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        "quote": "在真空中，$T _ { \\mu \\nu }$，爱因斯坦场方程可写为$R _ { \\mu \\nu } = 0$，因此在$\\boxed { } h _ { \\mu \\nu } = 0$的线性近似下，这些解被称为<u class=\"concept-term\" data-concept-identity=\"urn:uuid:5118e748-bc6f-482a-ad9a-7a158a9252a9\" data-concept-route=\"/concept-identities#concept-5118e748-bc6f-482a-ad9a-7a158a9252a9\" id=\"first-f02f8026ddd0613c5fb4-zh\">引力波(gravitational wave)</u>（更多细节见<a href=\"#problem-18-20\" class=\"cross-reference\" id=\"xref-08-general-relativity-19\" data-reference=\"problem-18-20\">习题18.20</a>）。",
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        "quote": "In vacuo, $T _ { \\mu \\nu }$ , Einstein’s field equations can be written $R _ { \\mu \\nu } = 0$ , so that in the linearized approximation we have $\\boxed { } h _ { \\mu \\nu } = 0$ ; these solutions are known as <u class=\"concept-term\" data-concept-identity=\"urn:uuid:5118e748-bc6f-482a-ad9a-7a158a9252a9\" data-concept-route=\"/concept-identities#concept-5118e748-bc6f-482a-ad9a-7a158a9252a9\" id=\"first-02b75935ddb66fb28ef9-en\">gravitational waves</u> (see <a href=\"#problem-18-20\" class=\"cross-reference\" id=\"xref-08-general-relativity-21\" data-reference=\"problem-18-20\">Problem 18.20</a> for further details).",
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