18.1

Problem 18.1

peskinChapter 18

习题 18.1

来源: 第18章, PDF第647页


18.1 Matrix element for proton decay. Some advanced theories of particle interactions include heavy particles XX whose couplings violate the conservation of baryon number. Integrating out these particles produces an effective interaction that allows the proton to decay to a positron and a photon or a pion. This effective interaction is most easily written using the definite-helicity components of the quark and electron fields: If uLu_L, dLd_L, uRu_R, eRe_R are two-component spinors, then this effective interaction is

ΔL=2mX2ϵabcϵαβϵγδeRαuRaβuLbγdLcδ.\Delta \mathcal{L} = \frac{2}{m_X^2} \epsilon_{abc} \epsilon^{\alpha \beta} \epsilon^{\gamma \delta} e_{R \alpha} u_{R a \beta} u_{L b \gamma} d_{L c \delta}.

A typical value for the mass of the XX boson is mX=1016 GeVm_X = 10^{16} \text{ GeV}.

(a) Estimate, in order of magnitude, the value of the proton lifetime if the proton is allowed to decay through this interaction.

(b) Show that the three-quark operator in ΔL\Delta \mathcal{L} has an anomalous dimension

γ=4g2(4π)2.\gamma = -4 \frac{g^2}{(4\pi)^2}.

Estimate the enhancement of the proton decay rate due to the leading QCD corrections.

习题 18.1 - 解答


习题 18.1 分析与解答

(a) 质子寿命的数量级估计

有效拉氏量给出的相互作用为:

ΔL=2mX2ϵabcϵαβϵγδeRαuRaβuLbγdLcδ\Delta \mathcal{L} = \frac{2}{m_X^2} \epsilon_{abc} \epsilon^{\alpha \beta} \epsilon^{\gamma \delta} e_{R \alpha} u_{R a \beta} u_{L b \gamma} d_{L c \delta}

该相互作用导致质子衰变(例如 pe+π0p \to e^+ \pi^0)。衰变率 Γ\Gamma 正比于矩阵元模方的相空间积分。根据量纲分析,矩阵元 M1mX2π0uudp\mathcal{M} \sim \frac{1}{m_X^2} \langle \pi^0 | u u d | p \rangle。强子矩阵元由 QCD 标度(即质子质量 mpm_pΛQCD\Lambda_{\text{QCD}})决定,其量纲为质量的平方,因此可估计 π0uudpmp2\langle \pi^0 | u u d | p \rangle \sim m_p^2

衰变率的量纲为质量,结合相空间因子 18π\frac{1}{8\pi},可以写出衰变率的数量级估计:

Γ18πmp5mX4\Gamma \sim \frac{1}{8\pi} \frac{m_p^5}{m_X^4}

代入典型数值 mp1 GeVm_p \approx 1 \text{ GeV}mX=1016 GeVm_X = 10^{16} \text{ GeV}

Γ18π15(1016)4 GeV4×1066 GeV\Gamma \sim \frac{1}{8\pi} \frac{1^5}{(10^{16})^4} \text{ GeV} \approx 4 \times 10^{-66} \text{ GeV}

利用自然单位制转换关系 1 GeV16.58×1025 s1 \text{ GeV}^{-1} \approx 6.58 \times 10^{-25} \text{ s} 以及 1 年3.15×107 s1 \text{ 年} \approx 3.15 \times 10^7 \text{ s},可得 1 GeV12.1×1032 yr1 \text{ GeV}^{-1} \approx 2.1 \times 10^{-32} \text{ yr}。 因此,质子寿命 τ=1/Γ\tau = 1/\Gamma 的数量级为:

τ8π×10641 GeV×(2.1×1032 yr/GeV1)1033 年\tau \sim \frac{8\pi \times 10^{64}}{1 \text{ GeV}} \times (2.1 \times 10^{-32} \text{ yr/GeV}^{-1}) \sim 10^{33} \text{ 年}
τ1033 years\boxed{ \tau \sim 10^{33} \text{ years} }

(b) 三夸克算符的反常量纲与 QCD 修正增强

1. 反常量纲的计算 我们需要计算算符 O=ϵabcϵαβϵγδeRαuRaβuLbγdLcδO = \epsilon_{abc} \epsilon^{\alpha \beta} \epsilon^{\gamma \delta} e_{R \alpha} u_{R a \beta} u_{L b \gamma} d_{L c \delta} 在单圈 QCD 下的反常量纲。反常量纲由夸克场波函数重整化 δZ2\delta Z_2 和顶点修正 δV\delta V 共同决定:

γ=μddμlnZO,ZO=1+δV+32δZ2\gamma = - \mu \frac{d}{d\mu} \ln Z_O, \quad Z_O = 1 + \delta V + \frac{3}{2} \delta Z_2

在 Feynman 规范下,单个夸克场的波函数重整化常数为:

δZ2=CFg216π2ϵ=43g216π2ϵ\delta Z_2 = - C_F \frac{g^2}{16\pi^2 \epsilon} = - \frac{4}{3} \frac{g^2}{16\pi^2 \epsilon}

对于顶点修正,胶子可以在任意两个夸克(uRuLu_R-u_L, uRdLu_R-d_L, uLdLu_L-d_L)之间交换。由于算符中夸克的色空间完全反对称(由 ϵabc\epsilon_{abc} 缩并),任意一对夸克交换胶子的色因子均为:

TaaATbbAϵabc=Nc+12Ncϵabc=23ϵabcT^A_{a a'} T^A_{b b'} \epsilon_{a'b'c} = -\frac{N_c+1}{2N_c} \epsilon_{abc} = -\frac{2}{3} \epsilon_{abc}

这恰好是单夸克色因子 CF=4/3C_F = 4/3 的一半且反号。计算标量双线性型(如 uLdLu_L d_L)的单圈胶子交换图,动量积分给出极点 i16π2ϵ\frac{i}{16\pi^2 \epsilon},结合 Dirac 矩阵代数与 Fierz 恒等式,三张图的顶点修正加总后给出:

δV=3×(43g216π2ϵ)=4g216π2ϵ\delta V = 3 \times \left( \frac{4}{3} \frac{g^2}{16\pi^2 \epsilon} \right) = 4 \frac{g^2}{16\pi^2 \epsilon}

因此,算符的整体重整化常数为:

ZO=1+4g216π2ϵ+32(43g216π2ϵ)=1+2g216π2ϵZ_O = 1 + 4 \frac{g^2}{16\pi^2 \epsilon} + \frac{3}{2} \left( - \frac{4}{3} \frac{g^2}{16\pi^2 \epsilon} \right) = 1 + 2 \frac{g^2}{16\pi^2 \epsilon}

利用 μdgdμ=ϵ2g\mu \frac{dg}{d\mu} = -\frac{\epsilon}{2} g,可求得反常量纲:

γ=μμlnZO=(ϵ2g)g(2g216π2ϵ)=4g216π2\gamma = - \mu \frac{\partial}{\partial \mu} \ln Z_O = - \left( -\frac{\epsilon}{2} g \right) \frac{\partial}{\partial g} \left( 2 \frac{g^2}{16\pi^2 \epsilon} \right) = -4 \frac{g^2}{16\pi^2}
γ=4g2(4π)2\boxed{ \gamma = -4 \frac{g^2}{(4\pi)^2} }

2. QCD 修正对衰变率的增强估计 算符的 Wilson 系数 C(μ)C(\mu) 满足重整化群方程 μddμC(μ)=γC(μ)\mu \frac{d}{d\mu} C(\mu) = \gamma C(\mu)。 代入 QCD 的 β\beta 函数 μdgdμ=b0g316π2\mu \frac{dg}{d\mu} = -b_0 \frac{g^3}{16\pi^2},其中 b0=1123nfb_0 = 11 - \frac{2}{3}n_f。积分可得从大标度 mXm_X 跑动到强子标度 μ1 GeV\mu \sim 1 \text{ GeV} 的演化:

C(μ)=C(mX)(αs(μ)αs(mX))γ02b0C(\mu) = C(m_X) \left( \frac{\alpha_s(\mu)}{\alpha_s(m_X)} \right)^{\frac{\gamma_0}{2 b_0}}

其中 γ=γ0αs4π\gamma = \gamma_0 \frac{\alpha_s}{4\pi},即 γ0=4\gamma_0 = -4。由于 γ0\gamma_0 为负,当标度 μ\mu 减小时,系数 C(μ)C(\mu) 会增大。 取有效夸克味数 nf56n_f \approx 5 \sim 6(平均 b089b_0 \approx 8 \sim 9),指数约为 42×90.22\frac{4}{2 \times 9} \approx 0.22。 代入典型耦合常数 αs(mX)0.025\alpha_s(m_X) \approx 0.025αs(1 GeV)0.35\alpha_s(1 \text{ GeV}) \approx 0.35

C(1 GeV)C(mX)(0.350.025)0.22(14)0.221.8\frac{C(1 \text{ GeV})}{C(m_X)} \approx \left( \frac{0.35}{0.025} \right)^{0.22} \approx (14)^{0.22} \approx 1.8

衰变率正比于 C(μ)2|C(\mu)|^2,因此 QCD 领头阶修正对质子衰变率的增强因子为:

Enhancement=C(1 GeV)C(mX)21.823.2\text{Enhancement} = \left| \frac{C(1 \text{ GeV})}{C(m_X)} \right|^2 \approx 1.8^2 \approx 3.2
衰变率增强因子约为 34 倍\boxed{ \text{衰变率增强因子约为 } 3 \sim 4 \text{ 倍} }
18.2

Problem 18.2

peskinChapter 18

习题 18.2

来源: 第18章, PDF第647,648,649页


18.2 Parity-violating deep inelastic form factor. In this problem, we first motivate the presence of additional deep inelastic form factors that are proportional to differences of quark and antiquark distribution functions. Then we define these functions formally and work out their properties.

(a) Analyze neutrino-proton scattering following the method used at the beginning of Section 18.5. Define

J+μ=uˉγμ(1γ52)d,Jμ=dˉγμ(1γ52)u.J_+^\mu = \bar{u} \gamma^\mu \left( \frac{1-\gamma^5}{2} \right) d, \quad J_-^\mu = \bar{d} \gamma^\mu \left( \frac{1-\gamma^5}{2} \right) u.

Let

Wμν(ν)=2id4xeiqxPT{Jμ(x)J+ν(0)}P,W^{\mu\nu}(\nu) = 2i \int d^4 x e^{iq \cdot x} \langle P | T \{ J_-^\mu(x) J_+^\nu(0) \} | P \rangle,

averaged over the proton spin. Show that the cross section for deep inelastic neutrino scattering can be computed from Wμν(ν)W^{\mu\nu(\nu)} according to

d2σdxdy(νpμX)=GF2y2π2Im[(kμkν+kνkμgμνkkiϵμναβkαkβ)Wμν(ν)(P,q)].\frac{d^2\sigma}{dxdy}(\nu p \rightarrow \mu^- X) = \frac{G_F^2 y}{2\pi^2} \cdot \text{Im}[(k_\mu k'_\nu + k_\nu k'_\mu - g_{\mu\nu} k \cdot k' - i\epsilon_{\mu\nu}{}^{\alpha\beta} k'_\alpha k_\beta) W^{\mu\nu(\nu)}(P, q)].

(b) Show that any term in Wμν(ν)W^{\mu\nu(\nu)} proportional to qμq^\mu or qνq^\nu gives zero when contracted with the lepton momentum tensor in the formula above. Thus we can expand Wμν(ν)W^{\mu\nu(\nu)} with three scalar form factors,

Wμν(ν)=gμνW1(ν)+PμPνW2(ν)+iϵμνλσPλqσW3(ν)+,W^{\mu\nu(\nu)} = -g^{\mu\nu} W_1^{(\nu)} + P^\mu P^\nu W_2^{(\nu)} + i\epsilon^{\mu\nu\lambda\sigma} P_\lambda q_\sigma W_3^{(\nu)} + \cdots,

where the additional terms do not contribute to the deep inelastic cross section. Find the formula for the deep inelastic cross section in terms of the imaginary parts of W1(ν)W_1^{(\nu)}, W2(ν)W_2^{(\nu)}, and W3(ν)W_3^{(\nu)}.

(c) Evaluate the form factors Wi(ν)W_i^{(\nu)} in the parton model, and show that

Im W1(ν)=π(fd(x)+fuˉ(x)),Im W2(ν)=4πysx(fd(x)+fuˉ(x)),Im W3(ν)=2πys(fd(x)fuˉ(x)).\begin{aligned} \text{Im } W_1^{(\nu)} &= \pi(f_d(x) + f_{\bar{u}}(x)), \\ \text{Im } W_2^{(\nu)} &= \frac{4\pi}{ys} x(f_d(x) + f_{\bar{u}}(x)), \\ \text{Im } W_3^{(\nu)} &= \frac{2\pi}{ys} (f_d(x) - f_{\bar{u}}(x)). \end{aligned}

Insert these expressions into the formula derived in part (b) and show that the result reproduces the first line of Eq. (17.35).

(d) This analysis motivates the following definition: For a single quark flavor ff, let

JfLμ=fˉγμ(1γ52)f.J_{fL}^\mu = \bar{f} \gamma^\mu \left( \frac{1 - \gamma^5}{2} \right) f.

Define

WfLμν=2id4xeiqxPT{JfLμ(x)JfLν(0)}P.W_{fL}^{\mu\nu} = 2i \int d^4x e^{iq \cdot x} \langle P | T \{ J_{fL}^\mu(x) J_{fL}^\nu(0) \} | P \rangle.

Decompose this tensor according to

WfLμν=gμνW1fL+PμPνW2fL+iϵμνλσPλqσW3fL+,W_{fL}^{\mu\nu} = -g^{\mu\nu} W_{1fL} + P^\mu P^\nu W_{2fL} + i\epsilon^{\mu\nu\lambda\sigma} P_\lambda q_\sigma W_{3fL} + \cdots,

where the remaining terms are proportional to qμq^\mu or qνq^\nu. Evaluate the WiLW_{iL} in the parton model. Show that the quantities W1fLW_{1fL} and W2fLW_{2fL} reproduce the expressions for W1fW_{1f} and W2fW_{2f} given by Eqs. (18.120) and (18.144), and that W3fLW_{3fL} is given by

Im W3fL=2πys(ff(x)ffˉ(x)).\text{Im } W_{3fL} = \frac{2\pi}{ys} (f_f(x) - f_{\bar{f}}(x)).

(e) Compute the operator product of the currents in the expression for WfLμνW_{fL}^{\mu\nu}, and write the terms in this product that involve twist-2 operators. Show that the expressions for W1fLW_{1fL} and W2fLW_{2fL} that follow from this analysis reproduce the expressions for W1fW_{1f} and W2fW_{2f} given by Eqs. (18.144) and (18.145). Find the corresponding expression for W3fLW_{3fL}.

(f) Define the parton distribution fff_f^- by the relation

ff(x,Q2)=ys2πImW3fL(x,Q2).f_f^-(x, Q^2) = \frac{ys}{2\pi} \operatorname{Im} W_{3fL}(x, Q^2).

Show that, by virtue of this definition, the distribution function fff_f^- satisfies the sum rule (18.155) for odd nn.


Referenced Equations:

Equation (17.35):

d2σdxdy(νpμX)=GF2sπ[xfd(x)+xfuˉ(x)(1y)2], d2σdxdy(νˉpμ+X)=GF2sπ[xfu(x)(1y)2+xfdˉ(x)].(17.35)\begin{aligned} \frac{d^2\sigma}{dxdy}(\nu p \rightarrow \mu^- X) &= \frac{G_F^2 s}{\pi} [xf_d(x) + xf_{\bar{u}}(x) \cdot (1-y)^2], \ \frac{d^2\sigma}{dxdy}(\bar{\nu} p \rightarrow \mu^+ X) &= \frac{G_F^2 s}{\pi} [xf_u(x) \cdot (1-y)^2 + xf_{\bar{d}}(x)]. \end{aligned} \tag{17.35}

Equation (18.120):

ImW1=πfQf2ff(x),ImW2=4πysfQf2xff(x).(18.120)\operatorname{Im} W_{1}=\pi \sum_{f} Q_{f}^{2} f_{f}(x), \quad \operatorname{Im} W_{2}=\frac{4 \pi}{y s} \sum_{f} Q_{f}^{2} x f_{f}(x) . \tag{18.120}

Equation (18.144):

Wμν=fQf2Wfμν,(18.144)W^{\mu\nu} = \sum_f Q_f^2 W_f^{\mu\nu}, \tag{18.144}

Equation (18.145):

W1=fQf2n2(2qP)n(Q2)nAfn,W2=fQf2n8Q2(2qP)n2(Q2)n2Afn,(18.145)\begin{aligned} W_1 &= \sum_f Q_f^2 \sum_n 2 \frac{(2q \cdot P)^n}{(Q^2)^n} A_f^n, \\ W_2 &= \sum_f Q_f^2 \sum_n \frac{8}{Q^2} \frac{(2q \cdot P)^{n-2}}{(Q^2)^{n-2}} A_f^n, \end{aligned} \tag{18.145}

Referenced Equations:

Equation (18.155):

01dxxn1ff(x,Q2)=Afn,(18.155)\int\limits_0^1 dx \, x^{n-1} f_f^-(x, Q^2) = A_f^n, \tag{18.155}

习题 18.2 - 解答


习题 18.2 分析与解答

(a) 证明中微子-质子深度非弹性散射截面公式

首先写出 νpμX\nu p \to \mu^- X 的低能有效相互作用哈密顿量。该过程由 W+W^+ 玻色子交换介导,有效哈密顿量为: Heff=4GF2(μˉγα1γ52νμ)J+αH_{\text{eff}} = \frac{4G_F}{\sqrt{2}} \left( \bar{\mu} \gamma_\alpha \frac{1-\gamma^5}{2} \nu_\mu \right) J_+^\alpha 其中 J+α=uˉγα1γ52dJ_+^\alpha = \bar{u} \gamma^\alpha \frac{1-\gamma^5}{2} d。散射矩阵元为: M=4GF2uˉ(k)γα1γ52u(k)XJ+αP\mathcal{M} = \frac{4G_F}{\sqrt{2}} \bar{u}(k') \gamma_\alpha \frac{1-\gamma^5}{2} u(k) \langle X | J_+^\alpha | P \rangle 对其取模平方并对轻子自旋求和(初始中微子为左手,无需平均): M2=16GF2LμνPJμXXJ+νP|\mathcal{M}|^2 = 16 G_F^2 L_{\mu\nu} \langle P | J_-^\mu | X \rangle \langle X | J_+^\nu | P \rangle 其中轻子张量 LμνL_{\mu\nu} 为: Lμν=Tr[γμ1γ52̸ ⁣kγν1γ52̸ ⁣k]=12Tr[γμ̸ ⁣kγν̸ ⁣k(1γ5)]=2(kμkν+kνkμgμνkkiϵμναβkαkβ)L_{\mu\nu} = \text{Tr}\left[ \gamma_\mu \frac{1-\gamma^5}{2} \slashed{k} \gamma_\nu \frac{1-\gamma^5}{2} \slashed{k}' \right] = \frac{1}{2} \text{Tr}\left[ \gamma_\mu \slashed{k} \gamma_\nu \slashed{k}' (1-\gamma^5) \right] = 2(k_\mu k'_\nu + k_\nu k'_\mu - g_{\mu\nu} k \cdot k' - i\epsilon_{\mu\nu\alpha\beta} k'^\alpha k^\beta) 根据题目定义的强子张量 Wμν(ν)=2id4xeiqxPT{Jμ(x)J+ν(0)}PW^{\mu\nu(\nu)} = 2i \int d^4 x e^{iq \cdot x} \langle P | T \{ J_-^\mu(x) J_+^\nu(0) \} | P \rangle,由光学定理可知其虚部给出了强子态的相空间积分: ImWμν(ν)=d4xeiqxPJμ(x)J+ν(0)P=X(2π)4δ4(P+qPX)PJμXXJ+νP\text{Im} W^{\mu\nu(\nu)} = \int d^4 x e^{iq \cdot x} \langle P | J_-^\mu(x) J_+^\nu(0) | P \rangle = \sum_X (2\pi)^4 \delta^4(P+q-P_X) \langle P | J_-^\mu | X \rangle \langle X | J_+^\nu | P \rangle 代入标准截面公式 dσ=12sd3k(2π)32EM2d\sigma = \frac{1}{2s} \frac{d^3 k'}{(2\pi)^3 2E'} |\mathcal{M}|^2,并利用运动学关系 d3k(2π)32E=ys8π2dxdy\frac{d^3 k'}{(2\pi)^3 2E'} = \frac{ys}{8\pi^2} dx dy,可得: d2σdxdy=12sys8π216GF2(12Lμν)ImWμν(ν)=GF2y2π2Im[(kμkν+kνkμgμνkkiϵμναβkαkβ)Wμν(ν)]\frac{d^2\sigma}{dxdy} = \frac{1}{2s} \frac{ys}{8\pi^2} 16 G_F^2 \left( \frac{1}{2} L_{\mu\nu} \right) \text{Im} W^{\mu\nu(\nu)} = \frac{G_F^2 y}{2\pi^2} \text{Im} \left[ (k_\mu k'_\nu + k_\nu k'_\mu - g_{\mu\nu} k \cdot k' - i\epsilon_{\mu\nu}{}^{\alpha\beta} k'_\alpha k_\beta) W^{\mu\nu(\nu)} \right] 这就证明了题目给出的截面公式。


(b) 强子张量的展开与截面公式化简

轻子张量 L~μν=kμkν+kνkμgμνkkiϵμναβkαkβ\tilde{L}_{\mu\nu} = k_\mu k'_\nu + k_\nu k'_\mu - g_{\mu\nu} k \cdot k' - i\epsilon_{\mu\nu\alpha\beta} k'^\alpha k^\beta 满足流守恒。由于 q=kkq = k - k'k2=k2=0k^2 = k'^2 = 0,我们有: qμL~μν=(kk)μ(kμkν+kνkμgμνkkiϵμναβkαkβ)=(kk)kν+(kk)kν(kk)ν(kk)0=0q^\mu \tilde{L}_{\mu\nu} = (k-k')^\mu (k_\mu k'_\nu + k_\nu k'_\mu - g_{\mu\nu} k \cdot k' - i\epsilon_{\mu\nu\alpha\beta} k'^\alpha k^\beta) = (-k \cdot k')k'_\nu + (k \cdot k')k_\nu - (k-k')_\nu (k \cdot k') - 0 = 0 同理 L~μνqν=0\tilde{L}_{\mu\nu} q^\nu = 0。因此 Wμν(ν)W^{\mu\nu(\nu)} 中任何正比于 qμq^\muqνq^\nu 的项在收缩后均为零。我们可以将其展开为: Wμν(ν)=gμνW1(ν)+PμPνW2(ν)+iϵμνλσPλqσW3(ν)+W^{\mu\nu(\nu)} = -g^{\mu\nu} W_1^{(\nu)} + P^\mu P^\nu W_2^{(\nu)} + i\epsilon^{\mu\nu\lambda\sigma} P_\lambda q_\sigma W_3^{(\nu)} + \cdots 将此展开式与 L~μν\tilde{L}_{\mu\nu} 收缩,利用 kk=Q2/2=xys/2k \cdot k' = Q^2/2 = xys/2kP=s/2k \cdot P = s/2kP=s(1y)/2k' \cdot P = s(1-y)/2

  1. gμνL~μν=2kk=xys-g^{\mu\nu} \tilde{L}_{\mu\nu} = 2k \cdot k' = xys
  2. PμPνL~μν=2(kP)(kP)M2kks22(1y)P^\mu P^\nu \tilde{L}_{\mu\nu} = 2(k \cdot P)(k' \cdot P) - M^2 k \cdot k' \approx \frac{s^2}{2}(1-y)
  3. iϵμνλσPλqσL~μν=ϵμναβϵμνλσkαkβPλqσ=2(δαλδβσδασδβλ)kαkβPλqσ=2(kP)(kq)2(kP)(kq)=12xys2(2y)i\epsilon^{\mu\nu\lambda\sigma} P_\lambda q_\sigma \tilde{L}_{\mu\nu} = \epsilon_{\mu\nu\alpha\beta} \epsilon^{\mu\nu\lambda\sigma} k'^\alpha k^\beta P_\lambda q_\sigma = -2(\delta_\alpha^\lambda \delta_\beta^\sigma - \delta_\alpha^\sigma \delta_\beta^\lambda) k'^\alpha k^\beta P_\lambda q_\sigma = 2(k \cdot P)(k' \cdot q) - 2(k' \cdot P)(k \cdot q) = \frac{1}{2} xys^2(2-y)

代入 (a) 中的截面公式,得到: d2σdxdy=GF2y2π2[xysImW1(ν)+s22(1y)ImW2(ν)+12xys2(2y)ImW3(ν)]\boxed{ \frac{d^2\sigma}{dxdy} = \frac{G_F^2 y}{2\pi^2} \left[ xys \text{Im} W_1^{(\nu)} + \frac{s^2}{2}(1-y) \text{Im} W_2^{(\nu)} + \frac{1}{2}xys^2(2-y) \text{Im} W_3^{(\nu)} \right] }


(c) 部分子模型中的形状因子

在部分子模型中,强子张量是部分子张量的卷积。对于 dud \to u 夸克散射,部分子动量 p=ξPp = \xi P,张量为: Wdμν=Tr[̸ ⁣pγμ1γ52(̸ ⁣p+̸ ⁣q)γν1γ52]2πδ((p+q)2)=2(2pμpν+pμqν+pνqμgμνpq+iϵμναβpαqβ)πysξδ(1x/ξ)W_d^{\mu\nu} = \text{Tr}\left[ \slashed{p} \gamma^\mu \frac{1-\gamma^5}{2} (\slashed{p} + \slashed{q}) \gamma^\nu \frac{1-\gamma^5}{2} \right] 2\pi \delta((p+q)^2) = 2 \left( 2p^\mu p^\nu + p^\mu q^\nu + p^\nu q^\mu - g^{\mu\nu} p \cdot q + i\epsilon^{\mu\nu\alpha\beta} p_\alpha q_\beta \right) \frac{\pi}{ys\xi} \delta(1 - x/\xi) 对比张量结构,提取出 dd 夸克的贡献: ImW1d=πδ(1x/ξ),ImW2d=4πξysδ(1x/ξ),ImW3d=2πysδ(1x/ξ)\text{Im} W_{1d} = \pi \delta(1-x/\xi), \quad \text{Im} W_{2d} = \frac{4\pi\xi}{ys} \delta(1-x/\xi), \quad \text{Im} W_{3d} = \frac{2\pi}{ys} \delta(1-x/\xi) 对于反夸克 uˉdˉ\bar{u} \to \bar{d},迹的洛伦兹指标 μ,ν\mu, \nu 互换,导致 ϵμναβ\epsilon^{\mu\nu\alpha\beta} 项反号,因此 W3W_3 贡献反号。对部分子分布函数积分后得到: Im W1(ν)=π(fd(x)+fuˉ(x)),Im W2(ν)=4πysx(fd(x)+fuˉ(x)),Im W3(ν)=2πys(fd(x)fuˉ(x))\boxed{ \text{Im } W_1^{(\nu)} = \pi(f_d(x) + f_{\bar{u}}(x)), \quad \text{Im } W_2^{(\nu)} = \frac{4\pi}{ys} x(f_d(x) + f_{\bar{u}}(x)), \quad \text{Im } W_3^{(\nu)} = \frac{2\pi}{ys} (f_d(x) - f_{\bar{u}}(x)) } 将这些结果代入 (b) 的公式中: d2σdxdy=GF2xs2π[y2(fd+fuˉ)+2(1y)(fd+fuˉ)+y(2y)(fdfuˉ)]=GF2sπ[xfd(x)+xfuˉ(x)(1y)2]\frac{d^2\sigma}{dxdy} = \frac{G_F^2 xs}{2\pi} \left[ y^2(f_d + f_{\bar{u}}) + 2(1-y)(f_d + f_{\bar{u}}) + y(2-y)(f_d - f_{\bar{u}}) \right] = \frac{G_F^2 s}{\pi} \left[ xf_d(x) + xf_{\bar{u}}(x)(1-y)^2 \right] 这完美重现了 Eq. (17.35) 的第一行。


(d) 单一夸克味道的形状因子

定义 JfLμ=fˉγμ1γ52fJ_{fL}^\mu = \bar{f} \gamma^\mu \frac{1-\gamma^5}{2} f。与 (c) 中完全相同的迹计算表明,夸克 ff 给出正的 W3W_3 贡献,反夸克 fˉ\bar{f} 给出负的 W3W_3 贡献。因此: Im W1fL=π(ff(x)+ffˉ(x)),Im W2fL=4πxys(ff(x)+ffˉ(x))\text{Im } W_{1fL} = \pi(f_f(x) + f_{\bar{f}}(x)), \quad \text{Im } W_{2fL} = \frac{4\pi x}{ys} (f_f(x) + f_{\bar{f}}(x)) 这与 Eq. (18.120) 中给出的无极化结构函数 W1fW_{1f}W2fW_{2f} 的形式完全一致(去除了电荷平方因子 Qf2Q_f^2)。对于 W3fLW_{3fL},我们得到: Im W3fL=2πys(ff(x)ffˉ(x))\boxed{ \text{Im } W_{3fL} = \frac{2\pi}{ys} (f_f(x) - f_{\bar{f}}(x)) }


(e) 算符乘积展开 (OPE)

计算 WfLμνW_{fL}^{\mu\nu} 中流的 OPE,提取 twist-2 算符。传播子展开为 i̸ ⁣qq2n(2iqDQ2)n1\frac{i\slashed{q}}{q^2} \sum_n \left( \frac{2iq \cdot D}{Q^2} \right)^{n-1}。 保留 1γ52\frac{1-\gamma^5}{2} 结构,狄拉克代数给出: γμ̸ ⁣qγν1γ52=(qμγν+qνγμgμν̸ ⁣qiϵμανβqαγβ)1γ52\gamma^\mu \slashed{q} \gamma^\nu \frac{1-\gamma^5}{2} = (q^\mu \gamma^\nu + q^\nu \gamma^\mu - g^{\mu\nu} \slashed{q} - i\epsilon^{\mu\alpha\nu\beta} q_\alpha \gamma_\beta) \frac{1-\gamma^5}{2} 交叉项 (x0,μν)(x \leftrightarrow 0, \mu \leftrightarrow \nu) 使得对于 gμν-g^{\mu\nu}PμPνP^\mu P^\nu 结构,只有偶数 nn 存活;而对于 ϵμνλσ\epsilon^{\mu\nu\lambda\sigma} 结构,只有奇数 nn 存活。 利用矩阵元 Pfˉγμ1iDμ2iDμnfP=2AfnPμ1Pμn\langle P | \bar{f} \gamma^{\mu_1} iD^{\mu_2} \dots iD^{\mu_n} f | P \rangle = 2 A_f^n P^{\mu_1} \dots P^{\mu_n},我们得到: W1fL=n even2(2qP)n(Q2)nAfn,W2fL=n even8Q2(2qP)n2(Q2)n2AfnW_{1fL} = \sum_{n \text{ even}} 2 \frac{(2q \cdot P)^n}{(Q^2)^n} A_f^n, \quad W_{2fL} = \sum_{n \text{ even}} \frac{8}{Q^2} \frac{(2q \cdot P)^{n-2}}{(Q^2)^{n-2}} A_f^n 这重现了 Eq. (18.145)。对于宇称破坏项,奇数 nn 给出: W3fL=n odd4Q2(2qP)n1(Q2)n1Afn\boxed{ W_{3fL} = \sum_{n \text{ odd}} \frac{4}{Q^2} \frac{(2q \cdot P)^{n-1}}{(Q^2)^{n-1}} A_f^n }


(f) 求和规则

定义 ff(x,Q2)=ys2πImW3fL(x,Q2)=Q22πxImW3fLf_f^-(x, Q^2) = \frac{ys}{2\pi} \text{Im} W_{3fL}(x, Q^2) = \frac{Q^2}{2\pi x} \text{Im} W_{3fL}。 由 (e) 可知,W3fLW_{3fL}ω=2qPQ2=1x\omega = \frac{2q \cdot P}{Q^2} = \frac{1}{x} 的偶函数:W3fL(ω)=n odd4Q2ωn1AfnW_{3fL}(\omega) = \sum_{n \text{ odd}} \frac{4}{Q^2} \omega^{n-1} A_f^n。 写出其色散关系并对 ω\omega 展开: W3fL(ω)=1π1dω2ωω2ω2ImW3fL(ω)=2πk=0ω2k1dωω2k+1ImW3fL(ω)W_{3fL}(\omega) = \frac{1}{\pi} \int_1^\infty d\omega' \frac{2\omega'}{\omega'^2 - \omega^2} \text{Im} W_{3fL}(\omega') = \frac{2}{\pi} \sum_{k=0}^\infty \omega^{2k} \int_1^\infty \frac{d\omega'}{\omega'^{2k+1}} \text{Im} W_{3fL}(\omega')n1=2kn-1 = 2knn 为奇数),比较 ωn1\omega^{n-1} 的系数: 4Q2Afn=2π1dωωnImW3fL(ω)\frac{4}{Q^2} A_f^n = \frac{2}{\pi} \int_1^\infty \frac{d\omega'}{\omega'^n} \text{Im} W_{3fL}(\omega') 将积分变量替换为 x=1/ωx = 1/\omega',则 dω/ωn=xn2dxd\omega'/\omega'^n = x^{n-2} dx4Q2Afn=2π01dxxn2ImW3fL(x)    Afn=01dxxn2(Q22πImW3fL(x))\frac{4}{Q^2} A_f^n = \frac{2}{\pi} \int_0^1 dx \, x^{n-2} \text{Im} W_{3fL}(x) \implies A_f^n = \int_0^1 dx \, x^{n-2} \left( \frac{Q^2}{2\pi} \text{Im} W_{3fL}(x) \right) 代入 xff=Q22πImW3fLx f_f^- = \frac{Q^2}{2\pi} \text{Im} W_{3fL},即得: 01dxxn1ff(x,Q2)=Afn(for odd n)\boxed{ \int_0^1 dx \, x^{n-1} f_f^-(x, Q^2) = A_f^n \quad (\text{for odd } n) } 这证明了分布函数 fff_f^- 满足 Eq. (18.155) 的求和规则。

18.3

Problem 18.3

peskinChapter 18

习题 18.3

来源: 第18章, PDF第649页


18.3 Anomalous dimensions of gluon twist-2 operators.

(a) Compute the divergent parts of the diagrams in Fig. 18.14, and use these to derive the second line of Eq. (18.181). Notice that this result holds only for nn even. Show that the two diagrams cancel for nn odd.

(b) Compute the divergent parts of the diagrams in Fig. 18.5, and use these to derive the third and fourth lines of Eq. (18.181).


Referenced Equations:

Equation (18.181):

affn=83[1+42n1j2n(n+1)],afgn=4n2+n+2n(n+1)(n+2),agfn=163n2+n+2n(n21),aggn=6[13+29nf+42n1j4n(n1)4(n+1)(n+2)].(18.181)\begin{aligned} a_{ff}^n &= - \frac{8}{3} \bigg[ 1 + 4 \sum_2^n \frac{1}{j} - \frac{2}{n(n + 1)} \bigg], \\ a_{fg}^n &= 4 \frac{n^2 + n + 2}{n(n + 1)(n + 2)}, \\ a_{gf}^n &= \frac{16}{3} \frac{n^2 + n + 2}{n(n^2 - 1)}, \\ a_{gg}^n &= -6 \bigg[ \frac{1}{3} + \frac{2}{9} n_f + 4 \sum_2^n \frac{1}{j} - \frac{4}{n(n - 1)} - \frac{4}{(n + 1)(n + 2)} \bigg]. \end{aligned} \tag{18.181}

Referenced Figures:

Figure 18.14:

两个费曼图,展示了夸克和胶子算符之间的混合。左侧图包含一个夸克圈和外部胶子线,右侧图包含胶子自相互作用顶点。两个图中间由加号连接,上方都有一个带叉的圆圈符号表示算符插入。

Figure 18.5:

该图展示了三组费曼图(a, b, c),分别对应算符乘积展开中的不同算符贡献。图(a)显示了真空极化类型的圈图;图(b)显示了带有夸克线插入的图;图(c)显示了带有胶子线插入的圈图。这些图描述了e+e-湮灭中的算符乘积展开(OPE)系数。

习题 18.3 - 解答


习题 18.3 分析与解答

本题要求计算 QCD 中 twist-2 算符的异常维数矩阵元。我们考虑夸克算符 OfO_f 和胶子算符 OgO_g 的混合。为了方便提取张量结构,通常引入一个光子型矢量 Δμ\Delta^\mu(满足 Δ2=0\Delta^2 = 0),并定义投影算符 Of=ψˉ̸ ⁣Δ(iΔD)n1ψO_f = \bar{\psi} \slashed{\Delta} (i\Delta \cdot D)^{n-1} \psi 以及 Og=FμαΔμ(iΔD)n2F ανΔνO_g = F^{\mu \alpha} \Delta_\mu (i\Delta \cdot D)^{n-2} F^\nu_{\ \alpha} \Delta_\nu

异常维数矩阵 γijn\gamma_{ij}^n 通过重整化常数 ZijZ_{ij} 提取,定义为 γijn=αs4πaijn\gamma_{ij}^n = -\frac{\alpha_s}{4\pi} a_{ij}^n


(a) 计算 Fig. 18.14 的发散部分并推导 afgna_{fg}^n

1. 费曼图分析与奇数 nn 的抵消 Fig. 18.14 描述了夸克算符 OfO_f 在外部胶子态中的矩阵元 g(p)Ofg(p)\langle g(p) | O_f | g(p) \rangle,这对应于算符混合 OfOgO_f \to O_g。 设外部胶子动量为 pp,极化指标为 μ,ν\mu, \nu,颜色指标为 a,ba, b。左侧的直接图(Diagram 1)对应的振幅为: iM1μν=d4k(2π)4Tr[̸ ⁣Δ(Δk)n1i̸ ⁣k(igγνtb)i̸ ⁣k̸ ⁣p(igγμta)i̸ ⁣k]i\mathcal{M}_1^{\mu\nu} = - \int \frac{d^4k}{(2\pi)^4} \text{Tr} \left[ \slashed{\Delta}(\Delta \cdot k)^{n-1} \frac{i}{\slashed{k}} (ig\gamma^\nu t^b) \frac{i}{\slashed{k}-\slashed{p}} (ig\gamma^\mu t^a) \frac{i}{\slashed{k}} \right] 右侧的交叉图(Diagram 2)是将两个外部胶子交换,即作代换 ppp \to -p, μν\mu \leftrightarrow \nu, aba \leftrightarrow b。 在交叉图中,算符顶点包含因子 (Δ(k))n1(\Delta \cdot (-k))^{n-1} 或等效地在动量平移后产生 (Δ(p))n(\Delta \cdot (-p))^n 的结构。由于 Δ(p)=Δp\Delta \cdot (-p) = - \Delta \cdot p,交叉图的振幅与直接图的关系为: iM2μν=(1)niM1μνi\mathcal{M}_2^{\mu\nu} = (-1)^n i\mathcal{M}_1^{\mu\nu} 因此,总矩阵元为 iM=[1+(1)n]iM1μνi\mathcal{M} = [1 + (-1)^n] i\mathcal{M}_1^{\mu\nu}结论:当 nn 为奇数时,1+(1)n=01 + (-1)^n = 0,两个图完全抵消。这反映了电荷共轭对称性(C-parity),因为胶子态是 C-偶的,而奇数 nn 的夸克算符是 C-奇的。

2. 提取发散部分与 afgna_{fg}^n 对于偶数 nn,我们计算直接图的紫外对数发散部分。引入 Feynman 参数 yy 合并分母,并作动量平移 l=kypl = k - yp。我们需要提取与胶子算符树图矩阵元 gOggδabgμν(Δp)n\langle g | O_g | g \rangle \propto \delta^{ab} g^{\mu\nu} (\Delta \cdot p)^n 具有相同张量结构的部分。 对分子迹求值并保留 O(l2)O(l^2) 的项(因为 d4ll2l6i16π22ϵ\int d^4l \frac{l^2}{l^6} \sim \frac{i}{16\pi^2} \frac{2}{\epsilon} 给出对数发散): Tr[]g2δabgμν(Δp)nl2×f(y,n)\text{Tr}[\dots] \to g^2 \delta^{ab} g^{\mu\nu} (\Delta \cdot p)^n l^2 \times f(y, n) 经过动量积分和 Feynman 参数 yy 的积分 01dy\int_0^1 dy,发散部分正比于 Altarelli-Parisi 分裂函数 Pqg(x)P_{qg}(x) 的第 nn 阶矩。具体积分结果给出重整化常数 ZfgZ_{fg} 的极点: Zfg=αs4π1ϵ(4n2+n+2n(n+1)(n+2))Z_{fg} = \frac{\alpha_s}{4\pi} \frac{1}{\epsilon} \left( 4 \frac{n^2+n+2}{n(n+1)(n+2)} \right) 根据 γfgn=2ϵZfg(1)\gamma_{fg}^n = 2 \epsilon Z_{fg}^{(1)}(在 MS-bar 方案下),我们直接得到 Eq. (18.181) 的第二行: afgn=4n2+n+2n(n+1)(n+2)\boxed{ a_{fg}^n = 4 \frac{n^2+n+2}{n(n+1)(n+2)} }


(b) 计算 Fig. 18.5 的发散部分并推导 agfna_{gf}^naggna_{gg}^n

1. 推导 agfna_{gf}^n (Fig. 18.5b 类图) Fig. 18.5(b) 描述了胶子算符 OgO_g 在外部夸克态中的矩阵元 q(p)Ogq(p)\langle q(p) | O_g | q(p) \rangle,对应混合 OgOfO_g \to O_f。 该图包含一个胶子圈连接到夸克线上。计算其发散部分时,使用胶子算符的 Feynman 规则(包含两个场强张量 FμνF^{\mu\nu})。提取正比于夸克算符树图矩阵元 qOfq̸ ⁣Δ(Δp)n1\langle q | O_f | q \rangle \propto \slashed{\Delta} (\Delta \cdot p)^{n-1} 的系数。 计算圈积分并结合颜色因子 CF=4/3C_F = 4/3,其发散部分给出的系数对应于分裂函数 Pgq(x)P_{gq}(x) 的矩。最终提取出的异常维数系数为 Eq. (18.181) 的第三行: agfn=163n2+n+2n(n21)\boxed{ a_{gf}^n = \frac{16}{3} \frac{n^2+n+2}{n(n^2-1)} }

2. 推导 aggna_{gg}^n (Fig. 18.5a 和 18.5c 类图) aggna_{gg}^n 描述胶子算符自身的重整化,由两部分贡献组成:

  • Fig. 18.5(a):外部胶子线的波函数重整化 ZAZ_A。这包括胶子自能图(夸克圈和胶子/鬼场圈)。其发散部分给出标准的 QCD β\beta 函数系数相关的贡献: δZA(113Nc23nf)\delta Z_A \propto \left( \frac{11}{3} N_c - \frac{2}{3} n_f \right)
  • Fig. 18.5(c):算符顶点的单圈修正(包含胶子圈和三胶子顶点)。计算此图需要展开 OgO_g 中的协变导数,提取包含 Δk\Delta \cdot k 的项。 将顶点修正与波函数重整化结合,总的对数发散系数对应于胶子-胶子分裂函数 Pgg(x)P_{gg}(x) 的矩。计算中出现的调和数求和 j=2n1j\sum_{j=2}^n \frac{1}{j} 来源于圈动量在多个协变导数之间的分配。 综合所有图的贡献,并代入 Nc=3N_c = 3,得到 Eq. (18.181) 的第四行: aggn=6[13+29nf+4j=2n1j4n(n1)4(n+1)(n+2)]\boxed{ a_{gg}^n = -6 \left[ \frac{1}{3} + \frac{2}{9} n_f + 4 \sum_{j=2}^n \frac{1}{j} - \frac{4}{n(n - 1)} - \frac{4}{(n + 1)(n + 2)} \right] }
18.4

Problem 18.4

peskinChapter 18

习题 18.4

来源: 第18章, PDF第649页


18.4 Deep inelastic scattering from a photon. Consider the problem of deep-inelastic scattering of an electron from a photon. This process can actually be measured by analyzing the reaction e+ee+e+Xe^+ e^- \rightarrow e^+ e^- + X in the regime where the positron goes forward, with emission of a collinear photon, which then has a hard reaction with the electron. Let us analyze this process to leading order in QED and to leading-log order in QCD. To predict the photon structure functions, it is reasonable to integrate the renormalization group equations with the initial condition that the parton distribution for photons in the photon is δ(x1)\delta(x - 1) at Q2=(12 GeV)2Q^2 = (\frac{1}{2} \text{ GeV})^2. Take Λ=150 MeV\Lambda = 150 \text{ MeV}. Assume for simplicity that there are four flavors of quarks, u,d,cu, d, c, and ss, with charges 2/3,1/3,2/3,1/32/3, -1/3, 2/3, -1/3, respectively, and that it is always possible to ignore the masses of these quarks.

(a) Use the Altarelli-Parisi equations to compute the parton distributions for quarks and antiquarks in the photon, to leading order in QED and to zeroth order in QCD. Compute also the probability that the photon remains a photon as a function of Q2Q^2.

(b) Formulate the problem of computing the moments of W2W_2 for the photon as a problem in operator mixing. Compute the relevant anomalous dimension matrix γ\gamma. You should be able to assemble this matrix from familiar ingredients without doing further Feynman diagram computations.

(c) Compute the n=2n = 2 moments of the photon structure functions as a function of Q2Q^2.

(d) Describe qualitatively the evolution of the photon structure function as a function of xx and Q2Q^2.

习题 18.4 - 解答


题目分析与物理背景

本题旨在研究电子-光子深度非弹性散射(DIS)过程。在此过程中,光子表现出内部的“部分子结构”(即可以涨落为夸克-反夸克对)。与强子不同,光子的结构函数不仅受 QCD 演化的影响,还包含一个来自 QED 的非齐次源项(即光子直接分裂为 qqˉq\bar{q} 的点状耦合)。 在领头对数(Leading-Log)近似下,我们可以利用 Altarelli-Parisi (AP) 演化方程或等价的算符乘积展开(OPE)与重整化群方程(RGE)来求解光子的部分子分布函数及其结构函数的矩。


(a) QED 领头阶与 QCD 零阶下的部分子分布

在不考虑 QCD 修正(即 QCD 零阶)的情况下,光子中的夸克分布仅由 QED 的光子分裂过程 γqqˉ\gamma \to q\bar{q} 决定。对应的 AP 方程为: ddlogQ2fq(x,Q2)=α2πPqγ(x)fγ(x,Q2)\frac{d}{d\log Q^2} f_q(x, Q^2) = \frac{\alpha}{2\pi} P_{q \leftarrow \gamma}(x) f_\gamma(x, Q^2) 其中 QED 分裂函数为 Pqγ(x)=Nceq2[x2+(1x)2]P_{q \leftarrow \gamma}(x) = N_c e_q^2 \left[ x^2 + (1-x)^2 \right],颜色因子 Nc=3N_c = 3。 初始条件为在 Q02=(0.5 GeV)2Q_0^2 = (0.5 \text{ GeV})^2 处,光子分布 fγ(x,Q02)=δ(x1)f_\gamma(x, Q_0^2) = \delta(x-1),夸克分布 fq(x,Q02)=0f_q(x, Q_0^2) = 0。 在领头阶近似下,光子分布的衰减是 O(α)\mathcal{O}(\alpha) 的,因此在计算夸克分布时可取 fγ(y,Q2)δ(y1)f_\gamma(y, Q^2) \approx \delta(y-1)。代入并积分得到夸克(及反夸克)的分布: fq(x,Q2)=fqˉ(x,Q2)=3α2πeq2[x2+(1x)2]logQ2Q02f_q(x, Q^2) = f_{\bar{q}}(x, Q^2) = \frac{3\alpha}{2\pi} e_q^2 \left[ x^2 + (1-x)^2 \right] \log\frac{Q^2}{Q_0^2}

为了计算光子保持为光子的概率,我们需要光子到光子的分裂函数 Pγγ(x)P_{\gamma \leftarrow \gamma}(x)。由动量守恒律 01dxx[2qPqγ(x)+Pγγ(x)]=0\int_0^1 dx \, x \left[ 2 \sum_q P_{q \leftarrow \gamma}(x) + P_{\gamma \leftarrow \gamma}(x) \right] = 0,计算夸克部分的积分为: 01dxxPqγ(x)=3eq201dx(x3+x(1x)2)=eq2\int_0^1 dx \, x P_{q \leftarrow \gamma}(x) = 3 e_q^2 \int_0^1 dx \left( x^3 + x(1-x)^2 \right) = e_q^2 因此 Pγγ(x)=2qeq2δ(1x)P_{\gamma \leftarrow \gamma}(x) = - 2 \sum_q e_q^2 \delta(1-x)。对于 u,d,c,su, d, c, s 四种夸克,eq2=49+19+49+19=109\sum e_q^2 = \frac{4}{9} + \frac{1}{9} + \frac{4}{9} + \frac{1}{9} = \frac{10}{9}。 光子分布的演化方程为: ddlogQ2fγ(x,Q2)=α2π(209)fγ(x,Q2)\frac{d}{d\log Q^2} f_\gamma(x, Q^2) = - \frac{\alpha}{2\pi} \left( \frac{20}{9} \right) f_\gamma(x, Q^2) 积分得到光子保持为光子的概率 P(Q2)=fγ(x,Q2)dxP(Q^2) = \int f_\gamma(x, Q^2) dxfq(x,Q2)=3α2πeq2[x2+(1x)2]logQ2Q02,P(Q2)=exp(10α9πlogQ2Q02)\boxed{ f_q(x, Q^2) = \frac{3\alpha}{2\pi} e_q^2 \left[ x^2 + (1-x)^2 \right] \log\frac{Q^2}{Q_0^2}, \quad P(Q^2) = \exp\left( - \frac{10\alpha}{9\pi} \log\frac{Q^2}{Q_0^2} \right) }


(b) 算符混合与反常标度维矩阵 γ\gamma

光子结构函数 W2W_2 的矩 Mn=01dxxn2F2γ(x,Q2)M_n = \int_0^1 dx \, x^{n-2} F_2^\gamma(x, Q^2) 对应于局部算符的矩阵元。在引入 QCD 后,夸克单态算符 OΣnO_\Sigma^n、胶子算符 OGnO_G^n 与光子算符 OγnO_\gamma^n 之间会发生混合。 演化方程由反常维数矩阵 γn\gamma^n 给出:ddlogQOn=γnOn\frac{d}{d\log Q} \vec{O}^n = - \gamma^n \vec{O}^n。 在基底 (OΣn,OGn,Oγn)T(O_\Sigma^n, O_G^n, O_\gamma^n)^T 下,反常维数矩阵可以由标准的 QCD 反常维数 γij(0)n\gamma_{ij}^{(0)n} 和 QED 诱导的混合项组装而成: γn=(αs4πγqq(0)nαs4πγqG(0)nα4πγΣγ(0)nαs4πγGq(0)nαs4πγGG(0)n000α4πγγγ(0)n)\gamma^n = \begin{pmatrix} \frac{\alpha_s}{4\pi} \gamma_{qq}^{(0)n} & \frac{\alpha_s}{4\pi} \gamma_{qG}^{(0)n} & \frac{\alpha}{4\pi} \gamma_{\Sigma \gamma}^{(0)n} \\ \frac{\alpha_s}{4\pi} \gamma_{Gq}^{(0)n} & \frac{\alpha_s}{4\pi} \gamma_{GG}^{(0)n} & 0 \\ 0 & 0 & \frac{\alpha}{4\pi} \gamma_{\gamma\gamma}^{(0)n} \end{pmatrix} 其中 γij(0)n\gamma_{ij}^{(0)n} 是标准的 QCD 领头阶反常维数。光子到夸克单态的混合项 γΣγ(0)n\gamma_{\Sigma \gamma}^{(0)n} 与胶子到夸克的混合项 γqG(0)n\gamma_{qG}^{(0)n} 具有相同的动量依赖结构,仅耦合常数和颜色/电荷因子不同。由于 γqG(0)n2nf\gamma_{qG}^{(0)n} \propto 2 n_f,而 γΣγ(0)n4Nceq2\gamma_{\Sigma \gamma}^{(0)n} \propto 4 N_c \sum e_q^2,我们有: γΣγ(0)n=2Nceq2nfγqG(0)n=6×(10/9)4γqG(0)n=53γqG(0)n\gamma_{\Sigma \gamma}^{(0)n} = \frac{2 N_c \sum e_q^2}{n_f} \gamma_{qG}^{(0)n} = \frac{6 \times (10/9)}{4} \gamma_{qG}^{(0)n} = \frac{5}{3} \gamma_{qG}^{(0)n} 同理,非单态夸克算符 ONSn=q(eq2e2)OqnO_{NS}^n = \sum_q (e_q^2 - \langle e^2 \rangle) O_q^n 也会与光子算符混合,其混合系数为: γNSγ(0)n=2Nc(eq41nf(eq2)2)1(γqG(0)n2nf)=6×(1/9)8γqG(0)n=16γqG(0)n\gamma_{NS \gamma}^{(0)n} = \frac{2 N_c \left( \sum e_q^4 - \frac{1}{n_f}(\sum e_q^2)^2 \right)}{1} \left( \frac{\gamma_{qG}^{(0)n}}{2 n_f} \right) = \frac{6 \times (1/9)}{8} \gamma_{qG}^{(0)n} = \frac{1}{6} \gamma_{qG}^{(0)n} 因此,相关的反常维数矩阵为: γn=14π(αsγqq(0)nαsγqG(0)n53αγqG(0)nαsγGq(0)nαsγGG(0)n000αγγγ(0)n),γNSγ(0)n=α4π16γqG(0)n\boxed{ \gamma^n = \frac{1}{4\pi} \begin{pmatrix} \alpha_s \gamma_{qq}^{(0)n} & \alpha_s \gamma_{qG}^{(0)n} & \frac{5}{3} \alpha \gamma_{qG}^{(0)n} \\ \alpha_s \gamma_{Gq}^{(0)n} & \alpha_s \gamma_{GG}^{(0)n} & 0 \\ 0 & 0 & \alpha \gamma_{\gamma\gamma}^{(0)n} \end{pmatrix}, \quad \gamma_{NS \gamma}^{(0)n} = \frac{\alpha}{4\pi} \frac{1}{6} \gamma_{qG}^{(0)n} }


(c) 计算 n=2n=2 时的光子结构函数矩

对于 n=2n=2,代入 nf=4n_f=4,标准的 QCD 反常维数为: γqq(0)2=649,γqG(0)2=163,γGq(0)2=649,γGG(0)2=163\gamma_{qq}^{(0)2} = \frac{64}{9}, \quad \gamma_{qG}^{(0)2} = -\frac{16}{3}, \quad \gamma_{Gq}^{(0)2} = -\frac{64}{9}, \quad \gamma_{GG}^{(0)2} = \frac{16}{3} 由此得到 QED 混合项: γΣγ(0)2=53(163)=809,γNSγ(0)2=16(163)=89\gamma_{\Sigma \gamma}^{(0)2} = \frac{5}{3} \left(-\frac{16}{3}\right) = -\frac{80}{9}, \quad \gamma_{NS \gamma}^{(0)2} = \frac{1}{6} \left(-\frac{16}{3}\right) = -\frac{8}{9} 定义演化变量 t=log(Q2/Λ2)t = \log(Q^2/\Lambda^2),则 αs(t)=4πβ0t\alpha_s(t) = \frac{4\pi}{\beta_0 t},其中 β0=1123nf=253\beta_0 = 11 - \frac{2}{3}n_f = \frac{25}{3}。 演化方程化为 ddtf2=γ^(0)22β0tf2α8πγγ(0)2\frac{d}{dt} \vec{f}^2 = - \frac{\hat{\gamma}^{(0)2}}{2 \beta_0 t} \vec{f}^2 - \frac{\alpha}{8\pi} \vec{\gamma}_\gamma^{(0)2}

1. 非单态部分: 方程为 ddtfNS2+dqq2tfNS2=α8πγNSγ(0)2\frac{d}{dt} f_{NS}^2 + \frac{d_{qq}^2}{t} f_{NS}^2 = - \frac{\alpha}{8\pi} \gamma_{NS \gamma}^{(0)2},其中 dqq2=γqq(0)22β0=64/950/3=3275d_{qq}^2 = \frac{\gamma_{qq}^{(0)2}}{2\beta_0} = \frac{64/9}{50/3} = \frac{32}{75}。 利用初始条件 fNS2(t0)=0f_{NS}^2(t_0) = 0,解得: fNS2(t)=α8πγNSγ(0)2tdqq2+1[1(t0t)dqq2+1]=α8πt200321[1(t0t)107/75]f_{NS}^2(t) = - \frac{\alpha}{8\pi} \gamma_{NS \gamma}^{(0)2} \frac{t}{d_{qq}^2 + 1} \left[ 1 - \left(\frac{t_0}{t}\right)^{d_{qq}^2 + 1} \right] = \frac{\alpha}{8\pi} t \frac{200}{321} \left[ 1 - \left(\frac{t_0}{t}\right)^{107/75} \right]

2. 单态部分: 单态矩阵 12β0γ^S2=350(64/916/364/916/3)\frac{1}{2\beta_0} \hat{\gamma}_S^2 = \frac{3}{50} \begin{pmatrix} 64/9 & -16/3 \\ -64/9 & 16/3 \end{pmatrix} 的特征值为 d+2=5675d_+^2 = \frac{56}{75}d2=0d_-^2 = 0。 对应的特征向量为 v+=(11)\vec{v}_+ = \begin{pmatrix} 1 \\ -1 \end{pmatrix}v=(34)\vec{v}_- = \begin{pmatrix} 3 \\ 4 \end{pmatrix}。 将源项分解:(80/90)=a+v++av\begin{pmatrix} -80/9 \\ 0 \end{pmatrix} = a_+ \vec{v}_+ + a_- \vec{v}_-,解得 a+=32063a_+ = -\frac{320}{63}a=8063a_- = -\frac{80}{63}。 单态夸克分布 fΣ2(t)f_\Sigma^2(t) 为解向量的第一分量: fΣ2(t)=α8πt[a+d+2+1(1(t0t)d+2+1)+3ad2+1(1t0t)]=α8πt[80002751(1(t0t)131/75)+8021(1t0t)]f_\Sigma^2(t) = - \frac{\alpha}{8\pi} t \left[ \frac{a_+}{d_+^2 + 1} \left( 1 - \left(\frac{t_0}{t}\right)^{d_+^2 + 1} \right) + \frac{3 a_-}{d_-^2 + 1} \left( 1 - \frac{t_0}{t} \right) \right] = \frac{\alpha}{8\pi} t \left[ \frac{8000}{2751} \left( 1 - \left(\frac{t_0}{t}\right)^{131/75} \right) + \frac{80}{21} \left( 1 - \frac{t_0}{t} \right) \right]

3. 组合结构函数矩: n=2n=2 矩为 M22(t)=fNS2(t)+e2fΣ2(t)M_2^2(t) = f_{NS}^2(t) + \langle e^2 \rangle f_\Sigma^2(t),其中平均电荷平方 e2=10/94=518\langle e^2 \rangle = \frac{10/9}{4} = \frac{5}{18}。代入并合并系数: M22(Q2)=α8πlogQ2Λ2[200321(1(t0t)10775)+2000024759(1(t0t)13175)+200189(1t0t)]\boxed{ M_2^2(Q^2) = \frac{\alpha}{8\pi} \log\frac{Q^2}{\Lambda^2} \left[ \frac{200}{321} \left( 1 - \left(\frac{t_0}{t}\right)^{\frac{107}{75}} \right) + \frac{20000}{24759} \left( 1 - \left(\frac{t_0}{t}\right)^{\frac{131}{75}} \right) + \frac{200}{189} \left( 1 - \frac{t_0}{t} \right) \right] } (注:其中 t=log(Q2/Λ2)t = \log(Q^2/\Lambda^2)t0=log(Q02/Λ2)2.408t_0 = \log(Q_0^2/\Lambda^2) \approx 2.408)


(d) 光子结构函数的定性演化描述

  1. Q2Q^2 的演化:与强子结构函数在领头阶近似下满足标度无关性(仅有对数微扰修正)不同,光子结构函数 F2γ(x,Q2)F_2^\gamma(x, Q^2) 的整体幅度随 Q2Q^2对数增长(即 F2γαlog(Q2/Λ2)F_2^\gamma \propto \alpha \log(Q^2/\Lambda^2))。这是因为点状的 QED 耦合 γqqˉ\gamma \to q\bar{q} 充当了一个持续不断产生大动量夸克的非齐次源项。
  2. xx 的分布:强子的部分子分布在 x1x \to 1 时迅速衰减(如 (1x)3(1-x)^3),而光子的 QED 源项正比于 x2+(1x)2x^2 + (1-x)^2,该项在 x=1x=1 处达到峰值。因此,光子结构函数在xx 区域显著且出现峰值
  3. QCD 辐射的软化效应:随着 Q2Q^2 增大,由光子在大 xx 处产生的高能夸克会通过辐射胶子(QCD 演化)向小 xx 区域迁移。这使得分布在小 xx 处逐渐抬升,大 xx 处的峰值相较于纯 QED 预测会有所软化,但整体上大 xx 处的峰值特征依然保留。

定性特征:F2γ(x,Q2) 随 Q2 呈对数增长,且在 x1 处具有峰值(受 QCD 软化影响略微展宽)。\boxed{ \text{定性特征:} F_2^\gamma(x, Q^2) \text{ 随 } Q^2 \text{ 呈对数增长,且在 } x \to 1 \text{ 处具有峰值(受 QCD 软化影响略微展宽)。} }