3.1

Problem 3.1

srednickiChapter 3

习题 3.1

来源: 第3章, PDF第43页


3.1 Derive eq. (3.29) from eqs. (3.21), (3.24), and (3.28).


Referenced Equations:

Equation (3.21):

a(k)=d3xeikx[i0φ(x)+ωφ(x)]=id3xeikx0φ(x),(3.21)\begin{aligned} a(\mathbf{k}) &= \int d^3 x e^{-i k x} \left[ i \partial_0 \varphi(x) + \omega \varphi(x) \right] \\ &= i \int d^3 x e^{-i k x} \overleftrightarrow{\partial}_0 \varphi(x) \, , \end{aligned} \tag{3.21}

Equation (3.24):

Π(x)=φ˙(x)(3.24)\Pi(x) = \dot{\varphi}(x) \tag{3.24}

Equation (3.28):

[φ(x,t),φ(x,t)]=0,[Π(x,t),Π(x,t)]=0,[φ(x,t),Π(x,t)]=iδ3(xx).\begin{align} [\varphi(\mathbf{x}, t), \varphi(\mathbf{x}', t)] &= 0 , \\ [\Pi(\mathbf{x}, t), \Pi(\mathbf{x}', t)] &= 0 , \\ [\varphi(\mathbf{x}, t), \Pi(\mathbf{x}', t)] &= i\delta^3(\mathbf{x} - \mathbf{x}') . \tag{3.28} \\ \end{align}

Equation (3.29):

[a(k),a(k)]=0,[a(k),a(k)]=0,[a(k),a(k)]=(2π)32ω δ3(kk).\begin{align} [a(\mathbf{k}), a(\mathbf{k}')] &= 0 , \\ [a^\dagger(\mathbf{k}), a^\dagger(\mathbf{k}')] &= 0 , \\ [a(\mathbf{k}), a^\dagger(\mathbf{k}')] &= (2\pi)^3 2\omega \ \delta^3(\mathbf{k} - \mathbf{k}') . \tag{3.29} \\ \end{align}

习题 3.1 - 解答


物理背景与分析 本题旨在从自由标量场的等时对易关系(Equal-Time Commutation Relations, ETCR)出发,推导产生与湮灭算符 a(k)a^\dagger(\mathbf{k})a(k)a(\mathbf{k}) 的对易关系。这是正则量子化过程中的核心步骤,它将场算符的量子化条件转化为动量空间中粒子态的代数结构,从而建立起多粒子 Fock 空间。

推导过程

首先,根据式 (3.21) 和 (3.24),将湮灭算符 a(k)a(\mathbf{k}) 及其厄米共轭(产生算符) a(k)a^\dagger(\mathbf{k}) 用场算符 φ(x)\varphi(x) 和共轭动量 Π(x)\Pi(x) 表示。 已知四维内积 kx=ωktkxkx = \omega_k t - \mathbf{k} \cdot \mathbf{x},其中 ωk=k2+m2\omega_k = \sqrt{\mathbf{k}^2 + m^2}。将 Π(x)=0φ(x)\Pi(x) = \partial_0 \varphi(x) 代入式 (3.21) 可得:

a(k)=d3xeiωkt+ikx[ωkφ(x,t)+iΠ(x,t)]a(\mathbf{k}) = \int d^3 x e^{-i \omega_k t + i \mathbf{k} \cdot \mathbf{x}} \left[ \omega_k \varphi(\mathbf{x}, t) + i \Pi(\mathbf{x}, t) \right]

由于 φ(x)\varphi(x)Π(x)\Pi(x) 均为厄米算符,对上式取厄米共轭可得产生算符:

a(k)=d3xeiωktikx[ωkφ(x,t)iΠ(x,t)]a^\dagger(\mathbf{k}) = \int d^3 x e^{i \omega_k t - i \mathbf{k} \cdot \mathbf{x}} \left[ \omega_k \varphi(\mathbf{x}, t) - i \Pi(\mathbf{x}, t) \right]

由于算符 a(k)a(\mathbf{k})a(k)a^\dagger(\mathbf{k}) 是守恒量(不随时间演化),我们可以选择在同一时刻 tt 计算它们的对易子。

1. 计算 [a(k),a(k)][a(\mathbf{k}), a(\mathbf{k}')]

利用积分表达式展开对易子:

[a(k),a(k)]=d3xd3yeiωkt+ikxeiωkt+iky[ωkφ(x,t)+iΠ(x,t),ωkφ(y,t)+iΠ(y,t)][a(\mathbf{k}), a(\mathbf{k}')] = \int d^3 x \int d^3 y e^{-i \omega_k t + i \mathbf{k} \cdot \mathbf{x}} e^{-i \omega_{k'} t + i \mathbf{k}' \cdot \mathbf{y}} \left[ \omega_k \varphi(\mathbf{x}, t) + i \Pi(\mathbf{x}, t), \omega_{k'} \varphi(\mathbf{y}, t) + i \Pi(\mathbf{y}, t) \right]

利用式 (3.28) 给出的等时对易关系:

[φ(x,t),φ(y,t)]=0,[Π(x,t),Π(y,t)]=0,[φ(x,t),Π(y,t)]=iδ3(xy)[\varphi(\mathbf{x}, t), \varphi(\mathbf{y}, t)] = 0, \quad [\Pi(\mathbf{x}, t), \Pi(\mathbf{y}, t)] = 0, \quad [\varphi(\mathbf{x}, t), \Pi(\mathbf{y}, t)] = i\delta^3(\mathbf{x} - \mathbf{y})

展开被积函数中的对易子:

[ωkφ(x,t)+iΠ(x,t),ωkφ(y,t)+iΠ(y,t)]=iωk[φ(x,t),Π(y,t)]+iωk[Π(x,t),φ(y,t)]=iωk(iδ3(xy))+iωk(iδ3(xy))=(ωk+ωk)δ3(xy)\begin{aligned} &\left[ \omega_k \varphi(\mathbf{x}, t) + i \Pi(\mathbf{x}, t), \omega_{k'} \varphi(\mathbf{y}, t) + i \Pi(\mathbf{y}, t) \right] \\ &= i \omega_k [\varphi(\mathbf{x}, t), \Pi(\mathbf{y}, t)] + i \omega_{k'} [\Pi(\mathbf{x}, t), \varphi(\mathbf{y}, t)] \\ &= i \omega_k (i \delta^3(\mathbf{x} - \mathbf{y})) + i \omega_{k'} (-i \delta^3(\mathbf{x} - \mathbf{y})) \\ &= (-\omega_k + \omega_{k'}) \delta^3(\mathbf{x} - \mathbf{y}) \end{aligned}

将其代回积分中,并利用 δ\delta 函数完成对 y\mathbf{y} 的积分:

[a(k),a(k)]=d3xei(ωk+ωk)t+i(k+k)x(ωk+ωk)=ei(ωk+ωk)t(ωk+ωk)d3xei(k+k)x=ei(ωk+ωk)t(ωk+ωk)(2π)3δ3(k+k)\begin{aligned} [a(\mathbf{k}), a(\mathbf{k}')] &= \int d^3 x e^{-i (\omega_k + \omega_{k'}) t + i (\mathbf{k} + \mathbf{k}') \cdot \mathbf{x}} (-\omega_k + \omega_{k'}) \\ &= e^{-i (\omega_k + \omega_{k'}) t} (-\omega_k + \omega_{k'}) \int d^3 x e^{i (\mathbf{k} + \mathbf{k}') \cdot \mathbf{x}} \\ &= e^{-i (\omega_k + \omega_{k'}) t} (-\omega_k + \omega_{k'}) (2\pi)^3 \delta^3(\mathbf{k} + \mathbf{k}') \end{aligned}

由于 δ3(k+k)\delta^3(\mathbf{k} + \mathbf{k}') 要求 k=k\mathbf{k}' = -\mathbf{k},此时 ωk=(k)2+m2=ωk\omega_{k'} = \sqrt{(-\mathbf{k})^2 + m^2} = \omega_k。因此因子 (ωk+ωk)=0(-\omega_k + \omega_{k'}) = 0,从而得到:

[a(k),a(k)]=0\boxed{ [a(\mathbf{k}), a(\mathbf{k}')] = 0 }

2. 计算 [a(k),a(k)][a^\dagger(\mathbf{k}), a^\dagger(\mathbf{k}')]

对上述结果直接取厄米共轭,利用对易子的性质 [A,B]=[A,B][A, B]^\dagger = -[A^\dagger, B^\dagger],可得:

[a(k),a(k)]=[a(k),a(k)]=0[a^\dagger(\mathbf{k}), a^\dagger(\mathbf{k}')] = -[a(\mathbf{k}), a(\mathbf{k}')]^\dagger = 0

或者通过完全类似的积分计算,对易子部分变为 (ωkωk)δ3(xy)(\omega_k - \omega_{k'}) \delta^3(\mathbf{x} - \mathbf{y}),同样由于 δ3(k+k)\delta^3(\mathbf{k} + \mathbf{k}') 使得 ωk=ωk\omega_k = \omega_{k'},结果为零:

[a(k),a(k)]=0\boxed{ [a^\dagger(\mathbf{k}), a^\dagger(\mathbf{k}')] = 0 }

3. 计算 [a(k),a(k)][a(\mathbf{k}), a^\dagger(\mathbf{k}')]

展开对易子:

[a(k),a(k)]=d3xd3yeiωkt+ikxeiωktiky[ωkφ(x,t)+iΠ(x,t),ωkφ(y,t)iΠ(y,t)][a(\mathbf{k}), a^\dagger(\mathbf{k}')] = \int d^3 x \int d^3 y e^{-i \omega_k t + i \mathbf{k} \cdot \mathbf{x}} e^{i \omega_{k'} t - i \mathbf{k}' \cdot \mathbf{y}} \left[ \omega_k \varphi(\mathbf{x}, t) + i \Pi(\mathbf{x}, t), \omega_{k'} \varphi(\mathbf{y}, t) - i \Pi(\mathbf{y}, t) \right]

计算被积函数中的对易子:

[ωkφ(x,t)+iΠ(x,t),ωkφ(y,t)iΠ(y,t)]=iωk[φ(x,t),Π(y,t)]+iωk[Π(x,t),φ(y,t)]=iωk(iδ3(xy))+iωk(iδ3(xy))=(ωk+ωk)δ3(xy)\begin{aligned} &\left[ \omega_k \varphi(\mathbf{x}, t) + i \Pi(\mathbf{x}, t), \omega_{k'} \varphi(\mathbf{y}, t) - i \Pi(\mathbf{y}, t) \right] \\ &= -i \omega_k [\varphi(\mathbf{x}, t), \Pi(\mathbf{y}, t)] + i \omega_{k'} [\Pi(\mathbf{x}, t), \varphi(\mathbf{y}, t)] \\ &= -i \omega_k (i \delta^3(\mathbf{x} - \mathbf{y})) + i \omega_{k'} (-i \delta^3(\mathbf{x} - \mathbf{y})) \\ &= (\omega_k + \omega_{k'}) \delta^3(\mathbf{x} - \mathbf{y}) \end{aligned}

代回积分并对 y\mathbf{y} 积分:

[a(k),a(k)]=d3xei(ωkωk)t+i(kk)x(ωk+ωk)=ei(ωkωk)t(ωk+ωk)d3xei(kk)x=ei(ωkωk)t(ωk+ωk)(2π)3δ3(kk)\begin{aligned} [a(\mathbf{k}), a^\dagger(\mathbf{k}')] &= \int d^3 x e^{-i (\omega_k - \omega_{k'}) t + i (\mathbf{k} - \mathbf{k}') \cdot \mathbf{x}} (\omega_k + \omega_{k'}) \\ &= e^{-i (\omega_k - \omega_{k'}) t} (\omega_k + \omega_{k'}) \int d^3 x e^{i (\mathbf{k} - \mathbf{k}') \cdot \mathbf{x}} \\ &= e^{-i (\omega_k - \omega_{k'}) t} (\omega_k + \omega_{k'}) (2\pi)^3 \delta^3(\mathbf{k} - \mathbf{k}') \end{aligned}

狄拉克 δ\delta 函数 δ3(kk)\delta^3(\mathbf{k} - \mathbf{k}') 强制要求 k=k\mathbf{k}' = \mathbf{k},这蕴含着 ωk=ωk\omega_{k'} = \omega_k。 因此,时间演化相位因子 ei(ωkωk)t=e0=1e^{-i (\omega_k - \omega_{k'}) t} = e^0 = 1,且能量因子 (ωk+ωk)=2ωk(\omega_k + \omega_{k'}) = 2\omega_k。代入后得到最终结果:

[a(k),a(k)]=(2π)32ωkδ3(kk)\boxed{ [a(\mathbf{k}), a^\dagger(\mathbf{k}')] = (2\pi)^3 2\omega_k \delta^3(\mathbf{k} - \mathbf{k}') }

至此,式 (3.29) 的三个对易关系已全部推导完毕。

3.2

Problem 3.2

srednickiChapter 3

习题 3.2

来源: 第3章, PDF第43页


3.2 Use the commutation relations, eq. (3.29), to show explicitly that a state of the form

k1kna(k1)a(kn)0(3.33)|k_1 \dots k_n\rangle \equiv a^\dagger(\mathbf{k}_1) \dots a^\dagger(\mathbf{k}_n)|0\rangle \tag{3.33}

is an eigenstate of the hamiltonian, eq. (3.30), with eigenvalue ω1++ωn\omega_1 + \dots + \omega_n. The vacuum 0|0\rangle is annihilated by a(k)a(\mathbf{k}), a(k)0=0a(\mathbf{k})|0\rangle = 0, and we take Ω0=E0\Omega_0 = \mathcal{E}_0 in eq. (3.30).


Referenced Equations:

Equation (3.29):

[a(k),a(k)]=0,[a(k),a(k)]=0,[a(k),a(k)]=(2π)32ω δ3(kk).\begin{align} [a(\mathbf{k}), a(\mathbf{k}')] &= 0 , \\ [a^\dagger(\mathbf{k}), a^\dagger(\mathbf{k}')] &= 0 , \\ [a(\mathbf{k}), a^\dagger(\mathbf{k}')] &= (2\pi)^3 2\omega \ \delta^3(\mathbf{k} - \mathbf{k}') . \tag{3.29} \\ \end{align}

Equation (3.30):

H=dk~ ω a(k)a(k)+(E0Ω0)V,(3.30)H = \int \widetilde{dk} \ \omega \ a^\dagger(\mathbf{k}) a(\mathbf{k}) + (\mathcal{E}_0 - \Omega_0)V, \tag{3.30}

习题 3.2 - 解答


题目分析

本题要求证明由 nn 个产生算符作用在真空态上构成的多粒子态 k1kn|k_1 \dots k_n\rangle 是自由场哈密顿量 HH 的本征态,并求出其本征值。 根据题意,取 E0=Ω0\mathcal{E}_0 = \Omega_0,哈密顿量常数项抵消,式 (3.30) 简化为:

H=dk~ ωk a(k)a(k)H = \int \widetilde{dk} \ \omega_{\mathbf{k}} \ a^\dagger(\mathbf{k}) a(\mathbf{k})

其中,dk~\widetilde{dk} 是洛伦兹不变的相空间测度,其定义与对易关系式 (3.29) 相匹配,即 dk~=d3k(2π)32ωk\widetilde{dk} = \frac{d^3k}{(2\pi)^3 2\omega_{\mathbf{k}}}ωk\omega_{\mathbf{k}} 代表动量为 k\mathbf{k} 的粒子的能量。

要计算 HH 作用在态 k1kn|k_1 \dots k_n\rangle 上的结果,核心技巧是利用对易关系计算单粒子产生算符与哈密顿量的对易子 [H,a(p)][H, a^\dagger(\mathbf{p})],然后将 HH 逐次向右对易,直到其直接作用于真空态 0|0\rangle 上并将其湮灭。

解题过程

第一步:计算基本对易子 [H,a(p)][H, a^\dagger(\mathbf{p})]

利用算符对易关系恒等式 [AB,C]=A[B,C]+[A,C]B[AB, C] = A[B, C] + [A, C]B,我们计算哈密顿量密度与产生算符的对易关系:

[a(k)a(k),a(p)]=a(k)[a(k),a(p)]+[a(k),a(p)]a(k)[a^\dagger(\mathbf{k}) a(\mathbf{k}), a^\dagger(\mathbf{p})] = a^\dagger(\mathbf{k}) [a(\mathbf{k}), a^\dagger(\mathbf{p})] + [a^\dagger(\mathbf{k}), a^\dagger(\mathbf{p})] a(\mathbf{k})

根据式 (3.29) 给出的对易关系 [a(k),a(p)]=0[a^\dagger(\mathbf{k}), a^\dagger(\mathbf{p})] = 0 以及 [a(k),a(p)]=(2π)32ωk δ3(kp)[a(\mathbf{k}), a^\dagger(\mathbf{p})] = (2\pi)^3 2\omega_{\mathbf{k}} \ \delta^3(\mathbf{k} - \mathbf{p}),上式化简为:

[a(k)a(k),a(p)]=a(k)((2π)32ωk δ3(kp))[a^\dagger(\mathbf{k}) a(\mathbf{k}), a^\dagger(\mathbf{p})] = a^\dagger(\mathbf{k}) \left( (2\pi)^3 2\omega_{\mathbf{k}} \ \delta^3(\mathbf{k} - \mathbf{p}) \right)

将其代入哈密顿量 HH 的积分中:

[H,a(p)]=dk~ ωk [a(k)a(k),a(p)]=d3k(2π)32ωk ωk a(k)((2π)32ωk δ3(kp))=d3k ωk a(k)δ3(kp)\begin{align} [H, a^\dagger(\mathbf{p})] &= \int \widetilde{dk} \ \omega_{\mathbf{k}} \ [a^\dagger(\mathbf{k}) a(\mathbf{k}), a^\dagger(\mathbf{p})] \\ &= \int \frac{d^3k}{(2\pi)^3 2\omega_{\mathbf{k}}} \ \omega_{\mathbf{k}} \ a^\dagger(\mathbf{k}) \left( (2\pi)^3 2\omega_{\mathbf{k}} \ \delta^3(\mathbf{k} - \mathbf{p}) \right) \\ &= \int d^3k \ \omega_{\mathbf{k}} \ a^\dagger(\mathbf{k}) \delta^3(\mathbf{k} - \mathbf{p}) \end{align}

利用狄拉克 δ\delta 函数的性质完成对 k\mathbf{k} 的积分,得到:

[H,a(p)]=ωpa(p)(1)[H, a^\dagger(\mathbf{p})] = \omega_{\mathbf{p}} a^\dagger(\mathbf{p}) \tag{1}

这表明产生算符 a(p)a^\dagger(\mathbf{p}) 具有将系统能量增加 ωp\omega_{\mathbf{p}} 的作用。该关系也可等价写为:

Ha(p)=a(p)H+ωpa(p)(2)H a^\dagger(\mathbf{p}) = a^\dagger(\mathbf{p}) H + \omega_{\mathbf{p}} a^\dagger(\mathbf{p}) \tag{2}

第二步:确定哈密顿量对真空态的作用

已知真空态满足 a(k)0=0a(\mathbf{k})|0\rangle = 0,因此哈密顿量作用于真空态的结果为:

H0=dk~ ωk a(k)a(k)0=0(3)H|0\rangle = \int \widetilde{dk} \ \omega_{\mathbf{k}} \ a^\dagger(\mathbf{k}) a(\mathbf{k}) |0\rangle = 0 \tag{3}

即真空态的能量本征值为 00

第三步:计算 HH 对多粒子态 k1kn|k_1 \dots k_n\rangle 的作用

将哈密顿量作用于目标态:

Hk1kn=Ha(k1)a(k2)a(kn)0H |k_1 \dots k_n\rangle = H a^\dagger(\mathbf{k}_1) a^\dagger(\mathbf{k}_2) \dots a^\dagger(\mathbf{k}_n)|0\rangle

利用式 (2),将 HH 与最左侧的 a(k1)a^\dagger(\mathbf{k}_1) 交换位置:

Hk1kn=(a(k1)H+ω1a(k1))a(k2)a(kn)0H |k_1 \dots k_n\rangle = \left( a^\dagger(\mathbf{k}_1) H + \omega_1 a^\dagger(\mathbf{k}_1) \right) a^\dagger(\mathbf{k}_2) \dots a^\dagger(\mathbf{k}_n)|0\rangle

其中简记 ωiωki\omega_i \equiv \omega_{\mathbf{k}_i}。展开后得到:

Hk1kn=ω1a(k1)a(kn)0+a(k1)Ha(k2)a(kn)0H |k_1 \dots k_n\rangle = \omega_1 a^\dagger(\mathbf{k}_1) \dots a^\dagger(\mathbf{k}_n)|0\rangle + a^\dagger(\mathbf{k}_1) H a^\dagger(\mathbf{k}_2) \dots a^\dagger(\mathbf{k}_n)|0\rangle

继续将 HHa(k2)a^\dagger(\mathbf{k}_2) 交换位置:

Hk1kn=ω1k1kn+a(k1)(a(k2)H+ω2a(k2))a(kn)0=(ω1+ω2)k1kn+a(k1)a(k2)Ha(kn)0\begin{align} H |k_1 \dots k_n\rangle &= \omega_1 |k_1 \dots k_n\rangle + a^\dagger(\mathbf{k}_1) \left( a^\dagger(\mathbf{k}_2) H + \omega_2 a^\dagger(\mathbf{k}_2) \right) \dots a^\dagger(\mathbf{k}_n)|0\rangle \\ &= (\omega_1 + \omega_2) |k_1 \dots k_n\rangle + a^\dagger(\mathbf{k}_1) a^\dagger(\mathbf{k}_2) H \dots a^\dagger(\mathbf{k}_n)|0\rangle \end{align}

重复此过程(即通过数学归纳法),将 HH 逐次向右移动穿过所有的产生算符,每次交换都会产生一个对应的能量项 ωi\omega_i

Hk1kn=(ω1+ω2++ωn)a(k1)a(kn)0+a(k1)a(kn)H0H |k_1 \dots k_n\rangle = (\omega_1 + \omega_2 + \dots + \omega_n) a^\dagger(\mathbf{k}_1) \dots a^\dagger(\mathbf{k}_n)|0\rangle + a^\dagger(\mathbf{k}_1) \dots a^\dagger(\mathbf{k}_n) H |0\rangle

根据式 (3),最右侧的 H0=0H|0\rangle = 0,因此最后一项消失。最终得到:

Hk1kn=(ω1++ωn)k1knH |k_1 \dots k_n\rangle = (\omega_1 + \dots + \omega_n) |k_1 \dots k_n\rangle

结论

上述推导明确表明,态 k1kn|k_1 \dots k_n\rangle 是哈密顿量 HH 的本征态,其对应的本征值为各个单粒子能量之和。

Hk1kn=(ω1++ωn)k1kn\boxed{ H |k_1 \dots k_n\rangle = (\omega_1 + \dots + \omega_n) |k_1 \dots k_n\rangle }
3.3

Problem 3.3

srednickiChapter 3

习题 3.3

来源: 第3章, PDF第43页


3.3 Use U(Λ)1φ(x)U(Λ)=φ(Λ1x)U(\Lambda)^{-1}\varphi(x)U(\Lambda) = \varphi(\Lambda^{-1}x) to show that

U(Λ)1a(k)U(Λ)=a(Λ1k),U(Λ)1a(k)U(Λ)=a(Λ1k),(3.34)\begin{aligned} U(\Lambda)^{-1}a(\mathbf{k})U(\Lambda) &= a(\Lambda^{-1}\mathbf{k}) , \\ U(\Lambda)^{-1}a^\dagger(\mathbf{k})U(\Lambda) &= a^\dagger(\Lambda^{-1}\mathbf{k}) , \end{aligned} \tag{3.34}

and hence that

U(Λ)k1kn=Λk1Λkn,(3.35)U(\Lambda)|k_1 \dots k_n\rangle = |\Lambda k_1 \dots \Lambda k_n\rangle , \tag{3.35}

where k1kn=a(k1)a(kn)0|k_1 \dots k_n\rangle = a^\dagger(\mathbf{k}_1) \dots a^\dagger(\mathbf{k}_n)|0\rangle is a state of nn particles with momenta k1,,knk_1, \dots, k_n.

习题 3.3 - 解答


习题分析与物理背景

在相对论性量子场论中,标量场 φ(x)\varphi(x) 在洛伦兹变换下作为一个标量函数变换,即 U(Λ)1φ(x)U(Λ)=φ(Λ1x)U(\Lambda)^{-1}\varphi(x)U(\Lambda) = \varphi(\Lambda^{-1}x)。为了探究这一变换对动量空间中的产生算符 a(k)a^\dagger(\mathbf{k}) 和湮灭算符 a(k)a(\mathbf{k}) 的影响,我们需要利用自由标量场的傅里叶展开。

关键的物理概念在于洛伦兹不变的动量积分测度。通常,标量场展开为:

φ(x)=dk~[a(k)eikx+a(k)eikx]\varphi(x) = \int d\tilde{k} \left[ a(\mathbf{k}) e^{-ik \cdot x} + a^\dagger(\mathbf{k}) e^{ik \cdot x} \right]

其中 dk~d\tilde{k} 是洛伦兹不变测度(例如 dk~=d3k(2π)32ωkd\tilde{k} = \frac{d^3k}{(2\pi)^3 2\omega_k})。利用测度的不变性以及四维内积的洛伦兹不变性,我们可以直接提取出算符的变换规律。进而,通过在产生算符之间插入幺正算符的恒等式 U1U=IU^{-1}U = I,并结合真空态的洛伦兹不变性,可以推导出多粒子态的变换行为。


解题过程

(1) 证明产生与湮灭算符的变换规律

首先,写出标量场 φ(x)\varphi(x) 的傅里叶展开式:

φ(x)=dk~[a(k)eikx+a(k)eikx]\varphi(x) = \int d\tilde{k} \left[ a(\mathbf{k}) e^{-ik \cdot x} + a^\dagger(\mathbf{k}) e^{ik \cdot x} \right]

对场算符应用洛伦兹变换的幺正算符 U(Λ)U(\Lambda)

U(Λ)1φ(x)U(Λ)=dk~[U(Λ)1a(k)U(Λ)eikx+U(Λ)1a(k)U(Λ)eikx]U(\Lambda)^{-1}\varphi(x)U(\Lambda) = \int d\tilde{k} \left[ U(\Lambda)^{-1}a(\mathbf{k})U(\Lambda) e^{-ik \cdot x} + U(\Lambda)^{-1}a^\dagger(\mathbf{k})U(\Lambda) e^{ik \cdot x} \right]

根据题意,场算符的变换满足 U(Λ)1φ(x)U(Λ)=φ(Λ1x)U(\Lambda)^{-1}\varphi(x)U(\Lambda) = \varphi(\Lambda^{-1}x)。我们将 Λ1x\Lambda^{-1}x 代入场的展开式中:

φ(Λ1x)=dk~[a(k)eik(Λ1x)+a(k)eik(Λ1x)]\varphi(\Lambda^{-1}x) = \int d\tilde{k} \left[ a(\mathbf{k}) e^{-ik \cdot (\Lambda^{-1}x)} + a^\dagger(\mathbf{k}) e^{ik \cdot (\Lambda^{-1}x)} \right]

利用四维矢量的内积性质,我们知道 k(Λ1x)=(Λk)xk \cdot (\Lambda^{-1}x) = (\Lambda k) \cdot x。因此上式可以写为:

φ(Λ1x)=dk~[a(k)ei(Λk)x+a(k)ei(Λk)x]\varphi(\Lambda^{-1}x) = \int d\tilde{k} \left[ a(\mathbf{k}) e^{-i(\Lambda k) \cdot x} + a^\dagger(\mathbf{k}) e^{i(\Lambda k) \cdot x} \right]

为了与 U(Λ)1φ(x)U(Λ)U(\Lambda)^{-1}\varphi(x)U(\Lambda) 的表达式进行对比,我们对积分变量进行代换。令 k=Λkk' = \Lambda k,由于积分测度 dk~d\tilde{k} 是洛伦兹不变的,故有 dk~=dk~d\tilde{k}' = d\tilde{k}。同时,逆变换给出 k=Λ1kk = \Lambda^{-1}k'。代入积分中得到:

φ(Λ1x)=dk~[a(Λ1k)eikx+a(Λ1k)eikx]\varphi(\Lambda^{-1}x) = \int d\tilde{k}' \left[ a(\Lambda^{-1}\mathbf{k}') e^{-ik' \cdot x} + a^\dagger(\Lambda^{-1}\mathbf{k}') e^{ik' \cdot x} \right]

将积分哑变量 kk' 重新替换为 kk,我们得到:

φ(Λ1x)=dk~[a(Λ1k)eikx+a(Λ1k)eikx]\varphi(\Lambda^{-1}x) = \int d\tilde{k} \left[ a(\Lambda^{-1}\mathbf{k}) e^{-ik \cdot x} + a^\dagger(\Lambda^{-1}\mathbf{k}) e^{ik \cdot x} \right]

比较 U(Λ)1φ(x)U(Λ)U(\Lambda)^{-1}\varphi(x)U(\Lambda)φ(Λ1x)\varphi(\Lambda^{-1}x) 展开式中 eikxe^{-ik \cdot x}eikxe^{ik \cdot x} 的系数,由于平面波基底的线性独立性,必然有:

U(Λ)1a(k)U(Λ)=a(Λ1k)U(Λ)1a(k)U(Λ)=a(Λ1k)\boxed{ \begin{aligned} U(\Lambda)^{-1}a(\mathbf{k})U(\Lambda) &= a(\Lambda^{-1}\mathbf{k}) \\ U(\Lambda)^{-1}a^\dagger(\mathbf{k})U(\Lambda) &= a^\dagger(\Lambda^{-1}\mathbf{k}) \end{aligned} }

(2) 证明多粒子态的变换规律

已知 nn 粒子态定义为 k1kn=a(k1)a(kn)0|k_1 \dots k_n\rangle = a^\dagger(\mathbf{k}_1) \dots a^\dagger(\mathbf{k}_n)|0\rangle。我们需要计算 U(Λ)k1knU(\Lambda)|k_1 \dots k_n\rangle

首先,从前面得到的产生算符变换关系 U(Λ)1a(k)U(Λ)=a(Λ1k)U(\Lambda)^{-1}a^\dagger(\mathbf{k})U(\Lambda) = a^\dagger(\Lambda^{-1}\mathbf{k}) 出发。将该式中的 Λ\Lambda 替换为 Λ1\Lambda^{-1},得到:

U(Λ1)1a(k)U(Λ1)=a(Λk)U(\Lambda^{-1})^{-1}a^\dagger(\mathbf{k})U(\Lambda^{-1}) = a^\dagger(\Lambda\mathbf{k})

由于 UU 是洛伦兹群的幺正表示,满足 U(Λ1)=U(Λ)1U(\Lambda^{-1}) = U(\Lambda)^{-1},因此 U(Λ1)1=U(Λ)U(\Lambda^{-1})^{-1} = U(\Lambda)。上式即化简为:

U(Λ)a(k)U(Λ)1=a(Λk)U(\Lambda)a^\dagger(\mathbf{k})U(\Lambda)^{-1} = a^\dagger(\Lambda\mathbf{k})

现在,将 U(Λ)U(\Lambda) 作用于 nn 粒子态:

U(Λ)k1kn=U(Λ)a(k1)a(k2)a(kn)0U(\Lambda)|k_1 \dots k_n\rangle = U(\Lambda) a^\dagger(\mathbf{k}_1) a^\dagger(\mathbf{k}_2) \dots a^\dagger(\mathbf{k}_n) |0\rangle

在每一个产生算符之间插入恒等算符 I=U(Λ)1U(Λ)I = U(\Lambda)^{-1}U(\Lambda)

U(Λ)k1kn=[U(Λ)a(k1)U(Λ)1][U(Λ)a(k2)U(Λ)1][U(Λ)a(kn)U(Λ)1]U(Λ)0\begin{aligned} U(\Lambda)|k_1 \dots k_n\rangle &= \left[ U(\Lambda) a^\dagger(\mathbf{k}_1) U(\Lambda)^{-1} \right] \left[ U(\Lambda) a^\dagger(\mathbf{k}_2) U(\Lambda)^{-1} \right] \dots \left[ U(\Lambda) a^\dagger(\mathbf{k}_n) U(\Lambda)^{-1} \right] U(\Lambda) |0\rangle \end{aligned}

利用物理真空态的洛伦兹不变性,即 U(Λ)0=0U(\Lambda)|0\rangle = |0\rangle,并将前面推导的 U(Λ)a(k)U(Λ)1=a(Λk)U(\Lambda)a^\dagger(\mathbf{k})U(\Lambda)^{-1} = a^\dagger(\Lambda\mathbf{k}) 逐项代入:

U(Λ)k1kn=a(Λk1)a(Λk2)a(Λkn)0\begin{aligned} U(\Lambda)|k_1 \dots k_n\rangle &= a^\dagger(\Lambda\mathbf{k}_1) a^\dagger(\Lambda\mathbf{k}_2) \dots a^\dagger(\Lambda\mathbf{k}_n) |0\rangle \end{aligned}

根据多粒子态的定义,右侧正是动量分别为 Λk1,,Λkn\Lambda k_1, \dots, \Lambda k_nnn 粒子态。因此我们证明了:

U(Λ)k1kn=Λk1Λkn\boxed{ U(\Lambda)|k_1 \dots k_n\rangle = |\Lambda k_1 \dots \Lambda k_n\rangle }
3.4

Problem 3.4

srednickiChapter 3

习题 3.4

来源: 第3章, PDF第43页


3.4 Recall that T(a)1φ(x)T(a)=φ(xa)T(a)^{-1}\varphi(x)T(a) = \varphi(x - a), where T(a)exp(iPμaμ)T(a) \equiv \exp(-iP^\mu a_\mu) is the spacetime translation operator, and P0P^0 is identified as the hamiltonian HH.

a) Let aμa^\mu be infinitesimal, and derive an expression for [φ(x),Pμ][\varphi(x), P^\mu].

b) Show that the time component of your result is equivalent to the Heisenberg equation of motion iφ˙=[φ,H]i\dot{\varphi} = [\varphi, H].

c) For a free field, use the Heisenberg equation to derive the Klein-Gordon equation.

d) Define a spatial momentum operator

Pd3xΠ(x)φ(x).(3.36)\mathbf{P} \equiv - \int d^3x \, \Pi(x) \nabla \varphi(x) . \tag{3.36}

Use the canonical commutation relations to show that P\mathbf{P} obeys the relation you derived in part (a).

e) Express P\mathbf{P} in terms of a(k)a(\mathbf{k}) and a(k)a^\dagger(\mathbf{k}).

习题 3.4 - 解答


a) 推导 [φ(x),Pμ][\varphi(x), P^\mu]

已知时空平移算符为 T(a)exp(iPμaμ)T(a) \equiv \exp(-iP^\mu a_\mu),且满足 T(a)1φ(x)T(a)=φ(xa)T(a)^{-1}\varphi(x)T(a) = \varphi(x - a)。 当 aμa^\mu 为无穷小量时,我们可以将等式两侧保留至 aμa^\mu 的一阶项进行展开。 对于等式左侧,平移算符及其逆算符展开为: T(a)1iPμaμ,T(a)11+iPμaμT(a) \approx 1 - iP^\mu a_\mu, \quad T(a)^{-1} \approx 1 + iP^\mu a_\mu 代入左侧得到: (1+iPμaμ)φ(x)(1iPνaν)φ(x)+iaμPμφ(x)iaμφ(x)Pμ=φ(x)+iaμ[Pμ,φ(x)](1 + iP^\mu a_\mu)\varphi(x)(1 - iP^\nu a_\nu) \approx \varphi(x) + i a_\mu P^\mu \varphi(x) - i a_\mu \varphi(x) P^\mu = \varphi(x) + i a_\mu [P^\mu, \varphi(x)] 对于等式右侧,将场算符在 xx 处进行泰勒展开: φ(xa)φ(x)aμμφ(x)=φ(x)aμμφ(x)\varphi(x - a) \approx \varphi(x) - a^\mu \partial_\mu \varphi(x) = \varphi(x) - a_\mu \partial^\mu \varphi(x) 比较等式两侧的一阶项,得到: iaμ[Pμ,φ(x)]=aμμφ(x)i a_\mu [P^\mu, \varphi(x)] = - a_\mu \partial^\mu \varphi(x) 由于 aμa_\mu 是任意无穷小量,可将其消去,得到: i[Pμ,φ(x)]=μφ(x)i [P^\mu, \varphi(x)] = - \partial^\mu \varphi(x) 两边同乘 i-i 并利用对易子反对称性 [A,B]=[B,A][A, B] = -[B, A],得到最终结果: [φ(x),Pμ]=iμφ(x)\boxed{ [\varphi(x), P^\mu] = -i \partial^\mu \varphi(x) }

b) 证明其时间分量等价于海森堡运动方程

取 (a) 中结果的时间分量 μ=0\mu = 0[φ(x),P0]=i0φ(x)[\varphi(x), P^0] = -i \partial^0 \varphi(x) 已知 P0P^0 被等同于哈密顿量 HH。为了使该结果与标准的海森堡运动方程 iφ˙=[φ,H]i\dot{\varphi} = [\varphi, H] 符号完全一致,我们需要采用“多加”度规约定(mostly-plus metric signature)(,+,+,+)(-, +, +, +)。 在该度规下,坐标逆变与协变分量的关系为 xμ=(t,x)x^\mu = (t, \mathbf{x})xμ=(t,x)x_\mu = (-t, \mathbf{x}),因此导数算符满足 0=0=t\partial^0 = -\partial_0 = -\frac{\partial}{\partial t}。 代入上式可得: [φ(x),H]=i(φt)=iφ˙(x)[\varphi(x), H] = -i \left( -\frac{\partial \varphi}{\partial t} \right) = i \dot{\varphi}(x) 等式两边同乘 ii(注意 i2=1i^2 = -1),并交换对易子顺序: iφ˙(x)=[φ(x),H]\boxed{ i\dot{\varphi}(x) = [\varphi(x), H] } 这正是算符演化的海森堡运动方程。

c) 利用海森堡方程推导自由场的克莱因-高登方程

自由标量场的哈密顿量为: H=d3y12[Π(y)2+(yφ(y))2+m2φ(y)2]H = \int d^3y \, \frac{1}{2} \left[ \Pi(\mathbf{y})^2 + (\nabla_y \varphi(\mathbf{y}))^2 + m^2 \varphi(\mathbf{y})^2 \right] 利用等时正则对易关系 [φ(x),Π(y)]=iδ(3)(xy)[\varphi(\mathbf{x}), \Pi(\mathbf{y})] = i\delta^{(3)}(\mathbf{x}-\mathbf{y}) 以及 [φ(x),φ(y)]=0[\varphi(\mathbf{x}), \varphi(\mathbf{y})] = 0,计算 φ˙\dot{\varphi}φ˙(x)=i[φ(x),H]=id3y12[φ(x),Π(y)2]=id3yiδ(3)(xy)Π(y)=Π(x)\dot{\varphi}(\mathbf{x}) = -i [\varphi(\mathbf{x}), H] = -i \int d^3y \, \frac{1}{2} [\varphi(\mathbf{x}), \Pi(\mathbf{y})^2] = -i \int d^3y \, i\delta^{(3)}(\mathbf{x}-\mathbf{y}) \Pi(\mathbf{y}) = \Pi(\mathbf{x}) 接着计算 φ¨(x)=Π˙(x)=i[Π(x),H]\ddot{\varphi}(\mathbf{x}) = \dot{\Pi}(\mathbf{x}) = -i [\Pi(\mathbf{x}), H]。利用 [Π(x),Π(y)]=0[\Pi(\mathbf{x}), \Pi(\mathbf{y})] = 0[Π(x),φ(y)]=iδ(3)(xy)[\Pi(\mathbf{x}), \varphi(\mathbf{y})] = -i\delta^{(3)}(\mathbf{x}-\mathbf{y})[Π(x),H]=d3y12([Π(x),(yφ(y))2]+m2[Π(x),φ(y)2])[\Pi(\mathbf{x}), H] = \int d^3y \, \frac{1}{2} \left( [\Pi(\mathbf{x}), (\nabla_y \varphi(\mathbf{y}))^2] + m^2 [\Pi(\mathbf{x}), \varphi(\mathbf{y})^2] \right) 其中: [Π(x),(yφ(y))2]=2yφ(y)y[Π(x),φ(y)]=2yφ(y)y(iδ(3)(xy))[\Pi(\mathbf{x}), (\nabla_y \varphi(\mathbf{y}))^2] = 2 \nabla_y \varphi(\mathbf{y}) \cdot \nabla_y [\Pi(\mathbf{x}), \varphi(\mathbf{y})] = 2 \nabla_y \varphi(\mathbf{y}) \cdot \nabla_y (-i\delta^{(3)}(\mathbf{x}-\mathbf{y})) [Π(x),φ(y)2]=2φ(y)(iδ(3)(xy))[\Pi(\mathbf{x}), \varphi(\mathbf{y})^2] = 2 \varphi(\mathbf{y}) (-i\delta^{(3)}(\mathbf{x}-\mathbf{y})) 代入积分,并对第一项进行分部积分(假设边界项为零): [Π(x),H]=id3y[y2φ(y)δ(3)(xy)+m2φ(y)δ(3)(xy)]=i2φ(x)im2φ(x)[\Pi(\mathbf{x}), H] = -i \int d^3y \left[ -\nabla_y^2 \varphi(\mathbf{y}) \delta^{(3)}(\mathbf{x}-\mathbf{y}) + m^2 \varphi(\mathbf{y}) \delta^{(3)}(\mathbf{x}-\mathbf{y}) \right] = i \nabla^2 \varphi(\mathbf{x}) - i m^2 \varphi(\mathbf{x}) 因此: φ¨(x)=i(i2φ(x)im2φ(x))=2φ(x)m2φ(x)\ddot{\varphi}(\mathbf{x}) = -i \left( i \nabla^2 \varphi(\mathbf{x}) - i m^2 \varphi(\mathbf{x}) \right) = \nabla^2 \varphi(\mathbf{x}) - m^2 \varphi(\mathbf{x}) 移项并利用达朗贝尔算符 μμ=t2+2\partial_\mu \partial^\mu = -\partial_t^2 + \nabla^2(在 (,+,+,+)(-,+,+,+) 度规下),得到: (μμ+m2)φ(x)=0\boxed{ (\partial_\mu \partial^\mu + m^2)\varphi(x) = 0 } 此即克莱因-高登方程。

d) 证明空间动量算符 P\mathbf{P} 满足 (a) 中的关系

已知空间动量算符定义为: Pd3yΠ(y)yφ(y)\mathbf{P} \equiv - \int d^3y \, \Pi(\mathbf{y}) \nabla_y \varphi(\mathbf{y}) 计算 φ(x)\varphi(\mathbf{x})P\mathbf{P} 的对易子(注意 φ(x)\varphi(\mathbf{x})yφ(y)\nabla_y \varphi(\mathbf{y}) 对易): [φ(x),P]=d3y[φ(x),Π(y)]yφ(y)[\varphi(\mathbf{x}), \mathbf{P}] = - \int d^3y \, [\varphi(\mathbf{x}), \Pi(\mathbf{y})] \nabla_y \varphi(\mathbf{y}) 代入等时正则对易关系 [φ(x),Π(y)]=iδ(3)(xy)[\varphi(\mathbf{x}), \Pi(\mathbf{y})] = i\delta^{(3)}(\mathbf{x}-\mathbf{y})[φ(x),P]=d3yiδ(3)(xy)yφ(y)=iφ(x)[\varphi(\mathbf{x}), \mathbf{P}] = - \int d^3y \, i\delta^{(3)}(\mathbf{x}-\mathbf{y}) \nabla_y \varphi(\mathbf{y}) = -i \nabla \varphi(\mathbf{x})(,+,+,+)(-,+,+,+) 度规下,空间分量 μ=j\mu = j 满足 j=j=j\partial^j = \partial_j = \nabla^j。因此上式可写为分量形式: [φ(x),Pj]=ijφ(x)\boxed{ [\varphi(x), P^j] = -i \partial^j \varphi(x) } 这与 (a) 中推导的 [φ(x),Pμ]=iμφ(x)[\varphi(x), P^\mu] = -i \partial^\mu \varphi(x) 的空间分量完全一致。

e) 用产生和湮灭算符表达 P\mathbf{P}

写出自由标量场 φ(x)\varphi(\mathbf{x}) 和共轭动量 Π(x)\Pi(\mathbf{x})t=0t=0 时的动量空间展开式: φ(x)=d3k(2π)32ωk(a(k)eikx+a(k)eikx)\varphi(\mathbf{x}) = \int \frac{d^3k}{(2\pi)^3 \sqrt{2\omega_k}} \left( a(\mathbf{k}) e^{i\mathbf{k}\cdot\mathbf{x}} + a^\dagger(\mathbf{k}) e^{-i\mathbf{k}\cdot\mathbf{x}} \right) Π(x)=φ˙(x)=d3k(2π)32ωk(iωk)(a(k)eikxa(k)eikx)\Pi(\mathbf{x}) = \dot{\varphi}(\mathbf{x}) = \int \frac{d^3k}{(2\pi)^3 \sqrt{2\omega_k}} (-i\omega_k) \left( a(\mathbf{k}) e^{i\mathbf{k}\cdot\mathbf{x}} - a^\dagger(\mathbf{k}) e^{-i\mathbf{k}\cdot\mathbf{x}} \right) 计算 φ(x)\varphi(\mathbf{x}) 的空间梯度: φ(x)=d3k(2π)32ωk(ik)(a(k)eikxa(k)eikx)\nabla \varphi(\mathbf{x}) = \int \frac{d^3k'}{(2\pi)^3 \sqrt{2\omega_{k'}}} (i\mathbf{k}') \left( a(\mathbf{k}') e^{i\mathbf{k}'\cdot\mathbf{x}} - a^\dagger(\mathbf{k}') e^{-i\mathbf{k}'\cdot\mathbf{x}} \right) 将它们代入 P\mathbf{P} 的定义式中,并首先完成对 d3xd^3x 的空间积分。空间积分会产生狄拉克 δ\delta 函数 (2π)3δ(3)(k±k)(2\pi)^3 \delta^{(3)}(\mathbf{k} \pm \mathbf{k}'),从而消除 d3kd^3k' 的积分: P=d3k(2π)32ωk(ωkk)[a(k)a(k)a(k)a(k)a(k)a(k)+a(k)a(k)]\mathbf{P} = - \int \frac{d^3k}{(2\pi)^3 2\omega_k} (\omega_k \mathbf{k}) \left[ a(\mathbf{k})a(-\mathbf{k}) - a(\mathbf{k})a^\dagger(\mathbf{k}) - a^\dagger(\mathbf{k})a(\mathbf{k}) + a^\dagger(\mathbf{k})a^\dagger(-\mathbf{k}) \right] 由于积分域是对称的,且 k\mathbf{k} 是奇函数,而 a(k)a(k)a(\mathbf{k})a(-\mathbf{k})a(k)a(k)a^\dagger(\mathbf{k})a^\dagger(-\mathbf{k})kk\mathbf{k} \to -\mathbf{k} 下是偶函数,因此这两项的积分严格为零。剩下交叉项: P=d3k(2π)3k2[a(k)a(k)+a(k)a(k)]\mathbf{P} = \int \frac{d^3k}{(2\pi)^3} \frac{\mathbf{k}}{2} \left[ a(\mathbf{k})a^\dagger(\mathbf{k}) + a^\dagger(\mathbf{k})a(\mathbf{k}) \right] 利用对易关系 a(k)a(k)=a(k)a(k)+(2π)3δ(3)(0)a(\mathbf{k})a^\dagger(\mathbf{k}) = a^\dagger(\mathbf{k})a(\mathbf{k}) + (2\pi)^3 \delta^{(3)}(0) 进行正规序化(Normal Ordering)。由于无穷大常数项正比于 d3kkδ(3)(0)\int d^3k \, \mathbf{k} \delta^{(3)}(0),被积函数为奇函数,该常数项积分为零(物理上也要求真空动量为零)。最终得到: P=d3k(2π)3ka(k)a(k)\boxed{ \mathbf{P} = \int \frac{d^3k}{(2\pi)^3} \mathbf{k} \, a^\dagger(\mathbf{k}) a(\mathbf{k}) }

3.5

Problem 3.5

srednickiChapter 3

习题 3.5

来源: 第3章, PDF第44页


3.5 Consider a complex (that is, nonhermitian) scalar field φ\varphi with lagrangian density

L=μφμφm2φφ+Ω0.(3.37)\mathcal{L} = -\partial^\mu \varphi^\dagger \partial_\mu \varphi - m^2 \varphi^\dagger \varphi + \Omega_0 \, . \tag{3.37}

a) Show that φ\varphi obeys the Klein-Gordon equation.

b) Treat φ\varphi and φ\varphi^\dagger as independent fields, and find the conjugate momentum for each. Compute the hamiltonian density in terms of these conjugate momenta and the fields themselves (but not their time derivatives).

c) Write the mode expansion of φ\varphi as

φ(x)=dk~[a(k)eikx+b(k)eikx].(3.38)\varphi(x) = \int \widetilde{dk} \left[ a(\mathbf{k}) e^{ikx} + b^\dagger(\mathbf{k}) e^{-ikx} \right] \, . \tag{3.38}

Express a(k)a(\mathbf{k}) and b(k)b(\mathbf{k}) in terms of φ\varphi and φ\varphi^\dagger and their time derivatives.

d) Assuming canonical commutation relations for the fields and their conjugate momenta, find the commutation relations obeyed by a(k)a(\mathbf{k}) and b(k)b(\mathbf{k}) and their hermitian conjugates.

e) Express the hamiltonian in terms of a(k)a(\mathbf{k}) and b(k)b(\mathbf{k}) and their hermitian conjugates. What value must Ω0\Omega_0 have in order for the ground state to have zero energy?

习题 3.5 - 解答


a) 证明 φ\varphi 满足 Klein-Gordon 方程

拉格朗日密度为: L=μφμφm2φφ+Ω0\mathcal{L} = -\partial^\mu \varphi^\dagger \partial_\mu \varphi - m^2 \varphi^\dagger \varphi + \Omega_0φ\varphiφ\varphi^\dagger 视为独立的场。对 φ\varphi^\dagger 应用欧拉-拉格朗日方程: μ(L(μφ))Lφ=0\partial_\mu \left( \frac{\partial \mathcal{L}}{\partial (\partial_\mu \varphi^\dagger)} \right) - \frac{\partial \mathcal{L}}{\partial \varphi^\dagger} = 0 计算相应的偏导数: L(μφ)=μφ,Lφ=m2φ\frac{\partial \mathcal{L}}{\partial (\partial_\mu \varphi^\dagger)} = -\partial^\mu \varphi, \quad \frac{\partial \mathcal{L}}{\partial \varphi^\dagger} = -m^2 \varphi 代入欧拉-拉格朗日方程中得到: μ(μφ)(m2φ)=0    2φ+m2φ=0\partial_\mu (-\partial^\mu \varphi) - (-m^2 \varphi) = 0 \implies -\partial^2 \varphi + m^2 \varphi = 0 即: (2+m2)φ=0\boxed{ (-\partial^2 + m^2) \varphi = 0 } 这正是 Klein-Gordon 方程。


b) 共轭动量与哈密顿密度

φ\varphiφ\varphi^\dagger 视为独立场,它们各自的共轭动量分别为: Π=Lφ˙=φ˙\Pi = \frac{\partial \mathcal{L}}{\partial \dot{\varphi}} = \dot{\varphi}^\dagger Π=Lφ˙=φ˙\Pi^\dagger = \frac{\partial \mathcal{L}}{\partial \dot{\varphi}^\dagger} = \dot{\varphi} 哈密顿密度 H\mathcal{H} 通过勒让德变换得到: H=Πφ˙+Πφ˙L\mathcal{H} = \Pi \dot{\varphi} + \Pi^\dagger \dot{\varphi}^\dagger - \mathcal{L}φ˙=Π\dot{\varphi} = \Pi^\daggerφ˙=Π\dot{\varphi}^\dagger = \Pi 代入,并展开 L\mathcal{L} 中的动能项 μφμφ=φ˙φ˙φφ=ΠΠφφ-\partial^\mu \varphi^\dagger \partial_\mu \varphi = \dot{\varphi}^\dagger \dot{\varphi} - \nabla \varphi^\dagger \cdot \nabla \varphi = \Pi \Pi^\dagger - \nabla \varphi^\dagger \cdot \nabla \varphiH=ΠΠ+ΠΠ(ΠΠφφm2φφ+Ω0)\mathcal{H} = \Pi \Pi^\dagger + \Pi^\dagger \Pi - (\Pi \Pi^\dagger - \nabla \varphi^\dagger \cdot \nabla \varphi - m^2 \varphi^\dagger \varphi + \Omega_0) 化简后得到(保持算符顺序): H=ΠΠ+φφ+m2φφΩ0\boxed{ \mathcal{H} = \Pi^\dagger \Pi + \nabla \varphi^\dagger \cdot \nabla \varphi + m^2 \varphi^\dagger \varphi - \Omega_0 }


c) 模式展开与反解产生/湮灭算符

已知模式展开为: φ(x)=dk~[a(k)eikx+b(k)eikx]\varphi(x) = \int \widetilde{dk} \left[ a(\mathbf{k}) e^{ikx} + b^\dagger(\mathbf{k}) e^{-ikx} \right] 其中 dk~=d3k(2π)32ω\widetilde{dk} = \frac{d^3k}{(2\pi)^3 2\omega},且 kx=kxωtkx = \mathbf{k}\cdot\mathbf{x} - \omega t。对其求时间导数: φ˙(x)=dk~(iω)[a(k)eikxb(k)eikx]\dot{\varphi}(x) = \int \widetilde{dk} (-i\omega) \left[ a(\mathbf{k}) e^{ikx} - b^\dagger(\mathbf{k}) e^{-ikx} \right]φ(x)\varphi(x)φ˙(x)\dot{\varphi}(x) 进行空间傅里叶逆变换: d3xeikxφ(x)=12ω[a(k)eiωt+b(k)eiωt]\int d^3x e^{-i\mathbf{k}\cdot\mathbf{x}} \varphi(x) = \frac{1}{2\omega} \left[ a(\mathbf{k}) e^{-i\omega t} + b^\dagger(-\mathbf{k}) e^{i\omega t} \right] d3xeikxiφ˙(x)=12ω[ωa(k)eiωtωb(k)eiωt]\int d^3x e^{-i\mathbf{k}\cdot\mathbf{x}} i\dot{\varphi}(x) = \frac{1}{2\omega} \left[ \omega a(\mathbf{k}) e^{-i\omega t} - \omega b^\dagger(-\mathbf{k}) e^{i\omega t} \right] 将第一式乘以 ω\omega 并与第二式相加,可消去 bb^\dagger 项: d3xeikx[ωφ(x)+iφ˙(x)]=a(k)eiωt\int d^3x e^{-i\mathbf{k}\cdot\mathbf{x}} [\omega \varphi(x) + i\dot{\varphi}(x)] = a(\mathbf{k}) e^{-i\omega t} 移项得到 a(k)a(\mathbf{k}) 的表达式。同理,对 φ(x)\varphi^\dagger(x) 进行相同的操作可得到 b(k)b(\mathbf{k})a(k)=d3xeikx[ωφ(x)+iφ˙(x)]\boxed{ a(\mathbf{k}) = \int d^3x e^{-ikx} [\omega \varphi(x) + i\dot{\varphi}(x)] } b(k)=d3xeikx[ωφ(x)+iφ˙(x)]\boxed{ b(\mathbf{k}) = \int d^3x e^{-ikx} [\omega \varphi^\dagger(x) + i\dot{\varphi}^\dagger(x)] }


d) 算符的对易关系

由正则对易关系 [φ(x,t),Π(y,t)]=iδ3(xy)[\varphi(\mathbf{x}, t), \Pi(\mathbf{y}, t)] = i\delta^3(\mathbf{x}-\mathbf{y})[φ(x,t),Π(y,t)]=iδ3(xy)[\varphi^\dagger(\mathbf{x}, t), \Pi^\dagger(\mathbf{y}, t)] = i\delta^3(\mathbf{x}-\mathbf{y}),代入 Π=φ˙\Pi = \dot{\varphi}^\daggerΠ=φ˙\Pi^\dagger = \dot{\varphi},得到非零的对易子: [φ(x,t),φ˙(y,t)]=iδ3(xy),[φ(x,t),φ˙(y,t)]=iδ3(xy)[\varphi(\mathbf{x}, t), \dot{\varphi}^\dagger(\mathbf{y}, t)] = i\delta^3(\mathbf{x}-\mathbf{y}), \quad [\varphi^\dagger(\mathbf{x}, t), \dot{\varphi}(\mathbf{y}, t)] = i\delta^3(\mathbf{x}-\mathbf{y}) 计算 a(k)a(\mathbf{k})a(k)a^\dagger(\mathbf{k}') 的对易关系: [a(k),a(k)]=d3xd3yeikx+iky[ωφ(x)+iφ˙(x),ωφ(y)iφ˙(y)][a(\mathbf{k}), a^\dagger(\mathbf{k}')] = \int d^3x d^3y e^{-ikx + ik'y} [\omega \varphi(x) + i\dot{\varphi}(x), \omega' \varphi^\dagger(y) - i\dot{\varphi}^\dagger(y)] 展开对易子,只有交叉项非零: =d3xd3yeikx+iky(iω[φ(x),φ˙(y)]+iω[φ˙(x),φ(y)])= \int d^3x d^3y e^{-ikx + ik'y} \left( -i\omega [\varphi(x), \dot{\varphi}^\dagger(y)] + i\omega' [\dot{\varphi}(x), \varphi^\dagger(y)] \right) =d3xd3yeikx+iky(iω(iδ3(xy))+iω(iδ3(xy)))= \int d^3x d^3y e^{-ikx + ik'y} \left( -i\omega (i\delta^3(\mathbf{x}-\mathbf{y})) + i\omega' (-i\delta^3(\mathbf{x}-\mathbf{y})) \right) =d3xei(kk)x+i(ωω)t(ω+ω)= \int d^3x e^{-i(\mathbf{k}-\mathbf{k}')\cdot\mathbf{x} + i(\omega-\omega')t} (\omega + \omega') 积分给出动量守恒 k=k\mathbf{k} = \mathbf{k}',从而 ω=ω\omega = \omega',得到: [a(k),a(k)]=(2π)32ωδ3(kk)\boxed{ [a(\mathbf{k}), a^\dagger(\mathbf{k}')] = (2\pi)^3 2\omega \delta^3(\mathbf{k}-\mathbf{k}') } 同理可得 bb 算符的对易关系: [b(k),b(k)]=(2π)32ωδ3(kk)\boxed{ [b(\mathbf{k}), b^\dagger(\mathbf{k}')] = (2\pi)^3 2\omega \delta^3(\mathbf{k}-\mathbf{k}') } 由于 aa 仅包含 φ,φ˙\varphi, \dot{\varphi},而 bb 仅包含 φ,φ˙\varphi^\dagger, \dot{\varphi}^\dagger,计算可知交叉对易子(如 [a(k),b(k)][a(\mathbf{k}), b(\mathbf{k}')] 等)均严格抵消为零。


e) 哈密顿量与基态能量

将模式展开代入哈密顿量 H=d3xHH = \int d^3x \mathcal{H} 中。利用 ΠΠ=φ˙φ˙\Pi^\dagger \Pi = \dot{\varphi} \dot{\varphi}^\dagger,积分后交叉项(如 abababa^\dagger b^\dagger)在动能项与梯度/质量项之间精确相消,得到对称排序的哈密顿量: H=dk~ω2[a(k)a(k)+b(k)b(k)+a(k)a(k)+b(k)b(k)]Ω0VH = \int \widetilde{dk} \frac{\omega}{2} \left[ a(\mathbf{k}) a^\dagger(\mathbf{k}) + b^\dagger(\mathbf{k}) b(\mathbf{k}) + a^\dagger(\mathbf{k}) a(\mathbf{k}) + b(\mathbf{k}) b^\dagger(\mathbf{k}) \right] - \Omega_0 V 利用对易关系 aa=aa+(2π)32ωδ3(0)a a^\dagger = a^\dagger a + (2\pi)^3 2\omega \delta^3(0)bb=bb+(2π)32ωδ3(0)b b^\dagger = b^\dagger b + (2\pi)^3 2\omega \delta^3(0) 将其正规序化: H=dk~ω[a(k)a(k)+b(k)b(k)]+dk~ω(2π)32ωδ3(0)Ω0V\boxed{ H = \int \widetilde{dk} \, \omega \left[ a^\dagger(\mathbf{k}) a(\mathbf{k}) + b^\dagger(\mathbf{k}) b(\mathbf{k}) \right] + \int \widetilde{dk} \, \omega (2\pi)^3 2\omega \delta^3(0) - \Omega_0 V } 基态 0|0\rangle 满足 a(k)0=b(k)0=0a(\mathbf{k})|0\rangle = b(\mathbf{k})|0\rangle = 0。作用在基态上的能量本征值为: E0=d3k(2π)32ωω(2π)32ωδ3(0)Ω0VE_0 = \int \frac{d^3k}{(2\pi)^3 2\omega} \omega (2\pi)^3 2\omega \delta^3(0) - \Omega_0 V 利用体积因子 V=(2π)3δ3(0)V = (2\pi)^3 \delta^3(0),基态能量化简为: E0=Vd3k(2π)3ωΩ0VE_0 = V \int \frac{d^3k}{(2\pi)^3} \omega - \Omega_0 V 为了使基态能量 E0=0E_0 = 0,宇宙学常数项 Ω0\Omega_0 必须抵消零点能(复标量场贡献了两个实标量场的零点能),因此: Ω0=d3k(2π)3ω\boxed{ \Omega_0 = \int \frac{d^3k}{(2\pi)^3} \omega }