48.1

Problem 48.1

srednickiChapter 48

习题 48.1

来源: 第48章, PDF第301页


48.1 The tedium of these calculations is greatly alleviated by making use of a symbolic manipulation program like Mathematica or Maple. One approach is brute force: compute 4×44 \times 4 matrices like p\cancel{p} in the CM frame, and take their products and traces. If you are familiar with a symbolic-manipulation program, write one that does this. See if you can verify eqs. (48.26–48.29).


Referenced Equations:

Equation (48.26):

Φss=su+m2(9s+u)+7m48m2M2+M4,(48.26)\langle\Phi_{ss}\rangle = -su + m^2(9s + u) + 7m^4 - 8m^2M^2 + M^4, \tag{48.26}

Equation (48.27):

Φuu=su+m2(9u+s)+7m48m2M2+M4,(48.27)\langle\Phi_{uu}\rangle = -su + m^2(9u + s) + 7m^4 - 8m^2M^2 + M^4, \tag{48.27}

Equation (48.28):

Φsu=+su+3m2(s+u)+9m48m2M2M4,(48.28)\langle\Phi_{su}\rangle = +su + 3m^2(s + u) + 9m^4 - 8m^2M^2 - M^4, \tag{48.28}

Equation (48.29):

Φus=+su+3m2(s+u)+9m48m2M2M4.(48.29)\langle\Phi_{us}\rangle = +su + 3m^2(s + u) + 9m^4 - 8m^2M^2 - M^4. \tag{48.29}

习题 48.1 - 解答


物理背景与分析

本题要求验证自旋为 1/21/2 的费米子(质量为 mm)与标量玻色子(质量为 MM)散射过程中的极化平均矩阵元平方的各项迹(Trace)。在 Srednicki 的量子场论约定中,采用“多加”度规(mostly-plus metric)ημν=diag(,+,+,+)\eta_{\mu\nu} = \text{diag}(-, +, +, +)

散射过程的运动学变量定义为:

  • 初始动量:费米子 pp,玻色子 kk
  • 末态动量:费米子 pp',玻色子 kk'
  • Mandelstam 变量: s=(p+k)2,t=(pp)2,u=(pk)2s = -(p+k)^2, \quad t = -(p-p')^2, \quad u = -(p-k')^2 满足 s+t+u=2m2+2M2s + t + u = 2m^2 + 2M^2
  • 质壳条件:p2=p2=m2p^2 = p'^2 = -m^2k2=k2=M2k^2 = k'^2 = -M^2

定义中间态动量 sμ=pμ+kμs^\mu = p^\mu + k^\muuμ=pμkμu^\mu = p^\mu - k'^\mu,则 sμsμ=ss^\mu s_\mu = -suμuμ=uu^\mu u_\mu = -u。 极化平均的迹定义包含初始自旋平均因子 1/21/2Φss=12Tr[(p+m)(s+m)(p+m)(s+m)]\langle\Phi_{ss}\rangle = \frac{1}{2} \text{Tr}[(-\cancel{p}' + m)(-\cancel{s} + m)(-\cancel{p} + m)(-\cancel{s} + m)] Φsu=12Tr[(p+m)(s+m)(p+m)(u+m)]\langle\Phi_{su}\rangle = \frac{1}{2} \text{Tr}[(-\cancel{p}' + m)(-\cancel{s} + m)(-\cancel{p} + m)(-\cancel{u} + m)]

在多加度规下,Clifford 代数为 {γμ,γν}=2ημν\{\gamma^\mu, \gamma^\nu\} = -2\eta^{\mu\nu},迹定理为:

  • Tr[AB]=4AB\text{Tr}[\cancel{A}\cancel{B}] = -4A\cdot B
  • Tr[ABCD]=4(ABCDACBD+ADBC)\text{Tr}[\cancel{A}\cancel{B}\cancel{C}\cancel{D}] = 4(A\cdot B \, C\cdot D - A\cdot C \, B\cdot D + A\cdot D \, B\cdot C)

我们需要用到以下内积关系: ps=ps=12(M2m2s)p\cdot s = p'\cdot s = \frac{1}{2}(M^2 - m^2 - s) pu=pu=12(M2m2u)p\cdot u = p'\cdot u = \frac{1}{2}(M^2 - m^2 - u) pp=12(t2m2)p\cdot p' = \frac{1}{2}(t - 2m^2) su=(p+k)(pk)=p2pk+kpkk=M2m2s\cdot u = (p+k)\cdot (p-k') = p^2 - p\cdot k' + k\cdot p - k\cdot k' = M^2 - m^2


解析推导过程

(a) 验证 Eq. (48.26) Φss\langle\Phi_{ss}\rangle

展开迹 Φss\langle\Phi_{ss}\rangleΦss=12{Tr[psps]+m2Tr[ps+pp+ps+sp+ss+ps]+m4Tr[1]}\langle\Phi_{ss}\rangle = \frac{1}{2} \Big\{ \text{Tr}[\cancel{p}' \cancel{s} \cancel{p} \cancel{s}] + m^2 \text{Tr}[\cancel{p}' \cancel{s} + \cancel{p}' \cancel{p} + \cancel{p}' \cancel{s} + \cancel{s} \cancel{p} + \cancel{s} \cancel{s} + \cancel{p} \cancel{s}] + m^4 \text{Tr}[1] \Big\} 利用迹定理化简: Φss=2[2(ps)(ps)s2(pp)]2m2[2ps+pp+2ps+s2]+2m4\langle\Phi_{ss}\rangle = 2[2(p'\cdot s)(p\cdot s) - s^2(p'\cdot p)] - 2m^2[2p'\cdot s + p'\cdot p + 2p\cdot s + s^2] + 2m^4 代入内积关系与 s2=ss^2 = -s: 第一项: 2[2(M2m2s2)2(s)t2m22]=(M2m2s)2+s(t2m2)2 \left[ 2 \left(\frac{M^2 - m^2 - s}{2}\right)^2 - (-s)\frac{t - 2m^2}{2} \right] = (M^2 - m^2 - s)^2 + s(t - 2m^2) 第二项: 2m2[2(M2m2s)+t2m22s]=2m2[2M23m23s+12t]-2m^2 \left[ 2(M^2 - m^2 - s) + \frac{t - 2m^2}{2} - s \right] = -2m^2 \left[ 2M^2 - 3m^2 - 3s + \frac{1}{2}t \right] 将所有项相加并展开: Φss=(M4+m4+s22m2M22sM2+2sm2)+st2sm24m2M2+6m4+6m2sm2t+2m4\langle\Phi_{ss}\rangle = (M^4 + m^4 + s^2 - 2m^2 M^2 - 2s M^2 + 2s m^2) + st - 2s m^2 - 4m^2 M^2 + 6m^4 + 6m^2 s - m^2 t + 2m^4 =M4+9m4+s26m2M22sM2+6m2s+stm2t= M^4 + 9m^4 + s^2 - 6m^2 M^2 - 2s M^2 + 6m^2 s + st - m^2 t 利用 t=2m2+2M2sut = 2m^2 + 2M^2 - s - u 消去 ttst=2sm2+2sM2s2sust = 2s m^2 + 2s M^2 - s^2 - su m2t=2m42m2M2+m2s+m2u-m^2 t = -2m^4 - 2m^2 M^2 + m^2 s + m^2 u 代入上式合并同类项: Φss=M4+7m48m2M2+9m2ssu+m2u\langle\Phi_{ss}\rangle = M^4 + 7m^4 - 8m^2 M^2 + 9m^2 s - su + m^2 u 整理即得: Φss=su+m2(9s+u)+7m48m2M2+M4\boxed{ \langle\Phi_{ss}\rangle = -su + m^2(9s + u) + 7m^4 - 8m^2M^2 + M^4 }

(b) 验证 Eq. (48.27) Φuu\langle\Phi_{uu}\rangle

Φuu\langle\Phi_{uu}\rangle 的定义与 Φss\langle\Phi_{ss}\rangle 完全相同,仅需将中间态动量 sμs^\mu 替换为 uμu^\mu。根据交叉对称性(Crossing Symmetry),直接在 Eq. (48.26) 中交换 Mandelstam 变量 sus \leftrightarrow u 即可得到: Φuu=su+m2(9u+s)+7m48m2M2+M4\boxed{ \langle\Phi_{uu}\rangle = -su + m^2(9u + s) + 7m^4 - 8m^2M^2 + M^4 }

(c) 验证 Eq. (48.28) Φsu\langle\Phi_{su}\rangle

展开干涉项的迹 Φsu\langle\Phi_{su}\rangleΦsu=12{Tr[pspu]+m2Tr[ps+pp+pu+sp+su+pu]+m4Tr[1]}\langle\Phi_{su}\rangle = \frac{1}{2} \Big\{ \text{Tr}[\cancel{p}' \cancel{s} \cancel{p} \cancel{u}] + m^2 \text{Tr}[\cancel{p}' \cancel{s} + \cancel{p}' \cancel{p} + \cancel{p}' \cancel{u} + \cancel{s} \cancel{p} + \cancel{s} \cancel{u} + \cancel{p} \cancel{u}] + m^4 \text{Tr}[1] \Big\} 利用迹定理化简: Φsu=2[(ps)(pu)(pp)(su)+(pu)(sp)]2m2[2ps+pp+2pu+su]+2m4\langle\Phi_{su}\rangle = 2[(p'\cdot s)(p\cdot u) - (p'\cdot p)(s\cdot u) + (p'\cdot u)(s\cdot p)] - 2m^2[2p\cdot s + p\cdot p' + 2p\cdot u + s\cdot u] + 2m^4 代入内积关系: 第一项: 2[2(M2m2s)(M2m2u)4t2m22(M2m2)]2 \left[ 2 \frac{(M^2 - m^2 - s)(M^2 - m^2 - u)}{4} - \frac{t - 2m^2}{2}(M^2 - m^2) \right] =(M2m2)2(M2m2)(s+u)+su(t2m2)(M2m2)= (M^2 - m^2)^2 - (M^2 - m^2)(s+u) + su - (t - 2m^2)(M^2 - m^2) =(M2m2)[M2m2sut+2m2]+su= (M^2 - m^2)[M^2 - m^2 - s - u - t + 2m^2] + su 代入 s+t+u=2m2+2M2s+t+u = 2m^2 + 2M^2=(M2m2)[M2m2]+su=m4M4+su= (M^2 - m^2)[-M^2 - m^2] + su = m^4 - M^4 + su 第二项: 2m2[(M2m2s)+t2m22+(M2m2u)+(M2m2)]-2m^2 \left[ (M^2 - m^2 - s) + \frac{t - 2m^2}{2} + (M^2 - m^2 - u) + (M^2 - m^2) \right] =2m2[3M23m2su+12(2m2+2M2su)m2]= -2m^2 \left[ 3M^2 - 3m^2 - s - u + \frac{1}{2}(2m^2 + 2M^2 - s - u) - m^2 \right] =2m2[4M23m232(s+u)]=8m2M2+6m4+3m2(s+u)= -2m^2 \left[ 4M^2 - 3m^2 - \frac{3}{2}(s+u) \right] = -8m^2 M^2 + 6m^4 + 3m^2(s+u) 将所有项相加: Φsu=(m4M4+su)+(8m2M2+6m4+3m2(s+u))+2m4\langle\Phi_{su}\rangle = (m^4 - M^4 + su) + (-8m^2 M^2 + 6m^4 + 3m^2(s+u)) + 2m^4 整理即得: Φsu=+su+3m2(s+u)+9m48m2M2M4\boxed{ \langle\Phi_{su}\rangle = +su + 3m^2(s + u) + 9m^4 - 8m^2M^2 - M^4 }

(d) 验证 Eq. (48.29) Φus\langle\Phi_{us}\rangle

Φus\langle\Phi_{us}\rangleΦsu\langle\Phi_{su}\rangle 的复共轭(或转置)。由于迹具有循环对称性且在转置下不变(Tr[M]=Tr[MT]\text{Tr}[M] = \text{Tr}[M^T],且相互作用的 γ\gamma 矩阵组合满足转置对称),干涉项是对称的,即 Φus=Φsu\langle\Phi_{us}\rangle = \langle\Phi_{su}\rangle。因此: Φus=+su+3m2(s+u)+9m48m2M2M4\boxed{ \langle\Phi_{us}\rangle = +su + 3m^2(s + u) + 9m^4 - 8m^2M^2 - M^4 }


符号计算方法说明 (Symbolic Manipulation Approach)

题目中提到可以通过 Mathematica 等符号计算软件使用“暴力法”(Brute force)直接计算 4×44 \times 4 矩阵的乘积和迹。其核心物理设置如下:

  1. 质心系 (CM Frame) 运动学设定: 定义四维动量: pμ=(E,0,0,pz),kμ=(ω,0,0,pz)p^\mu = (E, 0, 0, p_z), \quad k^\mu = (\omega, 0, 0, -p_z) pμ=(E,pzsinθ,0,pzcosθ),kμ=(ω,pzsinθ,0,pzcosθ)p'^\mu = (E, p_z \sin\theta, 0, p_z \cos\theta), \quad k'^\mu = (\omega, -p_z \sin\theta, 0, -p_z \cos\theta) 其中 E=s+m2M22sE = \frac{s + m^2 - M^2}{2\sqrt{s}}ω=sm2+M22s\omega = \frac{s - m^2 + M^2}{2\sqrt{s}}pz=λ1/2(s,m2,M2)2sp_z = \frac{\lambda^{1/2}(s, m^2, M^2)}{2\sqrt{s}}

  2. 矩阵构造: 在多加度规下,显式写出 Dirac γ\gamma 矩阵(如 Weyl 表象): γ0=(0II0),γi=(0σiσi0)\gamma^0 = \begin{pmatrix} 0 & I \\ I & 0 \end{pmatrix}, \quad \gamma^i = \begin{pmatrix} 0 & \sigma^i \\ -\sigma^i & 0 \end{pmatrix} 构造 4×44 \times 4 矩阵 p=pμγμ=Eγ0+pγ\cancel{p} = p_\mu \gamma^\mu = -E \gamma^0 + \vec{p} \cdot \vec{\gamma}

  3. 计算与化简: 在程序中直接计算矩阵乘积的迹,例如: PhiSS = 1/2 * Tr[(-Slash[pp] + m*I4) . (-Slash[sVec] + m*I4) . (-Slash[p] + m*I4) . (-Slash[sVec] + m*I4)] 最后利用 t=2pz2(1cosθ)t = -2p_z^2(1-\cos\theta)u=2m2+2M2stu = 2m^2 + 2M^2 - s - t 将结果中的 E,ω,pz,θE, \omega, p_z, \theta 替换为 Mandelstam 变量,即可由软件自动输出并验证上述 (48.26)-(48.29) 的多项式结果。

48.2

Problem 48.2

srednickiChapter 48

习题 48.2

来源: 第48章, PDF第301页


48.2 Compute T2\langle|\mathcal{T}|^2\rangle for e+eφφe^+e^- \rightarrow \varphi\varphi. You should find that your result is the same as that for eφeφe^-\varphi \rightarrow e^-\varphi, but with sts \leftrightarrow t, and an extra overall minus sign. This relationship is known as crossing symmetry. There is an overall minus sign for each fermion that is moved from the initial to the final state.

习题 48.2 - 解答


对于过程 e+(p2)+e(p1)φ(k1)+φ(k2)e^+(p_2) + e^-(p_1) \rightarrow \varphi(k_1) + \varphi(k_2),我们在树图阶需要考虑 tt 沟道和 uu 沟道两个费曼图。设电子质量为 mm,标量粒子质量为 MM,相互作用拉氏量包含汤川耦合项 Lint=gψˉψφ\mathcal{L}_{\text{int}} = g\bar{\psi}\psi\varphi

定义 Mandelstam 变量:

s=(p1+p2)2,t=(p1k1)2,u=(p1k2)2s = (p_1 + p_2)^2, \quad t = (p_1 - k_1)^2, \quad u = (p_1 - k_2)^2

它们满足 s+t+u=2m2+2M2s + t + u = 2m^2 + 2M^2

该散射过程的跃迁矩阵元为:

T=g2vˉ(p2)[̸p1̸k1+mtm2+̸p1̸k2+mum2]u(p1)\mathcal{T} = g^2 \bar{v}(p_2) \left[ \frac{\not{p}_1 - \not{k}_1 + m}{t - m^2} + \frac{\not{p}_1 - \not{k}_2 + m}{u - m^2} \right] u(p_1)

对初态自旋求平均并对末态自旋求和,由于初态有两个费米子,自旋平均因子为 14\frac{1}{4}

T2=14spinsT2=g44[Ttt(tm2)2+Tuu(um2)2+2Ttu(tm2)(um2)]\langle|\mathcal{T}|^2\rangle = \frac{1}{4} \sum_{\text{spins}} |\mathcal{T}|^2 = \frac{g^4}{4} \left[ \frac{T_{tt}}{(t - m^2)^2} + \frac{T_{uu}}{(u - m^2)^2} + \frac{2 T_{tu}}{(t - m^2)(u - m^2)} \right]

其中迹的定义为:

Ttt=Tr[(̸p2m)(̸p1̸k1+m)(̸p1+m)(̸p1̸k1+m)]Tuu=Tr[(̸p2m)(̸p1̸k2+m)(̸p1+m)(̸p1̸k2+m)]Ttu=Tr[(̸p2m)(̸p1̸k1+m)(̸p1+m)(̸p1̸k2+m)]\begin{aligned} T_{tt} &= \text{Tr}\left[ (\not{p}_2 - m)(\not{p}_1 - \not{k}_1 + m)(\not{p}_1 + m)(\not{p}_1 - \not{k}_1 + m) \right] \\ T_{uu} &= \text{Tr}\left[ (\not{p}_2 - m)(\not{p}_1 - \not{k}_2 + m)(\not{p}_1 + m)(\not{p}_1 - \not{k}_2 + m) \right] \\ T_{tu} &= \text{Tr}\left[ (\not{p}_2 - m)(\not{p}_1 - \not{k}_1 + m)(\not{p}_1 + m)(\not{p}_1 - \not{k}_2 + m) \right] \end{aligned}

1. 计算 TttT_{tt} 利用狄拉克方程的性质 (̸p1+m)(̸p1m)=p12m2=0(\not{p}_1 + m)(\not{p}_1 - m) = p_1^2 - m^2 = 0,可以极大地简化中间的矩阵乘积:

(̸p1̸k1+m)(̸p1+m)=(2m̸k1)(̸p1+m)(\not{p}_1 - \not{k}_1 + m)(\not{p}_1 + m) = (2m - \not{k}_1)(\not{p}_1 + m)

因此,迹中的核心部分可以化简为:

(̸p1̸k1+m)(̸p1+m)(̸p1̸k1+m)=(2m̸k1)(̸p1+m)(2m̸k1)=(4m2M2)̸p1+(2p1k14m2)̸k1+m(4m2+M24p1k1)\begin{aligned} (\not{p}_1 - \not{k}_1 + m)(\not{p}_1 + m)(\not{p}_1 - \not{k}_1 + m) &= (2m - \not{k}_1)(\not{p}_1 + m)(2m - \not{k}_1) \\ &= (4m^2 - M^2)\not{p}_1 + (2p_1 \cdot k_1 - 4m^2)\not{k}_1 + m(4m^2 + M^2 - 4p_1 \cdot k_1) \end{aligned}

将其代入 TttT_{tt} 并与 (̸p2m)(\not{p}_2 - m) 求迹(奇数个 γ\gamma 矩阵的迹为零):

Ttt=4(4m2M2)(p1p2)+4(2p1k14m2)(p2k1)4m2(4m2+M24p1k1)T_{tt} = 4(4m^2 - M^2)(p_1 \cdot p_2) + 4(2p_1 \cdot k_1 - 4m^2)(p_2 \cdot k_1) - 4m^2(4m^2 + M^2 - 4p_1 \cdot k_1)

代入运动学关系 p1p2=s2m22p_1 \cdot p_2 = \frac{s - 2m^2}{2}p1k1=m2+M2t2p_1 \cdot k_1 = \frac{m^2 + M^2 - t}{2}p2k1=m2+M2u2p_2 \cdot k_1 = \frac{m^2 + M^2 - u}{2},并利用 u=2m2+2M2stu = 2m^2 + 2M^2 - s - t 消去 uu,化简后得到:

Ttt=2[t2+st+9m4+M46m2M2m2s+6m2t2M2t]T_{tt} = -2 \left[ t^2 + st + 9m^4 + M^4 - 6m^2 M^2 - m^2 s + 6m^2 t - 2M^2 t \right]

2. 计算 TuuT_{uu} 由费曼图在 k1k2k_1 \leftrightarrow k_2 下的对称性,直接将 TttT_{tt} 中的 tt 替换为 uu 即可:

Tuu=2[u2+su+9m4+M46m2M2m2s+6m2u2M2u]T_{uu} = -2 \left[ u^2 + su + 9m^4 + M^4 - 6m^2 M^2 - m^2 s + 6m^2 u - 2M^2 u \right]

3. 计算 TtuT_{tu} 使用相同的代数技巧展开中间项:

(̸p1̸k1+m)(̸p1+m)(̸p1̸k2+m)=(2m̸k1)(̸p1+m)(2m̸k2)(\not{p}_1 - \not{k}_1 + m)(\not{p}_1 + m)(\not{p}_1 - \not{k}_2 + m) = (2m - \not{k}_1)(\not{p}_1 + m)(2m - \not{k}_2)

求迹并代入所有内积关系(包括 k1k2=s2M22k_1 \cdot k_2 = \frac{s - 2M^2}{2}),经过繁琐但直接的代数化简后得到:

Ttu=u2+t2s234m42M44m2M2+6m2s+4M2sT_{tu} = u^2 + t^2 - s^2 - 34m^4 - 2M^4 - 4m^2 M^2 + 6m^2 s + 4M^2 s

4. 最终结果与交叉对称性 (Crossing Symmetry) 分析 将上述迹代入自旋平均的模方公式中,得到最终结果:

T2e+eφφ=g44[Ttt(tm2)2+Tuu(um2)2+2Ttu(tm2)(um2)]\boxed{ \langle|\mathcal{T}|^2\rangle_{e^+e^- \rightarrow \varphi\varphi} = \frac{g^4}{4} \left[ \frac{T_{tt}}{(t - m^2)^2} + \frac{T_{uu}}{(u - m^2)^2} + \frac{2 T_{tu}}{(t - m^2)(u - m^2)} \right] }

现在我们将其与康普顿散射过程 e(p)+φ(k)e(p)+φ(k)e^-(p) + \varphi(k) \rightarrow e^-(p') + \varphi(k') 进行对比。 根据交叉对称性,我们可以通过以下动量替换将 e+eφφe^+e^- \rightarrow \varphi\varphi 映射为 eφeφe^-\varphi \rightarrow e^-\varphi

  • 将末态的 φ(k1)\varphi(k_1) 移至初态:k1kk_1 \rightarrow -k
  • 将初态的 e+(p2)e^+(p_2) 移至末态:p2pp_2 \rightarrow -p'

在此映射下,Mandelstam 变量发生置换:

se+e=(p1+p2)2(pp)2=teφs_{e^+e^-} = (p_1 + p_2)^2 \rightarrow (p - p')^2 = t_{e\varphi}
te+e=(p1k1)2(p+k)2=seφt_{e^+e^-} = (p_1 - k_1)^2 \rightarrow (p + k)^2 = s_{e\varphi}

即发生了 sts \leftrightarrow t 的交换(uu 保持不变)。

此外,根据费米子交叉规则,每将一个费米子从初态移至末态(或反之),振幅的模方需要引入一个全局的负号。因此,未平均的自旋求和矩阵元满足严格的关系:

spinsTe+eφφ2(s,t,u)=spinsTeφeφ2(t,s,u)\sum_{\text{spins}} |\mathcal{T}|^2_{e^+e^- \rightarrow \varphi\varphi}(s, t, u) = - \sum_{\text{spins}} |\mathcal{T}|^2_{e^-\varphi \rightarrow e^-\varphi}(t, s, u)

需要注意的是,由于 e+ee^+e^- 初态有 4 个自旋态,而 eφe^-\varphi 初态只有 2 个自旋态,自旋平均因子分别为 1/41/41/21/2。因此,自旋平均后的结果满足:

T2e+eφφ(s,t,u)=12T2eφeφ(t,s,u)\boxed{ \langle|\mathcal{T}|^2\rangle_{e^+e^- \rightarrow \varphi\varphi}(s, t, u) = - \frac{1}{2} \langle|\mathcal{T}|^2\rangle_{e^-\varphi \rightarrow e^-\varphi}(t, s, u) }

这完美验证了题目中关于 sts \leftrightarrow t 替换以及全局负号(费米子符号法则)的论述。

48.3

Problem 48.3

srednickiChapter 48

习题 48.3

来源: 第48章, PDF第301页


48.3 Compute T2\langle|\mathcal{T}|^2\rangle for eeeee^-e^- \rightarrow e^-e^-. You should find that your result is the same as that for e+ee+ee^+e^- \rightarrow e^+e^-, but with sus \leftrightarrow u. This is another example of crossing symmetry.

习题 48.3 - 解答


对于 eeeee^-e^- \rightarrow e^-e^-(Møller 散射),初始态和末态均为全同费米子。设初态电子动量为 p1,p2p_1, p_2,末态电子动量为 p3,p4p_3, p_4。我们引入 Mandelstam 变量: s=(p1+p2)2,t=(p1p3)2,u=(p1p4)2s = (p_1 + p_2)^2, \quad t = (p_1 - p_3)^2, \quad u = (p_1 - p_4)^2 它们满足动量守恒关系 s+t+u=4m2s + t + u = 4m^2。在质心系中,各动量点积可用 Mandelstam 变量表示为: p1p2=p3p4=s2m2p_1 \cdot p_2 = p_3 \cdot p_4 = \frac{s}{2} - m^2 p1p3=p2p4=m2t2p_1 \cdot p_3 = p_2 \cdot p_4 = m^2 - \frac{t}{2} p1p4=p2p3=m2u2p_1 \cdot p_4 = p_2 \cdot p_3 = m^2 - \frac{u}{2}

根据 Feynman 规则,Møller 散射的树图振幅包含 tt 沟道和 uu 沟道两个图。由于末态是全同费米子,交换末态粒子会引入一个相对负号(泡利不相容原理): T=Tt+Tu=e2[uˉ3γμu1uˉ4γμu2tuˉ4γμu1uˉ3γμu2u]\mathcal{T} = \mathcal{T}_t + \mathcal{T}_u = -e^2 \left[ \frac{\bar{u}_3 \gamma^\mu u_1 \bar{u}_4 \gamma_\mu u_2}{t} - \frac{\bar{u}_4 \gamma^\mu u_1 \bar{u}_3 \gamma_\mu u_2}{u} \right]

我们需要计算对初态自旋求平均、对末态自旋求和的非极化振幅平方: T2=14spinsT2=14spins(Tt2+Tu22Re(TtTu))\langle |\mathcal{T}|^2 \rangle = \frac{1}{4} \sum_{\text{spins}} |\mathcal{T}|^2 = \frac{1}{4} \sum_{\text{spins}} \left( |\mathcal{T}_t|^2 + |\mathcal{T}_u|^2 - 2 \text{Re}(\mathcal{T}_t \mathcal{T}_u^*) \right)

1. 计算 tt 沟道项 14Tt2\frac{1}{4} \sum |\mathcal{T}_t|^2 利用 Casimir 技巧和迹定理 Tr[γμ(+m)γν(+m)]=4(AμBν+AνBμgμν(ABm2))\text{Tr}[\gamma^\mu (\not{A} + m) \gamma^\nu (\not{B} + m)] = 4(A^\mu B^\nu + A^\nu B^\mu - g^{\mu\nu}(A \cdot B - m^2)),可得: 14Tt2=e44t2Tr[γμ(̸p1+m)γν(̸p3+m)]Tr[γμ(̸p2+m)γν(̸p4+m)]\frac{1}{4} \sum |\mathcal{T}_t|^2 = \frac{e^4}{4t^2} \text{Tr}[\gamma^\mu (\not{p}_1 + m) \gamma^\nu (\not{p}_3 + m)] \text{Tr}[\gamma_\mu (\not{p}_2 + m) \gamma_\nu (\not{p}_4 + m)] =4e4t2[2(p1p2)(p3p4)+2(p1p4)(p2p3)2m2(p1p3+p2p4)+4m4]= \frac{4e^4}{t^2} \left[ 2(p_1 \cdot p_2)(p_3 \cdot p_4) + 2(p_1 \cdot p_4)(p_2 \cdot p_3) - 2m^2(p_1 \cdot p_3 + p_2 \cdot p_4) + 4m^4 \right] 代入 Mandelstam 变量: 14Tt2=2e4t2[(s2m2)2+(u2m2)2+4m2t]\frac{1}{4} \sum |\mathcal{T}_t|^2 = \frac{2e^4}{t^2} \left[ (s - 2m^2)^2 + (u - 2m^2)^2 + 4m^2 t \right] 展开并利用 s+u=4m2ts+u = 4m^2 - t 进一步化简: (s2m2)2+(u2m2)2+4m2t=s2+u24m2(s+u)+8m4+4m2t=s2+u2+8m2t8m4(s - 2m^2)^2 + (u - 2m^2)^2 + 4m^2 t = s^2 + u^2 - 4m^2(s+u) + 8m^4 + 4m^2 t = s^2 + u^2 + 8m^2 t - 8m^4 因此: 14Tt2=2e4t2(s2+u2+8m2t8m4)\frac{1}{4} \sum |\mathcal{T}_t|^2 = \frac{2e^4}{t^2} (s^2 + u^2 + 8m^2 t - 8m^4)

2. 计算 uu 沟道项 14Tu2\frac{1}{4} \sum |\mathcal{T}_u|^2 由对称性,将 tt 沟道结果中的 tut \leftrightarrow u 互换即可得到 uu 沟道项: 14Tu2=2e4u2(s2+t2+8m2u8m4)\frac{1}{4} \sum |\mathcal{T}_u|^2 = \frac{2e^4}{u^2} (s^2 + t^2 + 8m^2 u - 8m^4)

3. 计算干涉项 12ReTtTu-\frac{1}{2} \text{Re} \sum \mathcal{T}_t \mathcal{T}_u^* 干涉项的自旋求和对应于一个包含 8 个 γ\gamma 矩阵的大迹: 12ReTtTu=e42tuTr[γμ(̸p1+m)γν(̸p4+m)γμ(̸p2+m)γν(̸p3+m)]-\frac{1}{2} \text{Re} \sum \mathcal{T}_t \mathcal{T}_u^* = -\frac{e^4}{2tu} \text{Tr}\left[ \gamma^\mu (\not{p}_1 + m) \gamma^\nu (\not{p}_4 + m) \gamma_\mu (\not{p}_2 + m) \gamma_\nu (\not{p}_3 + m) \right] 利用 γ\gamma 矩阵的缩并恒等式 γμγμ=4\gamma^\mu \gamma_\mu = 4, γμγμ=2\gamma^\mu \not{A} \gamma_\mu = -2\not{A}, γμγμ=4AB\gamma^\mu \not{A} \not{B} \gamma_\mu = 4A \cdot B 等,先化简前三个括号: γμ(̸p1+m)γν(̸p4+m)γμ=2̸p4γν̸p1+4m(p1ν+p4ν)2m2γν\gamma^\mu (\not{p}_1 + m) \gamma^\nu (\not{p}_4 + m) \gamma_\mu = -2 \not{p}_4 \gamma^\nu \not{p}_1 + 4m(p_1^\nu + p_4^\nu) - 2m^2 \gamma^\nu 将其与剩余部分 (̸p2+m)γν(̸p3+m)(\not{p}_2 + m) \gamma_\nu (\not{p}_3 + m) 相乘并求迹,非零项(包含偶数个 γ\gamma 矩阵)为: Tint=2Tr[̸p4γν̸p1̸p2γν̸p3]2m2Tr[̸p4γν̸p1γν]+4m2(p1ν+p4ν)Tr[γν̸p3+̸p2γν]2m2Tr[γν̸p2γν̸p3]2m4Tr[γνγν]T_{\text{int}} = -2 \text{Tr}[\not{p}_4 \gamma^\nu \not{p}_1 \not{p}_2 \gamma_\nu \not{p}_3] - 2m^2 \text{Tr}[\not{p}_4 \gamma^\nu \not{p}_1 \gamma_\nu] + 4m^2 (p_1^\nu + p_4^\nu) \text{Tr}[\gamma_\nu \not{p}_3 + \not{p}_2 \gamma_\nu] - 2m^2 \text{Tr}[\gamma^\nu \not{p}_2 \gamma_\nu \not{p}_3] - 2m^4 \text{Tr}[\gamma^\nu \gamma_\nu] 逐项计算迹:

  1. 2Tr[̸p4(4p1p2)̸p3]=32(p1p2)(p3p4)-2 \text{Tr}[\not{p}_4 (4p_1 \cdot p_2) \not{p}_3] = -32(p_1 \cdot p_2)(p_3 \cdot p_4)
  2. 2m2Tr[̸p4(2̸p1)]=16m2(p1p4)-2m^2 \text{Tr}[\not{p}_4 (-2\not{p}_1)] = 16m^2(p_1 \cdot p_4)
  3. 4m2(p1ν+p4ν)4(p3ν+p2ν)=16m2(p1+p4)(p2+p3)4m^2 (p_1^\nu + p_4^\nu) 4(p_{3\nu} + p_{2\nu}) = 16m^2(p_1 + p_4) \cdot (p_2 + p_3)
  4. 2m2Tr[2̸p2̸p3]=16m2(p2p3)-2m^2 \text{Tr}[-2\not{p}_2 \not{p}_3] = 16m^2(p_2 \cdot p_3)
  5. 2m4(16)=32m4-2m^4 (16) = -32m^4

将上述结果相加并代入 Mandelstam 变量: Tint=32(s2m2)2+16m2(2m2u)+16m2(st)32m4T_{\text{int}} = -32\left(\frac{s}{2} - m^2\right)^2 + 16m^2\left(2m^2 - u\right) + 16m^2(s - t) - 32m^4 =8(s24m2s+4m4)+16m2(stu)= -8(s^2 - 4m^2 s + 4m^4) + 16m^2(s - t - u) 利用 t+u=4m2st + u = 4m^2 - s,有 stu=2s4m2s - t - u = 2s - 4m^2,代入上式: Tint=8s2+32m2s32m4+16m2(2s4m2)=8(s28m2s+12m4)T_{\text{int}} = -8s^2 + 32m^2 s - 32m^4 + 16m^2(2s - 4m^2) = -8(s^2 - 8m^2 s + 12m^4) 因此,干涉项为: e42tuTint=4e4tu(s28m2s+12m4)-\frac{e^4}{2tu} T_{\text{int}} = \frac{4e^4}{tu} (s^2 - 8m^2 s + 12m^4)

4. 综合结果与交叉对称性分析tt 沟道、uu 沟道和干涉项相加,得到 Møller 散射的完整非极化振幅平方: T2=2e4[s2+u2+8m2t8m4t2+s2+t2+8m2u8m4u2+2(s28m2s+12m4)tu]\langle |\mathcal{T}|^2 \rangle = 2e^4 \left[ \frac{s^2 + u^2 + 8m^2 t - 8m^4}{t^2} + \frac{s^2 + t^2 + 8m^2 u - 8m^4}{u^2} + \frac{2(s^2 - 8m^2 s + 12m^4)}{tu} \right]

对于 Bhabha 散射 (e+ee+ee^+e^- \rightarrow e^+e^-),其过程包含 ss 沟道和 tt 沟道,其振幅平方的已知结果为: TBhabha2=2e4[t2+u2+8m2s8m4s2+s2+u2+8m2t8m4t2+2(u28m2u+12m4)st]\langle |\mathcal{T}_{\text{Bhabha}}|^2 \rangle = 2e^4 \left[ \frac{t^2 + u^2 + 8m^2 s - 8m^4}{s^2} + \frac{s^2 + u^2 + 8m^2 t - 8m^4}{t^2} + \frac{2(u^2 - 8m^2 u + 12m^4)}{st} \right] 根据交叉对称性 (Crossing Symmetry),将 Bhabha 散射结果中的 ssuu 互换 (sus \leftrightarrow u): 2e4[t2+s2+8m2u8m4u2+u2+s2+8m2t8m4t2+2(s28m2s+12m4)ut]2e^4 \left[ \frac{t^2 + s^2 + 8m^2 u - 8m^4}{u^2} + \frac{u^2 + s^2 + 8m^2 t - 8m^4}{t^2} + \frac{2(s^2 - 8m^2 s + 12m^4)}{ut} \right] 这与我们刚刚推导出的 Møller 散射结果完全一致。

最终结果为:

T2=2e4[s2+u2+8m2t8m4t2+s2+t2+8m2u8m4u2+2(s28m2s+12m4)tu]\boxed{ \langle |\mathcal{T}|^2 \rangle = 2e^4 \left[ \frac{s^2 + u^2 + 8m^2 t - 8m^4}{t^2} + \frac{s^2 + t^2 + 8m^2 u - 8m^4}{u^2} + \frac{2(s^2 - 8m^2 s + 12m^4)}{tu} \right] }
48.4

Problem 48.4

srednickiChapter 48

习题 48.4

来源: 第48章, PDF第301,302,303页


48.4 Suppose that M>2mM > 2m, so that the scalar can decay to an electron-positron pair.

a) Compute the decay rate, summed over final spins.

b) Compute T2|\mathcal{T}|^2 for decay into an electron with spin s1s_1 and a positron with spin s2s_2. Take the fermion three-momenta to be along the zz axis, and let the xx-axis be the spin-quantization axis. You should find that T2=0|\mathcal{T}|^2 = 0 if s1=s2s_1 = -s_2, or if M=2mM = 2m (so that the outgoing three-momentum of each fermion is zero). Discuss this in light of conservation of angular momentum and of parity. (Prerequisite: 40.)

c) Compute T2|\mathcal{T}|^2 for decay into an electron with helicity s1s_1 and a positron with helicity s2s_2. (See section 38 for the definition of helicity.)

You should find that the decay rate is zero if s1=s2s_1 = -s_2. Discuss this in light of conservation of angular momentum and of parity.

d) Now consider changing the interaction to L1=igϕΨγ5Ψ\mathcal{L}_1 = ig\phi\overline{\Psi}\gamma_5\Psi, and compute the spin-summed decay rate. Explain (in light of conservation of angular momentum and of parity) why the decay rate is larger than it was without the iγ5i\gamma_5 in the interaction.

e) Repeat parts (b) and (c) for the new form of the interaction, and explain any differences in the results.

习题 48.4 - 解答


a) 计算自旋求和的衰变率

标量相互作用的拉格朗日量为 L1=gϕΨˉΨ\mathcal{L}_1 = g\phi\bar{\Psi}\Psi。衰变过程 ϕ(p)e(k1)+e+(k2)\phi(p) \to e^-(k_1) + e^+(k_2) 的跃迁矩阵元为: T=guˉs1(k1)vs2(k2)\mathcal{T} = g \bar{u}_{s_1}(k_1) v_{s_2}(k_2) 对末态自旋求和,矩阵元模方为: s1,s2T2=g2Tr[(̸k1+m)(̸k2m)]=4g2(k1k2m2)\sum_{s_1, s_2} |\mathcal{T}|^2 = g^2 \text{Tr}[(\not{k}_1 + m)(\not{k}_2 - m)] = 4g^2 (k_1 \cdot k_2 - m^2) 由动量守恒 p=k1+k2p = k_1 + k_2,有 M2=(k1+k2)2=2m2+2k1k2M^2 = (k_1 + k_2)^2 = 2m^2 + 2k_1 \cdot k_2,因此 k1k2=M22m2k_1 \cdot k_2 = \frac{M^2}{2} - m^2。代入上式得: s1,s2T2=2g2(M24m2)\sum_{s_1, s_2} |\mathcal{T}|^2 = 2g^2 (M^2 - 4m^2) 两体相空间积分为 dΠ2=18π14m2M2\int d\Pi_2 = \frac{1}{8\pi} \sqrt{1 - \frac{4m^2}{M^2}}。衰变率为: Γ=12MdΠ2s1,s2T2=12M18π14m2M22g2M2(14m2M2)\Gamma = \frac{1}{2M} \int d\Pi_2 \sum_{s_1, s_2} |\mathcal{T}|^2 = \frac{1}{2M} \frac{1}{8\pi} \sqrt{1 - \frac{4m^2}{M^2}} \cdot 2g^2 M^2 \left(1 - \frac{4m^2}{M^2}\right) Γ=g2M8π(14m2M2)3/2\boxed{ \Gamma = \frac{g^2 M}{8\pi} \left( 1 - \frac{4m^2}{M^2} \right)^{3/2} }

b) 计算 xx 轴自旋量子化下的 T2|\mathcal{T}|^2 并讨论

设电子和正电子的动量分别为 k1=kz^k_1 = k\hat{z}k2=kz^k_2 = -k\hat{z},其中 k=M2/4m2k = \sqrt{M^2/4 - m^2}。在标准表示下,旋量可写为: us1(k1)=(E+mχs1kσzE+mχs1),vs2(k2)=(kσzE+mηs2E+mηs2)u_{s_1}(k_1) = \begin{pmatrix} \sqrt{E+m} \chi_{s_1} \\ \frac{k\sigma_z}{\sqrt{E+m}} \chi_{s_1} \end{pmatrix}, \quad v_{s_2}(k_2) = \begin{pmatrix} \frac{-k\sigma_z}{\sqrt{E+m}} \eta_{s_2} \\ \sqrt{E+m} \eta_{s_2} \end{pmatrix} 矩阵元为: T=gus1γ0vs2=gχs1(E+mkσzE+mkσzE+mE+m)ηs2=2gkχs1σzηs2\mathcal{T} = g u_{s_1}^\dagger \gamma^0 v_{s_2} = g \chi_{s_1}^\dagger \left( \sqrt{E+m} \frac{-k\sigma_z}{\sqrt{E+m}} - \frac{k\sigma_z}{\sqrt{E+m}} \sqrt{E+m} \right) \eta_{s_2} = -2gk \chi_{s_1}^\dagger \sigma_z \eta_{s_2} 正电子的物理自旋与 vv 旋量描述的负能电子自旋相反。若正电子在 xx 轴的自旋为 s2s_2,则 ηs2\eta_{s_2} 必须是 σx\sigma_x 本征值为 s2-s_2 的本征态。而 χs1\chi_{s_1}σx\sigma_x 本征值为 s1s_1 的本征态。 由于 σz\sigma_zσx\sigma_x 反易位,σzηs2\sigma_z \eta_{s_2} 会翻转 σx\sigma_x 的本征值,使其变为 (s2)=s2-(-s_2) = s_2。因此,内积 χs1(σzηs2)\chi_{s_1}^\dagger (\sigma_z \eta_{s_2}) 仅当 s1=s2s_1 = s_2 时非零。 T2=4g2k2δs1,s2=g2(M24m2)δs1,s2\boxed{ |\mathcal{T}|^2 = 4g^2 k^2 \delta_{s_1, s_2} = g^2 (M^2 - 4m^2) \delta_{s_1, s_2} } 讨论

  1. 角动量守恒:初态标量粒子 J=0J=0。末态 e+ee^+e^- 的宇称为 P=(1)L+1P = (-1)^{L+1}。由于初态 P=+1P=+1,要求 LL 为奇数。为满足 J=0J=0,必须有 S=LS=L,故最低阶允许态为 L=1,S=1L=1, S=1(即 3P0^3P_0 态)。总自旋 S=1S=1 意味着自旋波函数是对称的。在 xx 轴基底中,满足 Jz=0J_z=0S=1S=1 态仅由 +,+|+,+\rangle,|-,-\rangle 组成,因此 s1=s2s_1 = -s_2 的跃迁被禁戒。
  2. 宇称守恒L=1L=1 意味着这是一个 pp 波衰变,存在离心势垒,振幅正比于动量 kk。当 M=2mM=2mk=0k=0,衰变率必然为零。

c) 计算螺旋度基底下的 T2|\mathcal{T}|^2 并讨论

螺旋度是自旋在动量方向上的投影。电子动量沿 +z^+\hat{z},螺旋度 λ1\lambda_1 即为 +z^+\hat{z} 方向的自旋,故 χλ1\chi_{\lambda_1}σz\sigma_z 本征值为 λ1\lambda_1 的态。 正电子动量沿 z^-\hat{z},螺旋度 λ2\lambda_2 是沿 z^-\hat{z} 的自旋,这意味着其沿 +z^+\hat{z} 的物理自旋为 λ2/2-\lambda_2/2。由于 vv 旋量自旋与物理自旋相反,ηλ2\eta_{\lambda_2} 必须是 σz\sigma_z 本征值为 λ2\lambda_2 的态。 代入矩阵元 T=2gkχλ1σzηλ2=2gkλ2χλ1ηλ2\mathcal{T} = -2gk \chi_{\lambda_1}^\dagger \sigma_z \eta_{\lambda_2} = -2gk \lambda_2 \chi_{\lambda_1}^\dagger \eta_{\lambda_2}。由于两者都是 σz\sigma_z 的本征态,内积仅在 λ1=λ2\lambda_1 = \lambda_2 时非零。 T2=g2(M24m2)δλ1,λ2\boxed{ |\mathcal{T}|^2 = g^2 (M^2 - 4m^2) \delta_{\lambda_1, \lambda_2} } 讨论: 角动量在 zz 轴的投影 Jz=Sz(e)+Sz(e+)=λ12+(λ22)=λ1λ22J_z = S_{z}(e^-) + S_{z}(e^+) = \frac{\lambda_1}{2} + \left(-\frac{\lambda_2}{2}\right) = \frac{\lambda_1 - \lambda_2}{2}。由于初态 J=0J=0,必须有 Jz=0J_z = 0,这严格要求 λ1=λ2\lambda_1 = \lambda_2。因此 λ1=λ2\lambda_1 = -\lambda_2 的衰变率为零。

d) 伪标量相互作用下的衰变率

新的拉格朗日量为 L1=igϕΨˉγ5Ψ\mathcal{L}_1 = ig\phi\bar{\Psi}\gamma_5\Psi。矩阵元为 T=iguˉs1(k1)γ5vs2(k2)\mathcal{T} = ig \bar{u}_{s_1}(k_1) \gamma_5 v_{s_2}(k_2)。 自旋求和的矩阵元模方为: s1,s2T2=g2Tr[(̸k1+m)γ5(̸k2m)(γ5)]=g2Tr[(̸k1+m)(̸k2+m)]=4g2(k1k2+m2)\sum_{s_1, s_2} |\mathcal{T}|^2 = g^2 \text{Tr}[(\not{k}_1 + m) \gamma_5 (\not{k}_2 - m) (-\gamma_5)] = g^2 \text{Tr}[(\not{k}_1 + m) (\not{k}_2 + m)] = 4g^2 (k_1 \cdot k_2 + m^2) 代入 k1k2=M22m2k_1 \cdot k_2 = \frac{M^2}{2} - m^2,得到 T2=2g2M2\sum |\mathcal{T}|^2 = 2g^2 M^2。衰变率为: Γ=g2M8π(14m2M2)1/2\boxed{ \Gamma = \frac{g^2 M}{8\pi} \left( 1 - \frac{4m^2}{M^2} \right)^{1/2} } 解释: 初态现在是伪标量(P=1P=-1)。末态宇称 P=(1)L+1=1P = (-1)^{L+1} = -1 要求 LL 为偶数。为满足 J=0J=0,必须有 L=0,S=0L=0, S=0(即 1S0^1S_0 态)。因为 L=0L=0ss 波衰变,不存在离心势垒,矩阵元在阈值 k0k \to 0 时不包含 k2k^2 的压低因子,因此衰变率比标量相互作用更大。

e) 伪标量相互作用下的自旋与螺旋度分析

矩阵元化简为: T=igus1γ0γ5vs2=igχs1(E+mE+mkσzE+mkσzE+m)ηs2=igMχs1ηs2\mathcal{T} = ig u_{s_1}^\dagger \gamma^0 \gamma_5 v_{s_2} = ig \chi_{s_1}^\dagger \left( \sqrt{E+m}\sqrt{E+m} - \frac{k\sigma_z}{\sqrt{E+m}}\frac{-k\sigma_z}{\sqrt{E+m}} \right) \eta_{s_2} = ig M \chi_{s_1}^\dagger \eta_{s_2}

  1. xx 轴自旋基底χs1\chi_{s_1} 具有 σx=s1\sigma_x = s_1,而 ηs2\eta_{s_2} 具有 σx=s2\sigma_x = -s_2。正交性要求内积仅在 s1=s2s_1 = -s_2 时非零。 T2=g2M2δs1,s2\boxed{ |\mathcal{T}|^2 = g^2 M^2 \delta_{s_1, -s_2} } 差异解释:末态是 S=0S=0 的单态(反对称)。单态在任何空间方向上的自旋投影必然相反,因此要求 s1=s2s_1 = -s_2(与 (b) 中的 s1=s2s_1 = s_2 相反)。此外,由于是 ss 波衰变,当 M=2mM=2mT2|\mathcal{T}|^2 不为零。

  2. 螺旋度基底χλ1\chi_{\lambda_1} 具有 σz=λ1\sigma_z = \lambda_1,而 ηλ2\eta_{\lambda_2} 具有 σz=λ2\sigma_z = \lambda_2。正交性要求内积仅在 λ1=λ2\lambda_1 = \lambda_2 时非零。 T2=g2M2δλ1,λ2\boxed{ |\mathcal{T}|^2 = g^2 M^2 \delta_{\lambda_1, \lambda_2} } 差异解释:选择定则 λ1=λ2\lambda_1 = \lambda_2 与 (c) 完全相同,因为无论相互作用形式如何,沿运动轴的角动量守恒 Jz=0J_z = 0 始终要求 λ1=λ2\lambda_1 = \lambda_2。唯一的区别是去除了 pp 波带来的动量压低因子 (M24m2)(M^2 - 4m^2),替换为了 M2M^2

48.5

Problem 48.5

srednickiChapter 48

习题 48.5

来源: 第48章, PDF第302页


48.5 The charged pion π\pi^- is represented by a complex scalar field ϕ\phi, the muon μ\mu^- by a Dirac field M\mathcal{M}, and the muon neutrino νμ\nu_\mu by a spin-projected Dirac field PLNP_L\mathcal{N}, where PL=12(1γ5)P_L = \frac{1}{2}(1-\gamma_5). The charged pion can decay to a muon and a muon antineutrino via the interaction

L1=2c1GFfπμϕMγμPLN+h.c.,(48.30)\mathcal{L}_1 = 2c_1 G_F f_\pi \partial_\mu \phi \overline{\mathcal{M}} \gamma^\mu P_L \mathcal{N} + \text{h.c.} , \tag{48.30}

where c1c_1 is the cosine of the Cabibbo angle, GFG_F is the Fermi constant, and fπf_\pi is the pion decay constant.

a) Compute the charged pion decay rate Γ\Gamma.

b) The charged pion mass is mπ=139.6 MeVm_\pi = 139.6 \text{ MeV}, the muon mass is mμ=105.7 MeVm_\mu = 105.7 \text{ MeV}, and the muon neutrino is massless. The Fermi constant is measured in muon decay to be GF=1.166×105 GeV2G_F = 1.166 \times 10^{-5} \text{ GeV}^{-2}, and the cosine of the Cabibbo angle is measured in nuclear beta decays to be c1=0.974c_1 = 0.974. The measured value of the charged pion lifetime is 2.603×108 s2.603 \times 10^{-8} \text{ s}. Determine the value of fπf_\pi in MeV. Your result is too large by 0.8%0.8\%, due to neglect of electromagnetic loop corrections.

习题 48.5 - 解答


针对带电 π\pi 介子衰变过程 π(p)μ(k1)+νˉμ(k2)\pi^-(p) \to \mu^-(k_1) + \bar{\nu}_\mu(k_2),基于给定的有效拉格朗日量进行分析与计算。

(a) 计算带电 π\pi 介子的衰变率 Γ\Gamma

1. 写出跃迁矩阵元 由相互作用拉格朗日量 L1=2c1GFfπμϕMγμPLN+h.c.\mathcal{L}_1 = 2c_1 G_F f_\pi \partial_\mu \phi \overline{\mathcal{M}} \gamma^\mu P_L \mathcal{N} + \text{h.c.},标量场 ϕ\phi 湮灭初态 π\pi^- 介子,产生一个动量因子 ipμ-ip_\mu。因此,该过程的不变矩阵元(记为 A\mathcal{A} 以区分缪子场 M\mathcal{M})为:

iA=i(2c1GFfπ)(ipμ)uˉ(k1)γμPLv(k2)i\mathcal{A} = i(2c_1 G_F f_\pi) (-ip_\mu) \bar{u}(k_1) \gamma^\mu P_L v(k_2)

即:

A=2c1GFfπpμuˉ(k1)γμPLv(k2)\mathcal{A} = 2c_1 G_F f_\pi p_\mu \bar{u}(k_1) \gamma^\mu P_L v(k_2)

2. 计算矩阵元模方与自旋求和 初态为自旋为 0 的 π\pi 介子,无需自旋平均;对末态费米子自旋求和。利用 PL=1γ52P_L = \frac{1-\gamma_5}{2} 及其性质 γ0PLγ0=PR\gamma^0 P_L^\dagger \gamma^0 = P_RγνPR=PLγν\gamma^\nu P_R = P_L \gamma^\nu,可得:

spinsA2=4c12GF2fπ2pμpνTr[(̸k1+mμ)γμPL̸k2γνPL]\sum_{\text{spins}} |\mathcal{A}|^2 = 4 c_1^2 G_F^2 f_\pi^2 p_\mu p_\nu \text{Tr}\left[ (\not{k}_1 + m_\mu) \gamma^\mu P_L \not{k}_2 \gamma^\nu P_L \right]

由于中微子无质量 (mν=0m_\nu = 0),且 PL̸k2γνPL≠k2PRγνPL≠k2γνPL2≠k2γνPLP_L \not{k}_2 \gamma^\nu P_L = \not{k}_2 P_R \gamma^\nu P_L = \not{k}_2 \gamma^\nu P_L^2 = \not{k}_2 \gamma^\nu P_L,迹化简为:

Tr[(̸k1+mμ)γμ̸k2γνPL]\text{Tr}\left[ (\not{k}_1 + m_\mu) \gamma^\mu \not{k}_2 \gamma^\nu P_L \right]

包含奇数个 γ\gamma 矩阵的项(即含 mμm_\mu 的项)迹为零,剩下:

Tr[̸k1γμ̸k2γνPL]=12Tr[̸k1γμ̸k2γν(1γ5)]\text{Tr}\left[ \not{k}_1 \gamma^\mu \not{k}_2 \gamma^\nu P_L \right] = \frac{1}{2} \text{Tr}\left[ \not{k}_1 \gamma^\mu \not{k}_2 \gamma^\nu (1-\gamma_5) \right]

利用狄拉克矩阵迹定理 Tr(γμγν)=4(aμbν+aνbμgμνab)\text{Tr}(\not{a}\gamma^\mu\not{b}\gamma^\nu) = 4(a^\mu b^\nu + a^\nu b^\mu - g^{\mu\nu} a \cdot b),而含 γ5\gamma_5 的项会产生完全反对称张量 ϵαμβν\epsilon^{\alpha\mu\beta\nu},当它与对称张量 pμpνp_\mu p_\nu 缩并时结果为零。因此:

pμpνTr[̸k1γμ̸k2γνPL]=2[2(pk1)(pk2)p2(k1k2)]p_\mu p_\nu \text{Tr}\left[ \not{k}_1 \gamma^\mu \not{k}_2 \gamma^\nu P_L \right] = 2 \left[ 2(p \cdot k_1)(p \cdot k_2) - p^2 (k_1 \cdot k_2) \right]

3. 运动学关系代入 由动量守恒 p=k1+k2p = k_1 + k_2,且 p2=mπ2p^2 = m_\pi^2, k12=mμ2k_1^2 = m_\mu^2, k22=0k_2^2 = 0,可得:

k1k2=12(p2k12k22)=mπ2mμ22k_1 \cdot k_2 = \frac{1}{2}(p^2 - k_1^2 - k_2^2) = \frac{m_\pi^2 - m_\mu^2}{2}
pk1=k12+k1k2=mπ2+mμ22p \cdot k_1 = k_1^2 + k_1 \cdot k_2 = \frac{m_\pi^2 + m_\mu^2}{2}
pk2=k22+k1k2=mπ2mμ22p \cdot k_2 = k_2^2 + k_1 \cdot k_2 = \frac{m_\pi^2 - m_\mu^2}{2}

代入前面的表达式中:

2(pk1)(pk2)p2(k1k2)=2(mπ2+mμ22)(mπ2mμ22)mπ2(mπ2mμ22)=12mμ2(mπ2mμ2)2(p \cdot k_1)(p \cdot k_2) - p^2 (k_1 \cdot k_2) = 2 \left( \frac{m_\pi^2 + m_\mu^2}{2} \right) \left( \frac{m_\pi^2 - m_\mu^2}{2} \right) - m_\pi^2 \left( \frac{m_\pi^2 - m_\mu^2}{2} \right) = \frac{1}{2} m_\mu^2 (m_\pi^2 - m_\mu^2)

因此,自旋求和后的矩阵元模方为:

spinsA2=4c12GF2fπ2×2×12mμ2(mπ2mμ2)=4c12GF2fπ2mμ2(mπ2mμ2)\sum_{\text{spins}} |\mathcal{A}|^2 = 4 c_1^2 G_F^2 f_\pi^2 \times 2 \times \frac{1}{2} m_\mu^2 (m_\pi^2 - m_\mu^2) = 4 c_1^2 G_F^2 f_\pi^2 m_\mu^2 (m_\pi^2 - m_\mu^2)

4. 计算两体衰变率π\pi 介子静止系中,两体衰变相空间给出的衰变率为:

Γ=k8πmπ2spinsA2\Gamma = \frac{|\mathbf{k}|}{8\pi m_\pi^2} \sum_{\text{spins}} |\mathcal{A}|^2

其中末态粒子动量大小为 k=mπ2mμ22mπ|\mathbf{k}| = \frac{m_\pi^2 - m_\mu^2}{2m_\pi}。代入可得:

Γ=mπ2mμ216πmπ3[4c12GF2fπ2mμ2(mπ2mμ2)]=c12GF2fπ2mμ24πmπ3(mπ2mμ2)2\Gamma = \frac{m_\pi^2 - m_\mu^2}{16\pi m_\pi^3} \left[ 4 c_1^2 G_F^2 f_\pi^2 m_\mu^2 (m_\pi^2 - m_\mu^2) \right] = \frac{c_1^2 G_F^2 f_\pi^2 m_\mu^2}{4\pi m_\pi^3} (m_\pi^2 - m_\mu^2)^2

整理成标准形式:

Γ=c12GF2fπ24πmπmμ2(1mμ2mπ2)2\boxed{ \Gamma = \frac{c_1^2 G_F^2 f_\pi^2}{4\pi} m_\pi m_\mu^2 \left( 1 - \frac{m_\mu^2}{m_\pi^2} \right)^2 }

(b) 确定 π\pi 介子衰变常数 fπf_\pi 的数值

1. 提取已知物理量并统一单位 已知参数:

  • mπ=139.6 MeVm_\pi = 139.6 \text{ MeV}
  • mμ=105.7 MeVm_\mu = 105.7 \text{ MeV}
  • GF=1.166×105 GeV2=1.166×1011 MeV2G_F = 1.166 \times 10^{-5} \text{ GeV}^{-2} = 1.166 \times 10^{-11} \text{ MeV}^{-2}
  • c1=0.974c_1 = 0.974
  • τ=2.603×108 s\tau = 2.603 \times 10^{-8} \text{ s}
  • 普朗克常数 6.58212×1022 MeVs\hbar \approx 6.58212 \times 10^{-22} \text{ MeV}\cdot\text{s}

2. 计算衰变宽度 Γ\Gamma 利用寿命与衰变宽度的关系 Γ=/τ\Gamma = \hbar / \tau

Γ=6.58212×1022 MeVs2.603×108 s2.5287×1014 MeV\Gamma = \frac{6.58212 \times 10^{-22} \text{ MeV}\cdot\text{s}}{2.603 \times 10^{-8} \text{ s}} \approx 2.5287 \times 10^{-14} \text{ MeV}

3. 求解 fπf_\pi 由 (a) 中得到的衰变率公式,反解 fπf_\pi

fπ=4πmπ3Γc12GF2mμ2(mπ2mμ2)2=2mπc1GFmμ(mπ2mμ2)πmπΓf_\pi = \sqrt{ \frac{4\pi m_\pi^3 \Gamma}{c_1^2 G_F^2 m_\mu^2 (m_\pi^2 - m_\mu^2)^2} } = \frac{2 m_\pi}{c_1 G_F m_\mu (m_\pi^2 - m_\mu^2)} \sqrt{\pi m_\pi \Gamma}

先计算部分中间项:

  • mπ2mμ2=139.62105.72=19488.1611172.49=8315.67 MeV2m_\pi^2 - m_\mu^2 = 139.6^2 - 105.7^2 = 19488.16 - 11172.49 = 8315.67 \text{ MeV}^2
  • 分母:c1GFmμ(mπ2mμ2)=0.974×(1.166×1011)×105.7×8315.679.9808×106 MeV1c_1 G_F m_\mu (m_\pi^2 - m_\mu^2) = 0.974 \times (1.166 \times 10^{-11}) \times 105.7 \times 8315.67 \approx 9.9808 \times 10^{-6} \text{ MeV}^{-1}
  • 根号项:πmπΓ=π×139.6×(2.5287×1014)1.109×10113.330×106 MeV\sqrt{\pi m_\pi \Gamma} = \sqrt{\pi \times 139.6 \times (2.5287 \times 10^{-14})} \approx \sqrt{1.109 \times 10^{-11}} \approx 3.330 \times 10^{-6} \text{ MeV}
  • 分子:2mππmπΓ=2×139.6×3.330×1069.297×104 MeV22 m_\pi \sqrt{\pi m_\pi \Gamma} = 2 \times 139.6 \times 3.330 \times 10^{-6} \approx 9.297 \times 10^{-4} \text{ MeV}^2

将分子分母相除:

fπ=9.297×104 MeV29.9808×106 MeV193.15 MeVf_\pi = \frac{9.297 \times 10^{-4} \text{ MeV}^2}{9.9808 \times 10^{-6} \text{ MeV}^{-1}} \approx 93.15 \text{ MeV}

(注:由于未包含电磁圈图修正,该树图级计算结果比真实物理值偏大近 0.8%0.8\%,修正后的真实值约为 92.4 MeV92.4 \text{ MeV},与题目说明完全吻合。)

fπ93.2 MeV\boxed{ f_\pi \approx 93.2 \text{ MeV} }