A variational Monte Carlo simulation of the helium atom generates a correlated Markov…

PHYSICS · Multi-part · Fermi University Physics · Scientific Practice & Experimental Methods · Mathematical Methods for Physics · Uncertainty in measurement

Scientific Computing for Physicists, Ch The uncertainty of a simulated number: inputs, sensitivity and correlated output

Problem

A variational Monte Carlo simulation of the helium atom generates a correlated Markov chain of local-energy samples EL(i)E_L^{(i)} (in Hartree), one per Monte Carlo step. A first run of N=214=16384N = 2^{14} = 16384 steps has sample standard deviation σE=0.384 Hartree\sigma_E = 0.384\,\mathrm{Hartree}, and blocking gives: bb: 1, 2, 4, 8, 16, 32, 64, 128, 256 σ^b\hat\sigma_b (Hartree): 0.0030, 0.0038, 0.0049, 0.0063, 0.0081, 0.0104, 0.0134, 0.0172, 0.0210 with σ^b\hat\sigma_b still rising by more than 20%20\% per doubling of bb even at the largest block size shown. ((a)) Decide whether this blocking curve has reached a plateau, and state what this implies about quoting a statistical error bar from this run. ((b)) State, in one sentence, why an ordinary bootstrap of the raw series, or a block bootstrap using an unconverged block size, would give a misleading standard error here. ((c)) An independent run, sixty-four times longer, with N′=220=1048576N' = 2^{20} = 1048576 steps and the same σE=0.384 Hartree\sigma_E = 0.384\,\mathrm{Hartree}, has a blocking curve that is level at σ^b=0.0240 Hartree\hat\sigma_b = 0.0240\,\mathrm{Hartree}, within its own scatter, at b=8192b = 8192, 1638416384 and 3276832768 (128, 64 and 32 blocks). Compute the statistical inefficiency ss, the integrated autocorrelation time τint\tau_{\rm int} (in steps), and the effective sample size NeffN_{\rm eff} for this longer run. ((d)) State what the first, short run means for assembling an uncertainty budget for the ground-state energy, and what must be done before that budget can be closed.

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