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添加247字节 、 2021年11月30日 (二) 12:42
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\Lambda^d \sim \left\{ \begin{array} {lc }(-\mu)^{d/2-1}, & 2<d<4 \\
 
\Lambda^d \sim \left\{ \begin{array} {lc }(-\mu)^{d/2-1}, & 2<d<4 \\
 
\\ \mu \ln(-\mu/kT), & d=4 \\ \\ -\mu , & d>4 . \end{array}\right. </math>|3={{EquationRef|19}}}}
 
\\ \mu \ln(-\mu/kT), & d=4 \\ \\ -\mu , & d>4 . \end{array}\right. </math>|3={{EquationRef|19}}}}
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<math>d>4</math> the singular <math>(-\mu)^{d/2-1}</math> is still present but is dominated by the mean-field <math>-\mu\ .</math>
 
<math>d>4</math> the singular <math>(-\mu)^{d/2-1}</math> is still present but is dominated by the mean-field <math>-\mu\ .</math>
   −
 
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This behavior is reflected again in the R'''enormalization-group theory''' [19-21].  In the simplest cases there are two competing fixed points for  the renormalization-group flows, one of them associated with <math>d</math>-dependent  
This behavior is reflected again in the [[renormalization-group theory]] [19-21].  In the simplest cases there are two competing fixed points for  the renormalization-group flows, one of them associated with <math>d</math>-dependent  
   
exponents that satisfy both the <math>d</math>-independent scaling relations and
 
exponents that satisfy both the <math>d</math>-independent scaling relations and
 
the hyperscaling relations, the other with the <math>d</math>-independent  
 
the hyperscaling relations, the other with the <math>d</math>-independent  
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as though it were a single spin in a re-scaled model.  Each block is
 
as though it were a single spin in a re-scaled model.  Each block is
 
of finite size so the spins in its interior contribute only analytic
 
of finite size so the spins in its interior contribute only analytic
terms to the free energy of the system. The part of the free-energy
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terms to the free energy of the system. The part of the free-energy
 
density (free energy per spin) that carries the critical-point
 
density (free energy per spin) that carries the critical-point
singularities and their exponents comes from the interactions between
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singularities and their exponents comes from the interactions between blocks. Let this free-energy density be <math>f(t,H)\ ,</math> a function of temperature through <math>t=T/T_c-1</math> and of the magnetic field <math>H\ .</math>  The correlation length is the same in the re-scaled picture as in the original, but measured as a number of lattice spacings it is smaller in the former by the factor <math>L\ .</math>  Thus, the re-scaled model is effectively further from its critical point than the original was from its; so with <math>H</math> and <math>t</math> both going to 0 as the critical point is approached, the effective <math>H</math> and <math>t</math>
blocks. Let this free-energy density be <math>f(t,H)\ ,</math> a
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in the re-scaled model are <math>L^xH</math> and <math>L^yt</math> with positive exponents <math>x</math> and <math>y\ ,</math> so increasing with <math>L\ .</math>  From the point of view of the original model the contribution to the singular part of the free energy made by the spins in each block is <math>L^df(t,H)\ ,</math> while that same quantity, from the point of the view of the re-scaled model, is <math>f(L^yt, L^xH)\ .</math>  Thus,  
function of temperature through <math>t=T/T_c-1</math> and of the
  −
magnetic field <math>H\ .</math>  The correlation length is the same in
  −
the re-scaled picture as in the original, but measured as a number of
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lattice spacings it is smaller in the former by the factor
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<math>L\ .</math>  Thus, the re-scaled model is effectively further from
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its critical point than the original was from its; so with
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<math>H</math> and <math>t</math> both going to 0 as the critical
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point is approached, the effective <math>H</math> and <math>t</math>
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in the re-scaled model are <math>L^xH</math> and <math>L^yt</math>
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with positive exponents <math>x</math> and <math>y\ ,</math> so
  −
increasing with <math>L\ .</math>  From the point of view of the
  −
original model the contribution to the singular part of the free
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energy made by the spins in each block is <math>L^df(t,H)\ ,</math>
  −
while that same quantity, from the point of the view of the re-scaled
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model, is <math>f(L^yt, L^xH)\ .</math>  Thus,  
      
:<math>\label{eq:20}
 
:<math>\label{eq:20}
 
f(L^yt,
 
f(L^yt,
 
L^xH) \equiv L^df(t,H); </math>
 
L^xH) \equiv L^df(t,H); </math>
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{{NumBlk|1=:|2=<math>f(L^yt,
 +
L^xH) \equiv L^df(t,H);</math>|3={{EquationRef|20}}}}
 +
 
   −
i.e., by \eqref{eq:1},
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i.e., by \eqref{eq:1}, <math>f(t,H)</math> is a homogeneous function of <math>t</math> and <math>H^{y/x}</math> of degree <math>d/y\ .</math>
<math>f(t,H)</math> is a homogeneous function of <math>t</math> and
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<math>H^{y/x}</math> of degree <math>d/y\ .</math>
      
Therefore, by \eqref{eq:2}, <math>f(t,H)=t^{d/y}
 
Therefore, by \eqref{eq:2}, <math>f(t,H)=t^{d/y}
\phi(H^{y/x}/t)=H^{d/x}\psi(t/H^{y/x})</math> where <math>\phi</math>
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\phi(H^{y/x}/t)=H^{d/x}\psi(t/H^{y/x})</math> where <math>\phi</math> and <math>\psi</math> are functions only of the ratio <math>H^{y/x}/t\ .</math>  At <math>H=0</math> the first of these gives <math>f(t,0)=\phi(0)t^{d/y}\ .</math> But two temperature derivatives of <math>f(t,0)</math> gives the contribution to the heat capacity per spin, diverging as <math>t^{-\alpha}\ ;</math> so <math>d/y=2-\alpha\ .</math>  Also, on the critical isotherm <math>(t=0)\ ,</math> the second relation above gives <math>f(0,H)=\psi(0)H^{d/x}\ .</math>  But the magnetization per spin is <math>-(\partial f/\partial H)_T\ ,</math> vanishing as <math>H^{d/x-1}\ ,</math> so <math>d/x-1=1/\delta\ .</math>  The exponents <math>d/x</math> and <math>d/y</math> have thus been identified in terms of the thermodynamic exponents: the heat-capacity exponent <math>\alpha</math> and the critical-isotherm exponent <math>\delta\ .</math>  In the meantime, again with <math>-(\partial
and <math>\psi</math> are functions only of the ratio
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f/\partial H)_T</math> the magnetization per spin, the homogeneity of form of <math>f(t,H)</math> in \eqref{eq:20} is equivalent to that of <math>H(t,M)</math> in \eqref{eq:7}, from which the scaling laws <math>\gamma=\beta(\delta-1)</math> and <math>\alpha +
<math>H^{y/x}/t\ .</math>  At <math>H=0</math> the first of these gives
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<math>f(t,0)=\phi(0)t^{d/y}\ .</math> But two temperature derivatives
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of <math>f(t,0)</math> gives the contribution to the heat capacity per
  −
spin, diverging as <math>t^{-\alpha}\ ;</math> so
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<math>d/y=2-\alpha\ .</math>  Also, on the critical isotherm
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<math>(t=0)\ ,</math> the second relation above gives
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<math>f(0,H)=\psi(0)H^{d/x}\ .</math>  But the magnetization per spin is
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<math>-(\partial f/\partial H)_T\ ,</math> vanishing as
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<math>H^{d/x-1}\ ,</math> so <math>d/x-1=1/\delta\ .</math>  The exponents
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<math>d/x</math> and <math>d/y</math> have thus been identified in
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terms of the thermodynamic exponents: the heat-capacity exponent
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<math>\alpha</math> and the critical-isotherm exponent
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<math>\delta\ .</math>  In the meantime, again with <math>-(\partial
  −
f/\partial H)_T</math> the magnetization per spin, the homogeneity of
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form of <math>f(t,H)</math> in \eqref{eq:20} is equivalent to
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that of <math>H(t,M)</math> in \eqref{eq:7}, from which the
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scaling laws <math>\gamma=\beta(\delta-1)</math> and <math>\alpha +
   
2\beta + \gamma =2</math> are known to follow.
 
2\beta + \gamma =2</math> are known to follow.
   −
A related argument yields the scaling law \eqref{eq:10} for the
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A related argument yields the scaling law \eqref{eq:10} for the correlation function <math>h(r,t)\ ,</math> with <math>H=0</math> again for simplicity.  In the re-scaled model, <math>t</math> becomes <math>L^yt\ ,</math> as before, while <math>r</math> becomes <math>r/L\ .</math>  There may also be a factor, say <math>L^p</math> with some exponent <math>p\ ,</math> relating the magnitudes of the original and rescaled functions; thus,  
correlation function <math>h(r,t)\ ,</math> with <math>H=0</math> again
  −
for simplicity.  In the re-scaled model, <math>t</math> becomes
  −
<math>L^yt\ ,</math> as before, while <math>r</math> becomes
  −
<math>r/L\ .</math>  There may also be a factor, say <math>L^p</math>
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with some exponent <math>p\ ,</math> relating the magnitudes of the
  −
original and rescaled functions; thus,  
      
:<math>\label{eq:21}
 
:<math>\label{eq:21}
 
h(r,t) \equiv
 
h(r,t) \equiv
 
L^{p}h(r/L,L^yt); </math>
 
L^{p}h(r/L,L^yt); </math>
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{{NumBlk|1=:|2=<math>h(r,t) \equiv
 +
L^{p}h(r/L,L^yt);</math>|3={{EquationRef|21}}}}
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i.e., <math>h(r,t)</math> is homogeneous of
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degree <math>p</math> in <math>r</math> and <math>t^{-1/y}\ .</math>
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i.e., <math>h(r,t)</math> is homogeneous of degree <math>p</math> in <math>r</math> and <math>t^{-1/y}\ .</math> Then from the alternative form \eqref{eq:2} of the property of homogeneity,  
Then from the alternative form \eqref{eq:2} of the property of
  −
homogeneity,  
      
:<math>\label{eq:22}
 
:<math>\label{eq:22}
 
h(r,t)\equiv r^p G(r/t^{-1/y}) </math>
 
h(r,t)\equiv r^p G(r/t^{-1/y}) </math>
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{{NumBlk|1=:|2=<math>h(r,t)h(r,t)\equiv r^p G(r/t^{-1/y})</math>|3={{EquationRef|22}}}}
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with
  −
a scaling function <math>G\ .</math>  Comparing this with
  −
\eqref{eq:10}, and recalling that the correlation length
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<math>\xi</math> diverges at the critical point as
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<math>t^{-\nu}</math> with exponent <math>\nu\ ,</math> we identify
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<math>p=-(d-2+\eta)</math> and <math>1/y=\nu\ .</math>  The scaling law
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<math>(2-\eta)\nu=\gamma\ ,</math> which was a consequence of the
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homogeneity of form of <math>h(r,t)\ ,</math> again holds, while from
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<math>1/y=\nu</math> and the earlier <math>d/y=2-\alpha</math> we now
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have the hyperscaling law \eqref{eq:17},
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<math>d\nu=2-\alpha\ .</math>
     −
The block-spin picture thus yields the critical-point scaling of the
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with a scaling function <math>G\ .</math>  Comparing this with \eqref{eq:10}, and recalling that the correlation length <math>\xi</math> diverges at the critical point as <math>t^{-\nu}</math> with exponent <math>\nu\ ,</math> we identify <math>p=-(d-2+\eta)</math> and <math>1/y=\nu\ .</math>  The scaling law <math>(2-\eta)\nu=\gamma\ ,</math> which was a consequence of the homogeneity of form of <math>h(r,t)\ ,</math> again holds, while from <math>1/y=\nu</math> and the earlier <math>d/y=2-\alpha</math> we now have the hyperscaling law \eqref{eq:17}, <math>d\nu=2-\alpha\ .</math>
thermodynamic and correlation functions, and both the
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<math>d</math>-independent and <math>d</math>-dependent relations
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The block-spin picture thus yields the critical-point scaling of the thermodynamic and correlation functions, and both the <math>d</math>-independent and <math>d</math>-dependent relations among the scaling exponents. The essence of this picture is confirmed in the renormalization-group theory [19,20].
among the scaling exponents. The essence of this picture is confirmed
  −
in the renormalization-group theory [19,20].
      
== References ==
 
== References ==
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* Cesar A. Hidalgo R. and Albert-Laszlo Barabasi (2008) [[Scale-free networks]]. Scholarpedia, 3(1):1716.
 
* Cesar A. Hidalgo R. and Albert-Laszlo Barabasi (2008) [[Scale-free networks]]. Scholarpedia, 3(1):1716.
  −
   
==See also==
 
==See also==
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