Holographic inflation is argued to imprint exact large-angle symmetries on the cosmic microwave background, most notably a vanishing temperature correlation at 90 degrees of angular separation.
Introduction to Superstring Theory
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abstract
These four lectures, addressed to an audience of graduate students in experimental high energy physics, survey some of the basic concepts in string theory. The purpose is to convey a general sense of what string theory is and what it has achieved. Since the characteristic scale of string theory is expected to be close to the Planck scale, the structure of strings probably cannot be probed directly in accelerator experiments. The most accessible experimental implication of superstring theory is supersymmetry at or below the TeV scale.
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Pattern of perturbations from a coherent quantum inflationary horizon
Holographic inflation is argued to imprint exact large-angle symmetries on the cosmic microwave background, most notably a vanishing temperature correlation at 90 degrees of angular separation.