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Cosmic Strings as the Source of Small-Scale Microwave Background Anisotropy
Levon Pogosian, S. -H. Henry Tye, Ira Wasserman +1
Cosmic string networks generate cosmological perturbations actively throughout the history of the universe. Thus, the string sourced anisotropy of the cosmic microwave background i…
Cosmic String Detection via Microlensing of Stars
David F. Chernoff, S. -H. Henry Tye
Cosmic superstrings are produced towards the end of the brane inflation. If the string tension is low enough, loops tend to be relatively long-lived. The resultant string network i…
Scaling of Multi-Tension Cosmic Superstring Networks
S. -H. Henry Tye, Ira Wasserman, Mark Wyman
Brane inflation in superstring theory ends when branes collide, initiating the hot big bang. Cosmic superstrings are produced during the brane collision. The cosmic superstrings pr…