classical no-hair conjecture
GPTKB entity
Statements (16)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
gptkb:physical_phenomenon
gptkb:conjecture |
| gptkbp:alternativeName |
gptkb:no-hair_theorem
|
| gptkbp:appliesTo |
astrophysical black holes
|
| gptkbp:contrastsWith |
gptkb:hairy_black_holes
|
| gptkbp:field |
gptkb:general_relativity
|
| gptkbp:implies |
black holes have no other observable features
|
| gptkbp:proposedBy |
gptkb:Werner_Israel
gptkb:Stephen_Hawking gptkb:Brandon_Carter |
| gptkbp:relatedTo |
gptkb:black_hole
|
| gptkbp:state |
black holes are characterized only by mass, charge, and angular momentum
|
| gptkbp:yearProposed |
1970s
|
| gptkbp:bfsParent |
gptkb:hairy_black_holes
|
| gptkbp:bfsLayer |
8
|
| https://www.w3.org/2000/01/rdf-schema#label |
classical no-hair conjecture
|