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Results for pixel and strip centimeter-scale AC-LGAD sensors with a 120 GeV proton beam
Indexado
WoS WOS:001410310700001
Scopus SCOPUS_ID:85215432941
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


Abstract



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.

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Disciplinas de Investigación



WOS
Physics, Particles & Fields
Instruments & Instrumentation
Spectroscopy
Nuclear Science & Technology
Physics, Nuclear
Scopus
Nuclear And High Energy Physics
Instrumentation
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



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

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Financiamiento



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

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



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.

Muestra la fuente de financiamiento declarada en la publicación.