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Detectability of inflation-produced gravitational waves

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arxiv astro-ph/9607066 v1 pith:U42FEAMO submitted 1996-07-12 astro-ph gr-qc

Detectability of inflation-produced gravitational waves

classification astro-ph gr-qc
keywords wavesgravitationalinflationanisotropybackgroundcosmiccrucialdetect
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Detection of the gravitational waves excited during inflation as quantum mechanical fluctuations is a key test of inflation and crucial to learning about the specifics of the inflationary model. We discuss the potential of Cosmic Background Radiation (CBR) anisotropy and polarization and of laser interferometers such as LIGO, VIRGO/GEO and LISA to detect these gravity waves.

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Cited by 2 Pith papers

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

  1. Directional Search for Persistent Gravitational Waves: Results from the First Part of LIGO-Virgo-KAGRA's Fourth Observing Run

    gr-qc 2025-10 conditional novelty 6.0

    An 8.3-year LIGO–Virgo–KAGRA search for persistent, direction-dependent gravitational waves finds no signal and yields the most restrictive upper limits to date on anisotropic backgrounds and targeted sources.

  2. High Frequency Spectrum of Primordial Gravitational Waves

    hep-ph 2026-01 unverdicted novelty 5.0

    High-frequency primordial gravitational waves extend to higher frequencies due to post-inflation inflaton dynamics, and their detailed spectrum shape can distinguish inflation models.