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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  
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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
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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
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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>
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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,  
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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
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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,
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L^xH) \equiv L^df(t,H);</math>|3={{EquationRef|20}}}}
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   −
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>
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<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}
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\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
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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 +
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<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
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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
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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,  
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correlation function <math>h(r,t)\ ,</math> with <math>H=0</math> again
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for simplicity.  In the re-scaled model, <math>t</math> becomes
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<math>L^yt\ ,</math> as before, while <math>r</math> becomes
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<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
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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,  
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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}}}}
   −
with
  −
a scaling function <math>G\ .</math>  Comparing this with
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\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>
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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].
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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.
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  −
   
==See also==
 
==See also==
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