Triple
T12177249
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Tolman–Oppenheimer–Volkoff equation |
E290118
|
entity |
| Predicate | relatedTo |
P37
|
FINISHED |
| Object |
Buchdahl bound
The Buchdahl bound is a theoretical limit in general relativity that constrains how compact a stable, spherically symmetric star can be before collapsing into a black hole.
|
E966303
|
NE FINISHED |
Provenance (5 batches)
| Stage | Batch ID | Job type | Status |
|---|---|---|---|
| creating | batch_69d6ab4d6c00819095a9a7c35de83cfb |
elicitation | completed |
| NER | batch_69d915fa6ff08190a1ddb3606c229cad |
ner | completed |
| NED1 | batch_69f5f6ab19288190a882c842d74a2e30 |
ned_source_triple | completed |
| NED2 | batch_69f601ef0a9c8190ac922562a8856def |
ned_description | completed |
| NEDg | batch_69f600b7385881909ddb86a1d39ff5d4 |
nedg | completed |
Created at: April 8, 2026, 9:50 p.m.