90.1

Problem 90.1

srednickiChapter 90

习题 90.1

来源: 第90章, PDF第554页


90.1 Verify that the covariant derivatives in eqs. (90.7–90.10) transform appropriately.


Referenced Equations:

Equation (90.10):

DμNR=(μirμ)NR .(90.10)D_\mu N_\text{R} = (\partial_\mu - ir_\mu)N_\text{R} \ . \tag{90.10}

Equation (90.7):

DμU=μUilμU+iUrμ ,(90.7)D_\mu U = \partial_\mu U - il_\mu U + iUr_\mu \ , \tag{90.7}

Equation (90.8):

DμU=μU+iUlμirμU ,(90.8)D_\mu U^\dagger = \partial_\mu U^\dagger + iU^\dagger l_\mu - ir_\mu U^\dagger \ , \tag{90.8}

Equation (90.9):

DμNL=(μilμ)NL ,(90.9)D_\mu N_\text{L} = (\partial_\mu - il_\mu)N_\text{L} \ , \tag{90.9}

习题 90.1 - 解答


为了验证协变导数在局域手征变换下的变换行为,我们首先需要明确理论的物理背景与各场量的变换规则。

在具有 SU(N)L×SU(N)RSU(N)_\text{L} \times SU(N)_\text{R} 局域手征对称性的规范理论中,设局域变换矩阵为 L(x)SU(N)LL(x) \in SU(N)_\text{L}R(x)SU(N)RR(x) \in SU(N)_\text{R}。各物质场在局域变换下的行为如下: NLNL=LNLN_\text{L} \to N_\text{L}' = L N_\text{L} NRNR=RNRN_\text{R} \to N_\text{R}' = R N_\text{R} UU=LURU \to U' = L U R^\dagger U(U)=RULU^\dagger \to (U^\dagger)' = R U^\dagger L^\dagger

为了保证拉格朗日量的局域规范不变性,引入了左手和右手规范场(联络)lμl_\murμr_\mu。作为非阿贝尔规范场,它们的变换规则为: lμlμ=LlμL+iLμLl_\mu \to l_\mu' = L l_\mu L^\dagger + i L \partial_\mu L^\dagger rμrμ=RrμR+iRμRr_\mu \to r_\mu' = R r_\mu R^\dagger + i R \partial_\mu R^\dagger

“协变导数变换行为恰当”意味着,协变导数作用在场上后,其整体的变换规律必须与原场完全一致。在推导中,我们将反复使用幺正矩阵的性质 LL=1L L^\dagger = 1,对其求导可得: (μL)L+L(μL)=0    L(μL)=(μL)L(\partial_\mu L) L^\dagger + L (\partial_\mu L^\dagger) = 0 \implies L (\partial_\mu L^\dagger) = - (\partial_\mu L) L^\dagger 同理对于 RR 矩阵有 R(μR)=(μR)RR (\partial_\mu R^\dagger) = - (\partial_\mu R) R^\dagger

下面逐一验证四个协变导数方程。


1. 验证方程 (90.9) 中的 DμNLD_\mu N_\text{L}

协变导数定义为 DμNL=(μilμ)NLD_\mu N_\text{L} = (\partial_\mu - il_\mu)N_\text{L}。在局域变换下: (DμNL)=(μilμ)NL(D_\mu N_\text{L})' = (\partial_\mu - il_\mu') N_\text{L}' 代入 NLN_\text{L}'lμl_\mu' 的表达式: (DμNL)=μ(LNL)i(LlμL+iLμL)(LNL)(D_\mu N_\text{L})' = \partial_\mu (L N_\text{L}) - i (L l_\mu L^\dagger + i L \partial_\mu L^\dagger) (L N_\text{L}) 利用乘积法则展开导数项,并分配规范场项: (DμNL)=(μL)NL+L(μNL)iLlμ(LL)NL+L(μL)LNL(D_\mu N_\text{L})' = (\partial_\mu L) N_\text{L} + L (\partial_\mu N_\text{L}) - i L l_\mu (L^\dagger L) N_\text{L} + L (\partial_\mu L^\dagger) L N_\text{L} 由于 LL=1L^\dagger L = 1,且利用前面提到的恒等式 L(μL)L=(μL)LL=μLL (\partial_\mu L^\dagger) L = - (\partial_\mu L) L^\dagger L = - \partial_\mu L,上式化简为: (DμNL)=(μL)NL+L(μNL)iLlμNL(μL)NL(D_\mu N_\text{L})' = (\partial_\mu L) N_\text{L} + L (\partial_\mu N_\text{L}) - i L l_\mu N_\text{L} - (\partial_\mu L) N_\text{L} 第一项与第四项相互抵消,提取公因子 LL(DμNL)=L(μNLilμNL)(D_\mu N_\text{L})' = L (\partial_\mu N_\text{L} - i l_\mu N_\text{L}) (DμNL)=L(DμNL)\boxed{ (D_\mu N_\text{L})' = L (D_\mu N_\text{L}) } 这表明 DμNLD_\mu N_\text{L} 确实像 NLN_\text{L} 一样作为 SU(N)LSU(N)_\text{L} 的基础表示进行变换。


2. 验证方程 (90.10) 中的 DμNRD_\mu N_\text{R}

协变导数定义为 DμNR=(μirμ)NRD_\mu N_\text{R} = (\partial_\mu - ir_\mu)N_\text{R}。其推导过程与 NLN_\text{L} 完全对称: (DμNR)=(μirμ)NR(D_\mu N_\text{R})' = (\partial_\mu - ir_\mu') N_\text{R}' (DμNR)=μ(RNR)i(RrμR+iRμR)(RNR)(D_\mu N_\text{R})' = \partial_\mu (R N_\text{R}) - i (R r_\mu R^\dagger + i R \partial_\mu R^\dagger) (R N_\text{R}) (DμNR)=(μR)NR+R(μNR)iRrμNR+R(μR)RNR(D_\mu N_\text{R})' = (\partial_\mu R) N_\text{R} + R (\partial_\mu N_\text{R}) - i R r_\mu N_\text{R} + R (\partial_\mu R^\dagger) R N_\text{R} 利用 R(μR)R=μRR (\partial_\mu R^\dagger) R = - \partial_\mu R,抵消掉导数项: (DμNR)=R(μNRirμNR)(D_\mu N_\text{R})' = R (\partial_\mu N_\text{R} - i r_\mu N_\text{R}) (DμNR)=R(DμNR)\boxed{ (D_\mu N_\text{R})' = R (D_\mu N_\text{R}) } 这表明 DμNRD_\mu N_\text{R}NRN_\text{R} 一样作为 SU(N)RSU(N)_\text{R} 的基础表示进行变换。


3. 验证方程 (90.7) 中的 DμUD_\mu U

协变导数定义为 DμU=μUilμU+iUrμD_\mu U = \partial_\mu U - il_\mu U + iUr_\mu。在局域变换下: (DμU)=μUilμU+iUrμ(D_\mu U)' = \partial_\mu U' - i l_\mu' U' + i U' r_\mu' 代入 U,lμ,rμU', l_\mu', r_\mu'(DμU)=μ(LUR)i(LlμL+iLμL)(LUR)+i(LUR)(RrμR+iRμR)(D_\mu U)' = \partial_\mu (L U R^\dagger) - i (L l_\mu L^\dagger + i L \partial_\mu L^\dagger) (L U R^\dagger) + i (L U R^\dagger) (R r_\mu R^\dagger + i R \partial_\mu R^\dagger) 展开第一项(包含三部分的导数): μ(LUR)=(μL)UR+L(μU)R+LU(μR)\partial_\mu (L U R^\dagger) = (\partial_\mu L) U R^\dagger + L (\partial_\mu U) R^\dagger + L U (\partial_\mu R^\dagger) 展开第二项(左规范场部分): i(LlμL+iLμL)LUR=iLlμUR+L(μL)LUR- i (L l_\mu L^\dagger + i L \partial_\mu L^\dagger) L U R^\dagger = - i L l_\mu U R^\dagger + L (\partial_\mu L^\dagger) L U R^\dagger 利用 L(μL)L=μLL (\partial_\mu L^\dagger) L = - \partial_\mu L,该项变为: iLlμUR(μL)UR- i L l_\mu U R^\dagger - (\partial_\mu L) U R^\dagger 展开第三项(右规范场部分): iLUR(RrμR+iRμR)=iLUrμRLURR(μR)i L U R^\dagger (R r_\mu R^\dagger + i R \partial_\mu R^\dagger) = i L U r_\mu R^\dagger - L U R^\dagger R (\partial_\mu R^\dagger) 利用 RR=1R^\dagger R = 1,该项变为: iLUrμRLU(μR)i L U r_\mu R^\dagger - L U (\partial_\mu R^\dagger) 将上述三部分相加,非协变的导数项 (μL)UR(\partial_\mu L) U R^\daggerLU(μR)L U (\partial_\mu R^\dagger) 均被精确抵消: (DμU)=L(μU)RiLlμUR+iLUrμR(D_\mu U)' = L (\partial_\mu U) R^\dagger - i L l_\mu U R^\dagger + i L U r_\mu R^\dagger 提取左侧的 LL 和右侧的 RR^\dagger(DμU)=L(μUilμU+iUrμ)R(D_\mu U)' = L (\partial_\mu U - i l_\mu U + i U r_\mu) R^\dagger (DμU)=L(DμU)R\boxed{ (D_\mu U)' = L (D_\mu U) R^\dagger } 这表明 DμUD_\mu UUU 一样作为双重基础表示(bifundamental representation)进行变换。


4. 验证方程 (90.8) 中的 DμUD_\mu U^\dagger

协变导数定义为 DμU=μU+iUlμirμUD_\mu U^\dagger = \partial_\mu U^\dagger + iU^\dagger l_\mu - ir_\mu U^\dagger。在局域变换下: (DμU)=μ(U)+i(U)lμirμ(U)(D_\mu U^\dagger)' = \partial_\mu (U^\dagger)' + i (U^\dagger)' l_\mu' - i r_\mu' (U^\dagger)' 代入 (U)=RUL(U^\dagger)' = R U^\dagger L^\dagger 以及规范场: (DμU)=μ(RUL)+i(RUL)(LlμL+iLμL)i(RrμR+iRμR)(RUL)(D_\mu U^\dagger)' = \partial_\mu (R U^\dagger L^\dagger) + i (R U^\dagger L^\dagger) (L l_\mu L^\dagger + i L \partial_\mu L^\dagger) - i (R r_\mu R^\dagger + i R \partial_\mu R^\dagger) (R U^\dagger L^\dagger) 展开导数项: μ(RUL)=(μR)UL+R(μU)L+RU(μL)\partial_\mu (R U^\dagger L^\dagger) = (\partial_\mu R) U^\dagger L^\dagger + R (\partial_\mu U^\dagger) L^\dagger + R U^\dagger (\partial_\mu L^\dagger) 展开左规范场项: iRUL(LlμL+iLμL)=iRUlμLRULL(μL)=iRUlμLRU(μL)i R U^\dagger L^\dagger (L l_\mu L^\dagger + i L \partial_\mu L^\dagger) = i R U^\dagger l_\mu L^\dagger - R U^\dagger L^\dagger L (\partial_\mu L^\dagger) = i R U^\dagger l_\mu L^\dagger - R U^\dagger (\partial_\mu L^\dagger) 展开右规范场项: i(RrμR+iRμR)RUL=iRrμUL+R(μR)RUL=iRrμUL(μR)UL- i (R r_\mu R^\dagger + i R \partial_\mu R^\dagger) R U^\dagger L^\dagger = - i R r_\mu U^\dagger L^\dagger + R (\partial_\mu R^\dagger) R U^\dagger L^\dagger = - i R r_\mu U^\dagger L^\dagger - (\partial_\mu R) U^\dagger L^\dagger 将三部分相加,非协变项 (μR)UL(\partial_\mu R) U^\dagger L^\daggerRU(μL)R U^\dagger (\partial_\mu L^\dagger) 再次被精确抵消: (DμU)=R(μU)L+iRUlμLiRrμUL(D_\mu U^\dagger)' = R (\partial_\mu U^\dagger) L^\dagger + i R U^\dagger l_\mu L^\dagger - i R r_\mu U^\dagger L^\dagger 提取左侧的 RR 和右侧的 LL^\dagger(DμU)=R(μU+iUlμirμU)L(D_\mu U^\dagger)' = R (\partial_\mu U^\dagger + i U^\dagger l_\mu - i r_\mu U^\dagger) L^\dagger (DμU)=R(DμU)L\boxed{ (D_\mu U^\dagger)' = R (D_\mu U^\dagger) L^\dagger } 这表明 DμUD_\mu U^\dagger 的变换行为与 UU^\dagger 完全一致。至此,四个协变导数的变换性质均验证完毕。

90.2

Problem 90.2

srednickiChapter 90

习题 90.2

来源: 第90章, PDF第554页


90.2 Verify that substituting eq. (90.11) into eq. (90.1) yields eq. (90.12).


Referenced Equations:

Equation (90.1):

L=14fπ2TrμUμU+v3Tr(MU+MU)+iNˉ ⁣ ⁣ ⁣/NmNNˉ(UPL+UPR)N12(gA1)iNˉγμ(UμUPL+UμUPR)N,(90.1)\begin{aligned} \mathcal{L} = &-\frac{1}{4} f_{\pi}^{2} \operatorname{Tr} \partial^{\mu} U^{\dagger} \partial_{\mu} U + v^{3} \operatorname{Tr}(M U + M^{\dagger} U^{\dagger}) \\ &+ i \bar{N} \partial \! \! \! / N - m_{N} \bar{N}(U^{\dagger} P_{L} + U P_{R}) N \\ &- \frac{1}{2}(g_{A} - 1) i \bar{N} \gamma^{\mu}(U \partial_{\mu} U^{\dagger} P_{L} + U^{\dagger} \partial_{\mu} U P_{R}) N, \end{aligned} \tag{90.1}

Equation (90.11):

N=(uPL+uPR)N ,(90.11)N = (uP_\text{L} + u^\dagger P_\text{R})\mathcal{N} \ , \tag{90.11}

Equation (90.12):

L=14fπ2Tr(μUμUilμUμUirμUμU+lμlμ+rμrμ2lμUrμU)+v3Tr(MU+MU)+iN ⁣ ⁣ ⁣/NmNNN+N(v ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/+12r~ ⁣ ⁣ ⁣/)NgAN(a ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/12r~ ⁣ ⁣ ⁣/)γ5N ,(90.12)\begin{aligned} \mathcal{L} = &-\tfrac{1}{4} f_\pi^2 \operatorname{Tr}(\partial^\mu U^\dagger \partial_\mu U - il^\mu U \overleftrightarrow{\partial}_\mu U^\dagger - ir^\mu U^\dagger \overleftrightarrow{\partial}_\mu U \\ &+ l^\mu l_\mu + r^\mu r_\mu - 2l^\mu U r_\mu U^\dagger) \\ &+ v^3 \operatorname{Tr}(MU + M^\dagger U^\dagger) + i\overline{\mathcal{N}} \partial \! \! \! / \mathcal{N} - m_N \overline{\mathcal{N}} \mathcal{N} \\ &+ \overline{\mathcal{N}} (v \! \! \! / + \tfrac{1}{2} \tilde{l} \! \! \! / + \tfrac{1}{2} \tilde{r} \! \! \! /) \mathcal{N} - g_A \overline{\mathcal{N}} (a \! \! \! / + \tfrac{1}{2} \tilde{l} \! \! \! / - \tfrac{1}{2} \tilde{r} \! \! \! /) \gamma_5 \mathcal{N} \ , \end{aligned} \tag{90.12}

习题 90.2 - 解答


要验证将核子场重定义公式 (90.11) 代入拉格朗日量 (90.1) 能够得到 (90.12),我们需要先明确物理背景:公式 (90.1) 是全局手征对称性下的拉格朗日量。为了得到包含外部规范场 lμl^\murμr^\mu 的局域形式 (90.12),必须首先将 (90.1) 中的普通导数升级为协变导数。

1. 引入协变导数与基本定义

引入外部左手和右手规范场 lμl_\murμr_\mu,介子场 UU 和核子场 NN 的协变导数分别为: DμU=μUilμU+iUrμD_\mu U = \partial_\mu U - i l_\mu U + i U r_\mu DμN=μNilμPLNirμPRND_\mu N = \partial_\mu N - i l_\mu P_L N - i r_\mu P_R N 其中投影算符 PL,R=1γ52P_{L,R} = \frac{1 \mp \gamma_5}{2} 满足 PL2=PLP_L^2 = P_L, PR2=PRP_R^2 = P_R, PLPR=0P_L P_R = 0 以及 PLγμ=γμPRP_L \gamma^\mu = \gamma^\mu P_R

定义介子场 U=u2U = u^2,并引入以下基本手征结构(不含外部场时的裸矢量和轴矢量场): vμ=i2(uμu+uμu),aμ=i2(uμuuμu)v_\mu = \frac{i}{2} (u^\dagger \partial_\mu u + u \partial_\mu u^\dagger), \quad a_\mu = \frac{i}{2} (u^\dagger \partial_\mu u - u \partial_\mu u^\dagger) 以及外部场在核子基底下的旋转形式: l~μ=ulμu,r~μ=urμu\tilde{l}_\mu = u^\dagger l_\mu u, \quad \tilde{r}_\mu = u r_\mu u^\dagger

核子场的重定义 (90.11) 及其狄拉克伴随形式为: N=(uPL+uPR)NN = (u P_L + u^\dagger P_R) \mathcal{N} Nˉ=Nγ0=N(uPL+uPR)γ0=Nˉ(uPR+uPL)\bar{N} = N^\dagger \gamma^0 = \mathcal{N}^\dagger (u^\dagger P_L + u P_R) \gamma^0 = \bar{\mathcal{N}} (u^\dagger P_R + u P_L)

下面分两步处理介子部分和核子部分。

2. 介子部分的展开

μUDμU\partial_\mu U \to D_\mu U 代入介子动能项 14fπ2Tr(DμUDμU)-\frac{1}{4} f_\pi^2 \operatorname{Tr}(D^\mu U^\dagger D_\mu U) 中: DμU=μU+iUlμirμUD_\mu U^\dagger = \partial_\mu U^\dagger + i U^\dagger l_\mu - i r_\mu U^\dagger 展开迹 Tr(DμUDμU)\operatorname{Tr}(D^\mu U^\dagger D_\mu U),利用迹的循环性质和 UU=1U U^\dagger = 1(从而有 (μU)U=UμU(\partial_\mu U) U^\dagger = - U \partial_\mu U^\dagger 等关系):

Tr(DμUDμU)=Tr(μUμU)+Tr(lμlμ)+Tr(rμrμ)2Tr(lμUrμU)iTr[lμ(UμU(μU)U)]iTr[rμ(UμU(μU)U)]\begin{aligned} \operatorname{Tr}(D^\mu U^\dagger D_\mu U) &= \operatorname{Tr}(\partial^\mu U^\dagger \partial_\mu U) + \operatorname{Tr}(l^\mu l_\mu) + \operatorname{Tr}(r^\mu r_\mu) - 2\operatorname{Tr}(l^\mu U r_\mu U^\dagger) \\ &\quad - i \operatorname{Tr}[l^\mu (U \partial_\mu U^\dagger - (\partial_\mu U) U^\dagger)] - i \operatorname{Tr}[r^\mu (U^\dagger \partial_\mu U - (\partial_\mu U^\dagger) U)] \end{aligned}

引入双向导数 AμB=AμB(μA)BA \overleftrightarrow{\partial}_\mu B = A \partial_\mu B - (\partial_\mu A) B,上式直接化简为 (90.12) 中的介子部分: Tr(μUμUilμUμUirμUμU+lμlμ+rμrμ2lμUrμU)\operatorname{Tr}(\partial^\mu U^\dagger \partial_\mu U - i l^\mu U \overleftrightarrow{\partial}_\mu U^\dagger - i r^\mu U^\dagger \overleftrightarrow{\partial}_\mu U + l^\mu l_\mu + r^\mu r_\mu - 2l^\mu U r_\mu U^\dagger)

3. 核子部分的推导

NNNˉ\bar{N} 代入核子拉格朗日量的各项中。

第一项:质量项

mNNˉ(UPL+UPR)N=mNNˉ(uPR+uPL)(u2PL+u2PR)(uPL+uPR)N=mNNˉ(uPR+uPL)(uPL+uPR)N=mNNˉ(uuPR+uuPL)N=mNNˉN\begin{aligned} -m_N \bar{N}(U^\dagger P_L + U P_R) N &= -m_N \bar{\mathcal{N}} (u^\dagger P_R + u P_L) (u^{\dagger 2} P_L + u^2 P_R) (u P_L + u^\dagger P_R) \mathcal{N} \\ &= -m_N \bar{\mathcal{N}} (u^\dagger P_R + u P_L) (u^\dagger P_L + u P_R) \mathcal{N} \\ &= -m_N \bar{\mathcal{N}} (u^\dagger u P_R + u u^\dagger P_L) \mathcal{N} = -m_N \bar{\mathcal{N}} \mathcal{N} \end{aligned}

第二项:动能与规范耦合项 将导数升级为协变导数 iNˉγμDμN=iNˉγμμN+Nˉγμ(lμPL+rμPR)Ni \bar{N} \gamma^\mu D_\mu N = i \bar{N} \gamma^\mu \partial_\mu N + \bar{N} \gamma^\mu (l_\mu P_L + r_\mu P_R) N。 先计算普通导数部分:

iNˉγμμN=iNˉγμ(uPL+uPR)μ[(uPL+uPR)N]=iNˉγμ(uuPL+uuPR)μN+iNˉγμ(uμuPL+uμuPR)N\begin{aligned} i \bar{N} \gamma^\mu \partial_\mu N &= i \bar{\mathcal{N}} \gamma^\mu (u^\dagger P_L + u P_R) \partial_\mu [ (u P_L + u^\dagger P_R) \mathcal{N} ] \\ &= i \bar{\mathcal{N}} \gamma^\mu (u^\dagger u P_L + u u^\dagger P_R) \partial_\mu \mathcal{N} + i \bar{\mathcal{N}} \gamma^\mu (u^\dagger \partial_\mu u P_L + u \partial_\mu u^\dagger P_R) \mathcal{N} \end{aligned}

利用 uμu=i(vμ+aμ)u^\dagger \partial_\mu u = -i(v_\mu + a_\mu)uμu=i(vμaμ)u \partial_\mu u^\dagger = -i(v_\mu - a_\mu),第二项变为: Nˉγμ[vμ(PL+PR)+aμ(PLPR)]N=Nˉv ⁣ ⁣ ⁣/NNˉa ⁣ ⁣ ⁣/γ5N\bar{\mathcal{N}} \gamma^\mu [ v_\mu (P_L + P_R) + a_\mu (P_L - P_R) ] \mathcal{N} = \bar{\mathcal{N}} v \! \! \! / \mathcal{N} - \bar{\mathcal{N}} a \! \! \! / \gamma_5 \mathcal{N} 再计算外部规范场部分:

Nˉγμ(lμPL+rμPR)N=Nˉγμ(uPL+uPR)(lμPL+rμPR)(uPL+uPR)N=Nˉγμ(ulμuPL+urμuPR)N=Nˉγμ(l~μPL+r~μPR)N=Nˉγμ[12(l~μ+r~μ)12(l~μr~μ)γ5]N\begin{aligned} \bar{N} \gamma^\mu (l_\mu P_L + r_\mu P_R) N &= \bar{\mathcal{N}} \gamma^\mu (u^\dagger P_L + u P_R) (l_\mu P_L + r_\mu P_R) (u P_L + u^\dagger P_R) \mathcal{N} \\ &= \bar{\mathcal{N}} \gamma^\mu (u^\dagger l_\mu u P_L + u r_\mu u^\dagger P_R) \mathcal{N} = \bar{\mathcal{N}} \gamma^\mu (\tilde{l}_\mu P_L + \tilde{r}_\mu P_R) \mathcal{N} \\ &= \bar{\mathcal{N}} \gamma^\mu \left[ \frac{1}{2}(\tilde{l}_\mu + \tilde{r}_\mu) - \frac{1}{2}(\tilde{l}_\mu - \tilde{r}_\mu)\gamma_5 \right] \mathcal{N} \end{aligned}

合并得到: iNˉγμDμN=iNˉ ⁣ ⁣ ⁣/N+Nˉ(v ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/+12r~ ⁣ ⁣ ⁣/)NNˉ(a ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/12r~ ⁣ ⁣ ⁣/)γ5Ni \bar{N} \gamma^\mu D_\mu N = i \bar{\mathcal{N}} \partial \! \! \! / \mathcal{N} + \bar{\mathcal{N}} \left( v \! \! \! / + \frac{1}{2} \tilde{l} \! \! \! / + \frac{1}{2} \tilde{r} \! \! \! / \right) \mathcal{N} - \bar{\mathcal{N}} \left( a \! \! \! / + \frac{1}{2} \tilde{l} \! \! \! / - \frac{1}{2} \tilde{r} \! \! \! / \right) \gamma_5 \mathcal{N}

第三项:轴矢量耦合项 同样使用协变导数:12(gA1)iNˉγμ(UDμUPL+UDμUPR)N-\frac{1}{2}(g_A - 1) i \bar{N} \gamma^\mu (U D_\mu U^\dagger P_L + U^\dagger D_\mu U P_R) N。 其中 UDμU=UμU+ilμiUrμUU D_\mu U^\dagger = U \partial_\mu U^\dagger + i l_\mu - i U r_\mu U^\daggerUDμU=UμUiUlμU+irμU^\dagger D_\mu U = U^\dagger \partial_\mu U - i U^\dagger l_\mu U + i r_\mu。 先计算普通导数部分:

12(gA1)iNˉγμ(uPL+uPR)(UμUPL+UμUPR)(uPL+uPR)N=12(gA1)iNˉγμ(uUμUuPL+uUμUuPR)N\begin{aligned} &-\frac{1}{2}(g_A - 1) i \bar{\mathcal{N}} \gamma^\mu (u^\dagger P_L + u P_R) (U \partial_\mu U^\dagger P_L + U^\dagger \partial_\mu U P_R) (u P_L + u^\dagger P_R) \mathcal{N} \\ &= -\frac{1}{2}(g_A - 1) i \bar{\mathcal{N}} \gamma^\mu (u^\dagger U \partial_\mu U^\dagger u P_L + u U^\dagger \partial_\mu U u^\dagger P_R) \mathcal{N} \end{aligned}

利用恒等式 uUμUu=uμu+μuu=2iaμu^\dagger U \partial_\mu U^\dagger u = u \partial_\mu u^\dagger + \partial_\mu u^\dagger u = 2i a_\mu 以及 uUμUu=uμu+μuu=2iaμu U^\dagger \partial_\mu U u^\dagger = u^\dagger \partial_\mu u + \partial_\mu u u^\dagger = -2i a_\mu,该部分化简为: 12(gA1)iNˉγμ(2iaμPL2iaμPR)N=(gA1)Nˉa ⁣ ⁣ ⁣/γ5N-\frac{1}{2}(g_A - 1) i \bar{\mathcal{N}} \gamma^\mu (2i a_\mu P_L - 2i a_\mu P_R) \mathcal{N} = -(g_A - 1) \bar{\mathcal{N}} a \! \! \! / \gamma_5 \mathcal{N} 再计算外部规范场部分:

12(gA1)iNˉγμ[(ilμiUrμU)PL+(iUlμU+irμ)PR]N=12(gA1)Nˉγμ[u(lμu2rμu2)uPL+u(u2lμu2+rμ)uPR]N=12(gA1)Nˉγμ[(l~μr~μ)PL(l~μr~μ)PR]N=12(gA1)Nˉ(l~ ⁣ ⁣ ⁣/r~ ⁣ ⁣ ⁣/)γ5N\begin{aligned} &-\frac{1}{2}(g_A - 1) i \bar{N} \gamma^\mu [ (i l_\mu - i U r_\mu U^\dagger) P_L + (-i U^\dagger l_\mu U + i r_\mu) P_R ] N \\ &= \frac{1}{2}(g_A - 1) \bar{\mathcal{N}} \gamma^\mu [ u^\dagger (l_\mu - u^2 r_\mu u^{\dagger 2}) u P_L + u (-u^{\dagger 2} l_\mu u^2 + r_\mu) u^\dagger P_R ] \mathcal{N} \\ &= \frac{1}{2}(g_A - 1) \bar{\mathcal{N}} \gamma^\mu [ (\tilde{l}_\mu - \tilde{r}_\mu) P_L - (\tilde{l}_\mu - \tilde{r}_\mu) P_R ] \mathcal{N} \\ &= -\frac{1}{2}(g_A - 1) \bar{\mathcal{N}} (\tilde{l} \! \! \! / - \tilde{r} \! \! \! /) \gamma_5 \mathcal{N} \end{aligned}

合并得到: (gA1)Nˉ(a ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/12r~ ⁣ ⁣ ⁣/)γ5N-(g_A - 1) \bar{\mathcal{N}} \left( a \! \! \! / + \frac{1}{2} \tilde{l} \! \! \! / - \frac{1}{2} \tilde{r} \! \! \! / \right) \gamma_5 \mathcal{N}

4. 综合结果

将上述所有核子项相加,注意到动能项中产生的轴矢量部分 Nˉ(a ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/12r~ ⁣ ⁣ ⁣/)γ5N-\bar{\mathcal{N}}(a \! \! \! / + \frac{1}{2}\tilde{l} \! \! \! / - \frac{1}{2}\tilde{r} \! \! \! /)\gamma_5 \mathcal{N} 与轴矢量耦合项 (gA1)Nˉ(a ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/12r~ ⁣ ⁣ ⁣/)γ5N-(g_A - 1)\bar{\mathcal{N}}(a \! \! \! / + \frac{1}{2}\tilde{l} \! \! \! / - \frac{1}{2}\tilde{r} \! \! \! /)\gamma_5 \mathcal{N} 完美合并为 gA-g_A 的系数项。结合介子部分,最终得到完整的拉格朗日量:

L=14fπ2Tr(μUμUilμUμUirμUμU+lμlμ+rμrμ2lμUrμU)+v3Tr(MU+MU)+iN ⁣ ⁣ ⁣/NmNNN+N(v ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/+12r~ ⁣ ⁣ ⁣/)NgAN(a ⁣ ⁣ ⁣/+12l~ ⁣ ⁣ ⁣/12r~ ⁣ ⁣ ⁣/)γ5N \boxed{ \begin{aligned} \mathcal{L} = &-\tfrac{1}{4} f_\pi^2 \operatorname{Tr}(\partial^\mu U^\dagger \partial_\mu U - il^\mu U \overleftrightarrow{\partial}_\mu U^\dagger - ir^\mu U^\dagger \overleftrightarrow{\partial}_\mu U \\ &+ l^\mu l_\mu + r^\mu r_\mu - 2l^\mu U r_\mu U^\dagger) \\ &+ v^3 \operatorname{Tr}(MU + M^\dagger U^\dagger) + i\overline{\mathcal{N}} \partial \! \! \! / \mathcal{N} - m_N \overline{\mathcal{N}} \mathcal{N} \\ &+ \overline{\mathcal{N}} (v \! \! \! / + \tfrac{1}{2} \tilde{l} \! \! \! / + \tfrac{1}{2} \tilde{r} \! \! \! /) \mathcal{N} - g_A \overline{\mathcal{N}} (a \! \! \! / + \tfrac{1}{2} \tilde{l} \! \! \! / - \tfrac{1}{2} \tilde{r} \! \! \! /) \gamma_5 \mathcal{N} \ \end{aligned} }

这正是公式 (90.12),验证完毕。

90.3

Problem 90.3

srednickiChapter 90

习题 90.3

来源: 第90章, PDF第554页


90.3 Compute the rate for the decay process τπντ\tau^- \rightarrow \pi^- \nu_\tau. Look up the measured value and compare with your result.

习题 90.3 - 解答


1. 物理背景与有效拉氏量

τπντ\tau^- \rightarrow \pi^- \nu_\tau 是一个典型的轻子半轻衰变过程,由 WW^- 玻色子介导。由于涉及的能量尺度(τ\tau 质量 mτ1.777 GeVm_\tau \approx 1.777 \text{ GeV})远小于 WW 玻色子的质量,我们可以使用费米有效四费米子相互作用理论来描述该过程。

有效拉氏量为: Leff=GF2Vud[dˉγμ(1γ5)u][νˉτγμ(1γ5)τ]+h.c.\mathcal{L}_{\text{eff}} = -\frac{G_F}{\sqrt{2}} V_{ud} [\bar{d} \gamma^\mu (1-\gamma^5) u] [\bar{\nu}_\tau \gamma_\mu (1-\gamma^5) \tau] + \text{h.c.} 其中 GFG_F 是费米常数,VudV_{ud} 是 CKM 矩阵元。

对于强子部分,由于 π\pi^- 是赝标介子(自旋为0,宇称为负),矢量流部分 dˉγμu\bar{d}\gamma^\mu u 的真空到单 π\pi 态的矩阵元为零,只有轴矢流部分有贡献。我们引入 π\pi 介子衰变常数 fπf_\pi 来参数化该强子矩阵元(此处采用 fπ130 MeVf_\pi \approx 130 \text{ MeV} 的约定): π(pπ)dˉγμ(1γ5)u0=π(pπ)dˉγμγ5u0=ifπpπμ\langle \pi^-(p_\pi) | \bar{d} \gamma^\mu (1-\gamma^5) u | 0 \rangle = - \langle \pi^-(p_\pi) | \bar{d} \gamma^\mu \gamma^5 u | 0 \rangle = -i f_\pi p_\pi^\mu

2. 跃迁矩阵元与模方计算

结合轻子部分,该衰变过程的费曼振幅(矩阵元)为: M=GF2Vud(ifπpπμ)[uˉ(pν)γμ(1γ5)u(pτ)]\mathcal{M} = \frac{G_F}{\sqrt{2}} V_{ud} (i f_\pi p_\pi^\mu) [\bar{u}(p_\nu) \gamma_\mu (1-\gamma^5) u(p_\tau)]

利用动量守恒 pπμ=pτμpνμp_\pi^\mu = p_\tau^\mu - p_\nu^\mu,我们可以将 pπμp_\pi^\mu 缩并入轻子流中。利用狄拉克方程 uˉ(pν)̸pν=0\bar{u}(p_\nu) \not{p}_\nu = 0(忽略中微子质量)以及 ̸pτu(pτ)=mτu(pτ)\not{p}_\tau u(p_\tau) = m_\tau u(p_\tau),并注意到 γ5\gamma^5γμ\gamma^\mu 反对易: pπμuˉ(pν)γμ(1γ5)u(pτ)=uˉ(pν)(̸pτ̸pν)(1γ5)u(pτ)p_\pi^\mu \bar{u}(p_\nu) \gamma_\mu (1-\gamma^5) u(p_\tau) = \bar{u}(p_\nu) (\not{p}_\tau - \not{p}_\nu) (1-\gamma^5) u(p_\tau) =uˉ(pν)̸pτ(1γ5)u(pτ)=uˉ(pν)(1+γ5)̸pτu(pτ)=mτuˉ(pν)(1+γ5)u(pτ)= \bar{u}(p_\nu) \not{p}_\tau (1-\gamma^5) u(p_\tau) = \bar{u}(p_\nu) (1+\gamma^5) \not{p}_\tau u(p_\tau) = m_\tau \bar{u}(p_\nu) (1+\gamma^5) u(p_\tau)

因此,振幅简化为: M=iGF2Vudfπmτ[uˉ(pν)(1+γ5)u(pτ)]\mathcal{M} = i \frac{G_F}{\sqrt{2}} V_{ud} f_\pi m_\tau [\bar{u}(p_\nu) (1+\gamma^5) u(p_\tau)]

对初态 τ\tau 自旋求平均,对末态中微子自旋求和,计算矩阵元模方: M2=12spinsM2=12GF22Vud2fπ2mτ2Tr[(1+γ5)(̸pτ+mτ)(1γ5)̸pν]\overline{|\mathcal{M}|^2} = \frac{1}{2} \sum_{\text{spins}} |\mathcal{M}|^2 = \frac{1}{2} \frac{G_F^2}{2} |V_{ud}|^2 f_\pi^2 m_\tau^2 \text{Tr}\left[ (1+\gamma^5) (\not{p}_\tau + m_\tau) (1-\gamma^5) \not{p}_\nu \right] 利用迹定理 Tr[odd number of γ]=0\text{Tr}[\text{odd number of } \gamma] = 0 以及 (1+γ5)(1γ5)=0(1+\gamma^5)(1-\gamma^5) = 0,提取非零项: M2=GF24Vud2fπ2mτ2Tr[2(1γ5)̸pτ̸pν]\overline{|\mathcal{M}|^2} = \frac{G_F^2}{4} |V_{ud}|^2 f_\pi^2 m_\tau^2 \text{Tr}\left[ 2(1-\gamma^5) \not{p}_\tau \not{p}_\nu \right] =GF24Vud2fπ2mτ2×8(pτpν)=2GF2Vud2fπ2mτ2(pτpν)= \frac{G_F^2}{4} |V_{ud}|^2 f_\pi^2 m_\tau^2 \times 8 (p_\tau \cdot p_\nu) = 2 G_F^2 |V_{ud}|^2 f_\pi^2 m_\tau^2 (p_\tau \cdot p_\nu)

由运动学关系 pπ2=(pτpν)2    mπ2=mτ22pτpνp_\pi^2 = (p_\tau - p_\nu)^2 \implies m_\pi^2 = m_\tau^2 - 2 p_\tau \cdot p_\nu,可得 2pτpν=mτ2mπ22 p_\tau \cdot p_\nu = m_\tau^2 - m_\pi^2。代入上式: M2=GF2Vud2fπ2mτ2(mτ2mπ2)\overline{|\mathcal{M}|^2} = G_F^2 |V_{ud}|^2 f_\pi^2 m_\tau^2 (m_\tau^2 - m_\pi^2)

3. 相空间与衰变率公式

对于两体衰变,在 τ\tau 静止系中的衰变率公式为: Γ=pπ8πmτ2M2\Gamma = \frac{|\vec{p}_\pi|}{8\pi m_\tau^2} \overline{|\mathcal{M}|^2} 其中末态粒子的动量大小为 pπ=mτ2mπ22mτ|\vec{p}_\pi| = \frac{m_\tau^2 - m_\pi^2}{2m_\tau}

将动量和矩阵元模方代入衰变率公式: Γ(τπντ)=mτ2mπ216πmτ3GF2Vud2fπ2mτ2(mτ2mπ2)\Gamma(\tau^- \rightarrow \pi^- \nu_\tau) = \frac{m_\tau^2 - m_\pi^2}{16\pi m_\tau^3} G_F^2 |V_{ud}|^2 f_\pi^2 m_\tau^2 (m_\tau^2 - m_\pi^2) 整理得到最终的解析表达式: Γ(τπντ)=GF2Vud2fπ2mτ316π(1mπ2mτ2)2\boxed{ \Gamma(\tau^- \rightarrow \pi^- \nu_\tau) = \frac{G_F^2 |V_{ud}|^2 f_\pi^2 m_\tau^3}{16\pi} \left(1 - \frac{m_\pi^2}{m_\tau^2}\right)^2 }

4. 数值计算与实验对比

代入标准物理常数(参考 PDG 数据):

  • GF1.166×105 GeV2G_F \approx 1.166 \times 10^{-5} \text{ GeV}^{-2}
  • Vud0.974|V_{ud}| \approx 0.974
  • fπ0.1302 GeVf_\pi \approx 0.1302 \text{ GeV}
  • mτ1.777 GeVm_\tau \approx 1.777 \text{ GeV}
  • mπ0.140 GeVm_\pi \approx 0.140 \text{ GeV}

计算衰变宽度 Γ\GammaΓ(1.166×105)2×(0.974)2×(0.1302)2×(1.777)316π(1(0.1401.777)2)2 GeV\Gamma \approx \frac{(1.166 \times 10^{-5})^2 \times (0.974)^2 \times (0.1302)^2 \times (1.777)^3}{16\pi} \left(1 - \left(\frac{0.140}{1.777}\right)^2\right)^2 \text{ GeV} Γ1.36×1010×0.949×0.01695×5.6150.265×0.9877 GeV2.41×1013 GeV\Gamma \approx \frac{1.36 \times 10^{-10} \times 0.949 \times 0.01695 \times 5.61}{50.265} \times 0.9877 \text{ GeV} \approx 2.41 \times 10^{-13} \text{ GeV}

为了与实验测量值对比,我们计算其分支比 (Branching Ratio, B\mathcal{B})。已知 τ\tau 的实验寿命 ττ2.903×1013 s\tau_\tau \approx 2.903 \times 10^{-13} \text{ s},对应的总衰变宽度为: Γtot=ττ6.582×1025 GeVs2.903×1013 s2.267×1012 GeV\Gamma_{\text{tot}} = \frac{\hbar}{\tau_\tau} \approx \frac{6.582 \times 10^{-25} \text{ GeV}\cdot\text{s}}{2.903 \times 10^{-13} \text{ s}} \approx 2.267 \times 10^{-12} \text{ GeV}

理论预测的分支比为: Bth=ΓΓtot2.41×10132.267×101210.6%\mathcal{B}_{\text{th}} = \frac{\Gamma}{\Gamma_{\text{tot}}} \approx \frac{2.41 \times 10^{-13}}{2.267 \times 10^{-12}} \approx 10.6\%

查阅实验测量值 (PDG): 目前粒子物理数据组 (PDG) 给出的测量值为: Bexp(τπντ)=(10.82±0.05)%\mathcal{B}_{\text{exp}}(\tau^- \rightarrow \pi^- \nu_\tau) = (10.82 \pm 0.05)\%

对比结论: Bth10.6%vsBexp10.82%\boxed{ \mathcal{B}_{\text{th}} \approx 10.6\% \quad \text{vs} \quad \mathcal{B}_{\text{exp}} \approx 10.82\% } 理论计算结果与实验测量值高度吻合。约 2%2\% 的微小差异主要来源于我们在树图阶(Tree-level)计算中忽略了电磁辐射修正(Radiative corrections)以及 fπf_\piVudV_{ud} 参数提取时的微小不确定性。

90.4

Problem 90.4

srednickiChapter 90

习题 90.4

来源: 第90章, PDF第554页


90.4 a) Verify eq. (90.43).

b) Compute the total neutron decay rate. Given the measured neutron lifetime τ=886 s\tau = 886 \text{ s}, and using GF=1.166×105 GeV2G_{\text{F}} = 1.166 \times 10^{-5} \text{ GeV}^{-2} and c1=0.974c_1 = 0.974, compute gAg_{\text{A}}. Your answer is about 4% too high, because we neglected loop corrections, and the Coulomb interaction between the outgoing electron and proton.


Referenced Equations:

Equation (90.43):

T2=16GF2c12(1+3gA2)mnmpEeEνˉ×[1+apepνˉEeEνˉ+Az^peEe+Bz^pνˉEνˉ],(90.43)\begin{aligned} \langle |\mathcal{T}|^2 \rangle &= 16 G_F^2 c_1^2 (1 + 3g_A^2) m_n m_p E_e E_{\bar{\nu}} \\ &\quad \times \left[ 1 + a \frac{\mathbf{p}_e \cdot \mathbf{p}_{\bar{\nu}}}{E_e E_{\bar{\nu}}} + A \frac{\hat{\mathbf{z}} \cdot \mathbf{p}_e}{E_e} + B \frac{\hat{\mathbf{z}} \cdot \mathbf{p}_{\bar{\nu}}}{E_{\bar{\nu}}} \right], \end{aligned} \tag{90.43}

习题 90.4 - 解答


a) 验证公式 (90.43)

先分析矩阵元与张量结构 中子 β\beta 衰变 np+e+νˉen \to p + e^- + \bar{\nu}_e 的有效费米相互作用矩阵元为: T=GFc12[uˉpγμ(1gAγ5)un][uˉeγμ(1γ5)vν]\mathcal{T} = \frac{G_F c_1}{\sqrt{2}} \left[ \bar{u}_p \gamma^\mu (1 - g_A \gamma_5) u_n \right] \left[ \bar{u}_e \gamma_\mu (1 - \gamma_5) v_\nu \right] 对末态轻子自旋求和,并考虑极化中子(静止系中自旋矢量为 sμ=(0,z^)s^\mu = (0, \hat{\mathbf{z}}))和非极化质子,矩阵元模方可分解为轻子张量与强子张量的缩并: T2=GF2c122LμνHμν\langle |\mathcal{T}|^2 \rangle = \frac{G_F^2 c_1^2}{2} L^{\mu\nu} H_{\mu\nu}

计算轻子张量 LμνL^{\mu\nu} 利用狄拉克矩阵的迹定理(约定 ϵ0123=+1\epsilon^{0123} = +1): Lμν=Tr[̸peγμ(1γ5)̸pνγν(1γ5)]=2Tr[̸peγμ̸pνγν(1γ5)]=8(peμpνν+peνpνμgμνpepν+iϵμανβpeαpνβ)\begin{aligned} L^{\mu\nu} &= \text{Tr}\left[ \not{p}_e \gamma^\mu (1 - \gamma_5) \not{p}_\nu \gamma^\nu (1 - \gamma_5) \right] = 2 \text{Tr}\left[ \not{p}_e \gamma^\mu \not{p}_\nu \gamma^\nu (1 - \gamma_5) \right] \\ &= 8 \left( p_e^\mu p_\nu^\nu + p_e^\nu p_\nu^\mu - g^{\mu\nu} p_e \cdot p_\nu + i \epsilon^{\mu\alpha\nu\beta} p_{e\alpha} p_{\nu\beta} \right) \end{aligned}

计算强子张量 HμνH_{\mu\nu} 在核子的非相对论极限下(pn(mn,0)p_n \approx (m_n, \mathbf{0}), pp(mp,0)p_p \approx (m_p, \mathbf{0})),核子流的非零分量为: J02mnmpχpχn,Ji2mnmpgAχpσiχnJ^0 \approx 2\sqrt{m_n m_p} \chi_p^\dagger \chi_n, \quad J^i \approx -2\sqrt{m_n m_p} g_A \chi_p^\dagger \sigma^i \chi_n 利用中子自旋密度矩阵 ρn=12(1+σs)\rho_n = \frac{1}{2}(1 + \boldsymbol{\sigma} \cdot \mathbf{s}) 对质子自旋求和,得到强子张量分量: H00=4mnmpH0i=Hi0=4mnmpgAsiHij=4mnmpgA2(δij+iϵijksk)\begin{aligned} H_{00} &= 4 m_n m_p \\ H_{0i} &= H_{i0} = -4 m_n m_p g_A s^i \\ H_{ij} &= 4 m_n m_p g_A^2 (\delta^{ij} + i \epsilon^{ijk} s^k) \end{aligned}

张量缩并 分项计算 LμνHμν=L00H00+L0iH0i+Li0Hi0+LijHijL^{\mu\nu} H_{\mu\nu} = L^{00}H_{00} + L^{0i}H_{0i} + L^{i0}H_{i0} + L^{ij}H_{ij}

  1. 00分量L00H00=8(EeEν+pepν)×4mnmp=32mnmp(EeEν+pepν)L^{00} H_{00} = 8(E_e E_\nu + \mathbf{p}_e \cdot \mathbf{p}_\nu) \times 4 m_n m_p = 32 m_n m_p (E_e E_\nu + \mathbf{p}_e \cdot \mathbf{p}_\nu)
  2. 0i与i0分量(注意 pνi=pνip_{\nu i} = -p_\nu^i): L0i+Li0=16(Eepνi+Eνpei)L^{0i} + L^{i0} = 16(E_e p_\nu^i + E_\nu p_e^i) (L0i+Li0)H0i=64mnmpgA(Eepνs+Eνpes)(L^{0i} + L^{i0}) H_{0i} = -64 m_n m_p g_A (E_e \mathbf{p}_\nu \cdot \mathbf{s} + E_\nu \mathbf{p}_e \cdot \mathbf{s})
  3. ij分量: 对称部分缩并:8[2peipνj+δij(EeEνpepν)]×4mnmpgA2δij=32mnmpgA2(3EeEνpepν)8[2p_e^i p_\nu^j + \delta^{ij}(E_e E_\nu - \mathbf{p}_e \cdot \mathbf{p}_\nu)] \times 4 m_n m_p g_A^2 \delta^{ij} = 32 m_n m_p g_A^2 (3E_e E_\nu - \mathbf{p}_e \cdot \mathbf{p}_\nu) 反对称部分缩并(利用 ϵiαjβpeαpνβϵijk(EepνkEνpek)\epsilon^{i\alpha j\beta} p_{e\alpha} p_{\nu\beta} \supset \epsilon^{ijk}(E_e p_\nu^k - E_\nu p_e^k)): 8iϵijk(EepνkEνpek)×4mnmpgA2(iϵijlsl)=64mnmpgA2(EepνsEνpes)8i \epsilon^{ijk} (E_e p_\nu^k - E_\nu p_e^k) \times 4 m_n m_p g_A^2 (i \epsilon^{ijl} s^l) = -64 m_n m_p g_A^2 (E_e \mathbf{p}_\nu \cdot \mathbf{s} - E_\nu \mathbf{p}_e \cdot \mathbf{s})

组合并提取公因子 将所有项相加,并提出公因子 32mnmpEeEν32 m_n m_p E_e E_\nu(注意 s=z^\mathbf{s} = \hat{\mathbf{z}}): T2=16GF2c12mnmpEeEν[(1+3gA2)+(1gA2)pepνEeEν2gA(1gA)pez^Ee2gA(1+gA)pνz^Eν]\begin{aligned} \langle |\mathcal{T}|^2 \rangle &= 16 G_F^2 c_1^2 m_n m_p E_e E_\nu \Bigg[ (1 + 3g_A^2) + (1 - g_A^2)\frac{\mathbf{p}_e \cdot \mathbf{p}_\nu}{E_e E_\nu} \\ &\quad - 2g_A(1 - g_A)\frac{\mathbf{p}_e \cdot \hat{\mathbf{z}}}{E_e} - 2g_A(1 + g_A)\frac{\mathbf{p}_\nu \cdot \hat{\mathbf{z}}}{E_\nu} \Bigg] \end{aligned} 提出 (1+3gA2)(1 + 3g_A^2),即可严格还原出公式 (90.43): T2=16GF2c12(1+3gA2)mnmpEeEνˉ×[1+apepνˉEeEνˉ+Az^peEe+Bz^pνˉEνˉ]\boxed{ \begin{aligned} \langle |\mathcal{T}|^2 \rangle &= 16 G_F^2 c_1^2 (1 + 3g_A^2) m_n m_p E_e E_{\bar{\nu}} \\ &\quad \times \left[ 1 + a \frac{\mathbf{p}_e \cdot \mathbf{p}_{\bar{\nu}}}{E_e E_{\bar{\nu}}} + A \frac{\hat{\mathbf{z}} \cdot \mathbf{p}_e}{E_e} + B \frac{\hat{\mathbf{z}} \cdot \mathbf{p}_{\bar{\nu}}}{E_{\bar{\nu}}} \right] \end{aligned} } 其中关联系数分别为:a=1gA21+3gA2,A=2gA(gA1)1+3gA2,B=2gA(gA+1)1+3gA2a = \frac{1 - g_A^2}{1 + 3g_A^2}, \quad A = \frac{2g_A(g_A - 1)}{1 + 3g_A^2}, \quad B = \frac{-2g_A(g_A + 1)}{1 + 3g_A^2}


b) 计算总衰变率与 gAg_A

计算总衰变率 Γ\Gamma 对全立体角积分时,包含 pe\mathbf{p}_epνˉ\mathbf{p}_{\bar{\nu}} 的一次项均积分为零,仅保留各项同性部分: T2unpol=16GF2c12(1+3gA2)mnmpEeEν\langle |\mathcal{T}|^2 \rangle_{\text{unpol}} = 16 G_F^2 c_1^2 (1 + 3g_A^2) m_n m_p E_e E_\nu 代入三体相空间衰变率公式(忽略质子反冲动能,Eν=ΔEeE_\nu = \Delta - E_e,其中 Δ=mnmp\Delta = m_n - m_p): dΓ=12mnT2unpold3pe(2π)32Eed3pν(2π)32Eνd3pp(2π)32mp(2π)4δ4(p)d\Gamma = \frac{1}{2m_n} \langle |\mathcal{T}|^2 \rangle_{\text{unpol}} \frac{d^3 p_e}{(2\pi)^3 2E_e} \frac{d^3 p_\nu}{(2\pi)^3 2E_\nu} \frac{d^3 p_p}{(2\pi)^3 2m_p} (2\pi)^4 \delta^4(\sum p) 完成对 pp\mathbf{p}_p 和中微子角度的积分后,得到关于电子能量的微分衰变率: dΓ=GF2c12(1+3gA2)2π3Eepe(ΔEe)2dEed\Gamma = \frac{G_F^2 c_1^2 (1 + 3g_A^2)}{2\pi^3} E_e |\mathbf{p}_e| (\Delta - E_e)^2 dE_e 积分得到总衰变率: Γ=GF2c12(1+3gA2)2π3me5f(q)\Gamma = \frac{G_F^2 c_1^2 (1 + 3g_A^2)}{2\pi^3} m_e^5 f(q) 其中无量纲相空间积分 f(q)f(q) 定义为(q=Δ/meq = \Delta / m_e): f(q)=1qxx21(qx)2dx=160q21(2q49q28)+14qln(q+q21)f(q) = \int_1^q x \sqrt{x^2 - 1} (q - x)^2 dx = \frac{1}{60}\sqrt{q^2 - 1}(2q^4 - 9q^2 - 8) + \frac{1}{4}q \ln(q + \sqrt{q^2 - 1})

代入数值计算 已知物理常数:

  • mn=939.565 MeV,mp=938.272 MeV    Δ=1.293 MeVm_n = 939.565 \text{ MeV}, m_p = 938.272 \text{ MeV} \implies \Delta = 1.293 \text{ MeV}
  • me=0.511 MeVm_e = 0.511 \text{ MeV}
  • q=1.293/0.511=2.5303q = 1.293 / 0.511 = 2.5303

计算相空间因子 f(2.5303)f(2.5303)f(2.5303)1.633f(2.5303) \approx 1.633 将衰变率与寿命联系起来 Γ=/τ\Gamma = \hbar / \tau,代入 =6.582×1025 GeVs\hbar = 6.582 \times 10^{-25} \text{ GeV}\cdot\text{s}Γ=6.582×1025 GeVs886 s=7.429×1028 GeV\Gamma = \frac{6.582 \times 10^{-25} \text{ GeV}\cdot\text{s}}{886 \text{ s}} = 7.429 \times 10^{-28} \text{ GeV} 计算理论常数部分(注意单位统一为 GeV): C=GF2c12me52π3f(q)=(1.166×105)2(0.974)2(0.511×103)52π3×1.633=1.183×1028 GeV\begin{aligned} C &= \frac{G_F^2 c_1^2 m_e^5}{2\pi^3} f(q) \\ &= \frac{(1.166 \times 10^{-5})^2 (0.974)^2 (0.511 \times 10^{-3})^5}{2\pi^3} \times 1.633 \\ &= 1.183 \times 10^{-28} \text{ GeV} \end{aligned}

求解 gAg_A 根据 Γ=C(1+3gA2)\Gamma = C(1 + 3g_A^2),可得: 1+3gA2=7.429×10281.183×1028=6.2801 + 3g_A^2 = \frac{7.429 \times 10^{-28}}{1.183 \times 10^{-28}} = 6.280 3gA2=5.280    gA2=1.760    gA1.3273g_A^2 = 5.280 \implies g_A^2 = 1.760 \implies g_A \approx 1.327

注:实验测量值为 gA1.27g_A \approx 1.27。由于我们忽略了库仑修正(费米函数 F(Z,E)F(Z, E) 会使相空间因子增大)以及辐射圈图修正,导致计算出的 gAg_A 偏高约 4%4\% (1.27×1.041.321.27 \times 1.04 \approx 1.32),这与题目描述完全一致。

gA1.33\boxed{ g_A \approx 1.33 }

90.5

Problem 90.5

srednickiChapter 90

习题 90.5

来源: 第90章, PDF第554页


90.5 Use your results from problems 88.7 and 89.5 to show that the neutron decay rate is enhanced by a factor of 1+2παln(MW/mp)1 + \frac{2}{\pi} \alpha \ln(M_{\text{W}}/m_p). How much of the 4% discrepancy is accounted for by this effect?

习题 90.5 - 解答


物理背景与题目分析

在标准模型中,中子 β\beta 衰变(np+e+νˉen \to p + e^- + \bar{\nu}_e)的树图级衰变速率由费米常数 GFG_F 和 CKM 矩阵元 VudV_{ud} 决定。然而,为了得到精确的理论预测,必须考虑电弱辐射修正。

根据前置习题(88.7 和 89.5)的结论:

  1. 习题 88.7 处理了 μ\mu 子衰变(μe+νˉe+νμ\mu^- \to e^- + \bar{\nu}_e + \nu_\mu)的单圈辐射修正。费米常数 GFG_F 正是由 μ\mu 子衰变寿命定义的,因此 μ\mu 子衰变的短距离辐射修正已被吸收到 GFG_F 的物理定义中。
  2. 习题 89.5 处理了夸克层次半轻子衰变(du+e+νˉed \to u + e^- + \bar{\nu}_e)的单圈辐射修正。由于夸克与轻子的电荷不同,半轻子衰变中的 WγW-\gamma 盒图(Box diagram)和顶点修正与纯轻子衰变不能完全抵消。

将全电弱理论在 MWM_W 能标下匹配到费米有效场论,并通过重整化群演化(或直接计算单圈反常维度)将能标跑动到强子能标 μmp\mu \sim m_p 时,有效拉格朗日量会获得一个对数增强的短距离修正因子。


第一部分:推导衰变速率的增强因子

由习题 89.5 的结果可知,在强子能标 μ=mp\mu = m_p 处,包含短距离辐射修正的有效拉格朗日量为: Leff=GF2Vud(1+απlnMWmp)[uˉγρ(1γ5)d][eˉγρ(1γ5)νe]+h.c.\mathcal{L}_{\text{eff}} = - \frac{G_F}{\sqrt{2}} V_{ud} \left( 1 + \frac{\alpha}{\pi} \ln\frac{M_W}{m_p} \right) \left[ \bar{u} \gamma^\rho (1-\gamma_5) d \right] \left[ \bar{e} \gamma_\rho (1-\gamma_5) \nu_e \right] + \text{h.c.}

这表明,与未包含该辐射修正的树图级振幅 M0\mathcal{M}_0 相比,修正后的跃迁振幅 M\mathcal{M} 变为: M=M0(1+απlnMWmp)\mathcal{M} = \mathcal{M}_0 \left( 1 + \frac{\alpha}{\pi} \ln\frac{M_W}{m_p} \right)

衰变速率 Γ\Gamma 正比于振幅模长的平方 M2|\mathcal{M}|^2。将其展开并只保留到精细结构常数 α\alpha 的领头阶(O(α)\mathcal{O}(\alpha)),我们得到: ΓM2=M02(1+απlnMWmp)2\Gamma \propto |\mathcal{M}|^2 = |\mathcal{M}_0|^2 \left( 1 + \frac{\alpha}{\pi} \ln\frac{M_W}{m_p} \right)^2 ΓΓ0(1+2απlnMWmp)\Gamma \approx \Gamma_0 \left( 1 + \frac{2\alpha}{\pi} \ln\frac{M_W}{m_p} \right)

因此,中子衰变速率被增强了如下因子: 1+2παln(MWmp)\boxed{ 1 + \frac{2}{\pi} \alpha \ln\left(\frac{M_W}{m_p}\right) }


第二部分:计算该效应解释的误差比例

接下来,我们将具体的物理常数代入上述增强因子中,以评估其数值大小:

  • 精细结构常数 α1137.036\alpha \approx \frac{1}{137.036}
  • WW 玻色子质量 MW80.38 GeVM_W \approx 80.38 \text{ GeV}
  • 质子质量 mp0.938 GeVm_p \approx 0.938 \text{ GeV}

首先计算对数项: ln(MWmp)=ln(80.380.938)ln(85.69)4.451\ln\left(\frac{M_W}{m_p}\right) = \ln\left(\frac{80.38}{0.938}\right) \approx \ln(85.69) \approx 4.451

计算相对修正量 ΔΓ/Γ0\Delta \Gamma / \Gamma_0ΔΓΓ0=2παln(MWmp)23.14159×1137.036×4.4510.02067\frac{\Delta \Gamma}{\Gamma_0} = \frac{2}{\pi} \alpha \ln\left(\frac{M_W}{m_p}\right) \approx \frac{2}{3.14159} \times \frac{1}{137.036} \times 4.451 \approx 0.02067

这意味着短距离电弱辐射修正使中子的理论衰变速率增加了约 2.07%2.07\%

题目指出,如果不考虑此效应,理论预测与实验数据之间存在约 4%4\% 的偏差(discrepancy)。该辐射修正效应所占的比例为: Accounted fraction=2.07%4%0.517\text{Accounted fraction} = \frac{2.07\%}{4\%} \approx 0.517

结论: 该短距离辐射修正效应解释了理论与实验之间 4%4\% 偏差中的约一半(具体约为 52%52\%)。

This effect accounts for approximately 52% of the 4% discrepancy.\boxed{ \text{This effect accounts for approximately } 52\% \text{ of the } 4\% \text{ discrepancy.} }

90.6

Problem 90.6

srednickiChapter 90

习题 90.6

来源: 第90章, PDF第554页


90.6 Compute the rate for the decay process ππ0eνˉe\pi^- \rightarrow \pi^0 e^- \bar{\nu}_e. Note that, since mπ+mπ0=4.594 MeVmπ0m_{\pi^+} - m_{\pi^0} = 4.594 \text{ MeV} \ll m_{\pi^0}, the outgoing π0\pi^0 is nonrelativistic. Compare your calculated rate with the measured value of 0.397 s10.397 \text{ s}^{-1} to determine c1c_1. Your answer is about 1% too low, due to neglect of loop corrections.

习题 90.6 - 解答


习题分析与物理背景

本题要求计算 ππ0eνˉe\pi^- \rightarrow \pi^0 e^- \bar{\nu}_e 的衰变率(即 pion beta decay)。该过程由弱相互作用的矢量流介导。根据守恒矢量流(CVC)假说,同位旋多重态之间的跃迁矩阵元完全由同位旋代数决定。由于 π\pi^-π0\pi^0 属于同一个同位旋三重态,强子流的矩阵元为 π0(p)Vμπ(p)=2(p+p)μ\langle \pi^0(p') | V^\mu | \pi^-(p) \rangle = \sqrt{2} (p + p')^\mu

有效拉格朗日量包含费米常数 GFG_F 和 CKM 矩阵元 c1Vudc_1 \equiv V_{ud}。由于质量差 Δm=mπmπ0=4.594 MeV\Delta m = m_{\pi^-} - m_{\pi^0} = 4.594 \text{ MeV} 远小于 mπ0m_{\pi^0},出射的 π0\pi^0 几乎静止,可以作非相对论近似处理。

推导过程

衰变的跃迁矩阵元为: M=GF2c1[2(p+p)μ][uˉeγμ(1γ5)vν]=GFc1(p+p)μuˉeγμ(1γ5)vν\mathcal{M} = \frac{G_F}{\sqrt{2}} c_1 \left[ \sqrt{2} (p+p')^\mu \right] \left[ \bar{u}_e \gamma_\mu (1-\gamma_5) v_\nu \right] = G_F c_1 (p+p')^\mu \bar{u}_e \gamma_\mu (1-\gamma_5) v_\nu

π0\pi^0 非相对论近似下,动量 p(mπ,0)p \approx (m_{\pi^-}, \vec{0})p(mπ0,0)p' \approx (m_{\pi^0}, \vec{0}),因此 (p+p)μ(2mπ,0)(p+p')^\mu \approx (2m_\pi, \vec{0})。 对电子和中微子的自旋求和后,矩阵元模方为: M2=GF2c12(2mπ)2Tr[γ0(1γ5)p ⁣ ⁣ ⁣/νγ0(1γ5)(p ⁣ ⁣ ⁣/e+me)]|\mathcal{M}|^2 = G_F^2 c_1^2 (2m_\pi)^2 \text{Tr}\left[ \gamma_0 (1-\gamma_5) p \! \! \! /_\nu \gamma_0 (1-\gamma_5) (p \! \! \! /_e + m_e) \right] 计算迹可得: M2=32GF2c12mπ2(EeEν+pepν)|\mathcal{M}|^2 = 32 G_F^2 c_1^2 m_\pi^2 (E_e E_\nu + \vec{p}_e \cdot \vec{p}_\nu)

衰变率由相空间积分给出。由于 π0\pi^0 极重,它几乎不带走动能,电子和中微子共享能量 Δm\Delta m。相空间积分为: dΓ=12mπ12mπ0M2d3pe(2π)32Eed3pν(2π)32Eν2πδ(ΔmEeEν)d\Gamma = \frac{1}{2m_{\pi^-}} \frac{1}{2m_{\pi^0}} |\mathcal{M}|^2 \frac{d^3 p_e}{(2\pi)^3 2E_e} \frac{d^3 p_\nu}{(2\pi)^3 2E_\nu} 2\pi \delta(\Delta m - E_e - E_\nu) 代入 M2|\mathcal{M}|^2 并利用 2mπ2mπ04mπ22m_{\pi^-} 2m_{\pi^0} \approx 4m_\pi^2,对中微子和电子的立体角积分(pepν\vec{p}_e \cdot \vec{p}_\nu 项积分为零),得到: dΓ=GF2c12π3pe2dpeEν2dEνδ(ΔmEeEν)d\Gamma = \frac{G_F^2 c_1^2}{\pi^3} p_e^2 dp_e E_\nu^2 dE_\nu \delta(\Delta m - E_e - E_\nu)EνE_\nu 积分并利用 pedpe=EedEep_e d p_e = E_e d E_e,得到总衰变率: Γ=GF2c12π3meΔmpeEe(ΔmEe)2dEe\Gamma = \frac{G_F^2 c_1^2}{\pi^3} \int_{m_e}^{\Delta m} p_e E_e (\Delta m - E_e)^2 dE_e

引入无量纲变量 x=Ee/mex = E_e / m_e 和上限 x0=Δm/mex_0 = \Delta m / m_e,衰变率可写为: Γ=GF2c12me5π3f(x0)\Gamma = \frac{G_F^2 c_1^2 m_e^5}{\pi^3} f(x_0) 其中无量纲积分 f(x0)f(x_0) 为: f(x0)=1x0xx21(x0x)2dxf(x_0) = \int_1^{x_0} x \sqrt{x^2-1} (x_0 - x)^2 dx

数值计算与结果

代入已知数值:

  • Δm=4.594 MeV\Delta m = 4.594 \text{ MeV}
  • me=0.511 MeVm_e = 0.511 \text{ MeV}
  • x0=4.594/0.5118.990x_0 = 4.594 / 0.511 \approx 8.990

计算积分 f(x0)f(x_0)f(x0)=x021x0xx21dx2x01x0x2x21dx+1x0x3x21dxf(x_0) = x_0^2 \int_1^{x_0} x \sqrt{x^2-1} dx - 2x_0 \int_1^{x_0} x^2 \sqrt{x^2-1} dx + \int_1^{x_0} x^3 \sqrt{x^2-1} dx 利用标准积分公式,代入 x0=8.990x_0 = 8.990 得到: f(8.990)80.82×237.7317.98×1612.95+11625.61838.7f(8.990) \approx 80.82 \times 237.73 - 17.98 \times 1612.95 + 11625.6 \approx 1838.7

将常数 GF=1.166×1011 MeV2G_F = 1.166 \times 10^{-11} \text{ MeV}^{-2} 代入,并使用自然单位制转换系数 =6.582×1022 MeVs\hbar = 6.582 \times 10^{-22} \text{ MeV}\cdot\text{s}(即 1 MeV=1.519×1021 s11 \text{ MeV} = 1.519 \times 10^{21} \text{ s}^{-1}): GF2me5π31.527×1025 MeV2.320×104 s1\frac{G_F^2 m_e^5}{\pi^3} \approx 1.527 \times 10^{-25} \text{ MeV} \approx 2.320 \times 10^{-4} \text{ s}^{-1} 因此理论衰变率为: Γth=(2.320×104 s1)×1838.7×c120.4266c12 s1\Gamma_{\text{th}} = (2.320 \times 10^{-4} \text{ s}^{-1}) \times 1838.7 \times c_1^2 \approx 0.4266 \, c_1^2 \text{ s}^{-1}

将理论值与实验测量值 Γexp=0.397 s1\Gamma_{\text{exp}} = 0.397 \text{ s}^{-1} 进行对比: 0.4266c12=0.397    c120.9306    c10.9650.4266 \, c_1^2 = 0.397 \implies c_1^2 \approx 0.9306 \implies c_1 \approx 0.965

真实值为 c1=Vud0.974c_1 = V_{ud} \approx 0.974。我们计算得到的 c10.965c_1 \approx 0.965 比真实值低了约 1%1\%,这正是由于在树图级别的计算中忽略了圈图辐射修正(如库仑修正等)所致。

c10.965\boxed{ c_1 \approx 0.965 }

90.7

Problem 90.7

srednickiChapter 90

习题 90.7

来源: 第90章, PDF第554页


90.7 Verify eq. (90.59). Express Γ\Gamma in eV.


Referenced Equations:

Equation (90.59):

Γ=α2mπ364π3fπ2.(90.59)\Gamma=\frac{\alpha^{2} m_{\pi}^{3}}{64 \pi^{3} f_{\pi}^{2}} . \tag{90.59}

习题 90.7 - 解答


第一部分:验证公式 (90.59)

1. 物理背景与有效拉格朗日量 中性 π\pi 介子衰变为双光子 (π0γγ\pi^0 \to \gamma\gamma) 的过程由手征反常(Adler-Bell-Jackiw 反常)主导。由反常给出的 π0\pi^0 与双光子相互作用的有效拉格朗日量为:

Leff=e232π2fππ0ϵμνρσFμνFρσ\mathcal{L}_{\text{eff}} = -\frac{e^2}{32\pi^2 f_{\pi}} \pi^0 \epsilon^{\mu\nu\rho\sigma} F_{\mu\nu} F_{\rho\sigma}

其中 ee 是基本电荷(满足 α=e2/4π\alpha = e^2/4\pi),fπf_{\pi}π\pi 介子衰变常数,Fμν=μAννAμF_{\mu\nu} = \partial_\mu A_\nu - \partial_\nu A_\mu 是电磁场张量。利用反对称性,拉格朗日量可化简为:

Leff=e28π2fππ0ϵμνρσμAνρAσ\mathcal{L}_{\text{eff}} = -\frac{e^2}{8\pi^2 f_{\pi}} \pi^0 \epsilon^{\mu\nu\rho\sigma} \partial_\mu A_\nu \partial_\rho A_\sigma

2. 跃迁矩阵元π0\pi^0 的动量为 pp,两个出射光子的动量和极化矢量分别为 (k1,ϵ1)(k_1, \epsilon_1)(k2,ϵ2)(k_2, \epsilon_2)。对场算符求变分时,由于末态有两个全同光子,会产生一个对称性因子 22。跃迁矩阵元 M\mathcal{M} 为:

iM=ie28π2fπ×2×ϵμνρσ(ik1μ)ϵ1ν(ik2ρ)ϵ2σi\mathcal{M} = -i \frac{e^2}{8\pi^2 f_{\pi}} \times 2 \times \epsilon^{\mu\nu\rho\sigma} (-i k_{1\mu}) \epsilon_{1\nu}^* (-i k_{2\rho}) \epsilon_{2\sigma}^*

代入 α=e2/4π\alpha = e^2/4\pi,整理得到:

M=απfπϵμνρσk1μϵ1νk2ρϵ2σ\mathcal{M} = \frac{\alpha}{\pi f_{\pi}} \epsilon^{\mu\nu\rho\sigma} k_{1\mu} \epsilon_{1\nu}^* k_{2\rho} \epsilon_{2\sigma}^*

3. 矩阵元模方与极化求和 计算衰变率需要对末态光子的极化求和。利用 Ward 恒等式,可以将极化求和替换为 ϵνϵνgνν\sum \epsilon_\nu^* \epsilon_{\nu'} \to -g_{\nu\nu'}

polM2=(απfπ)2ϵμνρσϵμνρσk1μk2ρk1μk2ρ(gνν)(gσσ)\sum_{\text{pol}} |\mathcal{M}|^2 = \left( \frac{\alpha}{\pi f_{\pi}} \right)^2 \epsilon^{\mu\nu\rho\sigma} \epsilon^{\mu'\nu'\rho'\sigma'} k_{1\mu} k_{2\rho} k_{1\mu'} k_{2\rho'} (-g_{\nu\nu'}) (-g_{\sigma\sigma'})

利用 Levi-Civita 张量的缩并恒等式 ϵμνρσϵμνρσ=2(δμμδρρδρμδμρ)\epsilon^{\mu\nu\rho\sigma} \epsilon_{\mu'\nu\rho'\sigma} = -2(\delta^\mu_{\mu'}\delta^\rho_{\rho'} - \delta^\mu_{\rho'}\delta^\rho_{\mu'}),上式化简为:

polM2=2(απfπ)2[(k1k1)(k2k2)(k1k2)2]\sum_{\text{pol}} |\mathcal{M}|^2 = -2 \left( \frac{\alpha}{\pi f_{\pi}} \right)^2 \left[ (k_1 \cdot k_1)(k_2 \cdot k_2) - (k_1 \cdot k_2)^2 \right]

由于光子是无质量的,k12=k22=0k_1^2 = k_2^2 = 0,因此:

polM2=2(απfπ)2(k1k2)2\sum_{\text{pol}} |\mathcal{M}|^2 = 2 \left( \frac{\alpha}{\pi f_{\pi}} \right)^2 (k_1 \cdot k_2)^2

由运动学关系 p=k1+k2p = k_1 + k_2,平方得 mπ2=2k1k2m_{\pi}^2 = 2k_1 \cdot k_2,即 k1k2=mπ2/2k_1 \cdot k_2 = m_{\pi}^2 / 2。代入上式得:

polM2=2(απfπ)2(mπ22)2=α2mπ42π2fπ2\sum_{\text{pol}} |\mathcal{M}|^2 = 2 \left( \frac{\alpha}{\pi f_{\pi}} \right)^2 \left( \frac{m_{\pi}^2}{2} \right)^2 = \frac{\alpha^2 m_{\pi}^4}{2\pi^2 f_{\pi}^2}

4. 衰变宽度计算 对于两体衰变,衰变宽度 Γ\Gamma 的一般公式为:

Γ=12mπ1SdΦ2polM2\Gamma = \frac{1}{2m_{\pi}} \frac{1}{S} \int d\Phi_2 \sum_{\text{pol}} |\mathcal{M}|^2

其中 SS 是末态全同粒子的对称因子,这里有两个光子,故 S=2!=2S = 2! = 2。两体相空间积分 dΦ2\int d\Phi_2 对于无质量末态粒子为 18π\frac{1}{8\pi}。 将所有部分代入:

Γ=12mπ1218πα2mπ42π2fπ2=α2mπ364π3fπ2\Gamma = \frac{1}{2m_{\pi}} \cdot \frac{1}{2} \cdot \frac{1}{8\pi} \cdot \frac{\alpha^2 m_{\pi}^4}{2\pi^2 f_{\pi}^2} = \frac{\alpha^2 m_{\pi}^3}{64\pi^3 f_{\pi}^2}

至此,公式 (90.59) 验证完毕。


第二部分:计算 Γ\Gamma 的数值 (单位: eV)

1. 物理常数取值 进行数值计算需要代入以下标准物理常数:

  • 精细结构常数:α1137.036\alpha \approx \frac{1}{137.036}
  • 中性 π\pi 介子质量:mπ134.977 MeV=1.34977×108 eVm_{\pi} \approx 134.977 \text{ MeV} = 1.34977 \times 10^8 \text{ eV}
  • π\pi 介子衰变常数:fπ92.28 MeV=9.228×107 eVf_{\pi} \approx 92.28 \text{ MeV} = 9.228 \times 10^7 \text{ eV} (注:此处采用 fπ92f_\pi \approx 92 MeV 的约定,部分文献记为 Fπ=2fπ130F_\pi = \sqrt{2}f_\pi \approx 130 MeV)

2. 数值代入与计算 将上述数值代入已验证的公式:

Γ=(1137.036)2×(1.34977×108 eV)364π3×(9.228×107 eV)2\Gamma = \frac{\left( \frac{1}{137.036} \right)^2 \times (1.34977 \times 10^8 \text{ eV})^3}{64 \pi^3 \times (9.228 \times 10^7 \text{ eV})^2}

分别计算分子和分母:

  • 分子:α2mπ3(5.325×105)×(2.459×1024 eV3)1.309×1020 eV3\alpha^2 m_{\pi}^3 \approx (5.325 \times 10^{-5}) \times (2.459 \times 10^{24} \text{ eV}^3) \approx 1.309 \times 10^{20} \text{ eV}^3
  • 分母:64π3fπ21984.4×(8.516×1015 eV2)1.690×1019 eV264 \pi^3 f_{\pi}^2 \approx 1984.4 \times (8.516 \times 10^{15} \text{ eV}^2) \approx 1.690 \times 10^{19} \text{ eV}^2

相除得到最终的衰变宽度:

Γ1.309×10201.690×1019 eV7.75 eV\Gamma \approx \frac{1.309 \times 10^{20}}{1.690 \times 10^{19}} \text{ eV} \approx 7.75 \text{ eV}

(该理论计算结果与 PDG 实验测量值 Γexp7.8 eV\Gamma_{\text{exp}} \approx 7.8 \text{ eV} 高度吻合)

Γ7.75 eV\boxed{\Gamma \approx 7.75 \text{ eV}}