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Particle and Astroparticle Physics Colloquium Hamburg
Gravitational Waves from the Big Bang - Inflation in String Theory after BICEP2
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Europe/Berlin
Auditorium (DESY Hamburg)
Auditorium
DESY Hamburg
Description
BICEP2 from Antarctica has given us the first clear evidence for primordial gravitational waves causing B-mode polarization at degree angular scales l < 100. If interpreted in the context of inflation, their signal corresponds to a tensor-to-scalar ratio 
, which disfavors r<0.01 at about 5σ. We will discuss the implications of this result for models of single-field slow-roll inflation. Due to the Lyth bound, the new data represent strong evidence against virtually all small-field models of inflation. We will discuss the need for protective symmetries such as shift symmetries in large-field inflation models which are now favored, and review the situation of string inflation and its large-field version of (axion) monodromy.
, which disfavors r<0.01 at about 5σ. We will discuss the implications of this result for models of single-field slow-roll inflation. Due to the Lyth bound, the new data represent strong evidence against virtually all small-field models of inflation. We will discuss the need for protective symmetries such as shift symmetries in large-field inflation models which are now favored, and review the situation of string inflation and its large-field version of (axion) monodromy.