Fermi brim — Fermio riba statusas T sritis fizika atitikmenys: angl. Fermi brim; Fermi limit vok. Fermi Grenze, f rus. граница Ферми, f pranc. seuil de Fermi, m … Fizikos terminų žodynas
Fermi-Grenze — Fermio riba statusas T sritis fizika atitikmenys: angl. Fermi brim; Fermi limit vok. Fermi Grenze, f rus. граница Ферми, f pranc. seuil de Fermi, m … Fizikos terminų žodynas
Fermi liquid — is a generic term for a quantum mechanical liquid of fermions that arises under certain physical conditions when the temperature is sufficiently low. The interaction between the particles of the many body system does not need to be small (see e.g … Wikipedia
Fermi paradox — The Fermi paradox is the apparent contradiction between high estimates of the probability of the existence of extraterrestrial civilizations and the lack of evidence for, or contact with, such civilizations.The extreme age of the universe and its … Wikipedia
Fermi–Dirac statistics — Statistical mechanics Thermodynamics · … Wikipedia
Fermi's golden rule — In quantum physics, Fermi s golden rule is a way to calculate the transition rate (probability of transition per unit time) from one energy eigenstate of a quantum system into a continuum of energy eigenstates, due to a perturbation. We consider… … Wikipedia
Fermi–Pasta–Ulam problem — In physics, the Fermi–Pasta–Ulam problem or FPU problem was the apparent paradox in chaos theory that many complicated enough physical systems exhibited almost exactly periodic behavior instead of ergodic behavior. One of the resolutions of the… … Wikipedia
seuil de Fermi — Fermio riba statusas T sritis fizika atitikmenys: angl. Fermi brim; Fermi limit vok. Fermi Grenze, f rus. граница Ферми, f pranc. seuil de Fermi, m … Fizikos terminų žodynas
Chandrasekhar limit — When a star starts running out of fuel, it usually cools off and collapses (possibly with a supernova) into one of three compact forms, depending on its total mass: a White Dwarf, a big lump of Carbon and Oxygen atoms, almost like one huge… … Wikipedia
Greisen–Zatsepin–Kuzmin limit — The Greisen–Zatsepin–Kuzmin limit (GZK limit) is a theoretical upper limit on the energy of cosmic rays (high energy charged particles from space) coming from distant sources. The limit is 5×1019 eV, or about 8 joules. The limit is set by slowing … Wikipedia