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1 Einstein’s Methods John D. Norton partment of History and Philosophy of Science University of Pittsburgh

1 Einstein’s Methods John D. Norton Department of History and Philosophy of Science University of Pittsburgh

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Page 1: 1 Einstein’s Methods John D. Norton Department of History and Philosophy of Science University of Pittsburgh

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Einstein’s MethodsJohn D. Norton

Department of History and Philosophy of ScienceUniversity of Pittsburgh

Page 2: 1 Einstein’s Methods John D. Norton Department of History and Philosophy of Science University of Pittsburgh

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What can we know of how Einstein made his discoveries?

1905 Special relativity1905 Light quantum1905 Atoms/Brownian motion1906 Specific heats1909 Wave particle duality1907-1915 General relativity1916 Gravitational waves1916 “A and B” coefficients1917 Relativistic cosmology1924-25 Bose Einstein statistics…and more

Inscrutable flashes of insight

ormethodical

exploration?

This talk.

Einstein thought a great deal about his methods.They changed almost completely in his lifetime.Through a remarkable manuscript, we can look over Einstein’s shoulder and watch the struggle unfold.

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The view of Einstein’s work on general relativity as driven by the tension of physical and formal ways of thinking was developed in a collaborative research group working on Einstein’s Zurich Notebook of 1912-1913 at the Max Planck Institut für Bildungsforschung and then at the Max Planck Institut für Wissenschaftgeschichte.

Michel Janssen, John Norton, Jürgen Renn, Tilman Sauer, John Stachel, et al.

General Relativity in the Making:Einstein's Zurich Notebook.

Vol. 1 The Genesis of General Relativity: Documents and Interpretation.

Vol. 2 The Genesis of General Relativity.

Vol. 3

Vol.4.

Dordrecht: Kluwer.

available now

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Exploit formal (usually mathematical) properties of emerging theory.Covariance principles. Group structure.

Theory construction via mathematical theorems. Geometrical methods assure automatic covariance.

Formal naturalness.

Extreme case: choose mathematically simplest law.

Based on physical principles with evident empirical support.

Principle of relativity. Conservation of energy.

Special weight to secure cases of clear physical meaning.

Newtonian limit. Static gravitational fields in GR.

Physical naturalness.

Extreme case: thought experiments direct

theory choice.

Physical versus Formalapproach approach

Considerable overlap. Often both are the same inferences in different guises.

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Physical approach illustrated

Principle of relativity requires that the electromagnetic field manifests as different mixtures of magnetic field B and electric field E according to motion of observer.

Based on Einstein’s 1905 magnet-conductor thought experiment.

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Formal approach illustrated

Write Maxwell’s equations using four-vector and six-vector (now antisymmetric second rank tensor) quantities and operators of Minkowski’s 1908 spacetime, geometrical approach.Satisfaction of the principle of relativity is automatic. €

∂F*ik

∂xk= 0

∂Fik

∂xl+

∂Fli

∂xk+

∂Fkl

∂xi= 0

Fik =

0 Bz −By −iEx

−Bz 0 Bx −iEy

By −Bx 0 −iEz

iEx iEy iEz 0

⎢ ⎢ ⎢ ⎢

⎥ ⎥ ⎥ ⎥

F 'ik =

0 B'z −B'y 0

−B'z 0 B'x 0

B'y −B'x 0 0

0 0 0 0

⎢ ⎢ ⎢ ⎢

⎥ ⎥ ⎥ ⎥

Sign and coordinate conventions after Pauli, Theory of Relativity, p. 78.

Lorentz transformation

Hyperbolic rotation in spacetime mixes

E’s and B’sPure magnetic field

Mixed magnetic and electric field

Frame dependence of decomposition of electromagnetic field is a consequence of spacetime geometry.

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Evolution of Einstein’s approaches

1902-1904 statistical physics1905 Brownian motion1905 Light quantum1905 Special relativity1906 Specific heats1909 Wave particle duality 1907-1915 General relativity1916 A and B coefficients1917 Relativististic cosmology1924-25 Bose-Einsteinstatistics1935 EPR

Phy

sica

lF

ormal

Five dimensional        unified field 1922-41 Distant parallelism 1928Bivector fields 1932-33

Unified field via non-       symmetric connection 1925- 1955

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Einstein’s early distain for higher mathematics in physics

Special relativity, light quantum use only calculus of many variables.

Marked reluctance to adopt Minkowski’s four-dimensional methods. He does not use them until 1912.

Quip: “I can hardly understant Laue’s book” [1911 textbook on special relativity that used Minkowski’s methods].

Four-dimensional methods disparaged as “superfluous learnedness.”

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Abraham’s 1912 theory of gravity…

Abraham’s theory is the simplest mathematically delivered by four-dimensional methods.

∂2Φ

∂x2+

∂2Φ

∂y2+

∂2Φ

∂z2+

∂2Φ

∂u2= 4πγν u=ict

Fx = −∂Φ∂x

, etc.where c=c )…Einstein’s idea!

…is condemned by Einstein for its purely formal basis.

“[it] has been created out of thin air, i.e. out of nothing by considerations of mathematical beauty, and is completely untenable.” (To Besso)

“totally untenable” (To Ehrenfest)

“incorrect is every respect” (To Lorentz)

“totally unacceptable” (To Wien)

“totally untenable” (To Zangger)

“…at the first moment (for 14 days) I too was totally “bluffed” by the beauty and simplicity of its formulas.” (To Besso)

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General relativity begins to turn the tide

In 1912, Einstein began work on the precursor to general relativity, the “Entwurf” theory of 1913 with the

mathematical assistance of Marcel Grossmann, who introduced Einstein to Ricci and Levi-Civita’s “absolute

differential calculus” (now called tensor calculus).

“I am now working exclusively on the gravitation problem and believe that I can overcome all difficulties with the help of a mathematician friend of mine here [Marcel Grossmann]. But one thing is certain: never before in my life have I toiled any where near as much, and I have gained enormous respect for mathematics, whose more subtle parts I considered until now, in my ignorance, as pure luxury. Compared with this problem, the original theory of relativity is child's play.”

Einstein to Sommerfeld, October 1912

Sommerfeld: edited Minkowski’s papers and wrote introductory papers on four-dimensional methods.

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Einstein and Grossmann’s “Entwurf…” 1913

Complete framework of general theory of relativity. Gravity as curvature of spacetime geometry.

One thing is missing…

The Einstein equations!

Gik = k (Tik – (1/2) gik T)

Gik = 0 source free case

Ricci tensor Gik is first contraction of Riemann curvature tensor Riklm

(Yes--the notation is non-standard.)

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The “Einstein Equations” are approached…

Einstein and Grossman present gravitational field equations that are not generally covariant and have no evident geometrical meaning.

Riemann curvature tensor“Christoffel’s four-index-symbol”

Its first contraction as the unique tensor candidate for inclusion is gravitational field equations.

“But it turns out that this tensor does not reduce to the [Newtonian] in the special case of an infinitely weak, static gravitational field.”

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Einstein’s “Zurich Notebook” A notebook of calculation Einstein kept while he worked on the “Entwurf” theory with Grossmann.

Einstein worked from both ends.

Einstein expected the physical and formal/mathematical approaches to give the same result.

When he erroneously thought they

did not, he chose the physical approach over the formal and selected equations that would torment him for over two years.

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Inside the cover…

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Einstein connects gravity and curvature of spacetime.

Einstein writes the spacetime metric for the first time as

ds2 = G dx dxG soon becomes g

p. 39L

Importing of special case of his 1907-1912 theory in which a variable c is the gravitational potential.

First attempts at gravitational field equations based on

physical reasoning of 1907-1912 theory.

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The physical approach to energy-momentum conservation…

Equations of motion for a speck of dust (geodesic)

Expressions for energy-momentum density and four-force density for a cloud of dust.

Combine: energy-momentum conservation for dust

∂∂xμμν

∑ gmν Θμν( ) − 12

∂gμν

∂xmμν∑ Θμν = 0

Rate of accumulation

energy-momentum

Force density

p.5R

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…and the formal approach to energy-momentum conservation.

∂∂xμμν

∑ gmν Θμν( ) − 12

∂gμν

∂xmμν∑ Θμν = 0

Is the conservation law

of the form

differential

operator

⎝ ⎜

⎠ ⎟Θ = 0?

Check: form

differential

operator

⎝ ⎜

⎠ ⎟metric

tensor

⎝ ⎜

⎠ ⎟

It should be 0 or a four-vector.

It vanishes!

Stimmt!p.5R

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The formal approach to the gravitational field equations

Following pages: Einstein shows how to select coordinate systems so that they do vanish.

p. 14L

Einstein writes the Riemann curvature tensor for the first time… with Grossmann’s help.

First contraction formed.

To recover Newtonian limit, three terms “should have vanished.”

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Failure of the formal approach

Einstein finds multiple problems with the gravitational field equations based on the Riemann curvature tensor.

“Special case [of the 1907-1912 theory] apparently incorrect”

p. 21R

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“Entwurf” gravitational field equations

Derived from a purely physical approach. Energy-momentum conservation.

pp. 26L-R

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Einstein’s short-lived methodological moral of 1914

The physical approach is superior to the formal approach.

“At the moment I do not especially feel like working, for I had to struggle horribly to discover what I described above. The general theory of invariants was only an impediment. The direct route proved to be the only feasible one. It is just difficult to understand why I had to grope around for so long before I found what was so near at hand.”

Einstein to Besso, March 1914

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Einstein snatches triumph from near disaster: Fall 1915.

David Hilbert in Göttingen applies formal methods to general field equations for Einstein’s theory

... and Einstein knows it.

Communications to the Göttingen Academy:Nov. 4 Almost generally covariant

field equations

Nov. 11 Almost generally covariant field equations

Nov. 18 Explanation of Mercury’s perihelion motion

Nov. 26 Einstein equations

Einstein realizes his “Entwurf” field equations are wrong and returns to seek generally covariant equations.

Communications to the Prussian Academy:

Nov. 20 Something very close to Einstein’s equations

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Einstein’s new methodological moral

Triumph of formal methods over physical considerations.

“Hardly anyone who has truly understood it can resist the charm of this theory; it signifies a real triumph of the method of the general differential calculus, founded by Gauss, Riemann, Christoffel, Ricci and Levi-Civita.”

Communication to Prussian Academy of Nov. 4, 1915

“I had already taken into consideration the only possible generally covariant equations, which now prove to be the right ones, three years ago with my friend Grossmann. Only with heavy hearts did we detach ourselves from them, since the physical discussion had apparently shown their incompatibility with Newton's law.”

Einstein to Hilbert Nov 18, 1915

“This time the most obvious was correct; however Grossmann and I believed that the conservation laws would not be satisfied and that Newton's law would not come out in the first approximation.”

Einstein to Besso, Dec. 10, 1915

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Hesitations

“Except for the agreement with reality, it is in any case a grand intellectual achievement.”

Einstein to Hermann Weyl, Apr. 6, 1918, on Weyl’s mathematically most natural, geometric unification of gravity and electromagnetism“It seems to me that you overrate

the value of formal points of view. These may be valuable when an already found truth needs to be formulated, but fail always as heuristic aids.”

Einstein to Felix Klein, 1917, on the conformal invariance of Maxwell’s equations

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Experience may suggest the appropriate mathematical concepts, but they most certainly cannot be deduced from it. Experience remains, of course, the sole criterion of the physical utility of a mathematical construction. But the creative principle resides in mathematics. In a certain sense, therefore, I hold it true that pure thought can grasp reality, as the ancients dreamed.”

Einstein’s manifesto of June 10, 1933

“If, then, it is true that the axiomatic basis of theoretical physics cannot be extracted from experience but must be freely invented, can we ever hope to find the right way? Nay, more, has this right way any existence outside our illusions? Can we hope to be guided safely by experience at all when there exist theories (such as classical mechanics) which to a large extent do justice to experience, without getting to the root of the matter?

Herbert Spenser Lecture, "On the Methods of Theoretical Physics," University of Oxford

I answer without hesitation that there is, in my opinion, a right way, and that we are capable of finding it. Our experience hitherto justifies us in believing that nature is the realization of the simplest conceivable mathematical ideas. I am convinced that we can discover by means of purely mathematical constructions the concepts and the laws connecting them with each other, which furnish the key to the understanding of natural phenomena.

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“I have learned something else from the theory of gravitation:no collection of empirical facts however comprehensive can ever lead to the setting up of such complicated equations [as non-linear field equations of the unified field]. A theory can be tested by experience, but there is no way from experience to the construction of a theory. Equations of such complexity as are the equations of the gravitational field can be found only through the discovery of a logically simple mathematical condition that determines the equations completely or almost completely. Once one has obtained those sufficiently strong formal conditions, one requires only little knowledge of facts for the construction of the theory; in the case of the equations of gravitation it is the four-dimensionality and the symmetric tensor as expression for the structure of space that, together with the invariance with respect to the continuous transformation group, determine the equations all but completely.”

Einstein’s search for unified field theory

Autobiographical Notes, 1946

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A concluding puzzle

"If you want to find out anything from the theoretical physicists about the methods they use, I advise you to stick closely to one principle: don't listen to their words, fix your attention on their deeds."

Einstein’s manifesto begins:

Why does he say this?!

To lessen the shock of the extraordinary view he is about to present that so fully contradicts the then present mainstream of philosophical thought?

Or to induce you to look at what physicists--Einstein and others--actually do so you come to reject the mainstream in favor of Einstein’s view?