Quantum Monte Carlo simulation with a black hole
arXiv:1603.00716 · doi:10.1103/PhysRevD.93.094505
Abstract
We perform quantum Monte Carlo simulations in the background of a classical black hole. The lattice discretized path integral is numerically calculated in the Schwarzschild metric and in its approximated metric. We study spontaneous symmetry breaking of a real scalar field theory. We observe inhomogeneous symmetry breaking induced by inhomogeneous gravitational field.
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