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Cosmic strings formed during inflation are expected to be either diluted over super-Hubble distances, i.e., invisible today, or to have crossed our past light cone very recently.
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R. Jeannerot, J. Rocher and M. Sakellariadou, How generic is cosmic string formation in SUSY GUTs , Phys. Rev. D68
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J. Rocher and M. Sakellariadou, D-term inflation, cosmic strings, and consistency with cosmic microwave background measurement , Phys. Rev. Lett. 94
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C. Gordon, W. Hu, D. Huterer and T. M. Crawford, Spontaneous isotropy breaking: a mechanism for cmb multipole alignments , Phys.Rev. D72
2005
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M. Cruz, M. Tucci, E. Martinez-Gonzalez and P. Vielva, The non-gaussian cold spot in wmap: significance, morphology and foreground contribution , Mon.Not.Roy.Astron.Soc. 369
2006
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2010
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P. Peter and C. Ringeval, A Boltzmann treatment for the vorton excess problem , JCAP 1305
2013
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2014
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J. J. Blanco-Pillado, K. D. Olum and B. Shlaer, The number of cosmic string loops , Phys.Rev. D89
2014
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T. Vachaspati and A. Vilenkin, Formation and evolution of cosmic strings , Phys. Rev. D30
2045
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