Republic of Armenia |
| ANID-Millennium Science Foundation |
| U.S. Department of Energy (DOE), Office of Science, Office of High Energy Physics Early Career Research program award |
| California Institute of Technology High Energy Physics |
| University of Illinois Chicago |
| Agradecimiento |
|---|
| We thank the Fermilab accelerator and FTBF personnel for the excellent performance of the accelerator and support of the test beam facility, in particular M. Kiburg, E. Niner, N. Pastika, E. Schmidt and T. Nebel. We also thank the SiDet department, in particular M. Jonas and H. Gonzalez, for preparing the readout board by mounting and wirebonding the LGAD sensors. Finally, we thank L. Uplegger for developing and maintaining the telescope tracking system. This document was prepared using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02- 07CH11359. This work was also supported by the U.S. Department of Energy (DOE), Office of Science, Office of High Energy Physics Early Career Research program award. This work was also supported by funding from University of Illinois Chicago under Contract DE-FG02- 94ER40865 with the U.S. Department of Energy (DOE), and Contract 418643 with Brookhaven National Laboratory. This work has also been supported by funding from the California Institute of Technology High Energy Physics under Contract DE-SC0011925 with the U.S. Department of Energy. This work was supported by the Science Committee of Republic of Armenia (Research projects No. 22AA-1C009 and 22rl-037). This work was supported by the Chilean ANID PIA/APOYO AFB230003 and ANID-Millennium Science Foundation-ICN2019_044. |
| We thank the Fermilab accelerator and FTBF personnel for the excellent performance of the accelerator and support of the test beam facility, in particular M. Kiburg, E. Niner, N. Pastika, E. Schmidt and T. Nebel. We also thank the SiDet department, in particular M. Jonas and H. Gonzalez, for preparing the readout board by mounting and wirebonding the LGAD sensors. Finally, we thank L. Uplegger for developing and maintaining the telescope tracking system. This document was prepared using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was also supported by the U.S. Department of Energy (DOE), Office of Science, Office of High Energy Physics Early Career Research program award. This work was also supported by funding from University of Illinois Chicago under Contract DE-FG02-94ER40865 with the U.S. Department of Energy (DOE), and Contract 418643 with Brookhaven National Laboratory. This work has also been supported by funding from the California Institute of Technology High Energy Physics under Contract DE-SC0011925 with the U.S. Department of Energy. This work was supported by the Science Committee of Republic of Armenia (Research projects No. 22AA-1C009 and 22rl-037). This work was supported by the Chilean ANID PIA/APOYO AFB230003 and ANID - Millennium Science Foundation - ICN2019_044. |
| We thank the Fermilab accelerator and FTBF personnel for the excellent performance of the accelerator and support of the test beam facility, in particular M. Kiburg, E. Niner, N. Pastika, E. Schmidt and T. Nebel. We also thank the SiDet department, in particular M. Jonas and H. Gonzalez, for preparing the readout board by mounting and wirebonding the LGAD sensors. Finally, we thank L. Uplegger for developing and maintaining the telescope tracking system. This document was prepared using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was also supported by the U.S. Department of Energy (DOE), Office of Science, Office of High Energy Physics Early Career Research program award. This work was also supported by funding from University of Illinois Chicago under Contract DE-FG02-94ER40865 with the U.S. Department of Energy (DOE), and Contract 418643 with Brookhaven National Laboratory. This work has also been supported by funding from the California Institute of Technology High Energy Physics under Contract DE-SC0011925 with the U.S. Department of Energy. This work was supported by the Science Committee of Republic of Armenia (Research projects No. 22AA-1C009 and 22rl-037). This work was supported by the Chilean ANID PIA/APOYO AFB230003 and ANID - Millennium Science Foundation - ICN2019_044. |