quasicompact surface - définition. Qu'est-ce que quasicompact surface
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Qu'est-ce (qui) est quasicompact surface - définition

KIND OF LARGE CARDINAL NUMBER
Quasicompact cardinal

Surface finish         
  • How a profilometer works
  • 500px
  • Examples of various lay patterns
SMALL, LOCAL DEVIATIONS OF A SURFACE FROM A PERFECTLY FLAT IDEAL; DEFINED BY THE THREE CHARACTERISTICS OF LAY, SURFACE ROUGHNESS, AND WAVINESS
Surface texture symbol; Surface texture; Surface topography
Surface finish, also known as surface texture or surface topography, is the nature of a surface as defined by the three characteristics of lay, surface roughness, and waviness.. It comprises the small, local deviations of a surface from the perfectly flat ideal (a true plane).
Parametric surface         
  • 1= ''z'' = (''R'' + ''r'' cos ''v'') cos ''u''}}.
  • Parametric surface forming a [[trefoil knot]], equation details in the attached source code.
SURFACE IN THE EUCLIDEAN SPACE
Parametrized surface; Parametrised surface; Parametrized Surface; Surface parameterisation; Parametric object
A parametric surface is a surface in the Euclidean space \R^3 which is defined by a parametric equation with two parameters Parametric representation is a very general way to specify a surface, as well as implicit representation. Surfaces that occur in two of the main theorems of vector calculus, Stokes' theorem and the divergence theorem, are frequently given in a parametric form.
Planetary surface         
  • surface]] of the [[Moon]], which consists of [[lunar regolith]] (photographed by [[Neil Armstrong]], July 1969).
  • Perseverance]] rover.
  • Perspective radar view of Titan's [[Bolsena Lacus]] (lower right) and other northern hemisphere hydrocarbon lakes
  • access-date=24 July 2015 }}</ref>
  • Full-sized image]])''
  • Sand dunes in the [[Namib Desert]] on Earth (top), compared with dunes in Belet on Titan
WHERE THE SOLID (OR LIQUID) MATERIAL OF THE OUTER CRUST ON CERTAIN TYPES OF ASTRONOMICAL OBJECTS CONTACTS THE ATMOSPHERE OR OUTER SPACE
Planet surface; Surface (astronomy); Surfacism; Surface chauvinism
A planetary surface is where the solid or liquid material of certain types of astronomical objects contacts the atmosphere or outer space. Planetary surfaces are found on solid objects of planetary mass, including terrestrial planets (including Earth), dwarf planets, natural satellites, planetesimals and many other small Solar System bodies (SSSBs).

Wikipédia

Subcompact cardinal

In mathematics, a subcompact cardinal is a certain kind of large cardinal number.

A cardinal number κ is subcompact if and only if for every A ⊂ H(κ+) there is a non-trivial elementary embedding j:(H(μ+), B) → (H(κ+), A) (where H(κ+) is the set of all sets of cardinality hereditarily less than κ+) with critical point μ and j(μ) = κ.

Analogously, κ is a quasicompact cardinal if and only if for every A ⊂ H(κ+) there is a non-trivial elementary embedding j:(H(κ+), A) → (H(μ+), B) with critical point κ and j(κ) = μ.

H(λ) consists of all sets whose transitive closure has cardinality less than λ.

Every quasicompact cardinal is subcompact. Quasicompactness is a strengthening of subcompactness in that it projects large cardinal properties upwards. The relationship is analogous to that of extendible versus supercompact cardinals. Quasicompactness may be viewed as a strengthened or "boldface" version of 1-extendibility. Existence of subcompact cardinals implies existence of many 1-extendible cardinals, and hence many superstrong cardinals. Existence of a 2κ-supercompact cardinal κ implies existence of many quasicompact cardinals.

Subcompact cardinals are noteworthy as the least large cardinals implying a failure of the square principle. If κ is subcompact, then the square principle fails at κ. Canonical inner models at the level of subcompact cardinals satisfy the square principle at all but subcompact cardinals. (Existence of such models has not yet been proved, but in any case the square principle can be forced for weaker cardinals.)

Quasicompactness is one of the strongest large cardinal properties that can be witnessed by current inner models that do not use long extenders. For current inner models, the elementary embeddings included are determined by their effect on P(κ) (as computed at the stage the embedding is included), where κ is the critical point. This prevents them from witnessing even a κ+ strongly compact cardinal κ.

Subcompact and quasicompact cardinals were defined by Ronald Jensen.