08–12 lug 2024
L'Aquila, Italy
Europe/Rome fuso orario

Development of SuperCDMS Silicon HVeV Detectors for Low Mass Dark Matter Searches and Studies of Low Energy Excess

10 lug 2024, 16:20
1O 10m
L'Aquila, Italy

L'Aquila, Italy

Plenary sessions: Palazzo dell’Emiciclo, Sala Ipogea Parallel sessions: Palazzo dell’Emiciclo, Sala Ipogea - GSSI Rectorate, Auditorium - GSSI, Sala Rossa (MLH)
Poster Light Dark Matter Poster session

Relatore

Kyle Kennard (Northwestern University)

Descrizione

The SuperCDMS-HVeV program has previously demonstrated competitive
sensitivities to electron-recoil [1] and nuclear-recoil [2] dark matter in the sub-
GeV mass range using voltage biased silicon crystals equipped with TES calorime-
ters. HVeV detectors have achieved excellent energy resolution through the
application of an electric field to the crystal that enables amplification via the
Neganov-Trofimov-Luke effect, allowing for eV-scale thresholds and enabling
low mass dark matter searches. However, recent direct-detection searches for
low mass dark matter including those from SuperCDMS [3], DAMIC [4], SEN-
SEI [5], CRESST [6], and EDELWEISS [7] have encountered an excess of events
at low-energy with unknown origin. As such, understanding the origin of these
events is crucial to the study dark matter. HVeV detectors are well-suited for
studies of this excess due to their excellent resolutions. New developments on
the original HVeV design seek to test hypotheses regarding the origin of low
energy events. In this poster, I will show two new iterations of HVeV detec-
tors each designed to test a different hypothesis. In the first new iteration of
HVeV detectors, an insulating layer is deposited between the crystal bulk and
the phonon sensors to reduce signal from the diffusion of charge carriers through
the crystal-sensor interface. The second iteration focuses on improving the po-
sition resolution of the HVeV detector in order to isolate stress-induced events
near the edge of the detector caused by mechanical clamping during operation.
References
[1] R. Agnese et al. “First Dark Matter Constraints from a SuperCDMS Single-
Charge Sensitive Detector”. In: Physical Review Letters 121.5 (Aug. 2018).
[2] M. F. Albakry et al. “Investigating the sources of low-energy events in a
SuperCDMS-HVeV detector”. In: Physical Review D 105.11 (June 2022).
[3] R. Agnese et al. “Low-mass dark matter search with CDMSlite”. In: Phys-
ical Review D 97.2 (Jan. 2018).
1
[4] I. Arnquist et al. “First Constraints from DAMIC-M on Sub-GeV Dark-
Matter Particles Interacting with Electrons”. In: Physical Review Letters
130.17 (Apr. 2023).
[5] Orr Abramoff et al. “SENSEI: Direct-Detection Constraints on Sub-GeV
Dark Matter from a Shallow Underground Run Using a Prototype Skipper
CCD”. In: Physical Review Letters 122.16 (Apr. 2019).
[6] A. H. Abdelhameed et al. “First results from the CRESST-III low-mass
dark matter program”. In: Physical Review D 100.10 (Nov. 2019).
[7] E. Armengaud et al. “Searching for low-mass dark matter particles with a
massive Ge bolometer operated above ground”. In: Physical Review D 99.8
(Apr. 2019).

Autore principale

Kyle Kennard (Northwestern University)

Coautore

Alejandro Rodriguez (Northwestern University) Benjamin Schmidt (KIT) Prof. Enectali Figueroa-Feliciano (Northwestern University) Grace Bratrud (Northwestern University) Lidabel Ovalle-Mateo (Northwestern University) Ran Chen (Northwestern University) Valentina Novati (LPSC-CNRS)

Materiali di presentazione

Non sono ancora presenti materiali