Feynman Path Integral Calculator

Discretize paths, sample trajectories, and evaluate quantum amplitudes. Switch potentials, tune slices, inspect action terms. Download clean CSV or PDF for reports and sharing.

Calculator Inputs

Use consistent units across all fields.
Common choice: ħ = 1 for dimensionless tests.
β acts like inverse temperature in Euclidean form.
Higher N reduces discretization error.
Increase samples to reduce statistical error.
Use a new seed to test stability.
For oscillatory real-time kernels, use Wick rotation externally.
Polynomial coefficients
V(x)=c0+c1 x+c2 x²+c3 x³+c4 x⁴+c5 x⁵+c6 x⁶
Tip: keep coefficients moderate for stability.

Example Data Table

Case Potential m ħ β x₀ → x_T N Samples Expected behavior
A Free 1 1 1 0 → 1 64 5000 Matches closed-form ρ_free.
B Harmonic (ω=1) 1 1 1 0 → 0 96 8000 Should approach analytic harmonic kernel.
C Quartic (λ=0.1) 1 1 0.5 -1 → 1 128 12000 Needs more samples; weights vary widely.
Use these as starting points, then increase N and samples until results stabilize.

Formula Used

This tool evaluates a discretized Euclidean (imaginary-time) path integral for a one-dimensional particle between fixed endpoints x₀ and x_T over time β.

Euclidean density matrix
ρ(x_T,β;x₀,0) = ∫ Dx(τ) exp( - (1/ħ) ∫₀^β [ m/2 (dx/dτ)² + V(x) ] dτ )

Using a time slicing with N steps (ε=β/N), and sampling free Brownian bridges, the interacting density matrix is estimated by reweighting:

ρ_V = ρ_free · ⟨ exp( - (ε/ħ) Σ_{j=0}^{N-1} V( (x_j+x_{j+1})/2 ) ) ⟩_free-bridge

The free normalization ρ_free is known exactly, so the estimator does not require an unknown overall constant. Statistical uncertainty is reported from the sample variance of the reweight factor.

How to Use This Calculator

  1. Choose consistent units for m, ħ, and your potential parameters.
  2. Set β and endpoints x₀, x_T.
  3. Pick N (start with 64–256) and a sample count (start with 5000+).
  4. Select a potential model and fill in its parameters.
  5. Press Compute. Results appear above the form under the header.
  6. Export with CSV/PDF buttons for documentation or audits.

Professional Article

1) Purpose of the Euclidean Path Integral

This calculator estimates the Euclidean density matrix ρ(xT,β;x0,0) by sampling paths and averaging a reweighting factor. In many workflows, β plays the role of inverse temperature, and the same kernel is used to extract ground-state information when β is large.

2) Discretization Data and Time Slicing

The time interval is split into N slices, with step size ε = β/N. With the default example β=1 and N=64, the step is ε≈0.015625. Increasing N reduces Trotter discretization error, but increases compute cost roughly linearly in N.

3) Free-Bridge Sampling Strategy

Paths are generated as a Gaussian random walk and then corrected to satisfy the endpoint constraint x(0)=x0, x(β)=xT. The per-slice diffusion scale is σ = √(ħ ε / m), so doubling m reduces typical fluctuations by about √2 at fixed β and N.

4) Midpoint Action Evaluation

The potential contribution is integrated using a midpoint rule, ∫V dτ ≈ ε Σ V((xj+xj+1)/2). This midpoint choice improves accuracy over left-point sampling for smooth potentials and makes the estimator less sensitive to oscillations between adjacent slices.

5) Built-in Potential Models and Parameters

The interface supports free, harmonic, quartic, double-well, linear, square-well, and a polynomial up to x⁶. For the harmonic model, the analytic kernel is also computed, enabling immediate validation. For stiff models (large ω, a, or V0), the weight distribution can become extremely broad.

6) Statistical Uncertainty and Scaling

The estimator uses ρ = ρfree · ⟨A⟩, where A = exp(-∫V/ħ). The reported standard error scales approximately as 1/√S with S samples, so increasing samples from 5,000 to 20,000 typically reduces Monte Carlo noise by about a factor of 2.

7) Convergence Diagnostics Provided

Along with ρ, the calculator reports the mean and spread of V(mid) and the mean of ∫V dτ. Large standard deviation of V(mid) or warnings about weight spread indicate slow convergence and a need for higher N and S.

8) Recommended Workflow for Reliable Results

Start with moderate settings (for example N=64–128, S≥5000), then increase N until the result changes less than your target tolerance. Next, increase S until the reported error bars are acceptably small. For the harmonic case, aim for agreement with the analytic kernel within the Monte Carlo uncertainty before moving to more complex potentials.

FAQs

1) Does this compute real-time propagators directly?

No. It evaluates an imaginary-time (Euclidean) kernel. For real-time propagation, you typically need contour methods or analytic continuation, which is numerically delicate for noisy Monte Carlo estimates.

2) Why does the tool use free-bridge sampling?

Free bridges are easy to sample and have an exact normalization. The potential is included by reweighting with exp(-∫V/ħ), which turns the path integral into a statistically estimable average.

3) How do I choose the number of slices N?

Increase N until results stabilize. A common pattern is doubling N (64→128→256) and checking that changes are smaller than your acceptable error, while monitoring computation time.

4) Why are the weights sometimes extremely small?

Large positive potentials, large β, or small ħ can make exp(-∫V/ħ) tiny. Reduce potential strength, reduce β, or increase samples to improve effective statistics.

5) What does “Mean ∫V dτ” tell me?

It is the sampled average of the potential integral along paths. Large values generally correspond to stronger suppression of amplitudes and can signal that the kernel will be very small and harder to estimate accurately.

6) Can I validate the method?

Yes. Select the harmonic potential and compare ρ_est against the displayed analytic harmonic kernel. Adjust N and samples until the difference is within the reported Monte Carlo uncertainty.

7) Is this suitable for multi-dimensional systems?

This implementation is one-dimensional. Extending to multiple dimensions requires vector paths, a higher computational load, and careful tuning of sampling and variance reduction to keep weight fluctuations manageable.

Related Calculators

black hole temperatureenergy momentum tensorbogoliubov transformationquantum circuit simulatorspontaneous symmetry breakingwigner d matrixredshift distance calculatorquantum tunneling calculatorpoisson bracket calculatorbeta function calculator

Important Note: All the Calculators listed in this site are for educational purpose only and we do not guarentee the accuracy of results. Please do consult with other sources as well.