pith. sign in

arxiv: 2011.12414 · v2 · pith:XQWJ5D7Jnew · submitted 2020-11-24 · 🌀 gr-qc · astro-ph.CO· astro-ph.IM· hep-ex· hep-ph

Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies

classification 🌀 gr-qc astro-ph.COastro-ph.IMhep-exhep-ph
keywords gravitationalwavechallengesexpectedfrequencieshigh-frequencyligoopportunities
0
0 comments X
read the original abstract

The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges and gains expected in gravitational wave searches at frequencies above the LIGO/Virgo band, with a particular focus on Ultra High-Frequency Gravitational Waves (UHF-GWs), covering the MHz to GHz range. The absence of known astrophysical sources in this frequency range provides a unique opportunity to discover physics beyond the Standard Model operating both in the early and late Universe, and we highlight some of the most promising gravitational sources. We review several detector concepts which have been proposed to take up this challenge, and compare their expected sensitivity with the signal strength predicted in various models. This report is the summary of the workshop "Challenges and opportunities of high-frequency gravitational wave detection" held at ICTP Trieste, Italy in October 2019, that set up the stage for the recently launched Ultra-High-Frequency Gravitational Wave (UHF-GW) initiative.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 20 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Search for High-Frequency Gravitational Waves via Geomagnetic Conversion with Radio Telescopes

    gr-qc 2026-06 unverdicted novelty 7.0

    First search for high-frequency gravitational waves via inverse Gertsenshtein conversion in Earth's magnetic field with VLA and ALMA sets new upper limits h_c ≲ 10^{-18} from 1 GHz to 1 THz.

  2. Bidirectional Internal Squeezing for Gravitational-Wave Detectors

    gr-qc 2026-05 conditional novelty 7.0

    Bidirectional internal squeezing using opposing optical parametric amplifiers saturates quantum noise lower bounds from internal dissipation and renders high-frequency signal-referred noise independent of arm and sign...

  3. Gravitational Gertsenshtein-Zeldovich mechanism for the Association between GW190425 and FRB 20190425A

    astro-ph.HE 2026-04 unverdicted novelty 7.0

    Kilohertz gravitational waves from a neutron star merger convert to electromagnetic waves near a magnetar via the Gertsenshtein-Zeldovich effect and are inverse Compton scattered to gigahertz frequencies to explain th...

  4. Quantum production of gravitational waves after inflation

    gr-qc 2025-07 unverdicted novelty 7.0

    Scalar metric perturbations after inflation break conformal invariance and induce quantum production of gravitons, generating a GW spectrum that peaks near GHz frequencies for standard primordial scalar power spectra.

  5. Gravitational Wave-Induced Freeze-In of Fermionic Dark Matter

    hep-ph 2024-05 unverdicted novelty 7.0

    Stochastic gravitational waves induce 1-loop freeze-in production of fermionic dark matter via in-in formalism, potentially explaining the observed abundance more efficiently than conventional mechanisms.

  6. Calling the Brane Next Door: The Kaluza-Klein Tower as a Gravitational Information Channel

    hep-th 2026-06 unverdicted novelty 6.0

    The Kaluza-Klein tower functions as a MIMO gravitational communication channel between branes, with modes acting as subchannels for encoding information via occupation, phases, and timing.

  7. A Unified Bogoliubov Approach to Primordial Gravitational Waves: From Inflation to Reheating

    hep-ph 2026-04 unverdicted novelty 6.0

    An improved Bogoliubov numerical method computes the full primordial GW spectrum from inflation to reheating and shows that inflaton anharmonicity imprints distinctive features at high frequencies.

  8. Polarization Formalism for Photon-Gravitational Wave Mixing Around Magnetars

    hep-ph 2026-06 unverdicted novelty 5.0

    Polarization formalism applied to Gertsenshtein mixing in magnetars yields bounds showing negligible stochastic GW background from magnetar EM emissions.

  9. Radio Emission from High-Frequency Gravitational Wave Point Sources

    hep-ph 2026-06 unverdicted novelty 5.0

    Radio telescopes outperform other experiments at detecting high-frequency gravitational waves from primordial black hole mergers and boson clouds through conversion to radio signals in magnetic fields.

  10. Gravitational waves from cosmic strings with friction: analytical approximations and parameter space

    astro-ph.CO 2026-05 unverdicted novelty 5.0

    Analytical approximations for the ultra-high-frequency GW peak sourced by friction-era cosmic string loops, with expanded observable parameter space.

  11. Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition

    hep-ph 2026-04 unverdicted novelty 5.0

    ALP-assisted first-order phase transitions can explain observed intergalactic magnetic fields and produce detectable gravitational waves, linking cosmology with particle physics searches.

  12. Beyond the Standard Model of Cosmology: Testing new paradigms with a Multiprobe Exploration of the Dark Universe

    astro-ph.CO 2026-04 unverdicted novelty 5.0

    Proposes primordial black holes from modified small-scale fluctuations and entropic acceleration in expanding spacetime as explanations for dark matter and dark energy.

  13. Gravitational Waves from Matter Perturbations of Spectator Scalar Fields

    hep-ph 2026-04 unverdicted novelty 5.0

    A spectator scalar field with strong portal coupling to the inflaton sources a stochastic gravitational wave background reaching Ω_GW h² ∼ 10^{-11} at frequencies 10^7-10^8 Hz for benchmark parameters σ/λ ≃ 10^4 and T...

  14. High-frequency gravitational wave transients from superradiance

    gr-qc 2026-04 unverdicted novelty 5.0

    Ultralight boson clouds around primordial black holes emit high-frequency gravitational wave transients via superradiance and binary-driven transitions, but the signals fall below current detector sensitivity at plaus...

  15. Probing Bose-enhanced Inflaton Decay with Gravitational Waves

    hep-ph 2026-01 unverdicted novelty 5.0

    Bose enhancement from a transient condensate of inflaton decay products dramatically increases decay efficiency and amplifies stochastic gravitational wave production to potentially observable levels.

  16. Equation of state during (p)reheating with trilinear interactions

    astro-ph.CO 2025-07 unverdicted novelty 5.0

    Lattice simulations show that the post-inflationary equation of state with trilinear interactions returns to zero after an initial deviation, substantially lowering stochastic gravitational wave amplitudes relative to...

  17. Relic gravitational waves from primordial gravitational collapses

    gr-qc 2025-04 unverdicted novelty 5.0

    Sound shell collisions from Hubble-scale primordial density perturbations generate a stochastic GW background whose peak frequency and amplitude scale with the Hubble horizon and shell abundance.

  18. Response of interferometers to the vacuum of quantum gravity

    hep-th 2024-09 unverdicted novelty 5.0

    Standard low-energy quantum gravity via effective graviton QFT predicts interferometer length variations of order the Planck length (~10^{-35} m), with no divergences indicating breakdown.

  19. The read-out electronics for the FLASH experiment

    physics.ins-det 2026-03 unverdicted novelty 4.0

    FLASH's read-out system uses MSAs as low-noise amplifiers and SDR techniques to capture and process ultra-weak signals from dark matter or high-frequency gravitational waves in the 117-360 MHz range.

  20. Gravitational waves production during preheating within GB gravity with monomial coupling

    gr-qc 2026-04 unverdicted novelty 3.0

    In Gauss-Bonnet inflation with monomial potential and coupling, gravitational waves from preheating produce a present-day energy density spectrum consistent with Planck constraints when the coupling strength, equation...