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Massachusetts Institute of Technology

The Search for High-Frequency Gravitational Waves with a Modified Axion Detector

Abstract

dc:description.abstract

ABRACADABRA-10cm has had great success as a lumped-element axion dark matter pathfinder experiment, with two published axion searches and an extensive background investigation. Now, using the electrodynamics of gravitational waves and a simple change of pickup structures, we are using the ABRACADABRA detector to search for high-frequency gravitational waves in the kHz to MHz range. These higher frequencies may indicate signs of in-spiraling primordial black holes, or other beyond the standard model phenomena. With careful calibration used to distinguish between the two signals, we introduce the first simultaneous search for both axions and gravitational waves using a lumped-element axion detector. In this thesis I will present on the high-frequency cryogenic ABRACADABRA-10cm detector, the background investigations of the detector and the design and first data from the ABRACADABRA-10cm high-frequency gravitational wave search.

Degree

thesis:*
Name thesis:degree_name
Doctoral
Department dc:contributor.department
Massachusetts Institute of Technology. Department of Physics
Grantor dc:publisher
Massachusetts Institute of Technology
Year dc:date.issued
2024

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Pappas, Kaliroë Mabelle West
Advisor dc:contributor.advisor
  • Winslow, Lindley

Rights

dc:rights
Statement dc:rights
  • In Copyright - Educational Use Permitted
  • Copyright retained by author(s)

Identifiers

dc:identifier.*
Handle dc:identifier.uri
https://hdl.handle.net/1721.1/157593
OAI identifier oai:identifier
oai:dspace.mit.edu:1721.1/157593

Chain of custody

source
Harvested from
MIT
Base URL
dspace.mit.edu/oai/request
Last updated
2026-07-22
Source record
OAI-PMH GetRecord
related terms
citation

Pappas, Kaliroë Mabelle West. The Search for High-Frequency Gravitational Waves with a Modified Axion Detector. Massachusetts Institute of Technology, 2024. https://hdl.handle.net/1721.1/157593