The Pentadimensional Tracking Space Detector project, R&D for space-borne LGAD Si-microstrip tracking detectors

21 Nov 2025, 09:20
20m
2F, Activities Center (Academia Sinica)

2F, Activities Center

Academia Sinica

128 Section 2, Academia Road, Nankang, Taipei 115201, Taiwan
ORAL New Ideas and Future Applications 8. New Ideas and Future Applications

Speaker

Mattia Barbanera (INFN Perugia)

Description

In the context of the Pentadimensional Tracking Space Detector project (PTSD), we are currently developing a demonstrator to increase the Technological Readiness Level of LGAD Si-microstrip tracking detectors for applications in space-borne instruments.

Low Gain Avalanche Diodes (LGAD) is a consolidated technology developed for particle detectors at colliders which allows for simultaneous and accurate time (<100 ps) and position (~ 10 μm) resolutions with segmented Si sensors. It is a candidate technology that could enable for the first time 5D tracking (position, charge, and time) in space using LGAD Si-microstrip tracking systems. The intrinsic gain of LGAD sensors may also allow to decrease the sensor thickness while achieving signal yields similar to those of Si-microstrips currently operated in Space.

In this contribution we discuss the ongoing activities for the design, development, and test of a breadboard laboratory model for verification of requirements, functionalities and space qualification of LGAD Si-microstrip devices for 5D tracking in space. We also present the study performed at the Italian Space Agency - Concurrent Engineering Facility (ASI-CEF) addressing the design of a LGAD-tracker flight-demonstrator to be housed in a 6U-XL CubeSat platform. The possible, successful operations in space of the demonstrator could confirm the TRL of Si-microstrip LGAD-trackers to 9, making it a viable and available technology for future mission opportunities for charged cosmic-ray and γ-ray instruments.

Authors

Dr Matteo Duranti (National Institute of Nuclear Physics (INFN, IT)) Mattia Barbanera (INFN Perugia) Dr Mattia Barbanera (National Institute of Nuclear Physics (INFN, IT)) Valerio Vagelli (Italian Space Agency (ASI, IT))

Co-authors

Dr Alberto Oliva (National Institute of Nuclear Physics (INFN, IT)) Dr Elisabetta Cavazzuti (Italian Space Agency (ASI, IT)) Dr Emilie Savin (National Institute of Nuclear Physics (INFN, IT)) Dr Jiayu Hu (National Institute of Nuclear Physics (INFN, IT)) Dr Marco Miliucci (Italian Space Agency (ASI, IT)) Dr Maria Barbara Negri (Italian Space Agency (ASI, IT)) Dr Maria Ionica (National Institute of Nuclear Physics (INFN, IT)) Martina Savinelli (National Institute of Nuclear Physics (INFN, IT), University of Perugia (IT)) Dr Matteo Mergè (Italian Space Agency (ASI, IT)) Dr Valerio Formato (National Institute of Nuclear Physics (INFN, IT))

Presentation materials