Supersymmetric quantum cosmology for Bianchi class A models

Abstract

The canonical theory of (N=1) supergravity, with a matrix representation for the gravitino covector-spinor, is applied to the Bianchi class A spatially homogeneous cosmologies. The full Lorentz constraint and its implications for the wave function of the universe are analyzed in detail. We found that in this model no physical states other than the trivial "rest frame" type occur.

10 pages, Revtex

References in corpus (8)

• Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
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• Diagonal quantum Bianchi type IX models in N=1 supergravity
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Cited by in corpus (4)

• Lorentz-breaking effects in scalar-tensor theories of gravity
• Shape Invariant Potentials in Supersymmetric Quantum Cosmology
• Midisuperspace Supersymmetric Quantum Cosmology
• On the local Lorentz invariance in N=1 supergravity