The Belle II Silicon Vertex Detector: Performance and Running Experience

S. Bacher, K. Adamczyk,H. Aihara,Tariq Aziz,Seema Bahinipati, G. Batignani,J. Baudot,Prafulla Kumar Behera,S. Bettarini, T. Bilka, A. Bozek, F. Buchsteiner,G. Casarosa, D. Červenkov,Yonghu Chen, L. Corona, T. Czank,S. Das,N. Dash,G. de Marino,Z. Doležal, G. Dujany, F. Forti,Markus Friedl, E. Ganiev, B. Gobbo,S. Halder, K. Hara,S. Hazra, T. Higuchi,Christian Irmler,A. Ishikawa,H. B. Jeon,Ya-Qiu Jin,C. Joo, M. Kaleta,A. B. Kaliyar,Jakub Kandra,K. H. Kang, P. Kapusta,Peter Kodys, T. Kohriki,Mukesh Kumar,Rajesh Kumar,Peter Kvasnicka,C. La Licata,K. Lalwani,Shih-Chang Lee, Y. B. Li, J. Libby,Surajit Maity, S. N. Mayekar,G. B. Mohanty, J.A.M. Grimaldo,T. Morii, K. Nakamura,Z. Natkaniec, Y. Onuki, W. Ostrowicz,A. Paladino,E. Paoloni,H. Park,K. K. Rao, I. Ripp-Baudot, G. Rizzo,N. Rout,Doyen Sahoo, C. Schwanda, J. Suzuki,Satoshi Tanaka, H. Tanigawa,R. Thalmeier, T. Tsuboyama, Y. Uematsu, O. Verbycka, L. Vitale, K. Wan,J. C. Webb, J. Wiechczynski, H. Yin,L. Zani, T. Zhang

Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020)(2021)

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摘要
In spring 2019 the fully equipped Belle II experiment started data taking at the energy of the Y(4S) resonance. The new vertex detector (VXD) consists of two inner layers of DEPFET pixels (PXD) and four outer layers of double-sided silicon strip detectors (SVD). It plays a crucial role in recording high-quality data in the new high-luminosity environment of the SuperKEKB collider, characterized by severe beam backgrounds. The SVD was operated reliably during the 2019 physics run, showing high stability of the noise levels and calibration parameters. The SVD performance, measured with first data, showed excellent hit and tracking efficiencies, high signal-to-noise ratio, and cluster energy distribution in fair agreement with the expectations. Detailed studies of the good spatial resolution achieved will be shown. The excellent hit-time resolution has also been measured, which will be exploited for background rejection in the coming years of running at higher luminosity.
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