Probing Gravitational Dark Matter with Ultra-high Frequency Gravitational Waves

Probing Gravitational Dark Matter with Ultra-high Frequency Gravitational Waves
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Summary

The study explores the connection between gravitational dark matter and ultra-high frequency gravitational waves, proposing a novel method to probe dark matter properties using gravitational wave measurements.

Highlights

  • Gravitational dark matter interacts purely through gravity, making it challenging to detect directly.
  • The production of dark matter and gravitational waves are related, offering a new avenue for probing dark matter.
  • The study focuses on a minimal scenario where dark matter is generated through the annihilation of standard model particles in the thermal plasma.
  • The gravitational wave spectrum is related to the mass and spin of dark matter particles.
  • Future gravitational wave experiments in the ultra-high frequency regime could shed light on dark matter properties.
  • The study assumes a regime where the temperature is below the Planck mass, ensuring gravitons do not thermalize.
  • The results demonstrate a connection between the amount of gravitational waves and pure gravitational dark matter due to their cogenesis in the early Universe.

Key Insights

  • The study reveals a tight connection between the amplitude of thermal gravitational waves and the properties of pure gravitational dark matter, offering a new method to probe dark matter using gravitational wave measurements.
  • The production of dark matter and gravitational waves share the same source, enabling the use of gravitational waves to probe dark matter properties, particularly its mass and spin.
  • The analysis assumes a minimal setup where dark matter interacts purely through gravity, and its production is related to the annihilation of standard model particles in the thermal plasma.
  • The gravitational wave spectrum is found to be related to the mass and spin of dark matter particles, providing a potential avenue for probing these properties using future gravitational wave experiments.
  • The study highlights the importance of considering the reheating phase in the early Universe, which can introduce corrections to the gravitational wave spectrum and affect the results.
  • The findings suggest that the measurement of gravitational wave amplitude in the ultra-high frequency regime could provide probes to the mass and spin of pure gravitational dark matter.
  • The study demonstrates the potential of gravitational wave astronomy to shed light on the nature of dark matter, particularly in scenarios where dark matter interacts purely through gravity.

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Citation

Xu, Y. (2024). Probing Gravitational Dark Matter with Ultra-high Frequency Gravitational Waves (Version 1). arXiv. https://doi.org/10.48550/ARXIV.2412.21137

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