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       <dc:date>2026-05-04T15:29:51+00:00</dc:date>
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        <title>statphys</title>
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        <dc:date>2023-09-05T15:46:55+00:00</dc:date>
        <dc:creator>Anonymous (anonymous@undisclosed.example.com)</dc:creator>
        <title>김민재:스터디:임계현상:1장._임계현상의_기본적_내용</title>
        <link>https://statphys.pknu.ac.kr/dokuwiki/doku.php?id=%EA%B9%80%EB%AF%BC%EC%9E%AC:%EC%8A%A4%ED%84%B0%EB%94%94:%EC%9E%84%EA%B3%84%ED%98%84%EC%83%81:1%EC%9E%A5._%EC%9E%84%EA%B3%84%ED%98%84%EC%83%81%EC%9D%98_%EA%B8%B0%EB%B3%B8%EC%A0%81_%EB%82%B4%EC%9A%A9&amp;rev=1693896415&amp;do=diff</link>
        <description>임계점과 질서변수

대부분의 경우 질량, 총 에너지, 자기 모멘트 등을 부피로 나누어 밀도로 나타낸 것을 역학적 변수라고 한다. 여기에 압력, 온도, 자기장과 같은 것들은 어떤 물리계가 놓인 외부적 상황을 나타낸다. 이런 것들을 외부 장이라 한다. 대부분의 경우, 외부장이 하나의 값으로 결정된다면 역학적 변수들은 그 값이 유일하게 결정될 수 있다. 하지만 몇 가지 특별한 역학적 변수들은 외부 장이 결정 되더라도 그 값을 결정 할 수 없다. 다음은 그러한 경우의 예이다.$H_2O$$T = 273~\text{K}$$p = 1~\text{atm}$$\rho$$(T_c,p_c)$$\boldsymbol{m}$$\boldsymbol{h}$$0$$T&gt;T_c$$T_c$$(T=T_c, h=0)$$T&gt;T_c$$m=0$$(h=0)$$\rho$$\boldsymbol{m}$$T_c~(K)$$_2$$_2$$\lambda-$$^4-$$^4$$\quad\sim\quad$$0K$$0$$T$$0$$T_c$$0$$T…</description>
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        <dc:date>2023-09-05T15:46:55+00:00</dc:date>
        <dc:creator>Anonymous (anonymous@undisclosed.example.com)</dc:creator>
        <title>김민재:스터디:임계현상:2장._여러_모형의_기본적_개념</title>
        <link>https://statphys.pknu.ac.kr/dokuwiki/doku.php?id=%EA%B9%80%EB%AF%BC%EC%9E%AC:%EC%8A%A4%ED%84%B0%EB%94%94:%EC%9E%84%EA%B3%84%ED%98%84%EC%83%81:2%EC%9E%A5._%EC%97%AC%EB%9F%AC_%EB%AA%A8%ED%98%95%EC%9D%98_%EA%B8%B0%EB%B3%B8%EC%A0%81_%EA%B0%9C%EB%85%90&amp;rev=1693896415&amp;do=diff</link>
        <description>순서 테스트</description>
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        <dc:date>2023-09-05T15:46:55+00:00</dc:date>
        <dc:creator>Anonymous (anonymous@undisclosed.example.com)</dc:creator>
        <title>김민재:스터디:임계현상:3장._가우스_근사</title>
        <link>https://statphys.pknu.ac.kr/dokuwiki/doku.php?id=%EA%B9%80%EB%AF%BC%EC%9E%AC:%EC%8A%A4%ED%84%B0%EB%94%94:%EC%9E%84%EA%B3%84%ED%98%84%EC%83%81:3%EC%9E%A5._%EA%B0%80%EC%9A%B0%EC%8A%A4_%EA%B7%BC%EC%82%AC&amp;rev=1693896415&amp;do=diff</link>
        <description>긴즈버그-란다우 모형

긴즈버그-란다우 모형은 시스템의 해밀토니안이 다음과 같이 적힐 수 있음을 가정하는 것이다.
$$\frac{H[\sigma]}{T}=\int d^{d}x[a_{0}+a_{2}\sigma^{2}+a_{4}\sigma^{4}+c(\nabla\sigma)^{2}-\boldsymbol h\cdot\boldsymbol\sigma]$$
여기서 $\sigma^{2},\,\sigma^{2},\,(\nabla\sigma)^{2}$는 다음과 같이 정의된다.

$$\sigma^{2}\equiv\boldsymbol\sigma(\boldsymbol x)\cdot\boldsymbol\sigma(\boldsymbol x)\equiv\sum_{i=1}^{n}(\sigma_{i}(x))^{2},$$
$$\sigma^{2}\equiv(\sigma^{2})^{2},$$
$$(\nabla\sigma)^2\equiv\sum_{\alpha=1}^d\sum_{i=1}^n\left(\frac{\parti…</description>
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        <dc:date>2023-09-05T15:46:55+00:00</dc:date>
        <dc:creator>Anonymous (anonymous@undisclosed.example.com)</dc:creator>
        <title>김민재:스터디:임계현상:미완료_계산</title>
        <link>https://statphys.pknu.ac.kr/dokuwiki/doku.php?id=%EA%B9%80%EB%AF%BC%EC%9E%AC:%EC%8A%A4%ED%84%B0%EB%94%94:%EC%9E%84%EA%B3%84%ED%98%84%EC%83%81:%EB%AF%B8%EC%99%84%EB%A3%8C_%EA%B3%84%EC%82%B0&amp;rev=1693896415&amp;do=diff</link>
        <description>긴즈버그 기준

식 $(3.26)$
$$ \Delta C = \frac{T_c^2{a_2^\prime}^2}{2a_4} $$

식 $(3.39)$
\begin{equation}
\begin{split}
C &amp;= n \left[ \frac{1}{2} \left( \frac{Ta_2^\prime}{c} \right)^2 (2\pi)^-d \int d^dk^\prime (1+{k^\prime}^2)^-2 \right] \xi^{4-d} + l.s \\
&amp;\equiv C_0\xi^{4-d} + l.s
\end{split}
\end{equation}

$$C_{0}\approx\left(\frac{Ta_{2}^{\prime}}{c}\right)^{2}(2\pi)^{2}$$
로 두고 $\xi^{-1}\equiv\left(\frac{a_{2}^{\prime}}{c}\right)^{\frac{1}{2}}|T-T_{c}|^{\frac{1}{2}}$을 사용하여 $\frac{C_{0}\xi^{4-d}}…</description>
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