Place: MPA Lecture Hall
Session 2: Observational Prospects
10:00-10:25 Expectation for Planck and beyond, Ben Wandelt [20+5]
10:25-10:50 Primordial non-Gaussianity and large-scale structure, Licia Verde [20+5]
10:50-11:15 Signatures of primordial non-Gaussianity in CMB and LSS, Kendrick Smith [20+5]
11:15-11:40 Break [25]
11:40-12:30 Discussion Session 2 [50] Moderator: Eiichiro Komatsu
- What do the current data tell us?
- How comfortable are we with the current results?
- What would be the expectations for the future?
- CMB bispectrum and scale-dependent bias: what else? (Galaxy bispectrum, etc?)
SUMMARY OF DISCUSSION SESSION 2: available here
12:30-14:00 Lunch [90]
Special talk: Non-Gaussianity measurement with Information Field Theory, Torsten Enßlin
Session 3: Multiple field
14:00-14:25 Curvaton, David Wands [20+5]
14:25-14:50 Distinctive non-Gaussianity from vector fields coupled to inflaton, Marco Peloso [20+5]
14:50-15:15 CMB bispectrum from higher-spin non-Gaussianities, Maresuke Shiraishi [20+5]
15:15-15:35 Poster Talks [2x10=20]
- "Signals of primordial magnetic fields in the CMB," Kerstin Kunze
- "Practical guide to compute fNL outside the horizon," Yuki Watanabe
- "Beyond the delta-N formalism," Atsushi Naruko
- "Non-Gaussian halo statistics from excursion sets," Marcello Musso
- "Scale-dependent bias with higher-order primordial non-Gaussianity - Use of the integrated perturbation theory," Shuichiro Yokoyama
- "The CMB bispectrum from non-linear dynamics," Guido Walter Pettinari
- "Fast estimation of gravitational and primordial bispectra in large-scale structures and a simple model for small scales," Marcel Schmittfull
- "A modal approach to the numerical calculation of primordial non-Gaussianities," Sébastien Renaux-Petel
- "Can Bianchi- and fNL-models explain the phase correlations in CMB data?" Heike Modest
- "Will primordial local-type non-Gaussianity change halo shapes?" Dalong Cheng
15:35-16:05 Break [30]
16:05-16:30 Non-Gaussianity and the adiabatic limit, Jeol Meyers [20+5]
16:30-16:55 Multifield reheating and the fate of primordial observables, Christian Byrnes [20+5]