Kamis, 24 Januari 2013
Albert's three children were from his relationship with his first wife, Mileva Marić, his daughter Lieserl being born a year before they married.
Albert Einstein's second wife was Elsa Einstein, whose mother Fanny Koch was the sister of Albert's mother, and whose father Rudolf Einstein was the son of Raphael Einstein, a brother of Albert's paternal grandfather. Thus Albert and Elsa were first cousins through their mothers and second cousins through their fathers.[2]
Albert Einstein's second wife was Elsa Einstein, whose mother Fanny Koch was the sister of Albert's mother, and whose father Rudolf Einstein was the son of Raphael Einstein, a brother of Albert's paternal grandfather. Thus Albert and Elsa were first cousins through their mothers and second cousins through their fathers.[2]
Einstein family
The Einstein family is the family of the famous scientist Albert Einstein. Einstein's great-great-great-great-grandfather, Jakob Weil, is his oldest recorded relative, born around the turn of the 18th century, and the family continues to this day. Albert Einstein's great-great-grandfather, Löb Moses Sontheimer (1745–1831), was also the grandfather of the prominent tenor Heinrich Sontheim (1820–1912) of Stuttgart.[1]
Awards and honors
Main article: Einstein's awards and honors
Einstein received numerous awards and honors, including the Nobel Prize in Physics.Publications
- The following publications by Albert Einstein are referenced in this article. A more complete list of his publications may be found at List of scientific publications by Albert Einstein.
- Einstein, Albert (1901), "Folgerungen aus den Capillaritätserscheinungen (Conclusions Drawn from the Phenomena of Capillarity)", Annalen der Physik 4 (3): 513, Bibcode 1901AnP...309..513E, doi:10.1002/andp.19013090306
- Einstein, Albert (1905a), "Über einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt (On a Heuristic Viewpoint Concerning the Production and Transformation of Light)", Annalen der Physik 17 (6): 132–148, Bibcode 1905AnP...322..132E, doi:10.1002/andp.19053220607 This annus mirabilis paper on the photoelectric effect was received by Annalen der Physik 18 March.
- Einstein, Albert (1905b), A new determination of molecular dimensions. This PhD thesis was completed 30 April and submitted 20 July.
- Einstein, Albert (1905c), "On the Motion – Required by the Molecular Kinetic Theory of Heat – of Small Particles Suspended in a Stationary Liquid", Annalen der Physik 17 (8): 549–560, Bibcode 1905AnP...322..549E, doi:10.1002/andp.19053220806. This annus mirabilis paper on Brownian motion was received 11 May.
- Einstein, Albert (1905d), "On the Electrodynamics of Moving Bodies", Annalen der Physik 17 (10): 891–921, Bibcode 1905AnP...322..891E, doi:10.1002/andp.19053221004. This annus mirabilis paper on special relativity was received 30 June.
- Einstein, Albert (1905e), "Does the Inertia of a Body Depend Upon Its Energy Content?", Annalen der Physik 18 (13): 639–641, Bibcode 1905AnP...323..639E,
Non-scientific legacy
While travelling, 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 1986[118]). Barbara Wolff, of The Hebrew University's Albert Einstein Archives, told the BBC that there are about 3,500 pages of private correspondence written between 1912 and 1955.[119]Einstein bequeathed the royalties from use of his image to The Hebrew University of Jerusalem. Corbis, successor to The Roger Richman Agency, licenses the use of his name and associated imagery, as agent for the university.[120]
In popular culture
Main article: Albert Einstein in popular culture
In the period before World War II, 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."[121]Einstein has been the subject of or inspiration for many novels, films, plays, and works of music.[122] He is a favorite model for depictions of mad scientists and absent-minded professors; his expressive face and distinctive hairstyle have been widely copied and exaggerated. Time magazine's Frederic Golden wrote that Einstein was "a cartoonist's dream come true".[123]
Botstein notes that music assumed a pivotal and permanent role in
Einstein's life from that period on. Although the idea of becoming a
professional himself was not on his mind at any time, among those with
whom Einstein played chamber music
were a few professionals, and he performed for private audiences and
friends. Chamber music also became a regular part of his social life
while living in Bern, Zurich, and Berlin, where he played with Max Planck and his son, among others. In 1931, while engaged in research at California Institute of Technology,
he visited the Zoellner family conservatory in Los Angeles and played
some of Beethoven and Mozart's works with members of the Zoellner Quartet,
recently retired from two decades of acclaimed touring all across the
United States; Einstein later presented the family patriarch with an
autographed photograph as a memento.[116][117] Near the end of his life, when the young Juilliard Quartet
visited him in Princeton, he played his violin with them; although they
slowed the tempo to accommodate his lesser technical abilities,
Botstein notes the quartet was "impressed by Einstein's level of
coordination and intonation."[115]
Love of music
Einstein developed an appreciation of music at an early age. His
mother played the piano reasonably well and wanted her son to learn the
violin, not only to instill in him a love of music but also to help him
assimilate German culture. According to conductor Leon Botstein, Einstein is said to have begun playing when he was five, but did not enjoy it at that age.[115]
When he turned thirteen, however, he discovered the violin sonatas of Mozart. "Einstein fell in love" with Mozart's music, notes Botstein, and learned to play music more willingly. According to Einstein, he taught himself to play by "ever practicing systematically," adding that "Love is a better teacher than a sense of duty."[115] At age seventeen, he was heard by a school examiner in Aarau as he played Beethoven's violin sonatas, the examiner stating afterward that his playing was "remarkable and revealing of 'great insight.'" What struck the examiner, writes Botstein, was that Einstein "displayed a deep love of the music, a quality that was and remains in short supply. Music possessed an unusual meaning for this student."[115]
When he turned thirteen, however, he discovered the violin sonatas of Mozart. "Einstein fell in love" with Mozart's music, notes Botstein, and learned to play music more willingly. According to Einstein, he taught himself to play by "ever practicing systematically," adding that "Love is a better teacher than a sense of duty."[115] At age seventeen, he was heard by a school examiner in Aarau as he played Beethoven's violin sonatas, the examiner stating afterward that his playing was "remarkable and revealing of 'great insight.'" What struck the examiner, writes Botstein, was that Einstein "displayed a deep love of the music, a quality that was and remains in short supply. Music possessed an unusual meaning for this student."[115]
Political and religious views
Main articles: Albert Einstein's political views and Albert Einstein's religious views
Einstein's views about religious belief have been collected from interviews and original writings. These views covered Judaism, theological determinism, agnosticism, and humanism. He also wrote much about ethical culture, opting for Spinoza's god over belief in a personal god.[114]
Einstein–Podolsky–Rosen paradox
Main article: EPR paradox
In 1935, Einstein returned to the question of quantum mechanics. He
considered how a measurement on one of two entangled particles would
affect the other. He noted, along with his collaborators, that by
performing different measurements on the distant particle, either of
position or momentum, different properties of the entangled partner
could be discovered without disturbing it in any way.He then used a hypothesis of local realism to conclude that the other particle had these properties already determined. The principle he proposed is that if it is possible to determine what the answer to a position or momentum measurement would be, without in any way disturbing the particle, then the particle actually has values of position or momentum.
This principle distilled the essence of Einstein's objection to quantum mechanics. As a physical principle, it was shown to be incorrect when the Aspect experiment of 1982 confirmed Bell's theorem, which had been promulgated in 1964.
Einstein refrigerator
Main article: Einstein refrigerator
In 1926, Einstein and his former student Leó Szilárd co-invented (and in 1930, patented) the Einstein refrigerator. This absorption refrigerator was then revolutionary for having no moving parts and using only heat as an input.[106] On 11 November 1930, U.S. Patent 1,781,541
was awarded to Albert Einstein and Leó Szilárd for the refrigerator.
Their invention was not immediately put into commercial production, as
the most promising of their patents were quickly bought up by the
Swedish company Electrolux to protect its refrigeration technology from competition.[107]Bohr versus Einstein
Main article: Bohr–Einstein debates
Schrödinger gas model
Einstein suggested to Erwin Schrödinger that he might be able to reproduce the statistics of a Bose–Einstein gas
by considering a box. 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. Erwin Schrödinger applied this to derive the thermodynamic properties of a semiclassical ideal gas. Schrödinger urged Einstein to add his name as co-author, although Einstein declined the invitation.[105]
This formulation is a form of second quantization, but it predates modern quantum mechanics. Erwin Schrödinger applied this to derive the thermodynamic properties of a semiclassical ideal gas. Schrödinger urged Einstein to add his name as co-author, although Einstein declined the invitation.[105]
Einstein–de Haas experiment
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.
They confirmed that this leads the bar to rotate, because the
electron's angular momentum changes as the magnetization changes. 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.
Other investigations
Einstein conducted other investigations that were unsuccessful and abandoned. These pertain to force, superconductivity, gravitational waves, and other research. Please see the main article for details.
The 1927 Solvay Conference in Brussels, a gathering of the world's top physicists. Einstein in the center.
In addition to longtime collaborators Leopold Infeld, Nathan Rosen, Peter Bergmann and others, Einstein also had some one-shot collaborations with various scientists.
Collaboration with other scientists
Equations of motion
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.
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.
Einstein–Cartan theory
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 1920s.
Wormholes
Einstein collaborated with others to produce a model of a wormhole.
His motivation was to model elementary particles with charge as a
solution of gravitational field equations, in line with the program
outlined in the paper "Do Gravitational Fields play an Important Role in
the Constitution of the Elementary Particles?". 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.
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.
Unified field 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 1950,
he described his "unified field theory" in a Scientific American article entitled "On the Generalized Theory of Gravitation".[104]
Although he continued to be lauded for his work, Einstein became
increasingly isolated in his research, and his efforts were ultimately
unsuccessful. 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.
Mainstream physics, in turn, largely ignored Einstein's approaches to
unification. Einstein's dream of unifying other laws of physics with
gravity motivates modern quests for a theory of everything and in particular string theory, where geometrical fields emerge in a unified quantum-mechanical setting.
Energy momentum pseudotensor
General relativity includes a dynamical spacetime, so it is difficult to see how to identify the conserved energy and momentum. Noether's theorem allows these quantities to be determined from a Lagrangian with translation invariance, but general covariance makes translation invariance into something of a gauge symmetry.
The energy and momentum derived within general relativity by Noether's
presecriptions do not make a real tensor for this reason.
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.
The use of non-covariant objects like pseudotensors was heavily criticized in 1917 by Erwin Schrödinger and others.
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.
The use of non-covariant objects like pseudotensors was heavily criticized in 1917 by Erwin Schrödinger and others.
Bose–Einstein statistics
In 1924, 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 noted that Bose's
statistics applied to some atoms as well as to the proposed light
particles, and submitted his translation of Bose's paper to the Zeitschrift für Physik. 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.[102] It was not until 1995 that the first such condensate was produced experimentally by Eric Allin Cornell and Carl Wieman using ultra-cooling equipment built at the NIST–JILA laboratory at the University of Colorado at Boulder.[103] Bose–Einstein statistics are now used to describe the behaviors of any assembly of bosons. Einstein's sketches for this project may be seen in the Einstein Archive in the library of the Leiden University.[82]
Modern quantum theory
Einstein was displeased with quantum theory and mechanics, despite its
acceptance by other physicists, stating "God doesn't play with dice." As
Einstein passed away at the age of 76 he still would not accept quantum
theory.[100] In 1917, 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.[101]
This article showed that the statistics of absorption and emission of
light would only be consistent with Planck's distribution law if the
emission of light into a mode with n photons would be enhanced
statistically compared to the emission of light into an empty mode. 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. Einstein discovered Louis de Broglie's
work, and supported his ideas, which were received skeptically at
first. 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. This paper would inspire Schrödinger's work of 1926.
Cosmology
In 1917, Einstein applied the General theory of relativity to model
the structure of the universe as a whole. He wanted the universe to be
eternal and unchanging, but this type of universe is not consistent with
relativity. To fix this, Einstein modified the general theory by
introducing a new notion, the cosmological constant. With a positive cosmological constant, the universe could be an eternal static sphere.[99]
Einstein in his office at the University of Berlin.
Einstein believed a spherical static universe is philosophically preferred, because it would obey Mach's principle. He had shown that general relativity incorporates Mach's principle to a certain extent in frame dragging by gravitomagnetic fields,
but he knew that Mach's idea would not work if space goes on forever.
In a closed universe, he believed that Mach's principle would hold.
Mach's principle has generated much controversy over the years.
Hole argument and Entwurf theory
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 1913 the Entwurf ("draft") theory was the result of these investigations. As its name suggests, it was a sketch of a theory, with the equations of motion supplemented by additional gauge fixing conditions. Simultaneously less elegant and more difficult than general relativity, after more than two years of intensive work Einstein abandoned the theory in November 1915 after realizing that the hole argument was mistaken.[98]
In June 1913 the Entwurf ("draft") theory was the result of these investigations. As its name suggests, it was a sketch of a theory, with the equations of motion supplemented by additional gauge fixing conditions. Simultaneously less elegant and more difficult than general relativity, after more than two years of intensive work Einstein abandoned the theory in November 1915 after realizing that the hole argument was mistaken.[98]
General relativity and the Equivalence Principle
General relativity (GR) is a theory of gravitation that was developed by Albert Einstein between 1907 and 1915. 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 Albert 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.[97] So in 1908 he published an article on acceleration under special relativity. In that article, he argued that free fall is really inertial motion, and that for a freefalling observer the rules of special relativity must apply. This argument is called the Equivalence principle. In the same article, Einstein also predicted the phenomenon of gravitational time dilation. In 1911, Einstein published another article expanding on the 1907 article, in which additional effects such as the deflection of light by massive bodies were predicted.
As Albert 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.[97] So in 1908 he published an article on acceleration under special relativity. In that article, he argued that free fall is really inertial motion, and that for a freefalling observer the rules of special relativity must apply. This argument is called the Equivalence principle. In the same article, Einstein also predicted the phenomenon of gravitational time dilation. In 1911, Einstein published another article expanding on the 1907 article, in which additional effects such as the deflection of light by massive bodies were predicted.
Zero-point energy
Einstein's physical intuition led him to note that Planck's oscillator
energies had an incorrect zero point. He modified Planck's hypothesis by
stating that the lowest energy state of an oscillator is equal to 1⁄2hf, to half the energy spacing between levels. This argument, which was made in 1913 in collaboration with Otto Stern, was based on the thermodynamics of a diatomic molecule which can split apart into two free atoms.
Theory of critical opalescence
Einstein returned to the problem of thermodynamic fluctuations, giving a
treatment of the density variations in a fluid at its critical point.
Ordinarily the density fluctuations are controlled by the second
derivative of the free energy with respect to the density. 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 Raleigh scattering, which is what happens when the fluctuation size is much smaller than the wavelength, and which explains why the sky is blue.[96]
Einstein quantitatively derived critical opalescence from a treatment
of density fluctuations, and demonstrated how both the effect and
Rayleigh scattering originate from the atomistic constitution of matter.
Wave–particle duality
Although the patent office promoted Einstein to Technical Examiner
Second Class in 1906, he had not given up on academia. In 1908, he
became a privatdozent at the University of Bern.[95] In "über die Entwicklung unserer Anschauungen über das Wesen und die Konstitution der Strahlung" ("The Development of Our Views on the Composition and Essence of Radiation"), on the quantization of light, and in an earlier 1909 paper, Einstein showed that Max Planck's energy quanta must have well-defined momenta and act in some respects as independent, point-like particles. This paper introduced the photon concept (although the name photon was introduced later by Gilbert N. Lewis in 1926) and inspired the notion of wave–particle duality in quantum mechanics.
Adiabatic principle and action-angle variables
Throughout the 1910s, 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 1898 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 1911 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. The law that the action variable is quantized was a basic principle of the quantum theory as it was known between 1900 and 1925.[citation needed]
Einstein contributed to these developments by linking them with the 1898 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 1911 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. The law that the action variable is quantized was a basic principle of the quantum theory as it was known between 1900 and 1925.[citation needed]
Quantized atomic vibrations
In 1907 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 different, 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.[94]
Photons and energy quanta
In a 1905 paper,[92] Einstein postulated that light itself consists of localized particles (quanta).
Einstein's light quanta were nearly universally rejected by all
physicists, including Max Planck and Niels Bohr. This idea only became
universally accepted in 1919, with Robert Millikan's detailed experiments on the photoelectric effect, and with the measurement of Compton scattering.
Einstein concluded that each wave of frequency f is associated with a collection of photons with energy hf each, where h is Planck's constant. 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.[93]
Einstein concluded that each wave of frequency f is associated with a collection of photons with energy hf each, where h is Planck's constant. 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.[93]
Theory of relativity and E = mc²
Einstein's "Zur Elektrodynamik bewegter Körper" ("On the
Electrodynamics of Moving Bodies") was received on 30 June 1905 and
published 26 September of that same year. It reconciles Maxwell's equations for electricity and magnetism with the laws of mechanics, by introducing major changes to mechanics close to the speed of light. This later became known as Einstein's special theory of relativity.
Consequences of this include the time-space frame of a moving body appearing to slow down and contract (in the direction of motion) when measured in the frame of the observer. This paper also argued that the idea of a luminiferous aether – one of the leading theoretical entities in physics at the time – was superfluous.[88]
In his paper on mass–energy equivalence Einstein produced E = mc2 from his special relativity equations.[89] Einstein's 1905 work on relativity remained controversial for many years, but was accepted by leading physicists, starting with Max Planck.[90][91]
Consequences of this include the time-space frame of a moving body appearing to slow down and contract (in the direction of motion) when measured in the frame of the observer. This paper also argued that the idea of a luminiferous aether – one of the leading theoretical entities in physics at the time – was superfluous.[88]
In his paper on mass–energy equivalence Einstein produced E = mc2 from his special relativity equations.[89] Einstein's 1905 work on relativity remained controversial for many years, but was accepted by leading physicists, starting with Max Planck.[90][91]
General principles
He articulated the principle of relativity. This was understood by Hermann Minkowski
to be a generalization of rotational invariance from space to
space-time. Other principles postulated by Einstein and later vindicated
are the principle of equivalence and the principle of adiabatic invariance of the quantum number.
Thermodynamic fluctuations and statistical physics
Albert Einstein's first paper[87] submitted in 1900 to Annalen der Physik was on capillary attraction. It was published in 1901 with the title "Folgerungen aus den Kapillarität Erscheinungen," which translates as "Conclusions from the capillarity phenomena". Two papers he published in 1902–1903 (thermodynamics) attempted to interpret atomic phenomena from a statistical point of view. These papers were the foundation for the 1905 paper on Brownian motion, which showed that Brownian movement can be construed as firm evidence that molecules exist. His research in 1903 and 1904 was mainly concerned with the effect of finite atomic size on diffusion phenomena.[87]
| Title (translated) | Area of focus | Received | Published | Significance |
|---|---|---|---|---|
| On a Heuristic Viewpoint Concerning the Production and Transformation of Light | Photoelectric effect | 18 March | 9 June | Resolved an unsolved puzzle by suggesting that energy is exchanged only in discrete amounts (quanta).[83] This idea was pivotal to the early development of quantum theory.[84] |
| On the Motion of Small Particles Suspended in a Stationary Liquid, as Required by the Molecular Kinetic Theory of Heat | Brownian motion | 11 May | 18 July | Explained empirical evidence for the atomic theory, supporting the application of statistical physics. |
| On the Electrodynamics of Moving Bodies | Special relativity | 30 June | 26 September | Reconciled Maxwell's equations for electricity and magnetism with the laws of mechanics by introducing major changes to mechanics close to the speed of light, resulting from analysis based on empirical evidence that the speed of light is independent of the motion of the observer.[85] Discredited the concept of a "luminiferous ether."[86] |
| Does the Inertia of a Body Depend Upon Its Energy Content? | Matter–energy equivalence | 27 September | 21 November | Equivalence of matter and energy, E = mc2 (and by implication, the ability of gravity to "bend" light), the existence of "rest energy", and the basis of nuclear energy. |
Scientific career
hroughout his life, Einstein published hundreds of books and articles.[8][10]
In addition to the work he did by himself he also collaborated with
other scientists on additional projects including the Bose–Einstein
statistics, the Einstein refrigerator and others.[82]
1905 – Annus Mirabilis papers
Main articles: Annus Mirabilis papers, Photoelectric effect, Special theory of relativity, and Mass–energy equivalence
The Annus Mirabilis papers are four articles pertaining to the photoelectric effect (which gave rise to quantum theory), Brownian motion, the special theory of relativity, and E = mc2 that Albert Einstein published in the Annalen der Physik scientific journal in 1905. These four works contributed substantially to the foundation of modern physics and changed views on space, time, and matter. The four papers are:
During the autopsy, the pathologist of Princeton Hospital, Thomas Stoltz Harvey, removed Einstein's brain for preservation without the permission of his family, in the hope that the neuroscience of the future would be able to discover what made Einstein so intelligent.[79] Einstein's remains were cremated and his ashes were scattered at an undisclosed location.[80][81]
In his lecture at Einstein's memorial, nuclear physicist Robert Oppenheimer summarized his impression of him as a person: "He was almost wholly without sophistication and wholly without worldliness . . . There was always with him a wonderful purity at once childlike and profoundly stubborn."[68]
In his lecture at Einstein's memorial, nuclear physicist Robert Oppenheimer summarized his impression of him as a person: "He was almost wholly without sophistication and wholly without worldliness . . . There was always with him a wonderful purity at once childlike and profoundly stubborn."[68]
Death
On 17 April 1955, Albert Einstein experienced internal bleeding caused by the rupture of an abdominal aortic aneurysm, which had previously been reinforced surgically by Dr. Rudolph Nissen in 1948.[76]
He took the draft of a speech he was preparing for a television
appearance commemorating the State of Israel's seventh anniversary with
him to the hospital, but he did not live long enough to complete it.[77]
Einstein refused surgery, saying: "I want to go when I want. It is
tasteless to prolong life artificially. I have done my share, it is time
to go. I will do it elegantly."[78] He died in Princeton Hospital early the next morning at the age of 76, having continued to work until near the end.
All my life I have dealt with objective matters, hence I lack both the
natural aptitude and the experience to deal properly with people and to
exercise official function. I am the more distressed over these
circumstances because my relationship with the Jewish people became my
strongest human tie once I achieved complete clarity about our
precarious position among the nations of the world.[54]:522[74][75]
As a member of the National Association for the Advancement of Colored People (NAACP) at Princeton who campaigned for the civil rights of African Americans, Einstein corresponded with civil rights activist W. E. B. Du Bois, and in 1946 Einstein called racism America's "worst disease".[70]
He later stated, "Race prejudice has unfortunately become an American
tradition which is uncritically handed down from one generation to the
next. The only remedies are enlightenment and education".[71]
Einstein in 1947
During the final stage of his life, Einstein transitioned to a vegetarian lifestyle,[72]
arguing that "the vegetarian manner of living by its purely physical
effect on the human temperament would most beneficially influence the
lot of mankind".[73]
After the death of Israel's first president, Chaim Weizmann, in November 1952, Prime Minister David Ben-Gurion offered Einstein the position of President of Israel, a mostly ceremonial post.[74] The offer was presented by Israel's ambassador in Washington, Abba Eban, who explained that the offer "embodies the deepest respect which the Jewish people can repose in any of its sons".[54]:522 However, Einstein declined, and wrote in his response that he was "deeply moved", and "at once saddened and ashamed" that he could not accept it:
After the death of Israel's first president, Chaim Weizmann, in November 1952, Prime Minister David Ben-Gurion offered Einstein the position of President of Israel, a mostly ceremonial post.[74] The offer was presented by Israel's ambassador in Washington, Abba Eban, who explained that the offer "embodies the deepest respect which the Jewish people can repose in any of its sons".[54]:522 However, Einstein declined, and wrote in his response that he was "deeply moved", and "at once saddened and ashamed" that he could not accept it:
U.S. citizenship
Einstein became an American citizen in 1940. Not long after settling
into his career at Princeton, he expressed his appreciation of the "meritocracy"
in American culture when compared to Europe. According to Isaacson, he
recognized the "right of individuals to say and think what they
pleased", without social barriers, and as result, the individual was
"encouraged" to be more creative, a trait he valued from his own early
education. Einstein writes:
What makes the new arrival devoted to this country is the democratic trait among the people. No one humbles himself before another person or class. . . American youth has the good fortune not to have its outlook troubled by outworn traditions.[55]:432As a member of the National Association for the Advancement of Colored People (NAACP) at Princeton who campaigned for the civil rights of African Americans, Einstein corresponded with civil rights activist W. E. B. Du Bois, and in 1946 Einstein called racism America's "worst disease".[70] He later stated, "Race prejudice has unfortunately become an American tradition which is uncritically handed down from one generation to the next. The only remedies are enlightenment and education".[71]
World War II and the Manhattan Project
In 1939, a group of Hungarian scientists that included emigre physicist Leó Szilárd attempted to alert Washington of ongoing Nazi atomic bomb research. The group's warnings were discounted.[65] Einstein and Szilárd, along with other refugees such as Edward Teller and Eugene Wigner, "regarded it as their responsibility to alert Americans to the possibility that German scientists might win the race to build an atomic bomb, and to warn that Hitler would be more than willing to resort to such a weapon."[54]:630[66]
In the summer of 1939, a few months before the beginning of World War
II in Europe, Einstein was persuaded to lend his prestige by writing a letter with Szilárd to President Franklin D. Roosevelt
to alert him of the possibility. The letter also recommended that the
U.S. government pay attention to and become directly involved in uranium
research and associated chain reaction research.
The letter is believed to be "arguably the key stimulus for the U.S. adoption of serious investigations into nuclear weapons on the eve of the U.S. entry into World War II".[67] President Roosevelt could not take the risk of allowing Hitler to possess atomic bombs first. As a result of Einstein's letter and his meetings with Roosevelt, the U.S. entered the "race" to develop the bomb, drawing on its "immense material, financial, and scientific resources" to initiate the Manhattan Project. It became the only country to successfully develop an atomic bomb during World War II.
For Einstein, "war was a disease . . . [and] he called for resistance to war." But in 1933, after Hitler assumed full power in Germany, "he renounced pacifism altogether . . . In fact, he urged the Western powers to prepare themselves against another German onslaught."[68]:110 In 1954, a year before his death, Einstein said to his old friend, Linus Pauling, "I made one great mistake in my life — when I signed the letter to President Roosevelt recommending that atom bombs be made; but there was some justification — the danger that the Germans would make them..."[69]
The letter is believed to be "arguably the key stimulus for the U.S. adoption of serious investigations into nuclear weapons on the eve of the U.S. entry into World War II".[67] President Roosevelt could not take the risk of allowing Hitler to possess atomic bombs first. As a result of Einstein's letter and his meetings with Roosevelt, the U.S. entered the "race" to develop the bomb, drawing on its "immense material, financial, and scientific resources" to initiate the Manhattan Project. It became the only country to successfully develop an atomic bomb during World War II.
For Einstein, "war was a disease . . . [and] he called for resistance to war." But in 1933, after Hitler assumed full power in Germany, "he renounced pacifism altogether . . . In fact, he urged the Western powers to prepare themselves against another German onslaught."[68]:110 In 1954, a year before his death, Einstein said to his old friend, Linus Pauling, "I made one great mistake in my life — when I signed the letter to President Roosevelt recommending that atom bombs be made; but there was some justification — the danger that the Germans would make them..."[69]
His affiliation with the Institute for Advance Studies would last until his death in 1955.[64] He was one of the four first selected (two of the others being John von Neumann and Kurt Gödel)
at the new Institute, where he soon developed a close friendship with
Gödel. The two would take long walks together discussing their work. His
last assistant was Bruria Kaufman, who later became a renowned physicist. During this period, Einstein tried to develop a unified field theory and to refute the accepted interpretation of quantum physics, both unsuccessfully.
Other scientists also fled to America. Among them were Nobel laureates and professors of theoretical physics. With so many other Jewish scientists now forced by circumstances to live in America, often working side by side, Einstein wrote to a friend, "For me the most beautiful thing is to be in contact with a few fine Jews—a few millennia of a civilized past do mean something after all." In another letter he writes, "In my whole life I have never felt so Jewish as now."[55]
Other scientists also fled to America. Among them were Nobel laureates and professors of theoretical physics. With so many other Jewish scientists now forced by circumstances to live in America, often working side by side, Einstein wrote to a friend, "For me the most beautiful thing is to be in contact with a few fine Jews—a few millennia of a civilized past do mean something after all." In another letter he writes, "In my whole life I have never felt so Jewish as now."[55]
Emigration to U.S. in 1933
In February 1933 while on a visit to the United States, Einstein
decided not to return to Germany due to the rise to power of the Nazis under Germany's new chancellor.[56][57] He visited American universities in early 1933 where he undertook his third two-month visiting professorship at the California Institute of Technology
in Pasadena. He and his wife Elsa returned by ship to Belgium at the
end of March. During the voyage they were informed that their cottage
was raided by the Nazis and his personal sailboat had been confiscated.
Upon landing in Antwerp
on 28 March, he immediately went to the German consulate where he
turned in his passport and formally renounced his German citizenship.[55]
In early April, he learned that the new German government had passed laws barring Jews from holding any official positions, including teaching at universities.[55] A month later, Einstein's works were among those targeted by Nazi book burnings, and Nazi propaganda minister Joseph Goebbels proclaimed, "Jewish intellectualism is dead."[55] Einstein also learned that his name was on a list of assassination targets, with a "$5,000 bounty on his head."[55] One German magazine included him in a list of enemies of the German regime with the phrase, "not yet hanged".[55]
He resided in Belgium for some months, before temporarily living in England.[58][59] In a letter to his friend, physicist Max Born, who also emigrated from Germany and lived in England, Einstein wrote, ". . . I must confess that the degree of their brutality and cowardice came as something of a surprise."[55]
Portrait taken in 1935 at Princeton
In October 1933 he returned to the U.S. and took up a position at the Institute for Advanced Study at Princeton, New Jersey, that required his presence for six months each year.[60][61]
He was still undecided on his future (he had offers from European
universities, including Oxford), but in 1935 he arrived at the decision
to remain permanently in the United States and apply for citizenship.[62][63]
In early April, he learned that the new German government had passed laws barring Jews from holding any official positions, including teaching at universities.[55] A month later, Einstein's works were among those targeted by Nazi book burnings, and Nazi propaganda minister Joseph Goebbels proclaimed, "Jewish intellectualism is dead."[55] Einstein also learned that his name was on a list of assassination targets, with a "$5,000 bounty on his head."[55] One German magazine included him in a list of enemies of the German regime with the phrase, "not yet hanged".[55]
He resided in Belgium for some months, before temporarily living in England.[58][59] In a letter to his friend, physicist Max Born, who also emigrated from Germany and lived in England, Einstein wrote, ". . . I must confess that the degree of their brutality and cowardice came as something of a surprise."[55]
On his return voyage, he also visited Palestine
for 12 days in what would become his only visit to that region. "He was
greeted with great British pomp, as if he were a head of state rather
than a theoretical physicist", writes Isaacson. This included a cannon
salute upon his arrival at the residence of the British high
commissioner, Sir Herbert Samuel.
During one reception given to him, the building was "stormed by throngs
who wanted to hear him". In Einstein's talk to the audience, he
expressed his happiness over the event:
I consider this the greatest day of my life. Before, I have always found something to regret in the Jewish soul, and that is the forgetfulness of its own people. Today, I have been made happy by the sight of the Jewish people learning to recognize themselves and to make themselves recognized as a force in the world.[55]:308
Travels abroad
Einstein visited New York City for the first time on 2 April 1921, where he received an official welcome by the Mayor,
followed by three weeks of lectures and receptions. He went on to
deliver several lectures at Columbia University and Princeton
University, and in Washington he accompanied representatives of the
National Academy of Science on a visit to the White House. On his return
to Europe he was the guest of the British statesman and philosopher Viscount Haldane in London, where he met several renowned scientific, intellectual and political figures, and delivered a lecture at King's College.[53]
In 1922, he traveled throughout Asia and later to Palestine, as part of a six-month excursion and speaking tour. His travels included Singapore, Ceylon, and Japan, where he gave a series of lectures to thousands of Japanese. His first lecture in Tokyo lasted four hours, after which he met the emperor and empress at the Imperial Palace where thousands came to watch. Einstein later gave his impressions of the Japanese in a letter to his sons:[54]:307 "Of all the people I have met, I like the Japanese most, as they are modest, intelligent, considerate, and have a feel for art."[54]:308
In 1922, he traveled throughout Asia and later to Palestine, as part of a six-month excursion and speaking tour. His travels included Singapore, Ceylon, and Japan, where he gave a series of lectures to thousands of Japanese. His first lecture in Tokyo lasted four hours, after which he met the emperor and empress at the Imperial Palace where thousands came to watch. Einstein later gave his impressions of the Japanese in a letter to his sons:[54]:307 "Of all the people I have met, I like the Japanese most, as they are modest, intelligent, considerate, and have a feel for art."[54]:308
During 1911, he had calculated that, based on his new theory of
general relativity, light from another star would be bent by the Sun's
gravity. That prediction was claimed confirmed by observations made by a
British expedition led by Sir Arthur Eddington during the solar eclipse of 29 May 1919. International media reports of this made Einstein world famous. On 7 November 1919, the leading British newspaper The Times printed a banner headline that read: "Revolution in Science – New Theory of the Universe – Newtonian Ideas Overthrown".[48]
Much later, questions were raised whether the measurements had been
accurate enough to support Einstein's theory. In 1980 historians John Earman and Clark Glymour published an analysis suggesting that Eddington had suppressed unfavorable results.[49]
The two reviewers found possible flaws in Eddington's selection of
data, but their doubts, although widely quoted and, indeed, now with a
"mythical" status almost equivalent to the status of the original
observations, have not been confirmed.[50][51] Eddington's selection from the data seems valid and his team indeed made astronomical measurements verifying the theory.[52]
In 1921, Einstein was awarded the Nobel Prize in Physics for his explanation of the photoelectric effect, as relativity was considered still somewhat controversial. He also received the Copley Medal from the Royal Society in 1925.
In 1921, Einstein was awarded the Nobel Prize in Physics for his explanation of the photoelectric effect, as relativity was considered still somewhat controversial. He also received the Copley Medal from the Royal Society in 1925.
Academic career
By 1908, he was recognized as a leading scientist, and he was appointed lecturer at the University of Bern. The following year, he quit the patent office and the lectureship to take the position of physics docent [44] at the University of Zurich. He became a full professor at Karl-Ferdinand University in Prague in 1911. In 1914, he returned to Germany after being appointed director of the Kaiser Wilhelm Institute for Physics (1914–1932)[45] and a professor at the Humboldt University of Berlin, with a special clause in his contract that freed him from most teaching obligations. He became a member of the Prussian Academy of Sciences. In 1916, Einstein was appointed president of the German Physical Society (1916–1918).[46][47]
Patent office
After graduating, Einstein spent almost two frustrating years searching for a teaching post, but Marcel Grossmann's father helped him secure a job in Bern,[37] at the Federal Office for Intellectual Property, the patent office, as an assistant examiner.[38] He evaluated patent applications
for electromagnetic devices. In 1903, Einstein's position at the Swiss
Patent Office became permanent, although he was passed over for
promotion until he "fully mastered machine technology".[39]
Much of his work at the patent office related to questions about transmission of electric signals and electrical-mechanical synchronization of time, two technical problems that show up conspicuously in the thought experiments that eventually led Einstein to his radical conclusions about the nature of light and the fundamental connection between space and time.[40]
With a few friends he met in Bern, Einstein started a small discussion group, self-mockingly named "The Olympia Academy", which met regularly to discuss science and philosophy. Their readings included the works of Henri Poincaré, Ernst Mach, and David Hume, which influenced his scientific and philosophical outlook.
Much of his work at the patent office related to questions about transmission of electric signals and electrical-mechanical synchronization of time, two technical problems that show up conspicuously in the thought experiments that eventually led Einstein to his radical conclusions about the nature of light and the fundamental connection between space and time.[40]
With a few friends he met in Bern, Einstein started a small discussion group, self-mockingly named "The Olympia Academy", which met regularly to discuss science and philosophy. Their readings included the works of Henri Poincaré, Ernst Mach, and David Hume, which influenced his scientific and philosophical outlook.
Langganan:
Postingan (Atom)