Asymptotic Supergraviton States in Matrix Theory
Jan Plefka, Andrew Waldron (NIKHEF, Amsterdam)

TL;DR
This paper analyzes the asymptotic supergraviton states in Matrix theory, deriving an effective potential and discussing implications for the 11D supergraviton S matrix using a canonical quantum mechanical approach.
Contribution
It introduces a canonical framework to identify asymptotic supergraviton states and derives an effective potential expansion in inverse separation.
Findings
Identifies free supergraviton states in Matrix theory
Derives an effective potential for supergravitons
Discusses computation of the 11D supergraviton S matrix
Abstract
We study the Matrix theory from a purely canonical viewpoint. In particular, we identify free particle asymptotic states of the model corresponding to the 11D supergraviton multiplet along with the split of the matrix model Hamiltonian into a free and an interacting part. Elementary quantum mechanical perturbation theory then yields an effective potential for these particles as an expansion in their inverse separation. We discuss how our scheme can be used to compute the Matrix theory result for the 11D supergraviton S matrix and briefly comment on non-eikonal and longitudinal momentum exchange processes.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
