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References
- 1
- For a review, see: ``The Monte Carlo Method in Condensed
Matter Physics,'' ed. by K. Binder (Springer, Berlin, Heidelberg 1992).
- 2
- H. Müller-Krumbhaar and K. Binder, J. Stat.
Phys. 8, 1 (1973).
- 3
- N. Madras and A. D. Sokal, J. Stat. Phys. 50, 109
(1988).
- 4
- A.M. Ferrenberg, D.P. Landau and K. Binder, J.
Stat. Phys 63, 867 (1991).
- 5
- A.M. Ferrenberg and R.H. Swendsen, Phys. Rev. Lett.
61, 2635 (1988); A.M. Ferrenberg and R.H. Swendsen, Phys. Rev. Lett.
63, 1195 (1989).
- 6
- R.H. Swendsen, J.-S. Wang and A.M. Ferrenberg, ``New
Monte Carlo Methods for Improved Efficiency of Computer Simulations'' in
reference [1].
- 7
- A.M. Ferrenberg and D.P. Landau, Phys. Rev. B
44, 5081 (1991).
- 8
- An old but excellent reference is: W. Feller, ``An
Introduction to Probability Theory and Its Applications,'' (Wiley, New York
1957).
- 9
- The definition of the integrated correlation time used here
differs from that used in some recent papers. See, for example reference [3].
- 10
- See for example: P.R. Bevington, ``Data reduction and
error analysis for the physical sciences,'' (McGraw-Hill, New York 1969).
- 11
- E. Ising, Z. Phys. 31, 2553 (1925).
- 12
- L. Onsager, Phys. Rev 65, 117 (1944).
- 13
- A.E. Ferdinand and M.E. Fisher, Phys. Rev
185, 832 (1969).
- 14
- N. Metropolis, A.W. Rosenbluth, M.N. Rosenbluth, A.H.
Teller, and E. Teller, J. Chem. Phys. 21, 1087 (1953).
- 15
- U. Wolff, Phys. Rev. Lett. 62, 361 (1989).
- 16
- C.-K. Hu, Phys. Rev. Lett. 69, 2739 (1992).
- 17
- P.W. Kasteleyn and C.M. Fortuin, J. Phys. Soc.
Jpn. Suppl. 26s, 11 (1969); C.M. Fortuin and P.W. Kasteleyn,
Physicsa (Utrecht) 57, 536 (1972).
- 18
- W. Janke, unpublished.
- 19
- E.Münger and M. Novotny, Phys. Rev. B 43, 5773 (1991).
- 20
- B.Berg and T. Neuhaus, Phys. Rev. Lett. 68, 9
(1992).
- 21
- B.Berg and T. Celik, Phys. Rev. Lett. 69, 2292
(1992).
- 22
- W. Janke and T. Sauer, Phys. Rev. E 49, 3475 (1994).
- 23
- A.M. Ferrenberg and D.P. Landau, unpublished.
Figure Captions
Fig. 1: Absolute error in E as a function of
for the d=2 Ising
model simulated at infinite temperature (
). The measured error is
compared to the theoretical error from (15) as well as the
Gaussian test model (16).
Fig. 2: Relative error in C as a function of
for the d=2 Ising
model simulated at infinite temperature (
). The measured error is
compared to the theoretical error from (15) as well as the
Gaussian test model (17).
Fig. 3: Comparison of the theoretical and measured relative error in E as a
function of
for the d=2 Ising model simulated at
(marked
by the vertical line). The simulations were performed with the
Metropolis algorithm.
Fig. 4: Comparison of the theoretical and measured relative error in
C as a function of
for the d=2 Ising model simulated at
. The vertical line indicates the simulated temperature.
Results obtained using the Metropolis algorithm are shown.
Fig. 5: Ratio of the deviation from the correct answer to the statistical
error for the d=2 Ising model simulated at
(marked by the
vertical line) using the Metropolis algorithm. The horizontal lines
represent
standard deviation.
Fig. 6: Comparison of the relative error in the energy for a
simulation with independent measurements to a Metropolis simulation
with correlations. The vertical line indicates the location of the
simulated temperature. Results for the d=2 Ising model are shown.
Fig. 7: Comparison of the relative error in E determined by Metropolis
and Wolff simulations for the d=2 Ising model. To simplifiy the
comparison, the error from the Wolff algorithm was rescaled to match
that of the Metropolis algorithm at the simulated temperature (marked
by the vertical line).
Fig. 8: Plot of the reweighted energy correlation time (
)
for the Metropolis and Wolff algorithms. Results for the d=2 Ising
model are shown. The simulations were performed at
, which is
marked by the vertical line.
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Thu Jun 22 14:26:19 EDT 1995