Buchdahl's theorem, named for Hans Adolf Buchdahl, is a result in general relativity that makes precise the idea that ordinary gravitating matter has a maximum sustainable density. For a static, spherically symmetric body of a given areal radius, the theorem gives an inequality the body's mass must satisfy under fairly general conditions, so a body that violated the bound couldn't exist as an ordinary static star. The bound, often called Buchdahl's bound, had already been noted by Karl Schwarzschild for the special case of a constant-density fluid, though it shouldn't be confused with the much smaller Schwarzschild radius.
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StatementFor static, spherically symmetric matter configurations under certain conditions, the mass must satisfy an inequality with the areal radius, Buchdahl's bound, expressing a maximal sustainable density for ordinary gravitating matter. 2 Classification
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Entity-backed identity for the statement-form enum value this theorem already carries, resolved to a mathematics concept by an explicit value-to-entity map (phase 3 bucket conversion, docs\design_entity_backed_browse_buckets_20260928.md). The statement-form fact itself stays on the theorem unchanged.
Sources
1. Wikipedia: Buchdahl's theorem
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In general relativity, Buchdahl's theorem, named after Hans Adolf Buchdahl, makes more precise the notion that there is a maximal sustainable density for ordinary gravitating matter.
View the Source 2. Buchdahl's theorem, Wikipedia
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It gives an inequality between the mass and radius that must be satisfied for static, spherically symmetric matter configurations under certain conditions.
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