8-Spinor Quantum Gravity

Quantum gravity has been so elusive because we have tried to approach it by two paths which can never meet: quantum mechanics and general relativity. These contradict each other not only in superdense regimes, but also in the vacuum. We explore a straight road to quantum gravity here–the one mandated by Clifford-algebra covariance. This bridges the gap from microscales–where the massive Dirac propagator is a sum over null zig-zags–to macroscales–where we see the energy-momentum current, *T and the resulting Einstein curvature, *G. For massive particles, *T flows in the “cosmic time” direction, y^0–centrifugally in an expanding universe. Neighboring centrifugal currents of *T present opposite spacetime vorticities *G to the boundaries of each others’ worldtubes, so they advect–i.e. attract, as we show here by integrating a Spin^c-4 Lagrangian by parts in the spinfluid regime. This boundary integral not only explains why stress-energy *T is the source for gravitational curvature *G, but also gives a value for the gravitational constant, kappa(x^0) that depends on the current scale factor of our expanding Friedmann 3-brane. On the microscopic scale, quantum gravity appears naturally as the statistical mechanics of null zig-zags of massive particles in “imaginary time,” y^0.