Hamiltonian Truncation Effective Theory
- University of Oregon
- Case Western Reserve University
- Durham University
- University of California, Davis
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 H_0 with eigenvalues below some energy cutoff E_\text{max} . 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 E_\text{max} . 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 1/E_\text{max} . The effective Hamiltonian is non-local, with the non-locality controlled in an expansion in powers of H_0/E_\text{max} . 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 \lambda\phi^4 theory, and compute the the leading 1/E_\text{max}^2 corrections to the effective Hamiltonian. We show that these corrections nontrivially satisfy the crucial property of separation of scales. Numerical diagonalization of the effective Hamiltonian gives residual errors of order 1/E_\text{max}^3 , as expected by our power counting. We also present the power counting for 3D \lambda \phi^4 theory and perform calculations that demonstrate the separation of scales in this theory.
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- SC0009999; SC0011640
- OSTI ID:
- 1879775
- Alternate ID(s):
- OSTI ID: 1905570
- Journal Information:
- SciPost Physics, Journal Name: SciPost Physics Journal Issue: 2 Vol. 13; ISSN 2542-4653
- Publisher:
- Stichting SciPostCopyright Statement
- Country of Publication:
- Netherlands
- Language:
- English
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