CMB constraints on cosmic strings and superstrings

We present the first complete Markov chain Monte Carlo analysis of cosmological models with evolving cosmic (super) string networks, using the unconnected segment model in the unequal-time correlator formalism. For ordinary cosmic string networks, we derive joint constraints on. cold dark matter (CDM) and string network parameters, namely the string tension G mu, the loop-chopping efficiency c(r), and the string wiggliness alpha. For cosmic superstrings, we obtain joint constraints on the fundamental string tension G mu(F), the string coupling g(s), the self-interaction coefficient c(s), and the volume of compact extra dimensions w. This constitutes the most comprehensive CMB analysis of Lambda CDM cosmology + strings to date. For ordinary cosmic string networks our updated constraint on the string tension, obtained using Planck2015 temperature and polarization data, is G mu < 1.1 x 10(-7) in relativistic units, while for cosmic superstrings our constraint on the fundamental string tension after marginalizing over g(s), c(s), and w is G mu(F) < 2.8 x 10(-8).