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Surname list
Reissner, also Reißner, is a German surname. Notable people with the surname include: Eric Reissner (1913–1996), German-American civil engineer, mathematician
Reissner
Exact solution in general relativity
In physics and astronomy, the Reissner–Nordström metric is a static solution to the Einstein–Maxwell field equations that corresponds to the gravitational
Reissner–Nordström_metric
Russian writer and revolutionary (1895–1926)
Larissa Mikhailovna Reissner (Russian: Лариса Михайловна Рейснер; 13 May [O.S. 1 May] 1895 – 9 February 1926) was a Russian writer and revolutionary. She
Larissa_Reissner
Baltic German anatomist (1824–1878)
Ernst Reissner (German: [ˈʁaɪsnɐ]; 24 September 1824 – 16 September 1878) was a Baltic German anatomist from Riga, Livonia. In 1851 he received his medical
Ernst_Reissner
German engineer and mathematician (1874–1967)
Hans Jacob Reissner, also known as Jacob Johannes Reissner (18 January 1874, Berlin – 2 October 1967, Mt. Angel, Oregon), was a German aeronautical engineer
Hans_Reissner
Theory used to calculate the deformations and stresses in plates
The Reissner–Mindlin theory of plates is an extension of Kirchhoff–Love plate theory that takes into account shear deformations through the thickness of
Reissner–Mindlin_plate_theory
German cyclist (born 2000)
Charlotte Reißner". ProCyclingStats. Retrieved 29 January 2024. "Lena Charlotte Reissner". UCI.org. Retrieved 29 January 2024. Lena Charlotte Reißner at UCI
Lena_Charlotte_Reißner
Spinal fiber
Reissner's fiber (named after Ernst Reissner) is a fibrous aggregation of secreted molecules extending from the subcommissural organ (SCO) through the
Reissner's_fiber
German-American mathematician
Max Erich (Eric) Reissner (January 5, 1913 – November 1, 1996) was a German-American civil engineer and mathematician, and Professor of Mathematics at
Eric_Reissner
German-born theoretical physicist (1879–1955)
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Albert_Einstein
Class of solutions to Einstein's field equation
family solutions, namely the Schwarzschild, nonextremal Reissner–Nordström and extremal Reissner–Nordström metrics, can be identified as Weyl-type metrics
Weyl_metrics
Maximum-security state prison for male prisoners, located in New York, US
develop a college-degree granting program. Under the leadership of Dr. Anne Reissner, Hudson Link for Higher Education in Prison was founded to restore college
Sullivan Correctional Facility
Sullivan_Correctional_Facility
Attraction of masses and energy
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Gravity
Mathematical model of the stresses within flat plates under loading
These are the Kirchhoff–Love theory of plates (classical plate theory) The Reissner–Mindlin theory of plates (first-order shear plate theory) The Kirchhoff–Love
Plate_theory
Membrane in the cochlea in the inner ear
The vestibular membrane, vestibular wall or Reissner's membrane is a membrane inside the cochlea of the inner ear. It separates the cochlear duct from
Vestibular_membrane
Black hole with electric charge
charge will be formed in nature. The two types of charged black holes are Reissner–Nordström black holes (without spin), and Kerr–Newman black holes (with
Charged_black_hole
Lower energy limit in string theory
spacetime, is simply M {\displaystyle M} for the Reissner-Nordström solution. The event horizon(s) of the Reissner-Nordström black hole are located at the radial
Bogomol'nyi–Prasad–Sommerfield bound
Bogomol'nyi–Prasad–Sommerfield_bound
Compact astronomical body
Schwarzschild black hole. Non-rotating charged black holes are described by the Reissner–Nordström metric, while the Kerr metric describes a non-charged rotating
Black_hole
Condition in which spacetime itself breaks down
values. Similarly, disappearing event horizons can also be seen with the Reissner–Nordström geometry of a charged black hole if the charge ( Q {\displaystyle
Gravitational_singularity
Hypothetical topological feature of spacetime
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Wormhole
1997 British television film
Reed Deborah Findlay as Mrs. Reed Kay Mellor as Mrs. Butterworth Sophie Reissner as Bertha Rochester "Jane Eyre (1997)". Radio Times. Retrieved 15 March
Jane_Eyre_(1997_film)
General-relativistic effect
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Gravitational_time_dilation
Region in spacetime from which nothing can escape
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Event_horizon
Null hypersurface in general relativity
Augustin-Louis Cauchy. The simplest example is the internal horizon of a Reissner–Nordström black hole. Under the averaged weak energy condition (AWEC),
Cauchy_horizon
Hypothetical quantum cosmological effect
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Hawking_radiation
Capital and largest city of Germany
Berlin Rising: Biography of a City. W.W. Norton. ISBN 978-0-393-03606-0. Reissner, Alexander (1984). Berlin 1675-1945: The Rise and Fall of a Metropolis
Berlin
Origins of Einstein's gravitation theory
symmetric charged object was discovered by Reissner and later rediscovered by Nordström, and is called the Reissner–Nordström solution. The black hole aspect
History_of_general_relativity
Theory of gravitation as curved spacetime
to electrically charged objects were taken, eventually resulting in the Reissner–Nordström solution, which is associated with electrically charged black
General_relativity
Physics concept expressed as E = mc²
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Mass–energy_equivalence
Field-equations in general relativity
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Einstein_field_equations
German mystic, hymn-writer and poet
Adam Reusner, also Reissner or Reißner (c. 1496 – 1575 (some claim 1572 or 1582)) in Mindelheim), was a German mystic, hymn-writer and poet. Reusner studied
Adam_Reusner
Class of solutions to Einstein's equation in general relativity
coordinates [ ρ , z , ϕ ] {\displaystyle [\rho ,z,\phi ]} . The extremal Reissner–Nordström spacetime is a typical conformastatic solution. In this case
Conformastatic_spacetimes
1903 novel by Wilhelm Jensen
Helen M. Downey Language German Genre Romance, novella Publisher Carl Reissner (Germany) Moffat, Yard & Co. (U.S.) George Allen & Unwin (U.K.) Publication date
Gradiva_(novel)
Statement of spherically symmetric spacetimes
geometry of a spherically symmetric charged star must be given by the Reissner–Nordström electrovacuum. In the Einstein-Maxwell theory, there exist spherically
Birkhoff's theorem (relativity)
Birkhoff's_theorem_(relativity)
Hypothetical object of spacetime
it contains. In the case of a black hole possessing an electric charge (Reissner-Nordström black hole) or an angular momentum (Kerr black hole), then the
White_hole
Theorem in general relativity
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Goldberg–Sachs_theorem
Exact solution for the Einstein field equations
corresponding solution for a charged, spherical, non-rotating body, the Reissner–Nordström metric, was discovered soon afterwards (1916–1918). However,
Kerr_metric
Two interrelated physics theories by Albert Einstein
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Theory_of_relativity
Equations in physical cosmology
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Friedmann_equations
a source of gravity, that is with mass 1910 — Hans Reissner and Gunnar Nordström define Reissner–Nordström singularity, Hermann Weyl solves special case
Timeline of black hole physics
Timeline_of_black_hole_physics
German military leader (1473–1528)
Adam Reißner, who was for a time Frundsberg's secretary and as such, witness to many of the events he described. Reinhard Baummann opines that Reißner did
Georg_von_Frundsberg
Polish revolutionary (1885–1939)
Comintern policy. However, the terminal illness of Radek's lover, Larissa Reissner, saw Radek lose his inhibitions and he began publicly criticising Stalin
Karl_Radek
Exact solution to the Einstein field equations
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Oppenheimer–Snyder_model
Raychaudhuri (Raychaudhuri equation), Tullio Regge (Regge calculus), Hans Reissner (Reissner–Nordström metric), Wolfgang Rindler (Rindler chart for Minkowski vacuum)
List of contributors to general relativity
List_of_contributors_to_general_relativity
Aspect of general relativity
nearly identical to those predicted by Newton's theory of gravity. The Reissner–Nordström solution, which analyzes a non-rotating spherically symmetric
Solutions of the Einstein field equations
Solutions_of_the_Einstein_field_equations
Key results in general relativity on gravitational singularities
types of black hole interiors, such as the Cauchy horizon of a charged (Reissner–Nordström) or rotating (Kerr) black hole. A singularity can be either strong
Penrose–Hawking singularity theorems
Penrose–Hawking_singularity_theorems
1984 graduate textbook by Robert M. Wald
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
General_Relativity_(book)
Classification used in differential geometry and general relativity
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Petrov_classification
Deformation of slabs under load
h . {\displaystyle w=w^{K}+{\frac {{\mathcal {M}}^{K}}{\kappa Gh}}\,.} Reissner-Stein theory for cantilever plates leads to the following coupled ordinary
Bending_of_plates
Equation in which all expressions are tensors
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Manifest_covariance
Strain caused by an external load
Kirchhoff–Love theory of plates (also called classical plate theory) the Mindlin–Reissner plate theory (also called the first-order shear theory of plates) The assumptions
Bending
Swiss astronomer (1898–1974)
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Fritz_Zwicky
Theory in physics
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Relativistic_chaos
Borras Marie Le Net 4:06.987 6 Germany Franziska Brauße Lena Charlotte Reißner Lisa Klein Mieke Kröger 4:08.349 Seventh place final 7 Australia Alexandra
Cycling at the 2024 Summer Olympics – Women's team pursuit
Cycling_at_the_2024_Summer_Olympics_–_Women's_team_pursuit
German aviation pioneer (1859–1935)
began in earnest at age 50 when he worked with engineer Hans Reissner in Aachen. Reissner had developed an all-metal aircraft, on which work first started
Hugo_Junkers
Concept in general relativity
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Einstein–Hilbert_action
Path of an object through spacetime
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
World_line
Tensor field in Riemannian geometry
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Riemann_curvature_tensor
American theoretical physicist (1911–2008)
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
John_Archibald_Wheeler
Solution of Einstein field equations
cases. It reduces to the Kerr metric as the charge Q goes to zero; the Reissner–Nordström metric as the angular momentum J (or a = J/M) goes to zero; the
Kerr–Newman_metric
English mathematical biologist
Institutions University of Bristol Thesis Stability of the inner horizon of the Reissner-Nordstrõm and Kerr black hole models (1977) Doctoral advisor Roger Penrose
John McNamara (mathematical biologist)
John_McNamara_(mathematical_biologist)
Hypothetical FTL transportation by warping space
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Alcubierre_drive
Physics principle that simultaneity depends on choice of reference frame
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Relativity_of_simultaneity
1915 experimental aircraft
having received details of the concept of heavier-than-air travel from Hans Reissner, a colleague and fellow professor at the Technische Hochschule in Aachen
Junkers_J_1
Finnish physicist (1881–1923)
solution was also found by Hans Reissner, Hermann Weyl and George Barker Jeffery, and it is nowadays known as the Reissner–Nordström metric. Nordström maintained
Gunnar_Nordström
Soviet cultural and artistic organization
84,000 (1920) Key people Anatoly Lunacharsky Alexander Bogdanov Larissa Reissner Fedor Kalinin Pavel Lebedev-Polianskii Valerian Pletnev Platon Kerzhentsev
Proletkult
Conjecture in physics
spacetime is perhaps the "superextremal" M < | Q | {\displaystyle M<|Q|} Reissner–Nordström solution, which contains a singularity at r = 0 {\displaystyle
Cosmic_censorship_hypothesis
Light bending by mass between source and observer
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Gravitational_lens
Approximate solution to Einstein's field equations
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Hartle–Thorne_metric
Trace radiation from the early universe
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Cosmic_microwave_background
Mathematical model combining space and time
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Spacetime
Cavity in the cochlea of the inner ear
duct, separated by the basilar membrane and the vestibular membrane (Reissner's membrane) respectively. The cochlear duct houses the organ of Corti. The
Cochlear_duct
Equation explaining structure of a spherical body of isotropic material
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Tolman–Oppenheimer–Volkoff equation
Tolman–Oppenheimer–Volkoff_equation
Football club
Halverkamps 30 DF GER Jella Veit 31 MF POL Tanja Pawollek 40 GK GER Sherly Schulz 41 MF SUI Lia Kamber 42 MF AUT Naika Reissner 77 FW BEL Jill Janssens
1._FC_Union_Berlin_(women)
Type of horizon in spacetime
Ergosphere Killing horizon Naked singularity Particle horizon Photon sphere Reissner–Nordström solution Schwarzschild metric Hawking, S. W. & Ellis, G. F. R
Absolute_horizon
Description of gravity using discrete values
Ruben (2022). "Quantum gravitational corrections to the entropy of a Reissner-Nordström black hole". Eur. Phys. J. C. 82 (3) 272. arXiv:2201.08293. Bibcode:2022EPJC
Quantum_gravity
condense to form a filamentous structure named Reissner's fiber. The subcommissural organ/Reissner's fiber complex is thought to be involved in the reabsorption
Subcommissural_organ
Hypothetical mechanism for extracting energy from rotating black holes
Holographic principle No-hair theorem Metrics Schwarzschild (Derivation) Kerr Reissner–Nordström Kerr–Newman Hayward Alternatives Nonsingular black hole models
Penrose_process
Spanish mechanical engineer
Colegio de Ingenieros de Caminos". CICCP. Retrieved 2025-01-10. "Eric Reissner Medal". International Association for Computational Mechanics. Retrieved
Eugenio_Oñate
Solution of Einstein field equations
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Kerr–Newman–de–Sitter_metric
Solution to Einstein field equations
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Gravitational_plane_wave
American mathematician and computer scientist
Solution of the Differential Equations of Conical Shells (advisor Eric Reissner). He taught at MIT from 1954 to 1958. McIlroy joined Bell Laboratories
Douglas_McIlroy
2019 video game
Developer Limbic Entertainment Publisher Kalypso Media Designers Andreas Reißner Knut Arnold Marcus Cool Leonard Tetzlaff Writers Chris Bateman Richard
Tropico_6
General relativity equation
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Mathisson–Papapetrou–Dixon equations
Mathisson–Papapetrou–Dixon_equations
Diagram of different points in spacetime
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Penrose_diagram
Physical phenomenon in electromagnetic field theory
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
Relativistic_electromagnetism
Name list
Brazilian judoka Larissa Queiroz (born 1984), Brazilian actress Larissa Reissner (1895–1926), Russian writer and revolutionary Larissa Riquelme (born 1985)
Larissa_(given_name)
Measured time difference as explained by relativity theory
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Time_dilation
Hamiltonian formulation of general relativity
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
ADM_formalism
Null singularity inside black holes
was first described in 2012 by Donald Marolf and Amos Ori for classical Reissner-Nordström and Kerr black holes. It was numerically confirmed for the spherical
Shock_singularity
more metrics were created to describe other kinds of black holes: the Reissner-Nordstrom metric, describing charged, nonspinning black holes, the Kerr
History_of_black_hole_physics
Solution to the Einstein field equations
-(r_{\text{s}}/(2r^{3}))c^{2}L} . Derivation of the Schwarzschild solution Reissner–Nordström metric (charged, non-rotating solution) Kerr metric (uncharged
Schwarzschild_metric
Government ministry of Austria
Command): Generalleutnant / Lieutenant General (3 Star General) Franz Reißner Stellvertretender Kommandant (Deputy Commander): Generalmajor / Major General
Ministry_of_Defence_(Austria)
Debate about credit for general relativity
Spherical: Schwarzschild (interior Tolman–Oppenheimer–Volkoff equation) Reissner–Nordström Axisymmetric: Kerr (Kerr–Newman) Weyl−Lewis−Papapetrou Taub–NUT
General relativity priority dispute
General_relativity_priority_dispute
Near-horizon limit of the global metric of a black hole
{\displaystyle r} is fixed in the near-horizon limit. The metric of extremal Reissner–Nordström black hole is d s 2 = − ( 1 − M r ) 2 d t 2 + ( 1 − M r ) − 2
Near-horizon_metric
Deviation from Kepler's third law
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Gravitomagnetic_clock_effect
Russian-American aviation pioneer (1889–1972)
Milton C. Shaw 1986: Orlan W. Boston 1987: Philip G. Hodge 1988: Eric Reissner 1989: William R. Sears 1990: Harley A. Wilhelm 1992: Daniel C. Drucker
Igor_Sikorsky
American engineer (1926–2022)
Milton C. Shaw 1986: Orlan W. Boston 1987: Philip G. Hodge 1988: Eric Reissner 1989: William R. Sears 1990: Harley A. Wilhelm 1992: Daniel C. Drucker
H._Norman_Abramson
Constant of motion in the Kerr-Newman spacetime
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Carter_constant
Tensor describing energy momentum density in spacetime
Quantum field theory in curved spacetime Solutions Schwarzschild (interior) Reissner–Nordström Einstein–Rosen waves Wormhole Gödel Kerr Kerr–Newman Kerr–Newman–de
Stress–energy_tensor
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