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博客园 - 【当耐特】

菲兹克斯喵

Lesson 17 引力波的功率 (2) Lesson 16 引力波的功率 Lesson 8 Atmospheres Lesson 16 习题课 Lesson 15 引力波 Lesson 14 Noether 定理 Lesson 7 Evolution Lesson 7 传粉的力量 Lesson 13 配分函数的一些应用 Lesson 12 Penrose 过程与 Hawking 辐射 Lesson 6 Homology Lesson 11 带电荷和旋转的黑洞 Lesson 6 进食行为 Lesson 11 配分函数 Lesson 10 Penrose 图 Lesson 5 Diffusion Lesson 9 微观量与宏观量的联系 Lesson 5 捕食行为 Lesson 8 Schwarzschild 黑洞 Lesson 9 Schwarzschild 黑洞 (2) Lesson 8 近独立子体系分布 Lesson 4 Ignition of the Sun Lesson 7 统计力学绪论 Lesson 4 讲座:乌贼和章鱼的行为与智能 Lesson 7 Killing 矢量场和 Lie 导数 Lesson 6 Schwarzschild 解 Lesson 6 Landau 相变理论 (二) Lesson 3 Lane - Emden Equation Lesson 5 Landau 相变理论 Lesson 3 动物的感知 Lesson 5 Einstein 场方程 Lesson 4 协变的物理定律 Lesson 3 等效原理 & 广义协变性原理 Lesson 4 热力学第三定律 Lesson 2 Equation of State Lesson 3 热力学关系 Lesson 2 神经生物学基础 Lesson 2 度规和联络 Lesson 1 简介 Lesson 1 Lorentz 变换 Lesson 2 热力学定律 Lesson 1 Introduction & Light Lesson 1 介绍 流星监控项目 II - 树莓派配置 Lesson 15 Green 函数法 Lesson 29 散射 (二) Lesson 15 Spatial Patterns & Self-Organization Lesson 14 积分变换 Lesson 29 散射 Lesson 28 散射 (一) Lesson 27 绝热近似 Lesson 14 Dynamics of biological networks (2) Lesson 13 分离变量法总结 Lesson 26 变分法 (二) Lesson 14 Spatial Statistics Lesson 27 带电粒子和电磁场的相互作用 Lesson 13 磁性材料 & 拓扑绝缘体 Lesson 25 变分法 Lesson 13 Fast Radio Burst Lesson 13 Dynamics of biological networks Lesson 24 含时微扰 Lesson 26 相对论中的能量和动量守恒 Lesson 13 On the Intersection between Astronomy and AI Lesson 25 电磁场变换 Lesson 12 超导 Lesson 23 Zeeman Effect Lesson 12 absorbing Lesson 12 China Jingping Labs and Related Physics Lesson 24 狭义相对论的速度变换 Lesson 22 微扰论 Lesson 11 Bessel 函数 Lesson 12 Time Series Analysis Lesson 23 狭义相对论 Lesson 21 能带理论 Lesson 11 量子多体系统 Lesson 11 Molecular Motor (3) Tianwen:The Beauty of the Cosmos Lesson 10 连带 Legendre 函数 Lesson 20 多电子原子 & 固体 Lesson 11 Truncated & Censored Data Lesson 21 偶极辐射 (二) Lesson 10 离子阱量子计算 & 超快分子摄影 Lesson 10 Molecular Motor (2) Lesson 19 多粒子系统 Neutron Stars Lesson 20 偶极辐射 Lesson 9 Legendre 多项式 (二) Lesson 18 双粒子系统 Lesson 10 Clustering & Classification Lesson 19 辐射 (二) Lesson 9 引力波探测 & 原子量子计算 Lesson 17 CG 系数 「三次量子化」:宏观量子能级及其相干叠加态 —— 解读今年的 Nobel Prize Lesson 9 Molecular Motor Exoplanet Lesson 18 辐射 Lesson 16 自旋 (二) Lesson 8 Legendre 多项式 Lesson 17 波导 Lesson 9 Density Estimation
Lesson 13 作用量原理
2026-04-08 · via 菲兹克斯喵

作用量原理:我们的目的是测地线方程,

d2xμdτ2+Γμνλdxνdτdxλdτ=0\frac{\text{d}^2x^\mu}{\text{d}\tau^2}+\Gamma^\mu{}_{\nu\lambda}\frac{\text{d}x^\nu}{\text{d}\tau}\frac{\text{d}x^\lambda}{\text{d}\tau} = 0

粒子的作用量表达为

IM=−∑nmn∫−∞∞dp[−gμν(xn)dxnμdpdxnνdp]1/2I_M = -\sum_nm_n\int_{-\infty}^\infty\text{d}p\left[-g_{\mu\nu}(x_n)\frac{\text{d}x_n^\mu}{\text{d}p}\frac{\text{d}x_n^\nu}{\text{d}p}\right]^{1/2}

我们想通过其变分得到测地线方程,有

δIM=−∑nmn∫−∞∞dp⋅12[−gμν(xn)dxnμdpdxnνdp]−1/2{−∂gμν∂xnλδxnλdxnμdpdxnνdp−gμν(xn)(ddpδxnμddpxnν+ddpxnμddpδxnν)}=−∑nmn∫−∞∞dτ⋅12{−∂gμν∂xnλδxnλdxnμdpdxnνdp−gμν(xn)(ddpδxnμddpxnν+ddpxnμddpδxnν)}=⋯⋯\begin{aligned} \delta I_M &=-\sum_nm_n\int_{-\infty}^\infty\text{d}p\cdot\frac{1}{2}\left[-g_{\mu\nu}(x_n)\frac{\text{d}x_n^\mu}{\text{d}p}\frac{\text{d}x_n^\nu}{\text{d}p}\right]^{-1/2}\Big\{-\frac{\partial g_{\mu\nu}}{\partial x_n^\lambda}\delta x_n^\lambda\frac{\text{d}x_n^\mu}{\text{d}p}\frac{\text{d}x_n^\nu}{\text{d}p}\\\\ &\quad -g_{\mu\nu}(x_n)\left(\frac{\text{d}}{\text{d}p}\delta x_n^\mu\frac{\text{d}}{\text{d}p}x_n^\nu+\frac{\text{d}}{\text{d}p}x_n^\mu\frac{\text{d}}{\text{d}p}\delta x_n^\nu\right) \Big\}\\\\ &= -\sum_nm_n\int_{-\infty}^\infty\text{d}\tau\cdot\frac{1}{2}\Big\{-\frac{\partial g_{\mu\nu}}{\partial x_n^\lambda}\delta x_n^\lambda\frac{\text{d}x_n^\mu}{\text{d}p}\frac{\text{d}x_n^\nu}{\text{d}p}-g_{\mu\nu}(x_n)\left(\frac{\text{d}}{\text{d}p}\delta x_n^\mu\frac{\text{d}}{\text{d}p}x_n^\nu+\frac{\text{d}}{\text{d}p}x_n^\mu\frac{\text{d}}{\text{d}p}\delta x_n^\nu\right) \Big\}\\\\ &= \cdots\cdots \end{aligned}

后面过程略,但是最后会得到 Christoffel 符号的定义式.

对于一个带电的体系,上面的作用量加一项场的部分和一项电荷之间相互作用的部分. 其中场的部分是

−14∫d4x⋅g1/2(x)Fμν(x)Fμν(x)-\frac{1}{4}\int\text{d}^4x\cdot g^{1/2}(x)F_{\mu\nu}(x)F^{\mu\nu}(x)

这里的 g1/2g^{1/2} 来源于张量密度,d4x\text{d}^4x 不是普通标量.

为求电荷相互作用的项,首先写出狭义相对论下的流:

Jμ(x)=∑nendxnμdtδ3(x−xn(t))=∑nendxnμdτdτdtδ3(x−xn(t))J^\mu(x) = \sum_ne_n\frac{\text{d}x_n^\mu}{\text{d}t}\delta^3(x-x_n(t)) = \sum_ne_n\frac{\text{d}x_n^\mu}{\text{d}\tau}\frac{\text{d}\tau}{\text{d}t}\delta^3(x-x_n(t))

简单地把 33 改成 44 就是四维形式,但是并不广义相对论协变,因为 δ4\delta^4 并不是标量,还需要乘一个张量密度的系数,

Jμ(x)=∑nen∫dτ⋅g1/2(xn(τ))dxnμdτδ4(x−xn(τ))J^\mu(x) = \sum_ne_n\int\text{d}\tau\cdot g^{1/2}(x_n(\tau))\frac{\text{d}x_n^\mu}{\text{d}\tau}\delta^4(x-x_n(\tau))

由流,得到粒子之间的电磁相互作用,

∫d4x⋅g1/2(x)Aμ(x)Jμ(x)=∫dτ∫d4x∑nδ4(x−xn(τ))Aμ(x)endxnμdτ=∑nen∫−∞∞dpdxnμ(p)dpAμ(xn(p))\begin{aligned} &\int\text{d}^4x\cdot g^{1/2}(x)A_\mu(x)J^\mu(x)\\\\ =&\int\text{d}\tau\int\text{d}^4x\sum_n\delta^4(x-x_n(\tau))A_\mu(x)e_n\frac{\text{d}x_n^\mu}{\text{d}\tau}\\\\ =&\sum_ne_n\int_{-\infty}^\infty\text{d}p\frac{\text{d}x_n^\mu(p)}{\text{d}p}A_\mu(x_n(p)) \end{aligned}

相对于之前无电荷的作用量,这里多了两项:

IM=−∑nmn∫−∞∞dp[−gμν(xn)dxnμdpdxnνdp]1/2−14∫d4x⋅g1/2(x)Fμν(x)Fμν(x)−∑nen∫−∞∞dpdxnμ(p)dpAμ(xn(p))\begin{aligned} I_M &=-\sum_nm_n\int_{-\infty}^\infty\text{d}p\left[-g_{\mu\nu}(x_n)\frac{\text{d}x_n^\mu}{\text{d}p}\frac{\text{d}x_n^\nu}{\text{d}p}\right]^{1/2}-\frac{1}{4}\int\text{d}^4x\cdot g^{1/2}(x)F_{\mu\nu}(x)F^{\mu\nu}(x)\\\\ &\quad -\sum_ne_n\int_{-\infty}^\infty\text{d}p\frac{\text{d}x_n^\mu(p)}{\text{d}p}A_\mu(x_n(p)) \end{aligned}

变分后,第一项和第三项都有 xnμx_n^\mu,对于第一项变分之后得到测地线方程,下面考虑对第三项变分,

δI3=∑n∫−∞∞dp⋅[dδxnμdpAμ(xn(p))+dxnμdp∂Aμ∂xν∣x=xn(p)δxnμ(p)]=∑nen∫−∞∞dp(−Fμνdxnμdp)δxν+boundary terms\begin{aligned} \delta I_3 &= \sum_n\int_{-\infty}^\infty\text{d}p\cdot\left[\frac{\text{d}\delta x_n^\mu}{\text{d}p} A_\mu(x_n(p))+\frac{\text{d}x_n^\mu}{\text{d}p}\left.\frac{\partial A_\mu}{\partial x^\nu}\right|_{x=x_n(p)}\delta x_n^\mu(p)\right]\\\\ &= \sum_ne_n\int_{-\infty}^\infty\text{d}p\left(-F_{\mu\nu}\frac{\text{d}x_n^\mu}{\text{d}p}\right)\delta x^\nu+\text{boundary terms} \end{aligned}

这里的第一项可以通过 integral by part,

dδxnμdpAμ(xn(p))⟶−δxnμ∂Aμ∂xν∣x=xn(p)dxnν(p)dp\frac{\text{d}\delta x_n^\mu}{\text{d}p}A_\mu(x_n(p))\longrightarrow -\delta x_n^\mu\left.\frac{\partial A_\mu}{\partial x^\nu}\right|_{x=x_n(p)}\frac{\text{d}x_n^\nu(p)}{\text{d}p}

电磁场部分,

δIA=∫d4xg(−14FμνFμν)\begin{aligned} \delta I_A &= \int\text{d}^4x\sqrt{g}\left(-\frac{1}{4}F_{\mu\nu}F^{\mu\nu}\right) \end{aligned}

其中后面 Fμν=∂μAν−∂νAμF^{\mu\nu}=\partial^\mu A^\nu-\partial^\nu A^\mu,是反对称的,所以可以写成 2∂μAν2\partial^\mu A^\nu. 之后对这个 AνA^\nu 做变分,

δIA=∫d4xg(−1)(∂μAν−∂νAμ)∂μδAν=∫d4xgFμν;ν\delta I_A = \int\text{d}^4x\sqrt{g}(-1)(\partial_\mu A_\nu-\partial_\nu A_\mu)\partial^\mu\delta A^\nu = \int\text{d}^4x\sqrt{g} F_{\mu\nu}{}^{;\nu}


下面用作用量原理推导场方程.

场的相互作用是 local 的,因为没有长程关联,也就没有双重的积分. 取一个标量的作用量,

IG=−116πG∫d4x⋅g1/2RI_G = -\frac{1}{16\pi G}\int\text{d}^4x\cdot g^{1/2} R

变分,

δ(g1/2R)=δ(g1/2gμνRμν)=δgμνg1/2Rμν+δg1/2R+g1/2gμνδRμν\begin{aligned} \delta\left(g^{1/2}R\right) &= \delta\left(g^{1/2}g^{\mu\nu}R_{\mu\nu}\right)\\\\ &= \delta g^{\mu\nu}g^{1/2}R_{\mu\nu}+\delta g^{1/2}R+g^{1/2}g^{\mu\nu}\delta R_{\mu\nu} \end{aligned}

最难处理的是最后这一项,因为根本不知道 RR 是什么. 但是我们知道 RμνR_{\mu\nu} 没缩并之前是由 Γ\Gamma 构成的,而且 δΓ\delta\Gamma 是 tensor (因为使得 Γ\Gamma 不是 tensor 的那一项变分的时候没有了). 因此

δRμν=something’s derivative\delta R_{\mu\nu} = \text{something's derivative}

这一项的贡献是

∫d4xg⋅DμJ~μ\int\text{d}^4x\sqrt{g}\cdot D_\mu \tilde J^\mu

由 Stokes 可以化为面积分,将面积趋于无穷大,此式得零. 因此这一项对运动方程没有贡献.

接下来处理第一项,

gνρgρσ=δμσ⟹δgμρgρσ+gμρδgρσ=0g_{\nu\rho}g^{\rho\sigma} = \delta_\mu{}^\sigma \Longrightarrow \delta g_{\mu\rho}g^{\rho\sigma}+g_{\mu\rho}\delta g^{\rho\sigma} = 0

所以 δgρσ=−gρμδgμνgνσ\delta g^{\rho\sigma}=-g^{\rho\mu}\delta g_{\mu\nu}g^{\nu\sigma}. 第二项是 δg1/2=12g1/2gμνδgμν\delta g^{1/2}=\displaystyle{\frac{1}{2}}g^{1/2}g^{\mu\nu}\delta g_{\mu\nu}. 最终得到

δIG=−116πG∫d4x(−Rρσ+12gρσR)g1/2δgρσ\delta I_G = -\frac{1}{16\pi G}\int\text{d}^4x\left(-R^{\rho\sigma}+\frac{1}{2}g^{\rho\sigma}R\right)g^{1/2}\delta g_{\rho\sigma}

这个变分要和物质场的变分合在一起等于零. 如果场方程要正确,那么物质场对 gρσg_{\rho\sigma} 变分必须得是能动张量. 这听起来很奇怪,不过这件事是正确的. 我们以一群粒子为例,

IM=−∑nmn∫−∞∞dp(−gμνdxnμdpdxnνdp)1/2I_M = -\sum_n m_n\int_{-\infty}^\infty\text{d}p\left(-g_{\mu\nu}\frac{\text{d}x_n^\mu}{\text{d}p}\frac{\text{d}x_n^\nu}{\text{d}p}\right)^{1/2}

gμνg_{\mu\nu} 变分,

δIM=−∑nmn∫−∞∞dp⋅12(−gμνdxnμdpdxnνdp)−1/2(−dxnμdpdxnνdpδgμν(xn))=∑nmn∫−∞∞dp⋅12dxnμdτdxnνdτδgμν(xn)=∫d4xg(x)∑nmn∫−∞∞dτ⋅12dxnμdτdxnνdτ⋅g(x)δ4(x−xn(τ))δgμν(x)\begin{aligned} \delta I_M &= -\sum_nm_n\int_{-\infty}^\infty\text{d}p\cdot\frac{1}{2}\left(-g_{\mu\nu}\frac{\text{d}x_n^\mu}{\text{d}p}\frac{\text{d}x_n^\nu}{\text{d}p}\right)^{-1/2}\left(-\frac{\text{d}x_n^\mu}{\text{d}p}\frac{\text{d}x_n^\nu}{\text{d}p}\delta g_{\mu\nu}(x_n)\right)\\\\ &=\sum_nm_n\int_{-\infty}^\infty\text{d}p\cdot\frac{1}{2}\frac{\text{d}x_n^\mu}{\text{d}\tau}\frac{\text{d}x_n^\nu}{\text{d}\tau}\delta g_{\mu\nu}(x_n)\\\\ &= \int\text{d}^4x\sqrt{g(x)}\sum_nm_n\int_{-\infty}^\infty\text{d}\tau\cdot\frac{1}{2}\frac{\text{d}x_n^\mu}{\text{d}\tau}\frac{\text{d}x_n^\nu}{\text{d}\tau}\cdot\sqrt{g(x)}\delta^4(x-x_n(\tau))\delta g_{\mu\nu}(x) \end{aligned}

而这个体系的能动张量是

Tμν(x)=∫dτ∑nmndxnμdτdxnνdτg1/2(x)δ4(x−xn(τ))T^{\mu\nu}(x) = \int\text{d}\tau\sum_nm_n\frac{\text{d}x_n^\mu}{\text{d}\tau}\frac{\text{d}x_n^\nu}{\text{d}\tau} g^{1/2}(x)\delta^4(x-x_n(\tau))

验证了结果.

提示

现在来思考一下为什么这件事情是对的.

S=∫dt⋅L(q,q˙)S = \int\text{d}t\cdot L(q,\dot{q})

的变分是

δS=∫t1t2(δLδqδq+δLδq˙δq˙)dt+L(q(t2),q˙(t2))Δt−L(q(t1),q˙(t1))‾δS2=∫t1t2[(δLδqδq−ddtδLδq˙)‾0−ddt(δLδq˙δq)]+δS2=δLδq˙δq∣t1t2+δS2=[−δLδq˙q˙+L(q(t),q˙(t))]t1t2=0\begin{aligned} \delta S &= \int_{t_1}^{t_2}\left(\frac{\delta L}{\delta q}\delta q+\frac{\delta L}{\delta \dot{q}}\delta\dot{q}\right)\text{d}t +\underset{\delta S_2}{\underline{L(q(t_2),\dot{q}(t_2))\Delta t-L(q(t_1),\dot{q}(t_1))}}\\\\ &= \int_{t_1}^{t_2}\left[\underset{0}{\underline{\left(\frac{\delta L}{\delta q}\delta q - \frac{\text{d}}{\text{d}t}\frac{\delta L}{\delta \dot{q}}\right)}}-\frac{\text{d}}{\text{d}t}\left(\frac{\delta L}{\delta \dot{q}}\delta q\right)\right]+\delta S_2\\\\ &= \left.\frac{\delta L}{\delta\dot{q}}\delta q\right|^{t_2}_{t_1}+\delta S_2\\\\ &= \left[-\frac{\delta L}{\delta \dot{q}}\dot{q}+L(q(t),\dot{q}(t))\right]^{t_2}_{t_1} = 0 \end{aligned}