Properties (51)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
gptkb:physicist
|
| gptkbp:associated_with |
the no-hair theorem
|
| gptkbp:description |
rotating charged black holes
|
| gptkbp:established |
Roy_P._Kerr_and_Erwin_Schrödinger
|
| gptkbp:expansion |
in the limit of large distances
|
| gptkbp:has_a |
ring singularity
|
| gptkbp:has_implications_for |
cosmology
|
| gptkbp:hasEvents |
inner event horizon
outer event horizon |
| https://www.w3.org/2000/01/rdf-schema#label |
Kerr-Newman solution
|
| gptkbp:includes |
angular momentum parameter
electric charge parameter mass parameter |
| gptkbp:is_a |
black hole solution
|
| gptkbp:is_a_time_for |
charged rotating black holes
can be used to explore the role of black holes in galaxy formation can be used to explore the relationship between gravity and electromagnetism can be used to study particle dynamics near black holes can be used to study the thermodynamics of black holes can be extended to higher dimensions can be used to explore the nature of singularities has a non-trivial topology has implications for black hole evaporation preserves the symmetry of the spacetime can be used to study the interaction of matter with black holes can be used to study the dynamics of accretion disks around black holes can be used to analyze the stability of orbits around black holes can be used to investigate the cosmic censorship hypothesis can be used to investigate the nature of spacetime near black holes can be used to study the effects of charge on black hole properties can be used to investigate the role of black holes in the universe. can be used to study the effects of rotation on black hole properties Einstein-Maxwell_equations |
| gptkbp:is_characterized_by |
three parameters: mass, charge, and angular momentum
|
| gptkbp:is_essential_for |
theoretical physics
understanding rotating black holes |
| gptkbp:is_evaluated_by |
Boyle coordinates
|
| gptkbp:is_involved_in |
the_Einstein_equations_with_electromagnetic_fields
|
| gptkbp:is_studied_in |
general relativity
numerical relativity its stability properties Penrose_diagrams |
| gptkbp:is_used_in |
the study of gravitational lensing
astrophysical jets the study of black hole thermodynamics |
| gptkbp:isConnectedTo |
quantum_gravity_theories
|
| gptkbp:related_to |
astrophysics
gravitational wave astronomy the_Penrose_process |
| gptkbp:standardFeatures |
gptkb:Kerr_solution
gptkb:Reissner-Nordström_solution |