Reissner-Nordström solution
GPTKB entity
Properties (47)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
gptkb:physicist
|
| gptkbp:associated_with |
electromagnetic fields
|
| gptkbp:can_be |
flat
charged particles in a gravitational field |
| gptkbp:description |
electrically charged black holes
|
| gptkbp:explores |
the nature of singularities
|
| gptkbp:has |
a charge parameter
a mass parameter a metric tensor two event horizons |
| https://www.w3.org/2000/01/rdf-schema#label |
Reissner-Nordström solution
|
| gptkbp:includes |
a singularity
|
| gptkbp:is_a |
static black hole solution
|
| gptkbp:is_a_subject_of |
modern physics
mathematical research black hole physics advanced physics courses |
| gptkbp:is_a_time_for |
charged black holes in vacuum
has implications for astrophysical observations. preserves spherical symmetry Einstein-Maxwell_equations |
| gptkbp:is_available_in |
a charged sphere in spacetime
|
| gptkbp:is_characterized_by |
mass and charge
|
| gptkbp:is_essential_for |
understanding black hole thermodynamics
theoretical models of the universe understanding gravitational collapse |
| gptkbp:is_evaluated_by |
spherical coordinates
|
| gptkbp:is_featured_in |
the effects of charge on black holes
|
| gptkbp:is_involved_in |
Kerr_solution_when_angular_momentum_is_zero
|
| gptkbp:is_part_of |
the broader study of general relativity
|
| gptkbp:is_studied_in |
general relativity
black hole evaporation the context of quantum gravity numerical relativity the stability of black holes |
| gptkbp:is_used_in |
theoretical physics
|
| gptkbp:isConnectedTo |
the study of gravitational waves
|
| gptkbp:isUsedFor |
Einstein's_equations_with_electromagnetic_stress-energy_tensor
|
| gptkbp:leads |
naked singularities
|
| gptkbp:previousName |
gptkb:Hermann_Reissner
Hans Nordström |
| gptkbp:related_to |
gptkb:Kerr-Newman_solution
cosmology astrophysics the concept of charge in general relativity theoretical predictions of black hole behavior |
| gptkbp:standardFeatures |
Schwarzschild solution
|