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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2017-09-26 11:19:54 -0400 | 
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2017-09-26 11:19:54 -0400 | 
| commit | 75153282053738f549f2737f0fe42a18bb17b5a6 (patch) | |
| tree | 4d289553e0594f632dfe468c35216b920e75e76a /essential-ising.tex | |
| parent | 80c08bc131afb141d0ed780bd7ebb939f4303dbd (diff) | |
| download | paper-75153282053738f549f2737f0fe42a18bb17b5a6.tar.gz paper-75153282053738f549f2737f0fe42a18bb17b5a6.tar.bz2 paper-75153282053738f549f2737f0fe42a18bb17b5a6.zip  | |
changed paper body to incorporate new analysis
Diffstat (limited to 'essential-ising.tex')
| -rw-r--r-- | essential-ising.tex | 67 | 
1 files changed, 29 insertions, 38 deletions
diff --git a/essential-ising.tex b/essential-ising.tex index d641a57..7dd6686 100644 --- a/essential-ising.tex +++ b/essential-ising.tex @@ -316,7 +316,8 @@ the presence of an external field. Briefly, the external field $H$ is applied  by adding an extra spin $s_0$ with coupling $|H|$ to all others  \cite{dimitrovic.1991.finite}. A quickly converging estimate for the  magnetization in the finite-size system was then made by taking -$M=\sgn(H)s_0\sum s_i$, i.e., the magnetization relative to the external spin. +$M=\sgn(H)s_0\sum s_i$, i.e., the magnetization relative to the external spin +\cite{kent-dobias.2018.wolff}.  Data was then taken for susceptibility and magnetization for  $T_\c-T,H\leq0.1$. This data, rescaled as appropriate to collapse onto a  single curve, is plotted in Fig.~\ref{fig:scaling_fits}. @@ -330,34 +331,23 @@ the susceptibility scaling function, then  $T\chi(t,0)|t|^\gamma=\lim_{X\to0}\fX^\twodee(X)=2AB^2/\pi$ and the constant  $A$ is fixed to $A=\pi\fX(0)/2B^2=2^{19/8}\pi^3(\arcsinh1)^{15/4}C_0^-$.  The  resulting scaling functions $\fX$ and $\fM$ are plotted as solid lines in -Fig.~\ref{fig:scaling_fits}. As can be seen, there is very good agreement -between our proposed functional forms and what is measured.  However, there -are systematic differences that can be seen most clearly in the magnetization. -Since our method is known to only be accurate for high moments of the free -energy, we should expect that low moments require corrections.  Therefore, we -also fit those corrections using  -\begin{align} -  \tilde\fX^\twodee(X)&=\fX^\twodee(X)+\sum_{n=0}^Nf_n(BX)\label{eq:sus_scaling_poly}\\ -  \tilde\fM^\twodee(X)&=\fM^\twodee(X)+\frac{T_\c}B\sum_{n=0}^NF_n(BX)\label{eq:mag_scaling_poly} -\end{align} -where $F_n'(Y)=f_n(Y)$ and -\[ -  \begin{aligned} -    f_n(Y)&=\frac{c_nx^n}{1+(\lambda Y)^{n+1}}\\ -    F_n(Y)&=\frac{c_n\lambda^{-(n+1)}}{n+1}\log(1+(\lambda Y)^{n+1}). -  \end{aligned} -  \label{eq:poly} -\] -The functions $f_n$ have been chosen to be pure integer power laws for small -argument, but vanish appropriately at large argument. This is necessary -because the susceptibility vanishes with $h|t|^{-\beta\delta}$ while bare -polynomial corrections would not.  We fit these functions to known moments of -the free energy's scaling function -\cite{mangazeev.2008.variational,mangazeev.2010.scaling} our numeric data -for $N=0$. The -resulting curves are also plotted as dashed lines in -Fig.~\ref{fig:scaling_fits}. Our singular scaling function with one low-order -correction appears to match data quite well. +Fig.~\ref{fig:scaling_fits}. Though there is good agreement +between our functional forms and what is measured, there +are systematic differences that can be seen most clearly in the +magnetization. This is to be expected based on our earlier discussion: these +scaling forms should only be expected to well-describe the singularity at the +abrupt transition. Our forms both exhibit incorrect low-order +coefficients at the transition (Fig.~\ref{fig:series}) and incorrect +asymptotics as $h|t|^{-\beta\delta}$ becomes very large. In forthcoming work, +we develop a method to incorporate the essential singularity in the scaling +functions into a form that also incorporates known properties of the scaling +functions in the rest of the configuration space using a Schofield-like +parameterization \cite{kent-dobias.2018.parametric}. Fig.~\ref{fig:scaling_fits} shows a result as a +dashed yellow line, which depicts the scaling form resulting from +incorporating our singularity and the known series expansions of the scaling +function at high temperature, low temperature, and at the critical isotherm to +quadratic order. The low-order series coefficients of this modified form are +also shown in Fig.~\ref{fig:series}.  \begin{figure}    \input{fig-susmag} @@ -370,10 +360,11 @@ correction appears to match data quite well.      and $H=0.1\times(1,2^{-1/4},\ldots,2^{-50/4})$. The solid blue lines      show our analytic results \eqref{eq:sus_scaling} and      \eqref{eq:mag_scaling}, the dashed yellow lines show  -    \eqref{eq:sus_scaling_poly} and \eqref{eq:mag_scaling_poly} for $N=0$, the -    dotted green lines show the same for $N=4$, and the red line show the -    polynomial resulting from truncating the series after the eight known -    terms. +    a scaling function modified to match known series expansions +    in several known limits, and the +    dotted green lines show the +    polynomial resulting from truncating the series after the eight terms +    reported by \cite{mangazeev.2008.variational,mangazeev.2010.scaling}.    }    \label{fig:scaling_fits}  \end{figure} @@ -383,11 +374,11 @@ correction appears to match data quite well.    \caption{      The series coefficients defined by $\tilde\fF(X)=\sum_nf_nX^n$. The blue      pluses correspond to the scaling form \eqref{eq:2d_free_scaling}, the -    yellow saltires correspond to that form with the first four coefficients -    fixed to known values (\eqref{eq:sus_scaling_poly} with $N=0$), the green -    stars correspond to that form with the first eight coefficients fixed to -    known values (\eqref{eq:sus_scaling_poly} with $N=4$), and the red squares -    correspond to the first eight coefficients. +    yellow saltires correspond to a scaling function modified to match known +    series expansions in several known limits, and the green +    stars +    correspond to the first eight coefficients from +    \cite{mangazeev.2008.variational,mangazeev.2010.scaling}.    }    \label{fig:series}  \end{figure}  | 
