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

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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Publication Details

Journal
Scientific Reports
Published
2026-08-24
DOI
https://doi.org/10.1038/s41598-026-68157-7
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
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article

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

Pragati Pradhan, P. B. Jones, Douglas Singleton
Scientific Reports
Pulsars and Gravitational Waves Research
article

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

Pragati Pradhan, P. B. Jones, Douglas Singleton
article en

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.

Scientific Reports
California State University, Fresno (US), Embry–Riddle Aeronautical University (US)
Openalex Percentile: Top 10%
Pulsars and Gravitational Waves Research
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