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Detecting parity violation from axion inflation with third generation detectors
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Detecting parity violation from axion inflation with third generation detectors
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A gravitational wave background is expected to emerge from the superposition of numerous gravitational wave sources of both astrophysical and cosmological origin. A number of cosmological models can have a parity violation, resulting in the generation of circularly polarised gravitational waves. We investigate the constraining power of third generation Einstein Telescope and Cosmic Explorer detectors, for a gravitational wave background generated by early universe axion inflation.
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Cited by 1 Pith paper
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A battle of designs: triangular vs. L-shaped detectors and parity violation in the gravitational-wave background
L-shaped Einstein Telescope designs outperform triangular designs for detecting a parity-violating gravitational-wave background, and ET alone cannot do it under current observational constraints.
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