Dynamical string tensions via a tension scalar induce de Sitter space on a brane and allow different-tension strings to serve as dark matter with hidden standard-model copies.
Guendelman, Escaping the Hagedorn Temperature in Cosmology and Warped Spaces with Dynamical Tension Strings, e-Print: 2105.02279 [hep-th]
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Constructing de Sitter space and Dark Matter with Dynamical Tension Strings
Dynamical string tensions via a tension scalar induce de Sitter space on a brane and allow different-tension strings to serve as dark matter with hidden standard-model copies.