The Effect of Boundaries in One-Loop Quantum Cosmology
Peter D. D'Eath, Giampiero Esposito

TL;DR
This paper investigates boundary conditions in one-loop quantum cosmology with supersymmetry, calculating zeta-function values for various fields and showing supersymmetry's divergence at one-loop level when boundaries are present.
Contribution
It provides explicit zeta-function calculations for different boundary conditions in supersymmetric quantum cosmology, highlighting the divergence of supersymmetry at one-loop with boundaries.
Findings
Zeta(0) values computed for multiple fields under specific boundary conditions.
Supersymmetry does not cancel divergences at one-loop in the presence of boundaries.
Boundary conditions significantly influence quantum amplitude calculations.
Abstract
The problem of boundary conditions in a supersymmetric theory of quantum cosmology is studied, with application to the one-loop prefactor in the quantum amplitude. Our background cosmological model is flat Euclidean space bounded by a three-sphere, and our calculations are based on the generalized Riemann zeta-function. One possible set of supersymmetric local boundary conditions involves field strengths for spins 1, 3/2 and 2, the undifferentiated spin-1/2 field, and a mixture of Dirichlet and Neumann conditions for spin 0. In this case the results we can obtain are: zeta(0)=7/45 for a complex scalar field, zeta(0)=11/360 for spin 1/2, zeta(0)= -77/180 (magnetic) and 13/180 (electric) for spin 1, and zeta(0)=112/45 for pure gravity when the linearized magnetic curvature is vanishing on . The zeta(0) values for gauge fields have been obtained by working only with physical degrees…
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
