Potential of Radio Telescopes as High-Frequency Gravitational Wave Detectors

Link:
Autor/in:
Erscheinungsjahr:
2021
Medientyp:
Text
Schlagworte:
  • Astrophysics - Cosmology and Nongalactic Astrophysics
  • General Relativity and Quantum Cosmology
  • High Energy Physics - Phenomenology
Beschreibung:

  • In the presence of magnetic fields, gravitational waves are converted into photons and vice versa. We demonstrate that this conversion leads to a distortion of the cosmic microwave background (CMB), which can serve as a detector for MHz to GHz gravitational wave sources active before reionization. The measurements of the radio telescope EDGES can be cast as a bound on the gravitational wave amplitude, hc-21(10-12) at 78 MHz, for the strongest (weakest) cosmic magnetic fields allowed by current astrophysical and cosmological constraints. Similarly, the results of ARCADE 2 imply hc-24(10-14) at 3-30 GHz. For the strongest magnetic fields, these constraints exceed current laboratory constraints by about 7 orders of magnitude. Future advances in 21 cm astronomy may conceivably push these bounds below the sensitivity of cosmological constraints on the total energy density of gravitational waves.
Lizenz:
  • info:eu-repo/semantics/openAccess
Quellsystem:
Forschungsinformationssystem der UHH

Interne Metadaten
Quelldatensatz
oai:www.edit.fis.uni-hamburg.de:publications/5c2f61da-1911-4f8e-8543-8a90d956396e