Why correlation function decay as power law at critical temperature point?

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At the critical temperature point, the correlation function decays as a power law due to the behavior of the correlation length, which approaches infinity. As one nears the critical point, the correlation length increases, causing distant parts of the system to influence each other significantly. This transition from exponential decay to algebraic decay occurs because, at the critical point, there is no characteristic length scale, leading to a lack of decay over any specific distance. The mathematical representation shows that the correlation functions become algebraic, indicating a universal behavior at criticality. Understanding this phenomenon is crucial in the study of phase transitions in statistical physics.
ndung200790
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Please teach me this:
In QTF theory of Schroeder,chapter 13.1 saying:
Just at t=0(t=\frac{T-T_{c}}{T_{c}}),the correlation should decay as power law.
Define the exponent \eta by the formula:
G(x)=\frac{1}{x^{d-2+\eta}}
where d is Euclidien space dimension.
I do not understand why at critical point, the correlation function decay as power law.Please give me a to favour to explain this.
Thank you very much in advance.
 
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I would like to add that I am saying about the second phase transition in statistical physics using method of Quantum Field Theory
 
as one approaches a critical point the correlation length starts increasing, i.e. units farther and farther away becomes aware of each others dynamics.
in math terms the correlation functions \sim e^{-r/\chi}, where \chi is the correlation length, and r is the distance from your origin. this \chi grows as one approaches the critical point.

this feature reaches its maximum at the critical point where \chi \rightarrow \infty, i.e. every part of the system becomes aware of every other part. this is the reason the correlation functions become algebraic from exponential. one can approximately see this effect if one writes r^{-a} = e^{-\frac{r}{r(a\ln{r})^{-1}}}. compare it with e^{-r/\chi}. one sees that in the critical case there is no length scale like \chi. hence correlation functions don't decay over any characteristic length scale. therefore they have algebraic decay, which lacks any length scale.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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