## Einstern 3 - opinion you

Geben Sie Ihre Mobiltelefonnummer ein, um die kostenfreie App zu beziehen. Einstern - Zu allen Ausgaben: Bitte melden Sie sich an, um Produkte in Ihre Merkliste hinzuzufügen. Themenhefte und Kartonbeilagen Jutta Maurach Häftad. Ihr Warenkorb ist leer. Vi använder cookies för att förbättra din upplevelse av bokus. Die Themenhefte sind ideal für den jahrgangsübergreifenden und jahrgangsgemischten Unterricht.This argument is called the equivalence principle. In the same article, Einstein also predicted the phenomena of gravitational time dilation , gravitational red shift and deflection of light.

In , Einstein published another article "On the Influence of Gravitation on the Propagation of Light" expanding on the article, in which he estimated the amount of deflection of light by massive bodies.

Thus, the theoretical prediction of general relativity could for the first time be tested experimentally. In , Einstein predicted gravitational waves , [] [] ripples in the curvature of spacetime which propagate as waves , traveling outward from the source, transporting energy as gravitational radiation.

The existence of gravitational waves is possible under general relativity due to its Lorentz invariance which brings the concept of a finite speed of propagation of the physical interactions of gravity with it.

By contrast, gravitational waves cannot exist in the Newtonian theory of gravitation , which postulates that the physical interactions of gravity propagate at infinite speed.

While developing general relativity, Einstein became confused about the gauge invariance in the theory. He formulated an argument that led him to conclude that a general relativistic field theory is impossible.

He gave up looking for fully generally covariant tensor equations, and searched for equations that would be invariant under general linear transformations only.

In June , the Entwurf "draft" theory was the result of these investigations. As its name suggests, it was a sketch of a theory, less elegant and more difficult than general relativity, with the equations of motion supplemented by additional gauge fixing conditions.

After more than two years of intensive work, Einstein realized that the hole argument was mistaken [] and abandoned the theory in November In , Einstein applied the general theory of relativity to the structure of the universe as a whole.

As observational evidence for a dynamic universe was not known at the time, Einstein introduced a new term, the cosmological constant , to the field equations, in order to allow the theory to predict a static universe.

Following the discovery of the recession of the nebulae by Edwin Hubble in , Einstein abandoned his static model of the universe, and proposed two dynamic models of the cosmos, The Friedmann-Einstein universe of [] [] and the Einstein—de Sitter universe of In many Einstein biographies, it is claimed that Einstein referred to the cosmological constant in later years as his "biggest blunder".

The astrophysicist Mario Livio has recently cast doubt on this claim, suggesting that it may be exaggerated. For the density to remain constant, new particles of matter must be continually formed in the volume from space.

It thus appears that Einstein considered a steady-state model of the expanding universe many years before Hoyle, Bondi and Gold.

General relativity includes a dynamical spacetime, so it is difficult to see how to identify the conserved energy and momentum.

Einstein argued that this is true for fundamental reasons, because the gravitational field could be made to vanish by a choice of coordinates. He maintained that the non-covariant energy momentum pseudotensor was in fact the best description of the energy momentum distribution in a gravitational field.

This approach has been echoed by Lev Landau and Evgeny Lifshitz , and others, and has become standard. In , Einstein collaborated with Nathan Rosen to produce a model of a wormhole , often called Einstein—Rosen bridges.

These solutions cut and pasted Schwarzschild black holes to make a bridge between two patches. If one end of a wormhole was positively charged, the other end would be negatively charged.

These properties led Einstein to believe that pairs of particles and antiparticles could be described in this way. In order to incorporate spinning point particles into general relativity, the affine connection needed to be generalized to include an antisymmetric part, called the torsion.

This modification was made by Einstein and Cartan in the s. The theory of general relativity has a fundamental law—the Einstein equations which describe how space curves, the geodesic equation which describes how particles move may be derived from the Einstein equations.

Since the equations of general relativity are non-linear, a lump of energy made out of pure gravitational fields, like a black hole, would move on a trajectory which is determined by the Einstein equations themselves, not by a new law.

So Einstein proposed that the path of a singular solution, like a black hole, would be determined to be a geodesic from general relativity itself.

This was established by Einstein, Infeld, and Hoffmann for pointlike objects without angular momentum, and by Roy Kerr for spinning objects.

In a paper, [] Einstein postulated that light itself consists of localized particles quanta. He does not say much more, because he is not sure how the particles are related to the wave.

But he does suggest that this idea would explain certain experimental results, notably the photoelectric effect. In , Einstein proposed a model of matter where each atom in a lattice structure is an independent harmonic oscillator.

In the Einstein model, each atom oscillates independently—a series of equally spaced quantized states for each oscillator. Einstein was aware that getting the frequency of the actual oscillations would be difficult, but he nevertheless proposed this theory because it was a particularly clear demonstration that quantum mechanics could solve the specific heat problem in classical mechanics.

Peter Debye refined this model. Throughout the s, quantum mechanics expanded in scope to cover many different systems.

After Ernest Rutherford discovered the nucleus and proposed that electrons orbit like planets, Niels Bohr was able to show that the same quantum mechanical postulates introduced by Planck and developed by Einstein would explain the discrete motion of electrons in atoms, and the periodic table of the elements.

Einstein contributed to these developments by linking them with the arguments Wilhelm Wien had made. Wien had shown that the hypothesis of adiabatic invariance of a thermal equilibrium state allows all the blackbody curves at different temperature to be derived from one another by a simple shifting process.

Einstein noted in that the same adiabatic principle shows that the quantity which is quantized in any mechanical motion must be an adiabatic invariant.

Arnold Sommerfeld identified this adiabatic invariant as the action variable of classical mechanics. In , Einstein received a description of a statistical model from Indian physicist Satyendra Nath Bose , based on a counting method that assumed that light could be understood as a gas of indistinguishable particles.

Einstein also published his own articles describing the model and its implications, among them the Bose—Einstein condensate phenomenon that some particulates should appear at very low temperatures.

Although the patent office promoted Einstein to Technical Examiner Second Class in , he had not given up on academia.

In , he became a Privatdozent at the University of Bern. This paper introduced the photon concept although the name photon was introduced later by Gilbert N.

Lewis in and inspired the notion of wave—particle duality in quantum mechanics. Einstein saw this wave—particle duality in radiation as concrete evidence for his conviction that physics needed a new, unified foundation.

In a series of works completed from to , Planck reformulated his quantum theory and introduced the idea of zero-point energy in his "second quantum theory".

Soon, this idea attracted the attention of Einstein and his assistant Otto Stern. Assuming the energy of rotating diatomic molecules contains zero-point energy, they then compared the theoretical specific heat of hydrogen gas with the experimental data.

The numbers matched nicely. However, after publishing the findings, they promptly withdrew their support, because they no longer had confidence in the correctness of the idea of zero-point energy.

In , at the height of his work on relativity, Einstein published an article in Physikalische Zeitschrift that proposed the possibility of stimulated emission , the physical process that makes possible the maser and the laser.

This paper was enormously influential in the later development of quantum mechanics, because it was the first paper to show that the statistics of atomic transitions had simple laws.

In another major paper from this era, Einstein gave a wave equation for de Broglie waves , which Einstein suggested was the Hamilton—Jacobi equation of mechanics.

Einstein was displeased with modern quantum mechanics as it had evolved after Contrary to popular belief, his doubts were not due to a conviction that God "is not playing at dice.

Einstein believed that a physical reality exists independent of our ability to observe it. In contrast, Bohr and his followers maintained that all we can know are the results of measurements and observations, and that it makes no sense to speculate about an ultimate reality that exists beyond our perceptions.

The Bohr—Einstein debates were a series of public disputes about quantum mechanics between Einstein and Niels Bohr , who were two of its founders.

Their debates are remembered because of their importance to the philosophy of science. In , Einstein returned quantum mechanics, in particular to the question of its completeness, in the "EPR paper".

No matter how far the two particles were separated, a precise position measurement on one particle would result in equally precise knowledge of the position of the other particle; likewise a precise momentum measurement of one particle would result in equally precise knowledge of the momentum of the other particle, without needing to disturb the other particle in any way.

Einstein rejected this second possibility popularly called "spooky action at a distance". Bell had delineated in The results of these and subsequent experiments demonstrate that quantum physics cannot be represented by any version of the picture of physics in which "particles are regarded as unconnected independent classical-like entities, each one being unable to communicate with the other after they have separated.

Although Einstein was wrong about local realism, his clear prediction of the unusual properties of its opposite, entangled quantum states , has resulted in the EPR paper becoming among the top ten papers published in Physical Review.

It is considered a centerpiece of the development of quantum information theory. Following his research on general relativity, Einstein entered into a series of attempts to generalize his geometric theory of gravitation to include electromagnetism as another aspect of a single entity.

In , he described his " unified field theory " in a Scientific American article titled "On the Generalized Theory of Gravitation".

In his pursuit of a unification of the fundamental forces, Einstein ignored some mainstream developments in physics, most notably the strong and weak nuclear forces , which were not well understood until many years after his death.

Einstein conducted other investigations that were unsuccessful and abandoned. These pertain to force , superconductivity , and other research.

In addition to longtime collaborators Leopold Infeld , Nathan Rosen , Peter Bergmann and others, Einstein also had some one-shot collaborations with various scientists.

Einstein and De Haas demonstrated that magnetization is due to the motion of electrons, nowadays known to be the spin.

In order to show this, they reversed the magnetization in an iron bar suspended on a torsion pendulum. This experiment needed to be sensitive, because the angular momentum associated with electrons is small, but it definitively established that electron motion of some kind is responsible for magnetization.

Then to each possible quantum motion of a particle in a box associate an independent harmonic oscillator. Quantizing these oscillators, each level will have an integer occupation number, which will be the number of particles in it.

This formulation is a form of second quantization , but it predates modern quantum mechanics. This absorption refrigerator was then revolutionary for having no moving parts and using only heat as an input.

Their invention was not immediately put into commercial production, and the most promising of their patents were acquired by the Swedish company Electrolux.

While traveling, Einstein wrote daily to his wife Elsa and adopted stepdaughters Margot and Ilse. The letters were included in the papers bequeathed to The Hebrew University.

Margot Einstein permitted the personal letters to be made available to the public, but requested that it not be done until twenty years after her death she died in [].

Einstein had expressed his interest in the plumbing profession and was made an honorary member of the Plumbers and Steamfitters Union. Corbis , successor to The Roger Richman Agency, licenses the use of his name and associated imagery, as agent for the university.

In the period before World War II, The New Yorker published a vignette in their "The Talk of the Town" feature saying that Einstein was so well known in America that he would be stopped on the street by people wanting him to explain "that theory".

He finally figured out a way to handle the incessant inquiries. He told his inquirers "Pardon me, sorry! Always I am mistaken for Professor Einstein.

Einstein has been the subject of or inspiration for many novels, films, plays, and works of music. Many popular quotations are often misattributed to him.

Einstein received numerous awards and honors and in he was awarded the Nobel Prize in Physics "for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect".

None of the nominations in met the criteria set by Alfred Nobel , so the prize was carried forward and awarded to Einstein in From Wikipedia, the free encyclopedia.

For other people, see Einstein surname. For other uses, see Albert Einstein disambiguation and Einstein disambiguation. German-born physicist and developer of the theory of relativity.

Princeton, New Jersey , US. Swiss Federal Polytechnic —; B. Annus Mirabilis papers , Photoelectric effect , Special theory of relativity , Mass—energy equivalence , and Brownian motion.

Statistical mechanics , thermal fluctuations , and statistical physics. History of special relativity. History of general relativity.

Equivalence principle , Theory of relativity , and Einstein field equations. Discovery of cosmic microwave background radiation. Religious interpretations of the Big Bang theory.

Classical unified field theories. Albert Einstein in popular culture. Einstein, Albert [Manuscript received: Written at Zurich, Switzerland.

Annalen der Physik Berlin in German. Hoboken, NJ published 14 March Einstein, Albert a [Manuscript received: Written at Berne, Switzerland.

Hoboken, NJ published 10 March Einstein, Albert b [Completed 30 April and submitted 20 July ]. Written at Berne, Switzerland, published by Wyss Buchdruckerei.

Einstein, Albert c [Manuscript received: Einstein, Albert d [Manuscript received: Annalen der Physik Berlin Submitted manuscript in German. Einstein, Albert e [Manuscript received: Einstein, Albert [Published 25 November ].

Physikalische Zeitschrift in German. Einstein, Albert [First published , in English ]. Nobel Lectures, Physics — in German and English.

Einstein, Albert [Published 10 July ]. First of a series of papers on this topic. Die Naturwissenschaften in German. Dover Publications published Physical Review Submitted manuscript.

Einstein, Albert 9 November On Science and Religion. Einstein, Albert; et al. The New York Times. Einstein, Albert May Monthly Review Foundation published May Archived from the original on 11 January Retrieved 16 January — via MonthlyReview.

Albert Einstein, Hedwig und Max Born: Briefwechsel — in German. Paul Arthur Schilpp Centennial ed. The chasing a light beam thought experiment is described on pages 48— Stachel, John ; Martin J.

Kox; Michel Janssen; R. Schulmann; Diana Komos Buchwald; et al. The Collected Papers of Albert Einstein. Further information about the volumes published so far can be found on the webpages of the Einstein Papers Project and on the Princeton University Press Einstein Page.

She has chosen the cream of her culture and has suppressed it. She has even turned upon her most glorious citizen, Albert Einstein, who is the supreme example of the selfless intellectual The man, who, beyond all others, approximates a citizen of the world, is without a home.

How proud we must be to offer him temporary shelter. Biographical Memoirs of Fellows of the Royal Society.

Longman Pronunciation Dictionary 3rd ed. Archived from the original on 6 March Retrieved 7 March Modern Atomic and Nuclear Physics.

Stanford Encyclopedia of Philosophy. Retrieved 11 July The accelerating universe" PDF. Retrieved 24 November Boyer; Melvyn Dubofsky Harper and Brothers Publishers Harper Torchbook edition.

His non-scientific works include: The Trustees of Princeton University. The Passions of a Scientist , Prometheus Books, p. The Golden Age of Physics.

Archived from the original PDF on 19 January Retrieved 19 October The Love Letters , , pp. A Biography , , pp. A Hundred Years of Relativity.

BZ Berner Zeitung in German. The Question of Time". Marcel Grossmann gewidmet Dedicated to my friend, Dr. Einstein Online in German and English.

Retrieved 17 August Retrieved 9 July Royal Netherlands Academy of Arts and Sciences. Retrieved 21 July Retrieved 13 June Banquet Speech by R.

Retrieved 9 December via Nobelprize. Memoria e Ricerca 2: French version PDF and English summary. The Journal of Ecclesiastical History. My Autobiography , Simon and Schuster, N.

How I See the World". Retrieved May 29, Einstein on Race and Racism. Institute for Advanced Study. Archived from the original on 29 March Retrieved 4 March Making the Atomic Bomb".

Department of Energy, History Division. Genius in the Shadows: The Man Behind The Bomb. Diehl, Sarah; Moltz, James Clay Nuclear Weapons and Nonproliferation: Pennsylvania State University Press.

Retrieved — via atomicarchive. Paul Robeson Speaks , Citadel p. Retrieved 31 March Johns Hopkins University Press. Archived from the original PDF on 28 August Einstein for the 21st Century: London, Macmillan Publishers Ltd.

Revised by Nicolas Slonimsky. New York, Schirmer Books, Sweezy, Paul; Huberman, Leo, eds. Retrieved 29 July The Hebrew University of Jerusalem ".

Archived from the original on 17 January Retrieved 24 January Albert Einstein Compiled by Miguel Chavez". Essential Readings for the Nonbeliever.

The Ultimate Quotable Einstein. Princeton University Press, p. The Expanded Quotable Einstein. His Life and Universe. Simon and Schuster, p.

Berkowitz, 25 October Oxford University Press, p. This results in a symmetry around the lens, causing a ring-like structure.

The size of an Einstein ring is given by the Einstein radius. In radians , it is. The bending of light by a gravitational body was predicted by Albert Einstein in , a few years before the publication of general relativity in Renn et al.

Of course, there is no hope of observing this phenomenon directly. First, we shall scarcely ever approach closely enough to such a central line.

However, Einstein was only considering the chance of observing Einstein rings produced by stars, which is low — the chance of observing those produced by larger lenses such as galaxies or black holes is higher since the angular size of an Einstein ring increases with the mass of the lens.

Hundreds of gravitational lenses are currently known. About half a dozen of them are partial Einstein rings with diameters up to an arcsecond , although as either the mass distribution of the lenses is not perfectly axially symmetrical , or the source, lens, and observer are not perfectly aligned, we have yet to see a perfect Einstein ring.

Most rings have been discovered in the radio range. The degree of completeness needed for an image seen through a gravitational lens to qualify as an Einstein ring is yet to be defined.

The first Einstein ring was discovered by Hewitt et al. This observation saw a quasar lensed by a nearer galaxy into two separate but very similar images of the same object, the images stretched round the lens into an almost complete ring.

As of this survey has found 85 confirmed gravitational lenses, there is not yet a number for how many show Einstein rings. This arises from the light from three galaxies at distances of 3, 6, and 11 billion light years.

Such rings help in understanding the distribution of dark matter , dark energy , the nature of distant galaxies, and the curvature of the universe.

The odds of finding such a double ring are 1 in 10, Sampling 50 suitable double rings would provide astronomers with a more accurate measurement of the dark matter content of the universe and the equation of state of the dark energy to within 10 percent precision.

To the right is a simulation depicting a zoom on a Schwarzschild black hole in the plane of the Milky Way between us and the centre of the galaxy.

The first Einstein ring is to the most distorted region of the picture and shows the galactic disc. The zoom then reveals a series of 4 extra rings, increasingly thinner and closer to the black hole shadow.

They are multiple images of the galactic disk. From Wikipedia, the free encyclopedia. Part of a series of articles about Gravitational lensing Einstein ring Formalism Strong lensing Microlensing Weak lensing Strong lens systems.

This section does not cite any sources. Please help improve this section by adding citations to reliable sources. Unsourced material may be challenged and removed.

Aktuelles im Bereich Grundschule. Sagen Divertiti Ihre Meinung zu diesem Artikel. Sie haben bereits bei einem früheren Besuch Artikel in Ihren Warenkorb gelegt. Aktuelles im Bereich Berufliche Bildung. Informationen zu den Zahlungsarten. Einer der beiden Artikel ist schneller versandfertig. Aktuelles im Bereich Mittlere Schulformen.### 3 einstern - apologise, but

Einstern - Zu allen Ausgaben: Amazon Business Kauf auf Rechnung. Einsterns Schwester - Sprache und Lesen - Ausgabe Aber auch als klassischer Lehrgang im Klassenverband überzeugt Einstern. Kunden, die diesen Artikel angesehen haben, haben auch angesehen. Konsequente Differenzierung Einige Kinder haben alle Arbeitsaufträge längst erledigt, andere benötigen noch Zeit und Hilfe, um die gleichen Aufgaben zu lösen. Geben Sie Ihre Mobiltelefonnummer ein, um die kostenfreie App zu beziehen. Bitte melden Sie sich an, um Produkte in Ihre Merkliste hinzuzufügen. Geld verdienen mit Amazon. Sie haben keinen Kindle? The first Einstein ring mikrozahlung paypal discovered by Hewitt et al. And one life is enough for me. The Einsteins were non-observant Ashkenazi Jewsand Albert attended a Catholic elementary school in Munich, from the age of 5, for three years. This paper introduced the photon concept although the name photon was introduced later by Gilbert N. Newcastle upon Tyne UK: Please help improve this section by adding citations**einstern 3**reliable sources. Retrieved 25 February Although the patent office promoted Einstein to Technical Examiner Second Class inhe cricket spielregeln not given up on academia. Berkowitz, 25 October Part of a series of articles top online casino with no deposit bonus Gravitational lensing Einstein ring Formalism Strong lensing Microlensing Weak lensing Strong lens systems. The accelerating universe" PDF. From Wikipedia, the free encyclopedia.

### 3 einstern - consider

Pluspunkt Deutsch - Leben in Deutschland Studio [express]. Als offenes Lehrwerk gibt es den Schülerinnen und Schülern die Möglichkeit, im eigenen Tempo selbstständig zu arbeiten, und unterstützt Sie bei der Aufgabe, einzelne Kinder gezielt zu fördern. Mathematik für Kinder der Unterstufe. Themenhefte und Kartonbeilagen ,,,,, im Schuber av Roland Bauer. Weitere Informationen finden Sie auf diesen Seiten: Cornelsen Verlag Reihen Einstern. Mein Ex Libris Jetzt anmelden. Warehouse Deals Reduzierte B-Ware. Aktuelles im Bereich Mittlere Schulformen. Warehouse Deals Reduzierte B-Ware.At the critical point, this derivative is zero, leading to large fluctuations. The effect of density fluctuations is that light of all wavelengths is scattered, making the fluid look milky white.

Einstein relates this to Rayleigh scattering , which is what happens when the fluctuation size is much smaller than the wavelength, and which explains why the sky is blue.

This paper predicted that, when measured in the frame of a relatively moving observer, a clock carried by a moving body would appear to slow down , and the body itself would contract in its direction of motion.

This paper also argued that the idea of a luminiferous aether —one of the leading theoretical entities in physics at the time—was superfluous.

Einstein originally framed special relativity in terms of kinematics the study of moving bodies. In , Hermann Minkowski reinterpreted special relativity in geometric terms as a theory of spacetime.

General relativity GR is a theory of gravitation that was developed by Einstein between and According to general relativity , the observed gravitational attraction between masses results from the warping of space and time by those masses.

General relativity has developed into an essential tool in modern astrophysics. It provides the foundation for the current understanding of black holes , regions of space where gravitational attraction is so strong that not even light can escape.

As Einstein later said, the reason for the development of general relativity was that the preference of inertial motions within special relativity was unsatisfactory, while a theory which from the outset prefers no state of motion even accelerated ones should appear more satisfactory.

In that article titled "On the Relativity Principle and the Conclusions Drawn from It", he argued that free fall is really inertial motion, and that for a free-falling observer the rules of special relativity must apply.

This argument is called the equivalence principle. In the same article, Einstein also predicted the phenomena of gravitational time dilation , gravitational red shift and deflection of light.

In , Einstein published another article "On the Influence of Gravitation on the Propagation of Light" expanding on the article, in which he estimated the amount of deflection of light by massive bodies.

Thus, the theoretical prediction of general relativity could for the first time be tested experimentally. In , Einstein predicted gravitational waves , [] [] ripples in the curvature of spacetime which propagate as waves , traveling outward from the source, transporting energy as gravitational radiation.

The existence of gravitational waves is possible under general relativity due to its Lorentz invariance which brings the concept of a finite speed of propagation of the physical interactions of gravity with it.

By contrast, gravitational waves cannot exist in the Newtonian theory of gravitation , which postulates that the physical interactions of gravity propagate at infinite speed.

While developing general relativity, Einstein became confused about the gauge invariance in the theory. He formulated an argument that led him to conclude that a general relativistic field theory is impossible.

He gave up looking for fully generally covariant tensor equations, and searched for equations that would be invariant under general linear transformations only.

In June , the Entwurf "draft" theory was the result of these investigations. As its name suggests, it was a sketch of a theory, less elegant and more difficult than general relativity, with the equations of motion supplemented by additional gauge fixing conditions.

After more than two years of intensive work, Einstein realized that the hole argument was mistaken [] and abandoned the theory in November In , Einstein applied the general theory of relativity to the structure of the universe as a whole.

As observational evidence for a dynamic universe was not known at the time, Einstein introduced a new term, the cosmological constant , to the field equations, in order to allow the theory to predict a static universe.

Following the discovery of the recession of the nebulae by Edwin Hubble in , Einstein abandoned his static model of the universe, and proposed two dynamic models of the cosmos, The Friedmann-Einstein universe of [] [] and the Einstein—de Sitter universe of In many Einstein biographies, it is claimed that Einstein referred to the cosmological constant in later years as his "biggest blunder".

The astrophysicist Mario Livio has recently cast doubt on this claim, suggesting that it may be exaggerated. For the density to remain constant, new particles of matter must be continually formed in the volume from space.

It thus appears that Einstein considered a steady-state model of the expanding universe many years before Hoyle, Bondi and Gold.

General relativity includes a dynamical spacetime, so it is difficult to see how to identify the conserved energy and momentum. Einstein argued that this is true for fundamental reasons, because the gravitational field could be made to vanish by a choice of coordinates.

He maintained that the non-covariant energy momentum pseudotensor was in fact the best description of the energy momentum distribution in a gravitational field.

This approach has been echoed by Lev Landau and Evgeny Lifshitz , and others, and has become standard. In , Einstein collaborated with Nathan Rosen to produce a model of a wormhole , often called Einstein—Rosen bridges.

These solutions cut and pasted Schwarzschild black holes to make a bridge between two patches. If one end of a wormhole was positively charged, the other end would be negatively charged.

These properties led Einstein to believe that pairs of particles and antiparticles could be described in this way. In order to incorporate spinning point particles into general relativity, the affine connection needed to be generalized to include an antisymmetric part, called the torsion.

This modification was made by Einstein and Cartan in the s. The theory of general relativity has a fundamental law—the Einstein equations which describe how space curves, the geodesic equation which describes how particles move may be derived from the Einstein equations.

Since the equations of general relativity are non-linear, a lump of energy made out of pure gravitational fields, like a black hole, would move on a trajectory which is determined by the Einstein equations themselves, not by a new law.

So Einstein proposed that the path of a singular solution, like a black hole, would be determined to be a geodesic from general relativity itself. This was established by Einstein, Infeld, and Hoffmann for pointlike objects without angular momentum, and by Roy Kerr for spinning objects.

In a paper, [] Einstein postulated that light itself consists of localized particles quanta. He does not say much more, because he is not sure how the particles are related to the wave.

But he does suggest that this idea would explain certain experimental results, notably the photoelectric effect. In , Einstein proposed a model of matter where each atom in a lattice structure is an independent harmonic oscillator.

In the Einstein model, each atom oscillates independently—a series of equally spaced quantized states for each oscillator.

Einstein was aware that getting the frequency of the actual oscillations would be difficult, but he nevertheless proposed this theory because it was a particularly clear demonstration that quantum mechanics could solve the specific heat problem in classical mechanics.

Peter Debye refined this model. Throughout the s, quantum mechanics expanded in scope to cover many different systems. After Ernest Rutherford discovered the nucleus and proposed that electrons orbit like planets, Niels Bohr was able to show that the same quantum mechanical postulates introduced by Planck and developed by Einstein would explain the discrete motion of electrons in atoms, and the periodic table of the elements.

Einstein contributed to these developments by linking them with the arguments Wilhelm Wien had made. Wien had shown that the hypothesis of adiabatic invariance of a thermal equilibrium state allows all the blackbody curves at different temperature to be derived from one another by a simple shifting process.

Einstein noted in that the same adiabatic principle shows that the quantity which is quantized in any mechanical motion must be an adiabatic invariant.

Arnold Sommerfeld identified this adiabatic invariant as the action variable of classical mechanics. In , Einstein received a description of a statistical model from Indian physicist Satyendra Nath Bose , based on a counting method that assumed that light could be understood as a gas of indistinguishable particles.

Einstein also published his own articles describing the model and its implications, among them the Bose—Einstein condensate phenomenon that some particulates should appear at very low temperatures.

Although the patent office promoted Einstein to Technical Examiner Second Class in , he had not given up on academia. In , he became a Privatdozent at the University of Bern.

This paper introduced the photon concept although the name photon was introduced later by Gilbert N. Lewis in and inspired the notion of wave—particle duality in quantum mechanics.

Einstein saw this wave—particle duality in radiation as concrete evidence for his conviction that physics needed a new, unified foundation.

In a series of works completed from to , Planck reformulated his quantum theory and introduced the idea of zero-point energy in his "second quantum theory".

Soon, this idea attracted the attention of Einstein and his assistant Otto Stern. Assuming the energy of rotating diatomic molecules contains zero-point energy, they then compared the theoretical specific heat of hydrogen gas with the experimental data.

The numbers matched nicely. However, after publishing the findings, they promptly withdrew their support, because they no longer had confidence in the correctness of the idea of zero-point energy.

In , at the height of his work on relativity, Einstein published an article in Physikalische Zeitschrift that proposed the possibility of stimulated emission , the physical process that makes possible the maser and the laser.

This paper was enormously influential in the later development of quantum mechanics, because it was the first paper to show that the statistics of atomic transitions had simple laws.

In another major paper from this era, Einstein gave a wave equation for de Broglie waves , which Einstein suggested was the Hamilton—Jacobi equation of mechanics.

Einstein was displeased with modern quantum mechanics as it had evolved after Contrary to popular belief, his doubts were not due to a conviction that God "is not playing at dice.

Einstein believed that a physical reality exists independent of our ability to observe it. In contrast, Bohr and his followers maintained that all we can know are the results of measurements and observations, and that it makes no sense to speculate about an ultimate reality that exists beyond our perceptions.

The Bohr—Einstein debates were a series of public disputes about quantum mechanics between Einstein and Niels Bohr , who were two of its founders.

Their debates are remembered because of their importance to the philosophy of science. In , Einstein returned quantum mechanics, in particular to the question of its completeness, in the "EPR paper".

No matter how far the two particles were separated, a precise position measurement on one particle would result in equally precise knowledge of the position of the other particle; likewise a precise momentum measurement of one particle would result in equally precise knowledge of the momentum of the other particle, without needing to disturb the other particle in any way.

Einstein rejected this second possibility popularly called "spooky action at a distance". Bell had delineated in The results of these and subsequent experiments demonstrate that quantum physics cannot be represented by any version of the picture of physics in which "particles are regarded as unconnected independent classical-like entities, each one being unable to communicate with the other after they have separated.

Although Einstein was wrong about local realism, his clear prediction of the unusual properties of its opposite, entangled quantum states , has resulted in the EPR paper becoming among the top ten papers published in Physical Review.

It is considered a centerpiece of the development of quantum information theory. Following his research on general relativity, Einstein entered into a series of attempts to generalize his geometric theory of gravitation to include electromagnetism as another aspect of a single entity.

In , he described his " unified field theory " in a Scientific American article titled "On the Generalized Theory of Gravitation".

In his pursuit of a unification of the fundamental forces, Einstein ignored some mainstream developments in physics, most notably the strong and weak nuclear forces , which were not well understood until many years after his death.

Einstein conducted other investigations that were unsuccessful and abandoned. These pertain to force , superconductivity , and other research.

In addition to longtime collaborators Leopold Infeld , Nathan Rosen , Peter Bergmann and others, Einstein also had some one-shot collaborations with various scientists.

Einstein and De Haas demonstrated that magnetization is due to the motion of electrons, nowadays known to be the spin. In order to show this, they reversed the magnetization in an iron bar suspended on a torsion pendulum.

This experiment needed to be sensitive, because the angular momentum associated with electrons is small, but it definitively established that electron motion of some kind is responsible for magnetization.

Then to each possible quantum motion of a particle in a box associate an independent harmonic oscillator. Quantizing these oscillators, each level will have an integer occupation number, which will be the number of particles in it.

This formulation is a form of second quantization , but it predates modern quantum mechanics. This absorption refrigerator was then revolutionary for having no moving parts and using only heat as an input.

Their invention was not immediately put into commercial production, and the most promising of their patents were acquired by the Swedish company Electrolux.

While traveling, Einstein wrote daily to his wife Elsa and adopted stepdaughters Margot and Ilse. The letters were included in the papers bequeathed to The Hebrew University.

Margot Einstein permitted the personal letters to be made available to the public, but requested that it not be done until twenty years after her death she died in [].

Einstein had expressed his interest in the plumbing profession and was made an honorary member of the Plumbers and Steamfitters Union. Corbis , successor to The Roger Richman Agency, licenses the use of his name and associated imagery, as agent for the university.

In the period before World War II, The New Yorker published a vignette in their "The Talk of the Town" feature saying that Einstein was so well known in America that he would be stopped on the street by people wanting him to explain "that theory".

He finally figured out a way to handle the incessant inquiries. He told his inquirers "Pardon me, sorry! Always I am mistaken for Professor Einstein.

Einstein has been the subject of or inspiration for many novels, films, plays, and works of music. Many popular quotations are often misattributed to him.

Einstein received numerous awards and honors and in he was awarded the Nobel Prize in Physics "for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect".

None of the nominations in met the criteria set by Alfred Nobel , so the prize was carried forward and awarded to Einstein in From Wikipedia, the free encyclopedia.

For other people, see Einstein surname. For other uses, see Albert Einstein disambiguation and Einstein disambiguation.

German-born physicist and developer of the theory of relativity. Princeton, New Jersey , US. Swiss Federal Polytechnic —; B. Annus Mirabilis papers , Photoelectric effect , Special theory of relativity , Mass—energy equivalence , and Brownian motion.

Statistical mechanics , thermal fluctuations , and statistical physics. History of special relativity. History of general relativity.

Equivalence principle , Theory of relativity , and Einstein field equations. Discovery of cosmic microwave background radiation.

Religious interpretations of the Big Bang theory. Classical unified field theories. Albert Einstein in popular culture.

Einstein, Albert [Manuscript received: Written at Zurich, Switzerland. Annalen der Physik Berlin in German. Hoboken, NJ published 14 March Einstein, Albert a [Manuscript received: Written at Berne, Switzerland.

Hoboken, NJ published 10 March Einstein, Albert b [Completed 30 April and submitted 20 July ]. Written at Berne, Switzerland, published by Wyss Buchdruckerei.

Einstein, Albert c [Manuscript received: Einstein, Albert d [Manuscript received: Annalen der Physik Berlin Submitted manuscript in German.

Einstein, Albert e [Manuscript received: Einstein, Albert [Published 25 November ]. Physikalische Zeitschrift in German. Einstein, Albert [First published , in English ].

Nobel Lectures, Physics — in German and English. Einstein, Albert [Published 10 July ]. First of a series of papers on this topic.

Die Naturwissenschaften in German. Dover Publications published Physical Review Submitted manuscript. Einstein, Albert 9 November On Science and Religion.

Einstein, Albert; et al. The New York Times. Einstein, Albert May Monthly Review Foundation published May Archived from the original on 11 January Retrieved 16 January — via MonthlyReview.

Albert Einstein, Hedwig und Max Born: Briefwechsel — in German. Paul Arthur Schilpp Centennial ed. The chasing a light beam thought experiment is described on pages 48— Stachel, John ; Martin J.

Kox; Michel Janssen; R. Schulmann; Diana Komos Buchwald; et al. The Collected Papers of Albert Einstein. Further information about the volumes published so far can be found on the webpages of the Einstein Papers Project and on the Princeton University Press Einstein Page.

She has chosen the cream of her culture and has suppressed it. She has even turned upon her most glorious citizen, Albert Einstein, who is the supreme example of the selfless intellectual The man, who, beyond all others, approximates a citizen of the world, is without a home.

How proud we must be to offer him temporary shelter. Biographical Memoirs of Fellows of the Royal Society. Longman Pronunciation Dictionary 3rd ed.

Archived from the original on 6 March Retrieved 7 March Modern Atomic and Nuclear Physics. Stanford Encyclopedia of Philosophy.

Retrieved 11 July The accelerating universe" PDF. Retrieved 24 November Boyer; Melvyn Dubofsky Harper and Brothers Publishers Harper Torchbook edition.

His non-scientific works include: The Trustees of Princeton University. The Passions of a Scientist , Prometheus Books, p. The Golden Age of Physics.

Archived from the original PDF on 19 January Retrieved 19 October The Love Letters , , pp. A Biography , , pp. A Hundred Years of Relativity.

BZ Berner Zeitung in German. The Question of Time". Marcel Grossmann gewidmet Dedicated to my friend, Dr.

Einstein Online in German and English. Retrieved 17 August Retrieved 9 July Royal Netherlands Academy of Arts and Sciences.

Retrieved 21 July Retrieved 13 June Banquet Speech by R. Retrieved 9 December via Nobelprize. Memoria e Ricerca 2: French version PDF and English summary.

The Journal of Ecclesiastical History. My Autobiography , Simon and Schuster, N. How I See the World". Retrieved May 29, Einstein on Race and Racism.

Institute for Advanced Study. Archived from the original on 29 March Retrieved 4 March Making the Atomic Bomb". Department of Energy, History Division.

Genius in the Shadows: The Man Behind The Bomb. Diehl, Sarah; Moltz, James Clay Nuclear Weapons and Nonproliferation: Pennsylvania State University Press.

Retrieved — via atomicarchive. Paul Robeson Speaks , Citadel p. Retrieved 31 March Johns Hopkins University Press. Archived from the original PDF on 28 August Einstein for the 21st Century: London, Macmillan Publishers Ltd.

Revised by Nicolas Slonimsky. New York, Schirmer Books, Sweezy, Paul; Huberman, Leo, eds. The first Einstein ring was discovered by Hewitt et al. This observation saw a quasar lensed by a nearer galaxy into two separate but very similar images of the same object, the images stretched round the lens into an almost complete ring.

As of this survey has found 85 confirmed gravitational lenses, there is not yet a number for how many show Einstein rings. This arises from the light from three galaxies at distances of 3, 6, and 11 billion light years.

Such rings help in understanding the distribution of dark matter , dark energy , the nature of distant galaxies, and the curvature of the universe.

The odds of finding such a double ring are 1 in 10, Sampling 50 suitable double rings would provide astronomers with a more accurate measurement of the dark matter content of the universe and the equation of state of the dark energy to within 10 percent precision.

To the right is a simulation depicting a zoom on a Schwarzschild black hole in the plane of the Milky Way between us and the centre of the galaxy.

The first Einstein ring is to the most distorted region of the picture and shows the galactic disc. The zoom then reveals a series of 4 extra rings, increasingly thinner and closer to the black hole shadow.

They are multiple images of the galactic disk. From Wikipedia, the free encyclopedia. Part of a series of articles about Gravitational lensing Einstein ring Formalism Strong lensing Microlensing Weak lensing Strong lens systems.

This section does not cite any sources. Please help improve this section by adding citations to reliable sources. Unsourced material may be challenged and removed.

April Learn how and when to remove this template message. The New York Times. Retrieved December 27, Retrieved March 5, Retrieved 22 April Archived from the original PDF on July 25, Explicit use of et al.

Monthly Notices of the Royal Astronomical Society. Retrieved 10 February Discovery and Analysis of a Double Einstein Ring".

Retrieved 9 June

Mehr lesen Weniger lesen. Sv union lohne Sie Ihre Mobiltelefonnummer ein, um die kostenfreie App zu beziehen. Aber auch als klassischer Lehrgang im Klassenverband überzeugt Einstern. Skickas inom vardagar. Fundamentum Mathematik und Physik - ink. Band 3 - Arbeitsheft. Ihr Warenkorb wurde nun mit diesen Artikeln ergänzt. Der Artikel wurde dem Warenkorb hinzugefügt. Derzeit tritt ein Problem beim Filtern der Rezensionen auf. Willkommen, schön sind Sie skrill email
Ich meine, dass Sie nicht recht sind. Ich kann die Position verteidigen. Schreiben Sie mir in PM, wir werden reden.

Wacker, welche Phrase..., der prГ¤chtige Gedanke

Ich kann zu diesem Thema viel sagen.

Ja, ich bin mit Ihnen bestimmt einverstanden