einstein

İngilizce - Türkçe

einstein teriminin İngilizce Türkçe sözlükte anlamı: {i} Einstein; (isim) Einstein
einstein diffusion equation: einstein yayınım eşitliği
einstein's law: einstein yasası
einstein's law of equivalents: einstein eşdeğerler yasası
einstein law of equivalents: (Fizik) einstein eşdeğerler yasası

Türkçe - Türkçe

einstein teriminin Türkçe Türkçe sözlükte anlamı
bose-einstein yoğunlaşması: Bozonlardan oluşan maddelerin mutlak sıfır sıcaklığına çok yakın değerlere kadar soğutulmasıyla ortaya çıkan maddenin bir hali. Bu süpersoğutulmuş maddede atomların büyük çoğunluğu en düşük kuantum durumlarına çöker ve böylece makroskopik skalada kuantum etkileri göstermeye başlar

İngilizce - İngilizce

einstein teriminin İngilizce İngilizce sözlükte anlamı: an extremely clever person
Can you believe he's just a kindergartener? It looks like they've got an Einstein in the family.; A surname; Albert Einstein, the world-famous 20th Century theoretical physicist who developed the theory of relativity
If Einstein, my dear / Were a toll booth cashier / I imagine he too would be.; One mole of photons, regardless of frequency, as used to measure irradiance; {i} family name; Albert Einstein (1879-1955) U.S. physicist (born in Germany), winner of the 1921 Nobel Prize in Physics, developer of the theory of relativity; brand name of a word processing program (Computers); A person who is considered to be very intelligent; Bose Einstein statistics Einstein's mass energy relation Einstein Albert; physicist born in Germany who formulated the special theory of relativity and the general theory of relativity; Einstein also proposed that light consists of discrete quantized bundles of energy (later called photons) (1879-1955); Albert Einstein (1879 - 1955) was a German-born, naturalized-American theoretical physicist who is famous for his theories of special and general relativity which related space, time, and motion He received the Nobel Prize in physics in 1921 for his explanation of the photoelectric effect In his most productive year in physics, 1905, he published his papers on the photoelectric effect, Brownian motion, and special relativity while discharging his duties as a Swiss Patent examiner in Berne He is the author of the most famous equation, E=mc2, which relates the quantities of mass and energy The theories of relativity explain the effects of the postulate that the speed of light appears to be the same when observed from any inertial reference frame, no matter what the speed of the observer He is considered the last of the three giants of the science of mechanics: Galileo, Newton, and Einstein; the amount of energy absorbed by one mole of material undergoing a photochemical reaction; physicist who came up with the Theory of Relativity and E=MC^2; someone who has exceptional intellectual ability and originality; "Mozart was a child genius"; "he's smart but he's no Einstein"; One mole of photons Although widely used, it is not an IUPAC sanctioned unit It is sometimes defined as the energy of one mole of photons This use is discouraged [IUPAC Photo]; incomprehensible
Einstein barrier: Also known as the light barrier, the speed of light viewed as an uncrossable barrier to acceleration from subluminal and superluminal speeds in special relativity
Tachyons exist on the other side of the Einstein barrier.
Einstein constant: Alternative form of Einstein's constant
Einstein field equation: A symmetric 4 x 4 tensor equation in general relativity in which the gravitational force is described as a curvature of spacetime caused by matter and energy
Einstein field equations: The Einstein field equation represented as a set of ten scalar equations
Einstein space: A Riemann space in which the contracted curvature tensor is proportional to the metric tensor
Einstein spaces: plural form of Einstein space
Einstein's constant: the coupling constant appearing in the Einstein field equation
Einstein-Rosen bridge: A type of wormhole, originally predicted by physicists Albert Einstein & Nathan Rosen, that is inherently unstable and collapses before any information or matter can pass through
Einstein theory: theory developed by Albert Einstein that all motion is relative
Einstein's law: equation developed by Albert Einstein which expresses the relation of mass and energy
Einstein's mass-energy relation: Relationship between mass (m) and energy (E) in Albert Einstein's special theory of relativity, expressed E = mc^2, where c equals 186,000 mi/second (300,000 km/second), the speed of light. Whereas mass and energy were viewed as distinct in earlier physical theories, in special relativity a body's mass can be converted into energy in accordance with Einstein's formula. Such a release of energy decreases the body's mass (see conservation law)
Bose-Einstein condensate: A gaseous superfluid phase of matter in which all the particles have the same quantum state
Albert Einstein: {i} (1879-1955) U.S. physicist (born in Germany), winner of the 1921 Nobel Prize in Physics, developer of the theory of relativity
Albert Einstein: a US physicist and mathematician, born in Germany, who developed the theory of relativity, which completely changed the way that scientists understand space and time. He was one of the greatest scientists ever born, and people sometimes use the name Einstein to talk about someone who is very intelligent (1879-1955). born March 14, 1879, Ulm, Württemberg, Ger. died April 18, 1955, Princeton, N.J., U.S. German-Swiss-U.S. scientist. Born to a Jewish family in Germany, he grew up in Munich, and his family moved to Switzerland in 1894. He became a junior examiner at the Swiss patent office in 1902 and began producing original theoretical work that laid many of the foundations for 20th-century physics. He received his doctorate from the University of Zürich in 1905, the same year he won international fame with the publication of three articles: one on Brownian motion, demonstrating the existence of molecules; one on the photoelectric effect, in which he demonstrated the particle nature of light; and one on his special theory of relativity, which included his formulation of the equivalence of mass and energy (E = mc^2). He held several professorships before becoming director of Berlin's Kaiser Wilhelm Institute in 1914. In 1915 he published his general theory of relativity, which was confirmed experimentally during a solar eclipse in 1919 with observations of the deviation of light passing near the Sun. He received a Nobel Prize in 1921 for his work on the photoelectric effect, his work on relativity still being controversial. He made important contributions to quantum field theory, and for decades he sought to discover the mathematical relationship between electromagnetism and gravitation, which he believed would be a first step toward discovering the common laws governing the behaviour of everything in the universe, but such a unified field theory eluded him. His theories of relativity and gravitation represented a profound advance over Newtonian physics and revolutionized scientific and philosophical inquiry. He resigned his position at the Prussian Academy when Adolf Hitler came to power and moved to Princeton, N.J., where he joined the Institute for Advanced Study. Though a longtime pacifist, he was instrumental in persuading Pres. Franklin Roosevelt in 1939 to initiate the Manhattan Project for the production of an atomic bomb, a technology his own theories greatly furthered, though he did not work on the project himself. The most eminent scientist in the world in the postwar years, he declined an offer to become the first prime minister of Israel and became a strong advocate for nuclear disarmament
Arik Einstein: {i} (born 1939) Israeli singer and songwriter
Bose-Einstein condensation: The physical process in which a Bose-Einstein condensate is formed
Bose-Einstein statistics: One of two possible ways (the other is Fermi-Dirac statistics) in which a collection of indistinguishable particles may occupy a set of available discrete energy states. The gathering of particles in the same state, which is characteristic of particles that obey Bose-Einstein statistics, accounts for the cohesive streaming of laser light and the frictionless creeping of superfluid helium (see superfluidity). The theory of this behaviour was developed in 1924-25 by Satyendra Nath Bose (1894-1974) and Albert Einstein. Bose-Einstein statistics apply only to those particles, called bosons, which have integer values of spin and so do not obey the Pauli exclusion principle
bose-einstein statistics: (physics) statistical law obeyed by a system of particles whose wave function is not changed when two particles are interchanged (the Pauli exclusion principle does not apply)