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| In [[Kaluza–Klein theory]], a unification of [[general relativity]] and [[electromagnetism]], the five-fimensional Kaluza–Klein–Riemann curvature tensor (or Kaluza–Klein–Riemann–Christoffel curvature tensor) is the generalization of the four-dimensional [[Riemann curvature tensor]] (or Riemann–Christoffel curvature tensor).
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| The [[Ising model]] is a prototypical model in [[statistical physics]]. The model consists of discrete variables that represent magnetic dipole moments of atomic "spins" that can be in one of two states (+1 or −1). The spins are arranged in a graph, usually a lattice (where the local structure repeats periodically in all directions), allowing each spin to interact with its neighbors.
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| The 1859 City of Adelaide colonial by-election was held on 13 May 1859 to elect one of six members for [[Electoral district of City of Adelaide|City of Adelaide]] in the [[South Australian House of Assembly]], after sitting member [[William Henville Burford]] resigned on 29 April 1859.
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| In [[differential geometry]] and in particular [[Yang–Mills theory]], Uhlenbeck's singularity theorem is a result allowing the removal of a [[Singularity (mathematics)|singularity]] of a [[Four-dimensional Yang–Mills theory|four-dimensional Yang–Mills]] field with finite energy using gauge. It states as a consequence that Yang–Mills fields with finite energy on flat [[euclidean space]] arise from Yang–Mills fields on the curved [[sphere]], its [[one-point compactification]].
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| [[Quaternion Lorentz Transformations]] <small>(Linear transformation of spacetime coordinates)</small>▼
| In [[special relativity]], a [[Lorentz transformation]] is a real [[linear transformation]] of the [[spacetime coordinates]] t, x, y, z that preserves the Minkowski invariant or [[spacetime interval]] <math display="block">c^2 \, t^2-x^2-y^2-z^2</math> Using the 4x4 [[metric tensor]] <math>\eta</math>, this is▼
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| data-sort-value=496 | [[Special:Contribs/DonaldWP|DonaldWP]] (496)▼
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| data-sort-value=66 | [[Special:Contribs/PikutaMe|PikutaMe]] (66)
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| [[Ian Smith (civil engineer)]] <small>(Canadian and Swiss civil engineer)</small>
| Ian F. C. Smith is a Canadian and Swiss [[civil engineer]]. He is Emeritus Professor at the [[École Polytechnique Fédérale de Lausanne]] (EPFL) in Switzerland and was the founding director of the [[Nemetschek#Georg_Nemetschek_Institute_-_Artificial_Intelligence_for_the_Built_World|TUM Georg Nemetschek Institute Artificial Intelligence for the Built World]] at the [[Technical University of Munich]] in Germany.
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| data-sort-value=18 | [[Special:Contribs/Ronal tarim|Ronal tarim]] (18)
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| [[Silvano Donati]] <small>(Italian physicist in the field of photonics)</small>
| Silvano Donati (born 19 August 1942) is a physicist in the field of [[photonics]]. He is an emeritus professor at the [[University of Pavia]] where he has been Full Professor for 30 years and created the Electro-Optical Engineering Group.
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| data-sort-value=35 | [[Special:Contribs/Fratilias|Fratilias]] (35)
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| Dora Reisser (born February 1942) is a former British actress and fashion designer.
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| Dmitry Volkov ({{langx|uk|Дмитро Васильович Волков}}; 3 July 1925 – 5 January 1996) — physicist. [[Doctor of Philosophy|PhD]] in 1956. Doctor of Physical and Mathematical Sciences ([[Habilitation]]) in 1968. Professor (1977). [[Academician]] of [[National Academy of Sciences of Ukraine]] (1988).
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| ''Amouna'' (Arabic: أمونة), or alternatively known as Amouna al Mazyouna (Arabic: أمونة المزيونة) is an Emirati children's animated series created by Amer Kokh. It premiered on 25 September 2015 and aired on [[:ar:قناة_ماجد_للأطفال|Majid Kids TV]]. the series about Amouna is going on a adventure with her brother, Ali and Seif.▼
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▲| data-sort-value=58 | [[Special:Contribs/RobinHarrisonfan2008|RobinHarrisonfan2008]] (58)
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| Stephen (Geoffrey) Lipson (born 8 January 1941) is an Israeli-British physicist. He is Emeritus Professor of Physics at [[Technion]].
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| In [[optics]], the Herschel's condition is a condition for an [[optical system]] to produce sharp images for objects over an extended axial range, i.e. for objects displaced along the optical axis. It was formulated by [[John Herschel]].▼
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| Thomas L. Gilbert (November 24, 1922 – May 19, 2016) was an American physicist, a specialist in statistical physics.
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▲| ''Amouna'' (Arabic: أمونة), or alternatively known as Amouna al Mazyouna (Arabic: أمونة المزيونة) is an Emirati children's animated series created by Amer Kokh. It premiered on 25 September 2015 and aired on [[:ar:قناة_ماجد_للأطفال|Majid Kids TV]]. the series about Amouna is going on a adventure with her brother, Ali and Seif.
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| Shaofan Li is a Chinese-American professor of applied and [[computational mechanics]] in the Department of [[Civil and Environmental Engineering]] at the [[University of California, Berkeley]].
▲| In [[optics]], the Herschel's condition is a condition for an [[optical system]] to produce sharp images for objects over an extended axial range, i.e. for objects displaced along the optical axis. It was formulated by [[John Herschel]].
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| [[Yang–Mills moduli space]] <small>(Moduli space of the Yang–Mills equations)</small>
| In [[gauge theory]], the Yang–Mills moduli space (short YM moduli space, also instanton moduli space) is the [[moduli space]] of the [[Yang–Mills equations]], hence the space of its solutions up to [[gauge]]. It is used in [[Donaldson's theorem]], proven in and improved in , which was listed as a contribution for [[Simon Donaldson]] winning the [[Fields Medal]] in 1986, and to defined the [[Donaldson invariant|Donaldson invariants]] used to study four-dimensional smooth manifolds (short 4-manifolds).
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| data-sort-value=3289 | [[Special:Contribs/Samuel Adrian Antz|Samuel Adrian Antz]] (3289)
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▲| 2025-07-07
▲| [[Quaternion Lorentz Transformations]] <small>(Linear transformation of spacetime coordinates)</small>
▲| In [[special relativity]], a [[Lorentz transformation]] is a real [[linear transformation]] of the [[spacetime coordinates]] t, x, y, z that preserves the Minkowski invariant or [[spacetime interval]] <math display="block">c^2 \, t^2-x^2-y^2-z^2</math> Using the 4x4 [[metric tensor]] <math>\eta</math>, this is
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▲| data-sort-value=496 | [[Special:Contribs/DonaldWP|DonaldWP]] (496)
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| 2025-08-12
| [[Plunging region]] <small>(Region just outside event horizons)</small>
| In [[astrophysics]], a plunging region is a region near a [[black hole]] in which [[matter]] can no longer follow [[circular orbits]] and will instead rapidly "plunge" towards the [[event horizon]] at nearly the [[speed of light]]. This region exists between the [[innermost stable circular orbit]] and the event horizon of the black hole.
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| data-sort-value=988 | [[Special:Contribs/Shocksingularity|Shocksingularity]] (988)
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<span style="font-style: italic; font-size: 85%;">Last updated by [[User:SDZeroBot|SDZeroBot]] <sup>''[[User:SD0001|operator]] / [[User talk:SD0001|talk]]''</sup> at 13:
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