如何证明真空引力平面波的极化张量具有横向性——郑大培教材公式推导疑问
我刚好对郑大培教授这本《相对论与引力》里的线性引力波推导很熟悉,帮你理清楚怎么用洛伦兹规范条件搞定那个让人头疼的迹项$h$,推导出公式(13.28):
首先明确教材里的符号定义,避免混淆:
- 线性近似下的度规:$g_{\mu\nu} = \eta_{\mu\nu} + h_{\mu\nu}$,其中$\eta_{\mu\nu}$是闵氏度规,$h_{\mu\nu}$是小幅度度规扰动
- 迹项:$h = \eta^{\mu\nu}h_{\mu\nu}$(也就是扰动度规的迹)
- 洛伦兹规范条件(13.18):$\partial^\mu h_{\mu\nu} - \frac{1}{2}\partial_\nu h = 0$,可以简化为 $\partial^\mu h_{\mu\nu} = \frac{1}{2}\partial_\nu h$
1. 写出线性化的里奇张量
教材里给出的线性化里奇张量表达式是:
$$R_{\mu\nu} = \frac{1}{2}\left(\partial_\mu\partial^\rho h_{\rho\nu} + \partial_\nu\partial^\rho h_{\rho\mu} - \partial_\mu\partial_\nu h - \square h_{\mu\nu}\right)$$
这里$\square = \eta^{\mu\nu}\partial_\mu\partial_\nu$是闵氏时空下的达朗贝尔算符。
2. 用洛伦兹规范消去交叉项
现在看里奇张量里的前两项$\partial_\mu\partial^\rho h_{\rho\nu}$和$\partial_\nu\partial^\rho h_{\rho\mu}$,这就是迹项$h$影响的地方——但我们可以直接用洛伦兹规范条件替换:
- 对于$\partial_\mu\partial^\rho h_{\rho\nu}$,根据规范条件$\partial^\rho h_{\rho\nu} = \frac{1}{2}\partial_\nu h$,代入后得到:
$$\partial_\mu\partial^\rho h_{\rho\nu} = \partial_\mu\left(\frac{1}{2}\partial_\nu h\right) = \frac{1}{2}\partial_\mu\partial_\nu h$$ - 同理,$\partial_\nu\partial^\rho h_{\rho\mu} = \frac{1}{2}\partial_\nu\partial_\mu h = \frac{1}{2}\partial_\mu\partial_\nu h$(偏导数的顺序可以交换)
把这两个结果代回里奇张量:
$$R_{\mu\nu} = \frac{1}{2}\left(\frac{1}{2}\partial_\mu\partial_\nu h + \frac{1}{2}\partial_\mu\partial_\nu h - \partial_\mu\partial_\nu h - \square h_{\mu\nu}\right)$$
括号里前两项相加等于$\partial_\mu\partial_\nu h$,再减去第三项$\partial_\mu\partial_\nu h$,直接抵消了!剩下的部分就非常简洁:
$$R_{\mu\nu} = -\frac{1}{2}\square h_{\mu\nu}$$
3. 计算里奇标量并代入爱因斯坦张量
接下来计算里奇标量$R = \eta^{\mu\nu}R_{\mu\nu}$,同样用洛伦兹规范简化:
$$R = \eta{\mu\nu}\cdot\frac{1}{2}\left(\partial_\mu\partial\rho h_{\rho\nu} + \partial_\nu\partial^\rho h_{\rho\mu} - \partial_\mu\partial_\nu h - \square h_{\mu\nu}\right)$$
对前两项求和时,利用规范条件$\partial^\rho h_{\rho\mu} = \frac{1}{2}\partial_\mu h$,可以得到:
$$\eta{\mu\nu}\partial_\mu\partial\rho h_{\rho\nu} = \partial\rho\partial\mu h_{\rho\mu} = \partial^\rho\left(\frac{1}{2}\partial_\rho h\right) = \frac{1}{2}\square h$$
所以里奇标量最终简化为:
$$R = \frac{1}{2}\square h - \square h = -\frac{1}{2}\square h$$
然后代入爱因斯坦张量的定义$G_{\mu\nu} = R_{\mu\nu} - \frac{1}{2}\eta_{\mu\nu}R$:
$$G_{\mu\nu} = -\frac{1}{2}\square h_{\mu\nu} - \frac{1}{2}\eta_{\mu\nu}\left(-\frac{1}{2}\square h\right) = -\frac{1}{2}\square\left(h_{\mu\nu} - \frac{1}{2}\eta_{\mu\nu}h\right)$$
这里注意教材里定义的迹反转扰动$\bar{h}{\mu\nu} = h{\mu\nu} - \frac{1}{2}\eta_{\mu\nu}h$,把它代入后,爱因斯坦张量就变成:
$$G_{\mu\nu} = -\frac{1}{2}\square \bar{h}_{\mu\nu}$$
4. 结合爱因斯坦场方程得到公式(13.28)
最后结合爱因斯坦场方程$G_{\mu\nu} = \frac{8\pi G}{c^4}T_{\mu\nu}$,两边同时乘以-2,就得到了教材里的公式(13.28):
$$\square \bar{h}{\mu\nu} = -\frac{16\pi G}{c^4}T{\mu\nu}$$
小结:迹项$h$的处理技巧
洛伦兹规范条件的核心就是把$\partial^\mu h_{\mu\nu}$和$\partial_\nu h$绑定,让里奇张量里包含$h$的交叉偏导项直接抵消,最后通过迹反转扰动把$h$的影响整合到$\bar{h}_{\mu\nu}$中,彻底摆脱单独处理迹项的麻烦。
内容的提问来源于stack exchange,提问作者Keith

