Automorphic representations of small nilpotent orbits, BPS conditions and new automorphic functions

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Event details

Date 26.11.2014
Hour 15:1516:15
Speaker Pierre Vanhove
Location
Category Conferences - Seminars
Maximally supersymmetric string theory compactified on (d—1)-dimensional torus (1<=d<=8) is invariant under U-duality groups G_d(Z)\ G_d/K_d  where G_d is the real split form of the simply laced lie group of rank d and K_d is the maximal compact subgroup. The connection between  string theory compactified on tori of various dimensions naturally leads  to the nested structure where lower rank G_d appear as parabolic subgroup of E8 which describes string theory in three dimensions.  Scattering amplitudes in string theory lead to automorphic functions under G_d(Z).  Conditions from string theory allow to derive the laplace equation satisfied by these functions, and for well choosen maximal parabolic subgroups the constant terms. As well, the support of the non-vanishing Fourier coefficients are determined by conditions from supersymmetry BPS conditions and correspond to nilpotent character variety orbits.  In this talk we will provide an explicit construction of these automorphic functions. We will show that  the wavefront sets of these automorphic forms are supported on only certain coadjoint nilpotent orbits: just the minimal and trivial orbits in the first non-trivial case, and just the next-to-minimal, minimal and trivial orbits in the second non-trivial case. Thus  the next-to-minimal representations occur automorphically for E6, E7, and E8, and hence the first two nontrivial low energy coefficients in scattering amplitudes can be thought of as exotic Theta-functions for these groups.  We will show that these automorphic representations are residues of Eisenstein series.  We will detail the arguments that the  automorphic representations attached to next nilpotent orbits in the Hasse diagram  are not Eisenstein series. For the case of SL(2,Z), we will provide a complete construction of this new automorphic function using Eisenstein automorphic distributions.  This is based on the work done with  Michael B. Green, Stephen D. Miller, Jorge G. Russo,[arXiv:1004.0163] Michael B. Green, Stephen D. Miller, [arXiv:1111.2983] Michael B. Green, Stephen D. Miller,[arXiv:1404.2192]

Practical information

  • Informed public
  • Free

Organizer

  • Natascha Fontana

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