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Cosmic String Structure at the Gravitational Radiation Scale
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abstract
We use our model of the small scale structure on cosmic strings to develop further the result of Siemens, Olum, and Vilenkin that the gravitational radiation length scale on cosmic strings is smaller than the previously assumed $\Gamma G\mu t$. We discuss some of the properties of cosmic string loops at this cutoff scale, and we argue that recent network simulations point to two populations of cosmic string loops, one near the horizon scale and one near the gravitational radiation cutoff.
Forward citations
Cited by 3 Pith papers
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Probing the gravitational wave background from cosmic strings with LISA
LISA is projected to probe cosmic string tensions G mu down to about 1e-17 and to measure spectral features from early-universe physics.
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Backreaction on an infinite helical cosmic string
For a small-amplitude helical breather cosmic string, gravitational backreaction produces energy loss matching Sakellariadou's power and a rotation of the generators that advances the oscillation phase.
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Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison
As provided, the manuscript body (random lasing) does not correspond to the abstract (cosmic string gravitational wave backgrounds at LISA), leaving the abstract's quantitative claims unsupported by any accessible text.
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