Cosmological and astrophysical constraints on superconducting cosmic strings
arXiv:1212.6687 · doi:10.1088/1475-7516/2013/07/012
Abstract
We investigate the cosmological and astrophysical constraints on superconducting cosmic strings (SCSs). SCS loops emit strong bursts of electromagnetic waves, which might affect various cosmological and astrophysical observations. We take into account the effect on the CMB anisotropy, CMB blackbody spectrum, BBN, observational implications on radio wave burst and X-ray or gamma-ray events, and stochastic gravitational wave background measured by pulsar timing experiments. We then derive constraints on the parameters of SCS from current observations and estimate prospects for detecting SCS signatures in on-going observations. As a result, we find that these constraints exclude broad parameter regions, and also that on-going radio wave observations can probe large parameter space.
31 pages, 9 figures
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- Inflation, String Theory and Cosmology
- Pulsar-timing measurement of the circular polarization of the stochastic gravitational-wave background
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- Massive black holes at high redshifts from superconducting cosmic strings
- Superconducting cosmic strings as sources of cosmological fast radio bursts
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- Gravitating superconducting solitons in the (3+1)-dimensional Einstein gauged non-linear sigma-model
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- Can Superconducting Cosmic Strings Piercing Seed Black Holes Generate Supermassive Black Holes in the Early Universe?
- Dynamical simulations of colliding superconducting strings
- Lumpy cosmic strings