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Cosmic string loops in the expanding universe

3 Pith papers cite this work, alongside 133 external citations. Polarity classification is still indexing.

3 Pith papers citing it
133 external citations · Pith
abstract

We study the production of loops in the cosmic string network in the expanding background by means of a numerical simulation exact in the flat-spacetime limit and first-order in the expansion rate. We find an initial regime characterized by production of small loops at the scale of the initial correlation length, but later we see the emergence of a scaling regime of loop production. This qualitatively agrees with earlier expectations derived from the results of flat-spacetime simulations. In the final scaling regime we find that the characteristic length of loops scales as $\sim 0.1 t$ in both radiation and matter eras.

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years

2026 2 2020 1

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UNVERDICTED 3

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representative citing papers

The landscape of QCD axion models

hep-ph · 2020-03-02 · unverdicted · novelty 2.0

Review classifies QCD axion models extending the standard mass-coupling window and updates bounds from cosmology, astrophysics, and experiments.

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Showing 3 of 3 citing papers.