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quasinilpotent element - traduction vers russe
Quasinilpotent operator; Quasinilpotent
quasinilpotent element
математика
квазинильпотентный элемент
set membership
ANY ONE OF THE DISTINCT OBJECTS THAT MAKE UP A SET IN SET THEORY
Element (math); Element (set theory); ∈; ∉; Element (set); Set membership; ∋; Set element; Element (statistics); In (set); Element (group theory); Membership (set theory); ∊; ∍; ∌; Belongs to; Membership relation; Element of; /in
математика
принадлежность множеству
chemical element
![[[Dmitri Mendeleev]]](https://commons.wikimedia.org/wiki/Special:FilePath/DIMendeleevCab.jpg?width=200 "[[Dmitri Mendeleev]]")
![[[Henry Moseley]]](https://commons.wikimedia.org/wiki/Special:FilePath/Henry Moseley.jpg?width=200 "[[Henry Moseley]]")
![[[Mendeleev]]'s 1869 [[periodic table]]: ''An experiment on a system of elements. Based on their atomic weights and chemical similarities.''](https://commons.wikimedia.org/wiki/Special:FilePath/Mendeleev's 1869 periodic table.svg?width=200 "[[Mendeleev]]'s 1869 [[periodic table]]: ''An experiment on a system of elements. Based on their atomic weights and chemical similarities.''")
![Periodic table showing the cosmogenic origin of each element in the Big Bang, or in large or small stars. Small stars can produce certain elements up to sulfur, by the [[alpha process]]. Supernovae are needed to produce "heavy" elements (those beyond iron and nickel) rapidly by neutron buildup, in the [[r-process]]. Certain large stars slowly produce other elements heavier than iron, in the [[s-process]]; these may then be blown into space in the off-gassing of [[planetary nebulae]]](https://commons.wikimedia.org/wiki/Special:FilePath/Nucleosynthesis periodic table.svg?width=200 "Periodic table showing the cosmogenic origin of each element in the Big Bang, or in large or small stars. Small stars can produce certain elements up to sulfur, by the [[alpha process]]. Supernovae are needed to produce \"heavy\" elements (those beyond iron and nickel) rapidly by neutron buildup, in the [[r-process]]. Certain large stars slowly produce other elements heavier than iron, in the [[s-process]]; these may then be blown into space in the off-gassing of [[planetary nebulae]]")
, black and white.png?width=200 "link=Periodic table")
![Abundances of the chemical elements in the Solar System. Hydrogen and helium are most common, from the Big Bang. The next three elements (Li, Be, B) are rare because they are poorly synthesized in the Big Bang and also in stars. The two general trends in the remaining stellar-produced elements are: (1) an alternation of abundance in elements as they have even or odd atomic numbers (the [[Oddo-Harkins rule]]), and (2) a general decrease in abundance as elements become heavier. Iron is especially common because it represents the minimum energy nuclide that can be made by fusion of helium in supernovae.](https://commons.wikimedia.org/wiki/Special:FilePath/SolarSystemAbundances.png?width=200 "Abundances of the chemical elements in the Solar System. Hydrogen and helium are most common, from the Big Bang. The next three elements (Li, Be, B) are rare because they are poorly synthesized in the Big Bang and also in stars. The two general trends in the remaining stellar-produced elements are: (1) an alternation of abundance in elements as they have even or odd atomic numbers (the [[Oddo-Harkins rule]]), and (2) a general decrease in abundance as elements become heavier. Iron is especially common because it represents the minimum energy nuclide that can be made by fusion of helium in supernovae.")
SPECIES OF ATOMS HAVING THE SAME NUMBER OF PROTONS IN THE ATOMIC NUCLEUS AND THE SAME CHEMICAL PROPERTIES, BUT NOT NESSARILY THE SAME MASS, OR THE SAME STABILITY (OR HALF-LIFETIME IF THEY ARE UNSTABLE)
Elemental substance; Chemical Elements; Pure element; Chemical elements; Chemical Element; Element (chemistry); Molecular and atomic elements; Chemical element name; Nutritional chemical elements; Physical Elements; History of chemical elements; Light element; Naturally occurring element; Elementary substance
химический элемент
Définition
transposon
[trans'p??z?n, tr?:ns-, -nz-]
¦ noun Genetics a segment of DNA that can be translocated as a whole from a site in one genome to another site in the same genome or to a different genome.
Origin
1970s: from transposition + -on.
Wikipédia
Nilpotent operator
In operator theory, a bounded operator T on a Hilbert space is said to be nilpotent if Tn = 0 for some n. It is said to be quasinilpotent or topologically nilpotent if its spectrum σ(T) = {0}.
