Monte Carlo Computation of Spectral Density Function in Real-Time Scalar Field Theory
Navid Abbasi, Ali Davody

TL;DR
This paper develops a non-perturbative Monte Carlo method to compute the spectral density function in real-time scalar field theory, overcoming the sign problem and enabling analysis beyond perturbation theory.
Contribution
It introduces a novel approach combining Schwinger-Dyson equations with a new analytical integral method and Monte Carlo simulations for spectral functions in real-time quantum field theory.
Findings
Non-perturbative spectral function obtained via Monte Carlo
Comparison with perturbative results shows significant differences
Full vertex function computed for real-time scattering amplitudes
Abstract
Non-perturbative study of "real-time" field theories is difficult due to the sign problem. We use Bold Schwinger-Dyson (SD) equations to study the real-time theory in beyond the perturbative regime. Combining SD equations in a particular way, we derive a non-linear integral equation for the two-point function. Then we introduce a new method by which one can analytically perform the momentum part of loop integrals in this equation. The price we must pay for such simplification is to numerically solve a non-linear integral equation for the spectral density function. Using Bold diagrammatic Monte Carlo method we find non-perturbative spectral function of theory and compare it with the one obtained from perturbation theory. At the end we utilize our Monte Carlo result to find the full vertex function as the basis for the computation of real-time scattering amplitudes.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
