Hamiltonian Truncation Effective Theory
arXiv:2110.08273 · doi:10.21468/SciPostPhys.13.2.011
Abstract
Hamiltonian truncation is a non-perturbative numerical method for calculating observables of a quantum field theory. The starting point for this method is to truncate the interacting Hamiltonian to a finite-dimensional space of states spanned by the eigenvectors of the free Hamiltonian with eigenvalues below some energy cutoff . In this work, we show how to treat Hamiltonian truncation systematically using effective field theory methodology. We define the finite-dimensional effective Hamiltonian by integrating out the states above . The effective Hamiltonian can be computed by matching a transition amplitude to the full theory, and gives corrections order by order as an expansion in powers of . The effective Hamiltonian is non-local, with the non-locality controlled in an expansion in powers of . The effective Hamiltonian is also non-Hermitian, and we discuss whether this is a necessary feature or an artifact of our definition. We apply our formalism to 2D theory, and compute the the leading corrections to the effective Hamiltonian. We show that these corrections non-trivially satisfy the crucial property of separation of scales. Numerical diagonalization of the effective Hamiltonian gives residual errors of order , as expected by our power counting. We also present the power counting for 3D theory and perform calculations that demonstrate the separation of scales in this theory.
51 pages, 9 figures, v2: Clarifications and additional discussion added in response to referee reports. Conclusions unchanged
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- Hamiltonian formulation of the -dimensional theory in a momentum-space Daubechies wavelet basis
- Higher-order structure of Hamiltonian truncation effective theory