13.1

Problem 13.1

peskinChapter 13

习题 13.1

来源: 第13章, PDF第466页


13.1 Correction-to-scaling exponent. For critical phenomena in 4ϵ4 - \epsilon dimensions, the irrelevant contributions that disappear most slowly are those associated with the deviation of the coupling constant λ\lambda from its fixed-point value. This gives the most important nonuniversal correction to the scaling laws derived in Section 13.1. By studying the solution of the Callan-Symanzik equation, show that if the bare value of λ\lambda differs slightly from λ\lambda_*, the Gibbs free energy receives a correction

G(M,t)G(M,t)(1+(λλ)tωνk^(tM1/β)).G(M, t) \rightarrow G(M, t) \cdot (1 + (\lambda - \lambda_*) t^{\omega \nu} \hat{k}(t M^{-1/\beta})).

This formula defines a new critical exponent ω\omega, called the correction-to-scaling exponent. Show that

ω=ddλβλ=ϵ+O(ϵ2).\omega = \frac{d}{d\lambda} \beta \bigg|_{\lambda_*} = \epsilon + \mathcal{O}(\epsilon^2).

习题 13.1 - 解答


习题分析

4ϵ4-\epsilon 维的临界现象中,系统的宏观物理量(如吉布斯自由能)在临界点附近表现出标度行为。这种标度行为可以通过重整化群的 Callan-Symanzik (CS) 方程来推导。当系统的裸耦合常数 λ\lambda 并不严格等于红外不动点 λ\lambda_* 时,耦合常数随能标的流动会给纯粹的标度律带来修正。由于 λ\lambda 趋向 λ\lambda_* 的速度由 β\beta 函数在不动点处的斜率决定,这自然引出了修正标度指数 ω\omega

下面分步通过求解 CS 方程来推导自由能的修正形式,并计算 ω\omegaϵ\epsilon 展开下的首阶结果。

1. Callan-Symanzik 方程与特征线解

吉布斯自由能 G(M,t,λ,μ)G(M, t, \lambda, \mu) 满足如下的 CS 方程:

[μμ+β(λ)λγm(λ)ttγ(λ)MM]G(M,t,λ,μ)=0\left[ \mu \frac{\partial}{\partial \mu} + \beta(\lambda) \frac{\partial}{\partial \lambda} - \gamma_m(\lambda) t \frac{\partial}{\partial t} - \gamma(\lambda) M \frac{\partial}{\partial M} \right] G(M, t, \lambda, \mu) = 0

利用特征线法,引入无量纲的流动参数 ρ\rho,定义跑动参数:

dλˉdlogρ=β(λˉ),λˉ(1)=λ\frac{d \bar{\lambda}}{d \log \rho} = \beta(\bar{\lambda}), \quad \bar{\lambda}(1) = \lambda
dlogtˉdlogρ=γm(λˉ),tˉ(1)=t\frac{d \log \bar{t}}{d \log \rho} = - \gamma_m(\bar{\lambda}), \quad \bar{t}(1) = t
dlogMˉdlogρ=γ(λˉ),Mˉ(1)=M\frac{d \log \bar{M}}{d \log \rho} = - \gamma(\bar{\lambda}), \quad \bar{M}(1) = M

CS 方程的解表明,自由能在标度变换下满足:

G(M,t,λ,μ)=G(Mˉ(ρ),tˉ(ρ),λˉ(ρ),ρμ)G(M, t, \lambda, \mu) = G(\bar{M}(\rho), \bar{t}(\rho), \bar{\lambda}(\rho), \rho \mu)

2. 不动点附近的参数演化

在红外极限(ρ0\rho \to 0)下,跑动耦合常数 λˉ\bar{\lambda} 趋向于红外不动点 λ\lambda_*,满足 β(λ)=0\beta(\lambda_*) = 0。在 λ\lambda_* 附近对 β\beta 函数进行泰勒展开:

β(λˉ)ω(λˉλ),其中ωdβdλλ\beta(\bar{\lambda}) \approx \omega (\bar{\lambda} - \lambda_*), \quad \text{其中} \quad \omega \equiv \frac{d\beta}{d\lambda}\bigg|_{\lambda_*}

代入 λˉ\bar{\lambda} 的流动方程并积分,得到:

λˉ(ρ)λ=(λλ)ρω\bar{\lambda}(\rho) - \lambda_* = (\lambda - \lambda_*) \rho^\omega

对于跑动温度 tˉ(ρ)\bar{t}(\rho),在 λ\lambda_* 附近展开反常标度维数 γm(λˉ)γm+γm(λˉλ)\gamma_m(\bar{\lambda}) \approx \gamma_m^* + \gamma_m'^* (\bar{\lambda} - \lambda_*),积分得到:

tˉ(ρ)=texp(1ργm(λˉ(ρ))dρρ)tργm[1γmω(λλ)(ρω1)]\bar{t}(\rho) = t \exp\left( - \int_1^\rho \gamma_m(\bar{\lambda}(\rho')) \frac{d\rho'}{\rho'} \right) \approx t \rho^{-\gamma_m^*} \left[ 1 - \frac{\gamma_m'^*}{\omega} (\lambda - \lambda_*) (\rho^\omega - 1) \right]

同理,跑动磁化强度 Mˉ(ρ)\bar{M}(\rho) 为:

Mˉ(ρ)Mργ[1γω(λλ)(ρω1)]\bar{M}(\rho) \approx M \rho^{-\gamma^*} \left[ 1 - \frac{\gamma'^*}{\omega} (\lambda - \lambda_*) (\rho^\omega - 1) \right]

3. 自由能的标度修正

由量纲分析,自由能密度 GG 的质量量纲为 dd

G(Mˉ,tˉ,λˉ,ρμ)=(ρμ)dΦ(Mˉ(ρμ)d/21+,tˉ(ρμ)2,λˉ)G(\bar{M}, \bar{t}, \bar{\lambda}, \rho \mu) = (\rho \mu)^d \Phi\left( \frac{\bar{M}}{(\rho \mu)^{d/2-1+\dots}}, \frac{\bar{t}}{(\rho \mu)^2}, \bar{\lambda} \right)

为了提取临界标度行为,我们选择特定的 ρ\rho 使得 tˉ(ρ)/(ρμ)2=1\bar{t}(\rho) / (\rho \mu)^2 = 1。在零阶近似下,tˉ(ρ)tργm\bar{t}(\rho) \approx t \rho^{-\gamma_m^*},因此:

tργm=ρ2μ2    ρt12+γm=tνt \rho^{-\gamma_m^*} = \rho^2 \mu^2 \implies \rho \propto t^{\frac{1}{2 + \gamma_m^*}} = t^\nu

其中 ν=1/(2+γm)\nu = 1/(2 + \gamma_m^*) 是关联长度的临界指数。 此时,修正项中的 ρω\rho^\omega 变为:

ρωtων\rho^\omega \propto t^{\omega \nu}

λˉ(ρ)\bar{\lambda}(\rho)tˉ(ρ)\bar{t}(\rho)Mˉ(ρ)\bar{M}(\rho) 代入无量纲函数 Φ\Phi 中,并在 λ\lambda_* 处展开。所有由于 λλ\lambda \neq \lambda_* 引起的一阶修正项均正比于 λˉ(ρ)λ(λλ)ρω\bar{\lambda}(\rho) - \lambda_* \propto (\lambda - \lambda_*) \rho^\omega。因此,自由能可以写为零阶标度项加上一阶修正项:

G(M,t)G0(M,t)[1+(λλ)tωνk^(tM1/β)]G(M, t) \rightarrow G_0(M, t) \left[ 1 + (\lambda - \lambda_*) t^{\omega \nu} \hat{k}(t M^{-1/\beta}) \right]

其中 k^\hat{k} 是依赖于标度不变量 tM1/βt M^{-1/\beta} 的无量纲函数。这就证明了修正标度指数 ω\omega 的存在及其定义。

4. 计算修正标度指数 ω\omega

d=4ϵd = 4 - \epsilon 维的 ϕ4\phi^4 理论中,单圈近似下的 β\beta 函数为:

β(λ)=ϵλ+316π2λ2+O(λ3)\beta(\lambda) = -\epsilon \lambda + \frac{3}{16\pi^2} \lambda^2 + \mathcal{O}(\lambda^3)

寻找非平凡的 Wilson-Fisher 不动点 λ0\lambda_* \neq 0,令 β(λ)=0\beta(\lambda_*) = 0

ϵλ+316π2λ2=0    λ=16π23ϵ+O(ϵ2)-\epsilon \lambda_* + \frac{3}{16\pi^2} \lambda_*^2 = 0 \implies \lambda_* = \frac{16\pi^2}{3} \epsilon + \mathcal{O}(\epsilon^2)

根据定义,计算 β\beta 函数在 λ\lambda_* 处的导数:

ω=dβdλλ=ϵ+616π2λ\omega = \frac{d\beta}{d\lambda}\bigg|_{\lambda_*} = -\epsilon + \frac{6}{16\pi^2} \lambda_*

λ\lambda_* 的表达式代入上式:

ω=ϵ+616π2(16π23ϵ)=ϵ+2ϵ=ϵ\omega = -\epsilon + \frac{6}{16\pi^2} \left( \frac{16\pi^2}{3} \epsilon \right) = -\epsilon + 2\epsilon = \epsilon

因此,我们得到修正标度指数的首阶结果:

ω=dβdλλ=ϵ+O(ϵ2)\boxed{ \omega = \frac{d\beta}{d\lambda}\bigg|_{\lambda_*} = \epsilon + \mathcal{O}(\epsilon^2) }
13.2

Problem 13.2

peskinChapter 13

习题 13.2

来源: 第13章, PDF第466页


13.2 The exponent η\eta. By combining the result of Problem 10.3 with an appropriate renormalization prescription, show that the leading term in γ(λ)\gamma(\lambda) in ϕ4\phi^4 theory is

γ=λ212(4π)4.\gamma = \frac{\lambda^2}{12(4\pi)^4}.

Generalize this result to the O(N)O(N)-symmetric ϕ4\phi^4 theory to derive Eq. (13.47). Compute the leading-order (ϵ2\epsilon^2) contribution to η\eta.


Referenced Equations:

Equation (13.47):

γ=(N+2)λ24(8π2)2+O(λ3).(13.47)\gamma = (N+2) \frac{\lambda^2}{4(8\pi^2)^2} + \mathcal{O}(\lambda^3). \tag{13.47}

习题 13.2 - 解答


习题分析与解答

1. 单一标量场 ϕ4\phi^4 理论中的反常标度因数 γ(λ)\gamma(\lambda)

ϕ4\phi^4 理论中,拉格朗日量为 L=12(ϕ)212m2ϕ2λ4!ϕ4\mathcal{L} = \frac{1}{2}(\partial\phi)^2 - \frac{1}{2}m^2\phi^2 - \frac{\lambda}{4!}\phi^4。波函数重整化常数 Z=1+δZZ = 1 + \delta_Z 由单粒子不可约(1PI)两点函数 Σ(p2)\Sigma(p^2) 的发散部分决定。为了抵消发散,要求 p2δZΣ(p2)p^2 \delta_Z - \Sigma(p^2) 为有限值。

根据习题 10.3 的结果,对 Σ(p2)\Sigma(p^2) 产生领头阶(O(λ2)\mathcal{O}(\lambda^2))贡献的是双圈“日落图”(sunset diagram)。其振幅为: iΣ(p)=(iλ)23!ddk(2π)dddq(2π)dik2iq2i(pkq)2-i\Sigma(p) = \frac{(-i\lambda)^2}{3!} \int \frac{d^d k}{(2\pi)^d} \frac{d^d q}{(2\pi)^d} \frac{i}{k^2} \frac{i}{q^2} \frac{i}{(p-k-q)^2} 在维数正规化(d=4ϵd = 4 - \epsilon)下,将动量积分转到欧几里得空间,积分的极点部分为: ddk(2π)dddq(2π)dik2iq2i(pkq)2=ip22ϵ(4π)4+finite\int \frac{d^d k}{(2\pi)^d} \frac{d^d q}{(2\pi)^d} \frac{i}{k^2} \frac{i}{q^2} \frac{i}{(p-k-q)^2} = -i \frac{p^2}{2\epsilon(4\pi)^4} + \text{finite} 代入自能表达式中,得到: iΣ(p)=λ26(ip22ϵ(4π)4)=iλ212ϵ(4π)4p2    Σ(p)=λ212ϵ(4π)4p2-i\Sigma(p) = -\frac{\lambda^2}{6} \left( -i \frac{p^2}{2\epsilon(4\pi)^4} \right) = i \frac{\lambda^2}{12\epsilon(4\pi)^4} p^2 \implies \Sigma(p) = -\frac{\lambda^2}{12\epsilon(4\pi)^4} p^2 为了消除发散,动能反项必须满足 δZ=pole part of Σ(p)p2\delta_Z = \text{pole part of } \frac{\Sigma(p)}{p^2},因此: δZ=λ212ϵ(4π)4\delta_Z = -\frac{\lambda^2}{12\epsilon(4\pi)^4} 在最小减除(MS)方案中,反常标度因数 γ(λ)\gamma(\lambda) 的定义为: γ(λ)=12μddμlnZ12β(λ)δZλ\gamma(\lambda) = \frac{1}{2} \mu \frac{d}{d\mu} \ln Z \approx \frac{1}{2} \beta(\lambda) \frac{\partial \delta_Z}{\partial \lambda} 代入领头阶的 β\beta 函数 β(λ)=ϵλ+O(λ2)\beta(\lambda) = -\epsilon \lambda + \mathcal{O}(\lambda^2),可得: γ(λ)=12(ϵλ)(2λ12ϵ(4π)4)=λ212(4π)4\gamma(\lambda) = \frac{1}{2} (-\epsilon \lambda) \left( -\frac{2\lambda}{12\epsilon(4\pi)^4} \right) = \frac{\lambda^2}{12(4\pi)^4} 这证明了单一标量场 ϕ4\phi^4 理论中 γ\gamma 的领头阶结果。


2. 推广至 O(N)O(N) 对称的 ϕ4\phi^4 理论并推导 Eq. (13.47)

对于 O(N)O(N) 对称理论,相互作用项为 ΔL=λ4(ϕiϕi)2\Delta \mathcal{L} = -\frac{\lambda}{4} (\phi^i \phi^i)^2。对应的四点顶点规则为: Vijkl=2iλ(δijδkl+δikδjl+δilδjk)V_{ijkl} = -2i\lambda (\delta_{ij}\delta_{kl} + \delta_{ik}\delta_{jl} + \delta_{il}\delta_{jk}) 计算外线指标为 aabb 的日落图时,需要对内部三个传播子的指标 i,j,ki, j, k 求和。顶点因子的收缩为: i,j,kVaijkVbijk=(2iλ)2i,j,k(δaiδjk+δajδik+δakδij)(δbiδjk+δbjδik+δbkδij)\sum_{i,j,k} V_{aijk} V_{bijk} = (-2i\lambda)^2 \sum_{i,j,k} (\delta_{ai}\delta_{jk} + \delta_{aj}\delta_{ik} + \delta_{ak}\delta_{ij}) (\delta_{bi}\delta_{jk} + \delta_{bj}\delta_{ik} + \delta_{bk}\delta_{ij}) 展开并利用 δii=N\delta_{ii} = N,上述指标求和给出 3Nδab+6δab=3(N+2)δab3N \delta_{ab} + 6 \delta_{ab} = 3(N+2)\delta_{ab}。因此,日落图的对称因子 1/3!1/3! 与顶点收缩结合后给出: iΣab(p)=13![4λ2×3(N+2)δab](ip22ϵ(4π)4)=iλ2(N+2)ϵ(4π)4p2δab-i\Sigma^{ab}(p) = \frac{1}{3!} \left[ -4\lambda^2 \times 3(N+2)\delta^{ab} \right] \left( -i \frac{p^2}{2\epsilon(4\pi)^4} \right) = i \frac{\lambda^2(N+2)}{\epsilon(4\pi)^4} p^2 \delta^{ab} 由此得到 O(N)O(N) 理论的波函数重整化反项为: δZ=λ2(N+2)ϵ(4π)4\delta_Z = -\frac{\lambda^2(N+2)}{\epsilon(4\pi)^4} 同理,利用 γ=12β(λ)δZλ\gamma = \frac{1}{2} \beta(\lambda) \frac{\partial \delta_Z}{\partial \lambda},得到 O(N)O(N) 理论的反常标度因数: γ(λ)=12(ϵλ)(2λ(N+2)ϵ(4π)4)=(N+2)λ2(4π)4\gamma(\lambda) = \frac{1}{2} (-\epsilon \lambda) \left( -\frac{2\lambda(N+2)}{\epsilon(4\pi)^4} \right) = \frac{(N+2)\lambda^2}{(4\pi)^4} 注意到 (4π)4=256π4=4(8π2)2(4\pi)^4 = 256\pi^4 = 4(8\pi^2)^2,将其代入分母,即成功推导出 Eq. (13.47)γ(λ)=(N+2)λ24(8π2)2+O(λ3)\gamma(\lambda) = (N+2) \frac{\lambda^2}{4(8\pi^2)^2} + \mathcal{O}(\lambda^3)


3. 计算临界指数 η\eta 的领头阶(O(ϵ2)\mathcal{O}(\epsilon^2))贡献

临界指数 η\eta 描述了在 Wilson-Fisher 不动点 λ\lambda_* 处两点关联函数的标度行为 G(p)p2+ηG(p) \sim p^{-2+\eta}。由 Callan-Symanzik 方程可知,它与反常标度因数的关系为: η=2γ(λ)\eta = 2\gamma(\lambda_*)d=4ϵd = 4 - \epsilon 维下,O(N)O(N) 理论的 β\beta 函数到单圈阶为: β(λ)=ϵλ+N+88π2λ2\beta(\lambda) = -\epsilon \lambda + \frac{N+8}{8\pi^2} \lambda^2β(λ)=0\beta(\lambda_*) = 0,解得 Wilson-Fisher 不动点的耦合常数为: λ=8π2ϵN+8\lambda_* = \frac{8\pi^2 \epsilon}{N+8}λ\lambda_* 代入前面求得的 γ(λ)\gamma(\lambda) 表达式中: γ(λ)=(N+2)14(8π2)2(8π2ϵN+8)2=N+24(N+8)2ϵ2\gamma(\lambda_*) = (N+2) \frac{1}{4(8\pi^2)^2} \left( \frac{8\pi^2 \epsilon}{N+8} \right)^2 = \frac{N+2}{4(N+8)^2} \epsilon^2 最终得到临界指数 η\eta 的领头阶贡献为: η=N+22(N+8)2ϵ2\boxed{ \eta = \frac{N+2}{2(N+8)^2} \epsilon^2 }

13.3

Problem 13.3

peskinChapter 13

习题 13.3

来源: 第13章, PDF第466,467,468页


13.3 The CPNCP^N model. The nonlinear sigma model discussed in the text can be thought of as a quantum theory of fields that are coordinates on the unit sphere. A slightly more complicated space of high symmetry is complex projective space,

CPNCP^N. This space can be defined as the space of (N+1)(N+1)-dimensional complex vectors (z1,,zN+1)(z_1, \dots, z_{N+1}) subject to the condition

jzj2=1,\sum_j |z_j|^2 = 1,

with points related by an overall phase rotation identified, that is,

(eiαz1,,eiαzN+1)identified with(z1,,zN+1).(e^{i\alpha}z_1, \dots, e^{i\alpha}z_{N+1}) \quad \text{identified with} \quad (z_1, \dots, z_{N+1}).

In this problem, we study the two-dimensional quantum field theory whose fields are coordinates on this space.

(a) One way to represent a theory of coordinates on CPNCP^N is to write a Lagrangian depending on fields zj(x)z_j(x), subject to the constraint, which also has the local symmetry

zj(x)eiα(x)zj(x),z_j(x) \rightarrow e^{i\alpha(x)} z_j(x),

independently at each point xx. Show that the following Lagrangian has this symmetry:

L=1g2[μzj2zjμzj2].\mathcal{L} = \frac{1}{g^2} [|\partial_\mu z_j|^2 - |z_j^* \partial_\mu z_j|^2].

To prove the invariance, you will need to use the constraint on the zjz_j, and its consequence

zjμzj=(μzj)zj.z_j^* \partial_\mu z_j = -(\partial_\mu z_j^*) z_j.

Show that the nonlinear sigma model for the case N=3N=3 can be converted to the CPNCP^N model for the case N=1N=1 by the substitution

ni=zσiz,n^i = z^* \sigma^i z,

where σi\sigma^i are the Pauli sigma matrices.

(b) To write the Lagrangian in a simpler form, introduce a scalar Lagrange multiplier λ\lambda which implements the constraint and also a vector Lagrange multiplier AμA_\mu to express the local symmetry. More specifically, show that the Lagrangian of the CPNCP^N model is obtained from the Lagrangian

L=1g2[Dμzj2λ(zj21)],\mathcal{L} = \frac{1}{g^2} [|D_\mu z_j|^2 - \lambda(|z_j|^2 - 1)],

where Dμ=(μ+iAμ)D_\mu = (\partial_\mu + iA_\mu), by functionally integrating over the fields λ\lambda and AμA_\mu.

(c) We can solve the CPNCP^N model in the limit NN \rightarrow \infty by integrating over the fields zjz_j. Show that this integral leads to the expression

Z=DADλexp[Ntrlog(D2λ)+ig2d2xλ],Z = \int DAD\lambda \exp \left[ -N \operatorname{tr} \log(-D^2 - \lambda) + \frac{i}{g^2} \int d^2 x \lambda \right],

where we have kept only the leading terms for NN \rightarrow \infty, g2Ng^2 N fixed. Using methods similar to those we used for the nonlinear sigma model, examine the conditions for minimizing the exponent with respect to λ\lambda and AμA_\mu. Show that these conditions have a solution at Aμ=0A_\mu = 0 and λ=m2>0\lambda = m^2 > 0. Show that, if g2g^2 is renormalized at the scale MM, mm can be written as

m=Mexp[2πg2N].m = M \exp \left[ -\frac{2\pi}{g^2 N} \right].

** (d) ** Now expand the exponent about Aμ=0A_\mu = 0. Show that the first nontrivial term in this expansion is proportional to the vacuum polarization of massive scalar fields. Evaluate this expression using dimensional regularization, and show that it yields a standard kinetic energy term for AμA_\mu. Thus the strange nonlinear field theory that we started with is finally transformed into a theory of (N+1)(N + 1) massive scalar fields interacting with a massless photon.

习题 13.3 - 解答


(a) 局域对称性与 O(3)O(3) 非线性 σ\sigma 模型到 CP1CP^1 的转换

1. 证明拉格朗日量的局域 U(1)U(1) 对称性

考虑拉格朗日量: L=1g2[μzj2zjμzj2]\mathcal{L} = \frac{1}{g^2} \left[ |\partial_\mu z_j|^2 - |z_j^* \partial_\mu z_j|^2 \right] 在局域相位变换 zj(x)eiα(x)zj(x)z_j(x) \rightarrow e^{i\alpha(x)} z_j(x) 下,导数项变为: μzjeiα(μzj+i(μα)zj)\partial_\mu z_j \rightarrow e^{i\alpha} (\partial_\mu z_j + i (\partial_\mu \alpha) z_j) 计算第一项 μzj2|\partial_\mu z_j|^2 的变换: μzj2(μzjiμαzj)(μzj+iμαzj)=μzj2+iμα(zjμzjμzjzj)+(μα)2zj2|\partial_\mu z_j|^2 \rightarrow (\partial_\mu z_j^* - i \partial_\mu \alpha z_j^*)(\partial_\mu z_j + i \partial_\mu \alpha z_j) = |\partial_\mu z_j|^2 + i \partial_\mu \alpha (z_j^* \partial_\mu z_j - \partial_\mu z_j^* z_j) + (\partial_\mu \alpha)^2 |z_j|^2 利用约束条件 jzj2=1\sum_j |z_j|^2 = 1 及其推论 zjμzj=(μzj)zjz_j^* \partial_\mu z_j = -(\partial_\mu z_j^*) z_j,上式化简为: μzj2μzj2+2iμα(zjμzj)+(μα)2|\partial_\mu z_j|^2 \rightarrow |\partial_\mu z_j|^2 + 2i \partial_\mu \alpha (z_j^* \partial_\mu z_j) + (\partial_\mu \alpha)^2 计算第二项 zjμzj2|z_j^* \partial_\mu z_j|^2 的变换。首先看括号内的项: zjμzjeiαzjeiα(μzj+iμαzj)=zjμzj+iμαzj2=zjμzj+iμαz_j^* \partial_\mu z_j \rightarrow e^{-i\alpha} z_j^* e^{i\alpha} (\partial_\mu z_j + i \partial_\mu \alpha z_j) = z_j^* \partial_\mu z_j + i \partial_\mu \alpha |z_j|^2 = z_j^* \partial_\mu z_j + i \partial_\mu \alpha 取模平方: zjμzj+iμα2=zjμzj2iμα(zjμzjμzjzj)+(μα)2|z_j^* \partial_\mu z_j + i \partial_\mu \alpha|^2 = |z_j^* \partial_\mu z_j|^2 - i \partial_\mu \alpha (z_j^* \partial_\mu z_j - \partial_\mu z_j^* z_j) + (\partial_\mu \alpha)^2 同样利用 zjμzj=(μzj)zjz_j^* \partial_\mu z_j = -(\partial_\mu z_j^*) z_j,得到: zjμzj2zjμzj2+2iμα(zjμzj)+(μα)2|z_j^* \partial_\mu z_j|^2 \rightarrow |z_j^* \partial_\mu z_j|^2 + 2i \partial_\mu \alpha (z_j^* \partial_\mu z_j) + (\partial_\mu \alpha)^2 将两项相减,所有含 μα\partial_\mu \alpha 的项完全抵消: LL\boxed{ \mathcal{L} \rightarrow \mathcal{L} } 因此该拉格朗日量具有局域 U(1)U(1) 规范对称性。

2. N=3N=3 非线性 σ\sigma 模型到 CP1CP^1 模型的转换

O(3)O(3) 非线性 σ\sigma 模型的场为三维单位矢量 nin^i,拉格朗日量为 LO(3)=12gO(3)2(μni)2\mathcal{L}_{O(3)} = \frac{1}{2g_{O(3)}^2} (\partial_\mu n^i)^2。 代入 ni=zσizn^i = z^* \sigma^i z(其中 zz 为两组分复矢量,N=1N=1),计算导数: μni=(μz)σiz+zσi(μz)\partial_\mu n^i = (\partial_\mu z^\dagger) \sigma^i z + z^\dagger \sigma^i (\partial_\mu z) 平方并求和,利用泡利矩阵的完备性关系 σabiσcdi=2δadδbcδabδcd\sigma^i_{ab} \sigma^i_{cd} = 2\delta_{ad}\delta_{bc} - \delta_{ab}\delta_{cd}(μni)2=σabiσcdi[μzazb+zaμzb][μzczd+zcμzd](\partial_\mu n^i)^2 = \sigma^i_{ab} \sigma^i_{cd} [ \partial_\mu z^*_a z_b + z^*_a \partial_\mu z_b ] [ \partial^\mu z^*_c z_d + z^*_c \partial^\mu z_d ] 展开并应用完备性关系,利用 zz=1z^\dagger z = 1zμz=μzzz^\dagger \partial_\mu z = -\partial_\mu z^\dagger z(μni)2=2[(μzz)(μzz)+2μz2+(zμz)(μzz)][μ(zz)μ(zz)](\partial_\mu n^i)^2 = 2 [ (\partial_\mu z^\dagger z)(\partial^\mu z^\dagger z) + 2|\partial_\mu z|^2 + (z^\dagger \partial^\mu z)(\partial_\mu z^\dagger z) ] - [ \partial_\mu (z^\dagger z) \partial^\mu (z^\dagger z) ] 由于 zz=1z^\dagger z = 1,最后一项为 0。且 (μzz)=(zμz)(\partial_\mu z^\dagger z) = -(z^\dagger \partial_\mu z),故 (μzz)2=(zμz)2=zμz2(\partial_\mu z^\dagger z)^2 = (z^\dagger \partial_\mu z)^2 = -|z^\dagger \partial_\mu z|^2(因为 zμzz^\dagger \partial_\mu z 是纯虚数)。 代入化简得到: (μni)2=4(μz2zμz2)(\partial_\mu n^i)^2 = 4 \left( |\partial_\mu z|^2 - |z^\dagger \partial_\mu z|^2 \right) 因此,O(3)O(3) 模型的拉格朗日量变为: LO(3)=2gO(3)2[μz2zμz2]\boxed{ \mathcal{L}_{O(3)} = \frac{2}{g_{O(3)}^2} \left[ |\partial_\mu z|^2 - |z^\dagger \partial_\mu z|^2 \right] } 这正是 CP1CP^1 模型的拉格朗日量(只需重新定义耦合常数 g2=gO(3)2/2g^2 = g_{O(3)}^2 / 2)。


(b) 引入辅助场重写拉格朗日量

考虑带有拉格朗日乘子 λ\lambda 和规范场 AμA_\mu 的拉格朗日量: L=1g2[Dμzj2λ(zj21)]\mathcal{L} = \frac{1}{g^2} \left[ |D_\mu z_j|^2 - \lambda(|z_j|^2 - 1) \right] 其中 Dμ=μ+iAμD_\mu = \partial_\mu + iA_\mu。 首先对 λ\lambda 进行泛函积分,这会产生一个 δ\delta 泛函 δ(zj21)\delta(|z_j|^2 - 1),从而严格实现约束 zj2=1|z_j|^2 = 1。 在约束成立的前提下,展开 Dμzj2|D_\mu z_j|^2Dμzj2=(μzjiAμzj)(μzj+iAμzj)=μzj2+iAμ(zjμzjμzjzj)+AμAμzj2|D_\mu z_j|^2 = (\partial_\mu z_j^* - iA_\mu z_j^*)(\partial^\mu z_j + iA^\mu z_j) = |\partial_\mu z_j|^2 + iA^\mu (z_j^* \partial_\mu z_j - \partial_\mu z_j^* z_j) + A_\mu A^\mu |z_j|^2 利用 zj2=1|z_j|^2 = 1zjμzj=μzjzjz_j^* \partial_\mu z_j = -\partial_\mu z_j^* z_j,上式化为: Dμzj2=μzj2+2iAμ(zjμzj)+AμAμ|D_\mu z_j|^2 = |\partial_\mu z_j|^2 + 2i A^\mu (z_j^* \partial_\mu z_j) + A_\mu A^\mu 接下来对 AμA_\mu 进行泛函积分。由于这是关于 AμA_\mu 的高斯积分,积分结果等价于将 AμA_\mu 的经典运动方程代回拉格朗日量。对 AμA_\mu 变分求极值: LAμ=1g2[2i(zjμzj)+2Aμ]=0    Aμ=i(zjμzj)\frac{\partial \mathcal{L}}{\partial A^\mu} = \frac{1}{g^2} \left[ 2i (z_j^* \partial_\mu z_j) + 2A_\mu \right] = 0 \implies A_\mu = -i (z_j^* \partial_\mu z_j) 将此 AμA_\mu 代回拉格朗日量: L=1g2[μzj2+2i(izjμzj)(zjμzj)+(izjμzj)2]\mathcal{L} = \frac{1}{g^2} \left[ |\partial_\mu z_j|^2 + 2i (-i z_j^* \partial_\mu z_j)(z_j^* \partial^\mu z_j) + (-i z_j^* \partial_\mu z_j)^2 \right] L=1g2[μzj2+2(zjμzj)2(zjμzj)2]=1g2[μzj2+(zjμzj)2]\mathcal{L} = \frac{1}{g^2} \left[ |\partial_\mu z_j|^2 + 2(z_j^* \partial_\mu z_j)^2 - (z_j^* \partial_\mu z_j)^2 \right] = \frac{1}{g^2} \left[ |\partial_\mu z_j|^2 + (z_j^* \partial_\mu z_j)^2 \right] 由于 zjμzjz_j^* \partial_\mu z_j 是纯虚数,其平方等于负的模平方,即 (zjμzj)2=zjμzj2(z_j^* \partial_\mu z_j)^2 = -|z_j^* \partial_\mu z_j|^2。因此: L=1g2[μzj2zjμzj2]\boxed{ \mathcal{L} = \frac{1}{g^2} \left[ |\partial_\mu z_j|^2 - |z_j^* \partial_\mu z_j|^2 \right] }


(c) 大 NN 极限与质量能隙方程

在泛函积分中积掉 NN 个复标量场 zjz_j。作用量中关于 zjz_j 的二次项为 d2x1g2zj(D2λ)zj\int d^2x \frac{1}{g^2} z_j^* (-D^2 - \lambda) z_j。高斯积分给出行列式 [det(D2λ)]N[\det(-D^2 - \lambda)]^{-N}。 将其写到指数上,并保留大 NN 领头项,配分函数变为: Z=DADλexp[Ntrlog(D2λ)+ig2d2xλ]Z = \int DA D\lambda \exp \left[ -N \operatorname{tr} \log(-D^2 - \lambda) + \frac{i}{g^2} \int d^2 x \lambda \right] 寻找指数的鞍点(极值条件)。对 AμA_\mu 变分,由于洛伦兹不变性和宇称对称性,真空中流的期望值为零,故存在解 Aμ=0A_\mu = 0。 在 Aμ=0A_\mu = 0 处,对 λ\lambda 变分得到间隙方程(设鞍点处 λ=m2>0\lambda = m^2 > 0): Ntr[12m2]+ig2d2x=0-N \operatorname{tr} \left[ \frac{-1}{-\partial^2 - m^2} \right] + \frac{i}{g^2} \int d^2x = 0 转到动量空间并进行 Wick 转动到欧几里得空间(k0=ikE0,k2=kE2k^0 = i k^0_E, k^2 = -k_E^2): Nd2kE(2π)21kE2+m2=1g2N \int \frac{d^2 k_E}{(2\pi)^2} \frac{1}{k_E^2 + m^2} = \frac{1}{g^2} 引入紫外截断 MM 计算积分: N4πlog(M2+m2m2)N4πlog(M2m2)=1g2\frac{N}{4\pi} \log\left(\frac{M^2 + m^2}{m^2}\right) \approx \frac{N}{4\pi} \log\left(\frac{M^2}{m^2}\right) = \frac{1}{g^2} 解此方程得到动态生成的质量 mmlog(Mm)=2πg2N    m=Mexp[2πg2N]\log\left(\frac{M}{m}\right) = \frac{2\pi}{g^2 N} \implies \boxed{ m = M \exp \left[ -\frac{2\pi}{g^2 N} \right] }


(d) 展开有效作用量与光子动能项的生成

Aμ=0A_\mu = 0 附近展开有效作用量 Ntrlog(D2m2)-N \operatorname{tr} \log(-D^2 - m^2)。 算符 D2m2=2m2iμAμ2iAμμ+A2-D^2 - m^2 = -\partial^2 - m^2 - i\partial_\mu A^\mu - 2i A^\mu \partial_\mu + A^2。记自由传播子逆为 Δ=2m2\Delta = -\partial^2 - m^2,微扰项为 δV=i(A)2iA+A2\delta V = -i(\partial \cdot A) - 2i A \cdot \partial + A^2。 利用 log(Δ+δV)=logΔ+Δ1δV12(Δ1δV)2+\log(\Delta + \delta V) = \log \Delta + \Delta^{-1} \delta V - \frac{1}{2} (\Delta^{-1} \delta V)^2 + \dots,提取 AμA_\mu 的二次项,这正是 NN 个质量为 mm 的复标量场的真空极化图(Vacuum Polarization)贡献: Seff(2)=12d2q(2π)2Aμ(q)Πμν(q)Aν(q)S_{\text{eff}}^{(2)} = \frac{1}{2} \int \frac{d^2 q}{(2\pi)^2} A_\mu(q) \Pi^{\mu\nu}(q) A_\nu(-q) 使用维数正规化(d=2ϵd=2-\epsilon)计算标量 QED 的真空极化张量 Πμν(q)\Pi^{\mu\nu}(q)。由规范不变性可知 Πμν(q)=(q2gμνqμqν)Π(q2)\Pi^{\mu\nu}(q) = (q^2 g^{\mu\nu} - q^\mu q^\nu) \Pi(q^2)。 单圈图包含泡泡图和蝌蚪图,结合费曼参数法,其横向部分的标量函数为: Π(q2)=2N(4π)d/2Γ(2d2)01dxx(1x)[m2x(1x)q2]2d/2\Pi(q^2) = \frac{2N}{(4\pi)^{d/2}} \Gamma\left(2-\frac{d}{2}\right) \int_0^1 dx \frac{x(1-x)}{[m^2 - x(1-x)q^2]^{2-d/2}}d2d \rightarrow 2 极限下,Γ(1)=1\Gamma(1) = 1,分母指数为 11Π(q2)=N2π01dxx(1x)m2x(1x)q2\Pi(q^2) = \frac{N}{2\pi} \int_0^1 dx \frac{x(1-x)}{m^2 - x(1-x)q^2} 在低能极限 q20q^2 \rightarrow 0 下展开: Π(0)=N2πm201dxx(1x)=N2πm2(1213)=N12πm2\Pi(0) = \frac{N}{2\pi m^2} \int_0^1 dx \, x(1-x) = \frac{N}{2\pi m^2} \left( \frac{1}{2} - \frac{1}{3} \right) = \frac{N}{12\pi m^2} 代回有效作用量,在坐标空间中,(q2gμνqμqν)AμAν(q^2 g^{\mu\nu} - q^\mu q^\nu) A_\mu A_\nu 对应于 12FμνFμν\frac{1}{2} F_{\mu\nu} F^{\mu\nu}。因此,有效拉格朗日量中产生了 AμA_\mu 的标准动能项: Lkin=N48πm2FμνFμν\boxed{ \mathcal{L}_{\text{kin}} = \frac{N}{48\pi m^2} F_{\mu\nu} F^{\mu\nu} } 这表明,原本没有动能项的辅助场 AμA_\mu 通过量子修正获得了标准的麦克斯韦动能项,成为一个动力学的无质量光子,而 zjz_j 场则表现为与之相互作用的 (N+1)(N+1) 个质量为 mm 的复标量场。