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\topmatter
 
\title Corrections to the critical temperature\\
in 2d Ising systems with Kac potentials
 \endtitle







\author M. Cassandro$^1$, R. Marra$^2$, E.
Presutti$^3$\endauthor 
 
\affil
$^1$ Dipartimento di Fisica, Universit\`a di Roma La Sapienza. P.le A. Moro,\\ 00185
Roma, Italy
 email: Cassandro\@vaxrom.infn.it \\
 $^2$Dipartimento di Fisica, Universit\`a di Roma Tor Vergata, via della Ricerca\\
Scientifica, 00133 Roma, Italy.
 email: Marra\@vaxtov.infn.it \\
 $^3$Dipartimento di Matematica, Universit\`a di Roma Tor Vergata, via della Ricerca
\\ Scientifica, 00133 Roma, Italy. email:presutti\@ irmtvm51.bitnet;\;
presutti\@mat.utovrm.it  
 \endaffil
 
 

 
 
\abstract {We consider a $d=2$ Ising system with a Kac
potential whose mean field critical temperature is 1. 
Calling  $\gam>0$ the Kac parameter,  we prove that
there exists $c^\star>0$ so that the true
inverse critical temperature $\beta_{\text{cr}}(\gam)> 1 + b
\gam^2\log\gam^{-1}$, for any $b<c^\star$ and $\gam$
correspondingly small.  We also show that  if
$\gam\to 0$ and $b\to c^\star$, suitably, then the 
correlation functions (normalized
and rescaled) converge to those of a non trivial
Euclidean field theory. } \endabstract
 
\thanks  The research has been partially
supported by CNR, GNFM \endthanks 
 
 \endtopmatter 
 
\document

\vskip -.5cm{\bf Keywords:} Kac potential, Ising model, critical fluctuations,
euclidean field theory.

\resetall
\redefine \firstpart {1} 
 \vskip1cm
 
In this short communication we study the corrections to the
critical temperature in a $d=2$ Ising model with Kac
potentials, (proofs
will follow in an extended version of this note). 
 Recall that the
Kac hamiltonian, [\rcite{K}], is
$$- \frac 12 \sum_{x\ne y}
J_\gam(x,y)\si(x)\si(y) \(1.1)$$
where the spins $\si(x)=\pm 1$, $x\in \Bbb Z^d$, and the
coupling strength is $$J_\gam(x,y) = c_\gam
\gam^d J(\gam|x-y|),\quad \sum_{y\ne x}
J_\gam(x,y)=1,\quad \int dr J(|r|)=1,\quad
D:= \int_{\Bbb R^2} dr J(|r|) r^2\(1.2)$$ We suppose
 $J(|r|)\ge 0$ and, to fix the ideas, we take $J$
``smooth",  $J(|r|)> 0$ for  $|r|< 1$ and  $J(|r|)=0$ for
$|r|\ge 1$.
$\gam>0$ is the scaling parameter of the Kac potential and
we want to study the behavior of the inverse critical
temperature $\beta_{{\text{cr}}}(\gam)$,  for the
system with interaction $J_\gam$, as $\gam\to 0$.
$c_\gam$ is a normalization constant
that goes to 1 as $\gam\to 0$. It has been introduced to
avoid spurious fluctuations of $\beta_{{\text{cr}}}(\gam)$
as $\gam$ varies: one should in fact compare systems at
different $\gam$ with the same total interaction strength
$\sum J_\gam(0,x)$.  The deviations of
$\beta_{{\text{cr}}}(\gam)$
 in [\rcite{BF}] are entirely due to the variations
of this quantity.
 
The deviations we are talking about are from the
Lebowitz-Penrose critical temperature
$\beta_{\text{cr}}^{\text{LP}}$, that,  with the convention
 \(1.2), is
equal to 1,  see,
[\rcite{LP}]. We believe that 
$\beta_{\text{cr}}(\gam)$ goes to 1 as $\gam\to 0$.
A more precise statement involves lower and upper bounds. 
For the latter we only have a conjecture:
 
 \proclaim
{ Conjecture}   For any $\beta>1$ there is
$\gam(\beta)>0$ so that for all $\gam\le \gam(\beta)$,
$\beta_{\text{cr}}(\gam)<\beta$.
 \endproclaim
 
(We are not aware of a proof of this conjecture, except in
cases where reflection positivity may be applied, as in the
original Kac potential, see [\rcite{BF}].  In general the
proof  should follow from a Peierles argument
complemented by some large deviation estimates and bounds on
the surface tension.  Some progresses on the last two issues
have been recently obtained, [\rcite{M}], [\rcite{ABCP}]).
 
The  other side of the bound comes from mean
 field: it is
known that $\beta_{\text{cr}}(\gam)\ge 
\beta_{\text{cr}}^{\text{LP}}=
1$, as we will discuss later.  Thus, assuming
the validity of the Conjecture, we 
 conclude that
$\beta_{\text{cr}}(\gam)\to 1$ as $\gam\to 0$.  The 
next question concerns  the rate
of convergence. Our results show that
$\beta_{\text{cr}}(\gam)>1$ (strictly, for $\gam>0$) and that
the deviations from 1 are responsible for the Wick
regularization and the convergence of
the block spin variables
to a non trivial Euclidean field theory.  
Let us be more precise, starting from the first statement:
 
\vskip.6cm
\proclaim{1. Theorem}
 
\nopagebreak
For any $b<c^\star:= 1/(\pi D)$, $D$ as in \(1.2), there is
$\gam(b)>0$ so that for all $0<\gam\le \gam(b)$
$$\beta_{\text{cr}}(\gam) \ge \beta_b(\gam):= 1 +b \gam^2
\log \gam^{-1} \(1.3)$$ \endproclaim
\vskip.6cm
This Theorem suggests to study the critical behavior by
letting  $b\to c^\star$ as $\gam\to 0$.  The analysis of
this limit is in the same spirit of the continuum limit
considered for instance
in the works of Aizenmann,
[\rcite{A1}], [\rcite{A2}], Sokal, [\rcite{S}], Fr\"olich,
[\rcite{F}],  and Brydges, Fr\"olich and Sokal, 
[\rcite{BFS}], and references therein, where they prove
convergence to $\phi^4$ in $d=2,3$ and to a Gaussian field
in higher dimensions, using, and exploiting, the relation
with Ising systems and Statistical Mechanics.  Our systems
do not seem to be included, at least explicitely, in the
class considered  in the above papers
 and we have worked out a specific proof that has the
advantage of making explicit the relation between the shift
of the critical temperature, the origin of the Wick
regularization term and the fluctuations
strength.
 
We study the convergence of the block spin variables, by
considering the normalized and scaled correlation
functions.  We denote by $<\cdot>_{b,\gam}$
the expectation with respect to the Gibbs measure with
interaction $J_\gam$ and inverse temperature
$\beta_b(\gam)$, see \(1.3).  
 By Theorem 1 for $\gam<\gam(b)$ there is only one Gibbs
state and no ambiguity may arise.  Sometimes later we will
write  $<\cdot>_{\beta,\gam}$, for the expectation with
respect to the Gibbs measure at the inverse
temperature $\beta$.
 
>From the
proof of Theorem 1 it follows that 
the correlations decay on
the scale 
$$\ell_{b,\gam} =
\frac{\gam^{-2}}{\sqrt{(c-b)\log\gam^{-1}}} \(1.4)$$
Thus, in interaction-length units, the correlation
length is
$$\gam\ell_{b,\gam}
=\frac{1}{\sqrt{\beta_{c^\star}(\gam) -\beta_b(\gam)}}
\(1.4a)$$ which shows that the mean field critical exponent
is ``correct" when the temperature ``is not too close" to
critical, i.e. $b<c^\star$, as in \(1.3). (This remark
complements that of Aizenmann about the validity of mean
field for computing critical exponents in  $d>4$,
see the beginning of Section 4 in [\rcite{A2}]).  Since
Theorem 1 does not tell  us that $\beta_{c^\star}(\gam)$ is
the true inverse critical temperature, the r.h.s. of \(1.4a)
is only  an upper
bound to  the critical exponent.  On the
other hand, since we prove in Theorem 2 below that our
system behaves as a massive local field theory when $b\to
c^\star$ and $\gam\to 0$ (suitably), we expect a change of
behavior when the distance from $\beta_{c^\star}(\gam)$ is
of the order of $\gam^2$  (which is the order of the term
 responsible for the appearence of the mass in the
teory).  Therefore, at these values of the inverse
temperature, the  n.n. Ising critical exponent should be
recovered.
 
 
We introduce the normalized and rescaled correlations
$$S_{b,\gam}(r_1,..,r_{2n}) = \gam^{-2n} \langle
\si(\ell_{b,\gam}r_1)\cdots \si(\ell_{b,\gam}r_{2n})
\rangle_{b,\gam} \(1.6)$$
where $\ell_{b,\gam}r_i$ should be replaced by its  integer
part, and all sites are supposed 
distinct. We have the following result:
 
\vskip.6cm\proclaim {2. Theorem}
 
\nopagebreak
There is $\eps_0>0$ and for any $\eps\le \eps_0$ there is
a sequence $b_\gam$ such that
$$\lim  \sqrt{(c-b_\gam)\log\gam^{-1}} =
\eps^{-1} \(1.6a)$$
and  for any $n$ and any distinct
$r_1,..,r_{2n}$,
$$\lim
S_{b,\gam}(r_1,..,r_{2n}) =
S^{(\eps)}(r_1,..,r_{2n})\(1.7)$$
The Schwinger functions $S^{(\eps)}$ are continuous in
$\{r_i\ne r_j\}$, and, for any test function
$\psi(r_1,..,r_{2n})$,
 $$\lim\int dr_1\cdots
dr_{2n}S_{b,\gam}(r_1,..,r_{2n}) \psi(r_1,..,r_{2n}) = \int
dr_1\cdots dr_{2n}S^{(\eps)}(r_1,..,r_{2n})
\psi(r_1,..,r_{2n}) \(1.8)$$ The functions
$S^{(\eps)}$ satisfy a recursive relation that is also
satisfied by the Schwinger functions of the $\phi^4$
Euclidean theory with interaction strength $\lambda =1$ and
mass $\eps^{-1}$.  In particular the truncated correlation
functions constructed from $S^{(\eps)}$  are not identically
0. \endproclaim
 
\vskip.6cm
 
Without entering into the proofs of the two Theorems, we
just want to outline some points that may be of interest. 
We  recall that by using the Dobrushin's techniques for
uniqueness of Gibbs measures, [\rcite{D}], we get for the
Vaserstein distance $R_x(\si,\si')$ between the conditional
probabilities at $x$ given two different boundary
conditions, $\si$ and $\si'$,
$$R_x(\si,\si') \le \beta \sum_{y\ne x}
J_\gam(x,y)\big|\si(y)-\si(y')\big| \(1.8i)$$
Recalling \(1.2) the Dobrushin's
uniqueness condition
$\beta \sum
J_\gam(x,y)<1$ is satisfied for all $\beta<1$
and all $\gam$, hence 
$\beta_{{\text{cr}}}(\gam)\ge 1$.  The same
analysis in [\rcite{D}] allows to derive bounds for the
correlation functions, which, in the case of the 2 point
correlations yields
$$\langle \si(0)
\si(x)\rangle_{\beta,\gam} \le \beta \sum_{y\ne 0}
J_\gam(x,y) \langle \si(0) \si(x)\rangle_{\beta,\gam} +
2\beta J_\gam(x,0)\(1.9)$$ hence
$$\langle \si(0) \si(x)\rangle_{\beta,\gam}
\le  2\Big( \big(1-\beta J_\gam\big)^{-1}\Big)_{x,0}
\(1.9a)$$ On the other hand, by  the DLR equations,
$$\langle \si(0) \si(x)\rangle_{\beta,\gam}
=\langle \si(0)\tanh \beta
h_\gam(x)\rangle_{\beta,\gam},\qquad
h_\gam(x) = \sum_{y\ne x} J_\gam(x,y)\si(y) \(1.11)$$
By Taylor expanding the hyperbolic tangent and retaining
only the first two terms (as it  can be rigorously
justified using Newmann's Gaussian inequalities,
[\rcite{N}], and \(1.9a)) we get
$$\langle \si(0) \si(x)\rangle_{\beta,\gam} \approx
\beta\langle \si(0)h_\gam(x)\rangle_{\beta,\gam} - \frac 13
\beta^3\langle \si(0)h_\gam(x)^3\rangle_{\beta,\gam} 
\(1.12)$$
Given  any $\beta<1$,  it
is not difficult to see, using the previous arguments,
that also the last term is of
higher order,  in the limit as $\gam\to 0$. 
We can then solve \(1.11) and, more generally we find that
for any  $n\ge 1$ and
any distinct $r_1,..,r_{2n}$ (and in any dimension $d$)
$$\lim_{\gam\to 0} \gam^{-2n}\langle \si(\gam^{-1}r_1)
\si(\gam^{-1}r_{2n})\rangle_{\beta,\gam} =
\sum_{\text{pairings}}\prod_{\ell=1}^n G\big( r_{i_\ell}-
r_{j_\ell}\big) \(1.10)$$
where $G=G_1$ and
$$G_t(r) = \frac{1}{2\pi Dt}e^{-r^2/2Dt} \(1.10a)$$
$D$ as in \(1.2).
The bound \(1.9) is quite accurate when $\beta<1$ is kept
fixed as $\gam\to 0$, but it starts deviating from the
correct one  as soon as
$\beta=1-\gam^2$.
We can rewrite  \(1.12) as
$$\langle \si(0) \si(x)\rangle_{\beta,\gam} \approx
(\beta-\beta^3 C_{\beta,\gam})
\langle \si(0)h_\gam(x)\rangle_{\beta,\gam}
-\frac 13 \beta^3\langle
\si(0)h_\gam(x)^3\rangle^T_{\beta,\gam}\(1.14)$$
where $\langle\cdot\rangle^T_{\beta,\gam}$ is the truncated
correlation function and
$$C_{\beta,\gam} = \langle
h_\gam(x)^2\rangle_{\beta,\gam}=
\gam^2\log\gam^{-1}[\frac{1}{\pi D} +
0\big(\frac{ 1}{\log \gam^{-1}}\big)],\quad
 \text{for $\beta=\beta_{b}(\gam)$, $b<c^\star$} \(1.15)$$
(An upper bound of the right order at $\beta = 1 -\gam^2$ 
follows directly from \(1.9)).  Because of the Gaussian
structure of the correlations, evidentiated by \(1.10), we
should have, and we actually do have that
 the truncated
correlation function  may be neglected as $\gam\to 0$.
 
>From \(1.14), \(1.15)  and after some computations, we 
then see
that the effective temperature is $$\beta-\beta^3
C_{\beta,\gam}= \beta-c^\star\gam^2
\log\gam^{-1}  +
0\big( \gam^{2})
 \(1.16)$$ 
This establishes the relation between the temperature shift
and the Wick regularization, (i.e. replacing a correleation
function by the truncated one). The
same mechanism was observed in [\rcite{BF}] in a $d=3$
lattice approximation of $\phi^4$, see also [\rcite{BFS}]. 
 
The hard part in the
proof of Theorems 1 and 2 is to extend the validity of the
above considerations beyond $\beta = 1$.  We achieve that by
making an ansatz on bounds on the 
correlation functions.  We then prove, (this part of the
argument is relatively simple),  that the ansatz is
consistent with the equations that are obtained by applying
the DLR equation to correlation functions of any 
 order (similar  to those in \(1.11) for the two body
terms).  We then need to prove that the actual correlations
satisfy the ansatz and this is done by a continuity argument
starting from $\beta = 1 -\gam^2$.  In this part we use
extensively Newmann's Gaussian inequalities and convexity
properties of the pressure to prove uniqueness of the even
correlation functions.  With this information we can then
modify the usual mean field argument for the magnetization
proving that also at $\beta_b(\gam)$, $b<c^\star$, it is
equal to 0, thus obtaining  Theorem 1.  To prove Theorem 2
we use Aizenmann inequality on the 4 point truncated
correlation function to have a closed inequality for the 2
points correlations, that can be solved till $b=c^\star$ if
$\eps^{-1}$ in \(1.6a) is large enough.  By
using an argument by contradiction we finally prove the
existence of a non trivial limit.
 
\vskip1.5cm
\heading{Concluding Remarks}\endheading
\vskip.2cm
\nopagebreak
 
Very schematically we present motivations and some of the
main open problems we would like to study.
 
 
\roster \item  Unsatisfactory: we would like to work at
 $\gam$
small but non zero and $\beta = \beta_{c^\star}-a\gam^2$,
$a>0$ and $a\to 0$. Aim: crossover from mean field to n.n.
Ising critical exponent, see the discussion following
\(1.4a).
 
\item 
Original motivation: Jona-Lasinio's proposal, [\rcite{J}],
of stochastic quantization via particle dynamics, in our
case the Glauber dynamics.  Namely to derive stochastic PDE's whose
invariant measure is the $\phi^4$ Euclidean field theory. 
This is the dynamical analogue of the approach to 
constructive $\phi^4$ theories via Ising models, with the
belief that, like in equilibrium, this may lead to
substantial simplifications.  Results in $d=1$ have been
already obtained, [\rcite{BPRS}] and [\rcite{BF1}].
 
\item \;\; $d=3$\;?
\endroster
\vskip2cm
\heading{Acknowledgments}\endheading
 
\nopagebreak
We are indebted to Lorenzo Bertini, Gianni Jona-Lasinio and
Enzo Olivieri for many helpful comments.
 
 
 
 \vskip1cm
\Refs
 
\nopagebreak
\widestnumber\key{99}
 
\ref\key \rtag {ABCP} \by Alberti, G. Bellettini,
M. Cassandro, E. Presutti \jour in preparation \endref
 
\vskip.4cm
\ref\key \rtag {A1}\by M. Aizenman \paper Geometric Analysis
of $\Phi^4$ Fields and Ising Models. Parts I and II.\jour
Commun. Math. Phys. \vol 86\pages 1--48\yr 1982
\endref
 
\vskip.4cm
\ref\key \rtag{A2}\by M. Aizenman \paper Rigorous Results on
the Critical Behavior  in Statistical Mechanics \paperinfo
in "Scaling and Self-Similarity in Physics"\ed. J.
Fr\"olich  \publ Birkhauser \publaddr Boston \yr1983 \endref
 
\vskip.4cm
\ref\key \rtag{BPRS}\by L. Bertini, E. Presutti, B.
R\"udiger, E. Saada \paper Dynamical Fluctuations at the
Critical Point: Convergence to a  Non Linear Stochastic PDE
\jour Probability Theory and its Applications \toappear
\endref
 
 
 
\vskip.4cm
\ref\key \rtag{BF}\by J. Bricmont and J. R. Fontaine
\paper Perturbation about the Mean Field Critical Point
\jour Commun. Math. Phys. \vol 86 \pages 337--362 \yr 1982
\endref
 
 \vskip.4cm
\ref\key \rtag{BFS}\by D.C. Brydges, J .Fr\"olich and A.
Sokal\paper A new proof of the existence and Nontriviality
of the continuum $\Phi^4_2$ and $\Phi^4_3$ Quantum Field
Theories \jour
 Commun. Math. Phys. \vol 91 \pages 141--186\yr1983
\endref
 
 
 
 \vskip.4cm
\ref\key \rtag{D} \by R. L. Dobrushin \paper Prescribing a
System of Random Variables by Conditional Distributions
\jour Theory Probab. Appl. \vol 15 \pages 458-486 \yr 1970
\endref
 
 \vskip.4cm
\ref\key \rtag{BF1} \by J. Fritz, B. R\"udiger 
 \jour In preparation  \endref
 
 
\vskip.4cm
\ref\key \rtag{F} \by J. Fr\"olich \paper On the Triviality
of $\lambda \Phi^4$ Theories and the Approach to the
Critical Point in $D>4$ dimensions\jour Nuclear Physics
B200[FS4] \pages 281--296 \yr 1982
\endref
 
\vskip.4cm
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\vskip2cm
\enddocument
