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2–6 Sept 2019
Europe/Zurich timezone

Probing higher spin fields from galaxy alignment

Not scheduled
25m

Description

ㅤNon-linear effects during inflation can generate primordial non-Gaussianities(PNG). Arkani-Hamed & Maldacena showed that an interaction between the inflaton and higher spin (s2) fields, which may be predicted in string theory, can generate angular dependent PNG. Specifically, the search of the imprint of spin (s4) fields can give us the evidences of string theory. As was argued by Schmidt et al., the anisotropy generated from spin-2 PNG can be explored by galaxy alignments. By extending this method, we examine the detectability of the imprint of spin-4 fields by galaxy alignments. I will state the relation between the higher moments with galaxy alignments and the PNG with higher spins.

Authors

Fabian Schmidt Kazuyuki Akitsu (Kavli IPMU) Yuko Urakawa

Co-author

Kiyotomo Ichiki (Nagoya University)

Presentation materials

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