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PreprintCC BY 4.0arXiv

Signatures in the local interstellar medium of electromagnetic radiation produced by neutron star gravitational waves

Abstract

The Voyager spacecraft have been detecting plasma oscillations of a few kHz for over 40 years. However, there is still no widely accepted hypothesis for the astrophysical source of the oscillations. Having entered the local interstellar medium, these detections have persisted, adding to the challenge of identifying the astrophysical source. Neutron stars were one of the earliest hypothesized candidates of the electromagnetic radiation responsible for the detected plasma oscillations, but no theoretical mechanism could be identified to explain the frequency of the oscillations. We explore the recently developed theory of co-production of electromagnetic radiation in gravitational wave backgrounds as a possible source of these low-frequency oscillations and investigate whether neutron stars could be the astrophysical source.

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BibTeX
@misc{jones2026signatures,
  title = {{Signatures in the local interstellar medium of electromagnetic radiation produced by neutron star gravitational waves}},
  author = {Preston Jones and Pragati Pradhan and Douglas Singleton},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.23865},
  eprint = {2609.23865},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.23865},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Signatures in the local interstellar medium of electromagnetic radiation produced by neutron star gravitational waves
AU  - Preston Jones
AU  - Pragati Pradhan
AU  - Douglas Singleton
PY  - 2026
DA  - 2026/09/20
PB  - arXiv
DO  - 10.48550/arxiv.2609.23865
UR  - https://arxiv.org/abs/2609.23865
AB  - The Voyager spacecraft have been detecting plasma oscillations of a few kHz for over 40 years. However, there is still no widely accepted hypothesis for the astrophysical source of the oscillations. Having entered the local interstellar medium, these detections have persisted, adding to the challenge of identifying the astrophysical source. Neutron stars were one of the earliest hypothesized candidates of the electromagnetic radiation responsible for the detected plasma oscillations, but no theoretical mechanism could be identified to explain the frequency of the oscillations. We explore the recently developed theory of co-production of electromagnetic radiation in gravitational wave backgrounds as a possible source of these low-frequency oscillations and investigate whether neutron stars could be the astrophysical source.
ER  -