Lessons from Einstein’s 1915 discovery of general relativity

Lee Smolin
There is a myth that Einstein’s discovery of general relativity was due to his following beautiful mathematics to discover new insights about nature. I argue that this is an incorrect reading of the history and that what Einstein did was to follow physical insights which arose from asking that the story we tell of how nature works be coherent.
1 The lessons of general relativity
2 Following Einstein’s path
3 Going beyond the standard model: which legacy to follow?
4 The search for new principles
5 Einstein’s unique approach to physics
…

Is E=mc^2 an exclusively relativistic result?

Qing-Ping Ma
The mass-energy formula E=mc2 is thought to be derived by Einstein from special relativity. The present study shows that since the formula has also been derived from classical physics by Einstein, it is not an exclusively relativistic result. The formula is implied by the classical electromagnetic momentum P=E/c and the Newtonian definition of momentum P=mv. Like momentum P=mv, E=mc2 applies to both classical physics and special relativity, if relativistic mass is used in the equation. The derivation by Einstein in 1905 is logically flawed as a relativistic proof and the truly relativistic formula should be E=E0/(1-v2/c2)1/2 derived by Laue in 1911 and Klein in 1918. If the energy measured in one reference frame is E0, it is E=E0/(1-v2/c2)1/2 in a reference frame moving at velocity v relative to the first frame….


General Relativity Still Making Waves

This year marks the 100th anniversary of Einstein’s general theory of relativity. In a series of papers published in November 1915 [1] and May 1916 [2], Einstein upended the Newtonian concept of gravitation as a force acting instantaneously over a great distance, and replaced it with the idea that gravity is “geometry,” a consequence of the curvature or warpage of space and time. Einstein’s theory has completely transformed our view of space, time, and the Universe. But it was only the beginning of a story that physicists are still writing.

Einstein and his general theory became celebrities in November 1919, when newspapers worldwide proclaimed “Einstein’s theory triumphs.” The occasion was the report by British astronomers that they had measured the bending of starlight by the Sun. The researchers had analyzed photographs of stars near the Sun during a total eclipse and found that the tiny displacements of their images, with respect to reference photographs, agreed better with Einstein’s theory than with Newton’s, which predicted half the effect [3]. Subsequent eclipse measurements tended to confirm Einstein, but some physicists and astronomers remained skeptical [4]. While Einstein’s theory successfully accounted for an anomaly in the orbit of Mercury, a third test of the theory, called the gravitational redshift, was initially a bust. Two 1917 observations failed to detect the predicted shift in the Sun’s spectral lines. It wasn’t until 1960 that the effect was finally measured in a laboratory experiment involving gamma rays [5].

The difficulty in testing the theory led many to think its effects were too small to be relevant, and, during the 1920s and 30s, interest in the theory declined. By 1960 it was relegated to the backwaters of physics and astronomy. The discovery of quasars in the early 1960s changed all this. The unprecedented outpouring of energy from these enigmatic objects required a powerful source, and some scientists turned to the relativistic black hole, the ultimate spacetime warper, for a solution. Technological advances and the advent of space exploration provided new tools that could properly test general relativity. Thus began a general relativity renaissance [6].

Today general relativity is at the forefront of physics and astronomy [7,8], and may be key to answering the big questions of our time: What is the origin of our Universe and what will its fate be? What does gravity look like on quantum scales? What are black holes? General relativity is now “big” science, involving kilometer-scale observatories designed to detect gravitational waves [9], and the world’s largest supercomputers are simulating the mergers of black holes [10]. Ideas from general relativity are feeding back into other fields like condensed matter and nuclear physics, which use Einstein’s mathematics to solve otherwise intractable problems [11]. The theory has found its way into daily life: relativistic effects must be accounted for if global positioning systems are to work properly [12,13]. It is even seeping into popular culture with general relativity featuring in Hollywood movies like Interstellar and The Theory of Everything.

The next century of general relativity looks to be as exciting as the first. The anticipated detection of gravitational waves should yield further confirmation of Einstein’s theory, and provide new ways of observing the Universe. More detailed studies of black holes may uncover how they form, grow, and whether their strong warping of space-time is as Einstein predicted. And theorists will continue to seek a formulation of gravity—possibly different from Einstein’s 1915 version—that achieves the long-sought quantum theory of gravity.

Clifford Will
Department of Physics,
University of Florida,
P.O. Box 118440,
Gainesville, Florida 32611-8440, USA

[1] A. Einstein, Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften, pp. 778–786, 799-801, 831-839, 844–847 (Berlin, 1915).
[2] A. Einstein, Die Grundlage der allgemeinen Relativitätstheorie, Ann. Phys. (Berlin) 354, 769 (1916).
[3] C. M. Will, The 1919 measurement of the deflection of light, Classical Quantum Gravity 32, 124001 (2015).
[4] J. Crelinsten, Einstein’s Jury: The Race to Test Relativity (Princeton University Press, Princeton, NJ, 2006).
[5] R. V. Pound and G. A. Rebka, Apparent Weight of Photons, Phys. Rev. Lett. 4, 337 (1960).
[6] C. M. Will, Was Einstein Right? Putting General Relativity to the Test (Basic Books, New York, 1993).
[7] General Relativity and Gravitation: A Centennial Perspective, edited by A. Ashtekar , (Cambridge University Press, Cambridge, England, 2015).
[8] C. M. Will, Focus issue: Milestones of general relativity, Classical Quantum Gravity 32, 124001 (2015).
[9] R. X. Adhikari, Gravitational radiation detection with laser interferometry, Rev. Mod. Phys. 86, 121 (2014).
[10] J. Centrella, J. G. Baker, B. J. Kelly, and J. R. van Meter, Black-hole binaries, gravitational waves, and numerical relativity, Rev. Mod. Phys. 82, 3069 (2010).
[11] S. A. Hartnoll, Lectures on holographic methods for condensed matter physics, Classical Quantum Gravity 26, 224002 (2009).
[12] C. M. Will, Einstein’s Relativity and Everyday Life, Physics Central Writers’ Gallery,
[13] N. Ashby, Relativity and the global positioning system, Phys. Today 55, 41 (2002).

Read also: 2015 – General Relativity’s Centennial


Steady-state cosmology: from Einstein to Hoyle

Cormac O’Raifeartaigh, Simon Mitton
We recently reported the discovery of an unpublished manuscript by Albert Einstein in which he attempted a ‘steady-state’ model of the universe, i.e., a cosmic model in which the expanding universe remains essentially unchanged due to a continuous formation of matter from empty space. The manuscript was apparently written in early 1931, many years before the steady-state models of Fred Hoyle, Hermann Bondi and Thomas Gold. We compare Einstein’s steady-state cosmology with that of Hoyle, Bondi and Gold and consider the reasons Einstein abandoned his model. The relevance of steady-state models for today’s cosmology is briefly reviewed.

To explain why a fth dimension might be unobserved in everyday life, Einstein and Bergmann describe a long thin tube, as sketched here. (The drawing that actually appears in their paper shows instead
a thin at strip, which illustrates the same idea.)

A Note On Einstein, Bergmann, and the Fifth Dimension

 To explain why a fth dimension might be unobserved in everyday life, Einstein and Bergmann describe a long thin tube, as sketched here. (The drawing that actually appears in their paper shows instead a thin at strip, which illustrates the same idea.)

To explain why a fifth dimension might be unobserved in everyday life, Einstein and Bergmann describe a long thin tube, as sketched here. (The drawing that actually appears in their paper shows instead
a thin at strip, which illustrates the same idea.)

Edward Witten
This note is devoted to a detail concerning the work of Albert Einstein and Peter Bergmann on unified theories of electromagnetism and gravitation in five dimensions.
In their paper of 1938, Einstein and Bergmann were among the first to introduce the modern viewpoint in which a four-dimensional theory that coincides with Einstein-Maxwell theory at long distances is derived from a five-dimensional theory with complete symmetry among all five dimensions.
But then they drew back, modifying the theory in a way that spoiled the five-dimensional symmetry and looks contrived to modern readers.
Why? According to correspondence of Peter Bergmann with the author, the reason was that the more symmetric version of the theory predicts the existence of a new long range field (a massless scalar field).
In 1938, Einstein and Bergmann did not wish to make this prediction. (Based on a lecture at the Einstein Centennial Celebration at the Library of Alexandria, June, 2005.


How Einstein Discovered Dark Energy

Alex Harvey
In 1917 Einstein published his Cosmological Considerations Concerning the General Theory of Relativity. In it was the first use of the cosmological constant. Shortly thereafter Schröodinger presented a note providing a solution to these same equations with the cosmological constant term transposed to the right hand side thus making it part of the stress-energy tensor. Einstein commented that if Schröodinger had something more than a mere mathematical convenience in mind he should describe its properties. Then Einstein detailed what some of these properties might be. In so doing, he gave the first description of Dark Energy. We present a translation of Schrödinger’s paper and Einstein’s response….
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Read also: The Cosmological Constant


5 Of Physics’s Greatest Sex Scandals

Physicists need love, too. Just ask Paul Frampton, the physics professor who was sentenced recently after an alleged scam involving drugs and a bikini model.
We know it can be hard to resist the temptation of bikini models on the Internet, but physicist Paul Frampton was duped pretty bad. The University of North Carolina professor flew to Bolivia to meet up with model Denise Milani, but Milani never showed up. Instead, a man with a briefcase claiming to be Milani’s intermediary sent Frampton on a drug smuggling mission. Frampton was arrested before he made it back the United States and convicted last week. We’re all fools in love, huh?

Frampton isn’t the only physicist to get caught up in a love scandal. Though most of them haven’t ended up in an Argentine prison, some did have awkward run-ins with the media. Check out these physicists who probably wish their sex lives were as invisible as dark matter.

Albert Einstein’s theory of relatives
The father of relativity wasn’t very good to his second first wife, Mileva Maric. He made her do all the housework, and in return, she got… well, nothing much in the love department. That’s because he was too busy taking lovers, including his cousin Elsa whom he later married. When asked about his love life, he would probably say, “It’s all relatives.” Zing!

Marie Curie’s radioactive love
Apparently, two Nobel prizes aren’t enough to get people off your back about that one affair you had. After Marie Curie’s husband died, she fell in love with his former student, Pierre Langevin. The man was married, so the French press made a big stink about it and started calling her a homewrecker and a Jew. For the record, Curie was not cheating on anyone herself (and was also not Jewish.)

Erwin Schrodinger’s mistresses
Here we have another physicist who wanted little do with his wife. Austrian physicist Erwin Schrodinger had several mistresses, one being the wife of his assistant, Arthur March. The weird part: March was cool with it and stepped in as the father of the child while his wife Hilde moved into the Schrodinger household.

Stephen Hawking and the sex clubs
It doesn’t really seem fair to pick on Hawking for a few reasons, the main one being that he currently doesn’t have a wife to cheat on, but the media did it anyway. Hawking apparently frequents the sex clubs, and the only reason that’s a scandal is because it is now horrendously public. No one’s getting hurt here, at the very least.
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