The Renewal of Einstein's Theory of Relativity in the Post-War Era


Albert Einstein in Vienna (1921); Wikimedia Commons.

The Renewal of Einstein's Theory of Relativity in the Post-War Era

Historians of Science at Department I of the MPIWG research the reinvention of Einstein’s Theory in the Post-War Era.

In November 1915, Albert Einstein published his theory of gravitation, thus attaining international renown which was to last unfailingly until the present day, long after his death. The history of his general theory of relativity, however, took a different course. It lost its appeal in the 1920s and did not experience a resurgence until the mid-1950s. Researchers at the Max Planck Institute for the History of Science have traced this surprising development.

In 2015, the general theory of relativity will be 100 years old. In November 1915, Albert Einstein gave weekly lectures to the Prussian Academy of Sciences in which he set out the fundamental field equations of his new theory and explained its application to the precession of the perihelion of Mercury.

Four years later, one of the basic predictions of the theory – the bending of light in the gravitational field of the sun – was impressively confirmed by a solar eclipse expedition on the island of Principe, which was led by Arthur S. Eddington. Einstein became, almost overnight, an international celebrity, and has been regarded as the epitome of the brilliant scientist ever since.

This unparalleled success story is often recounted and has been researched in great detail. Less well known is the subsequent history of the general theory of relativity which – in contrast to its sensational beginnings – took a somewhat surprising turn. Historian of Science Jean Eisenstaedt has shown that after the initial hype, interest in and research into the theory ebbed into a “low-watermark period”. This phase lasted from roughly the mid-1920s to the mid-1950s.

The low point was followed by a vigorous resurgence of interest, which physicist Clifford Will describes as the “renaissance” of the general relativity theory: Until then, the theory was used mainly to calculate minute corrections to the predictions of the Newtonian gravitational theory within our solar system. Now it became important for describing distant celestial bodies as well.


The image of a distant galaxy is distorted into a so-called Einstein Ring, due to the gravitational lensing effect, first predicted by Einstein himself on the basis of his general theory of relativity; Wikimedia Commons.

Their unexpected properties could be explained with the help of concepts newly derived from the theory: for example, the model of a black hole – an astronomical object with a gravitational field so strong that not even light can escape it.

The general theory of relativity returned to centre stage in the 1960s and 1970s. A half century after Einstein’s triumph, researchers who dealt with this theory and with black holes became the new superstars of physics – foremost among them the British physicist Stephen Hawking.

With the aim of studying these historical dynamics, Department I of the Max Planck Institute for the History of Science has established a Working Group in which historians of modern physics and international experts in general relativity and its history are combining their efforts. This work – partly in preparation for a major conference that is to be held on the occasion of the theory’s centennial in November (together with the Albert Einstein Institute in Potsdam-Golm) – is currently in full swing, and the project will present first results in the upcoming issue of Isis (authors: Alexander Blum, Roberto Lalli, Jürgen Renn).

These results have already shed light on the above-mentioned decline and subsequent resurgence of general relativity. The changed conditions for the sciences – and specifically physics – after World War II and during the Cold War are of course a major factor. After physicists had demonstrated their importance to national security by building the atomic bomb, a great deal of money flowed into physics research in the post-war years, and the number of young physics graduates surged on an unprecedented scale.

At the same time, technologies developed during the war opened up whole new fields of research. For example, methods developed in radar research to detect radio waves were now used to observe celestial bodies that did not happen to emit radiation in the spectral range perceived by the human eye, giving rise to the field of radio astronomy. In the early 1960s, the new field of study provided proof of distant star-like objects whose properties differ fundamentally from those of our sun: Despite being billions of light-years away, these quasars, as they became known, emit such powerful radiation that they can be detected by radio telescopes. In the context of general relativity, they were soon interpreted as black holes in the making.

However, it was by no means certain that research into general relativity could benefit from the boom in physics. Around 1950, general relativity was regarded as a highly esoteric and unproductive field. Nor could it have benefited directly from new astronomical observations, since new theoretical concepts to explain those observations had already been worked out in the late 1950s and early 1960s. In order to benefit from these developments, physicists first had to re-invent the general relativity theory.

During the decades of neglect, the general relativity theory was essentially a field of mathematical and philosophical interest: Remote from concrete physical questions and highly complex in structure, the Einstein field equations provided a fertile field of activity for mathematicians.

At the same time, with its novel concept of curved spacetime, the theory formed the basis for experiments for elaborating a unified theory of the whole of physics or a theory that could explain the development of the universe as a whole (cosmology). However, these early experiments were driven principally by fundamental philosophical questions and had little to do with mainstream physics research.


This nearly perfect sphere was used in the Gravity Probe B satellite experiment to test the curvature of spacetime near earth, as predicted the general theory of relativity. Here it is seen refracting an image of that theory's inventor; Wikimedia Commons.

That all began to change in the 1950s: New mobility made it easier for international scientists to meet who, until that time, were working  in relative isolation on peripheral problems of physics relating to general relativity. A key event was a conference in Bern in 1955, which proved to be a starting point for the establishment of an international community of physicists who call themselves “relativists”.

The conference was held on the occasion of the 50th anniversary of the special theory of relativity. Of course, Albert Einstein was invited as a guest of honour. His death several months before the conference was taken as a sign by the participants that it was now up to them to continue the Einstein tradition.

To a certain extent, the institutionalisation of this community in subsequent years – through regular conferences, specialist journals and a lively exchange of young scientists between the far-flung centres of this research – followed the model of established subdisciplines of physics, such as nuclear physics. However, in comparison to nuclear physicists, the general relativity and gravitation community had to invent itself from scratch to a much greater extent. For this reason, it was a pioneer in the field of international networking.

In order to create such a community, physicists first had to formulate common questions. In the process, an increased number of physical questions came to the fore. One example is the calculation and possible proof of the existence of gravitational waves; another, the nature of gravitational fields of very dense, massive stars.

These questions brought relativists in contact with other subdisciplines of physics, as such dense objects could be – and in fact had to be – described using nuclear physics methods. The relativists developed the theoretical concepts which, in the wake of astronomical discoveries in the early 1960s, impressively established the general relativity theory as an empirical physical theory with an unexpected scope of applications – a status that has been consolidated in the intervening 50 years.

Further Information

Watch the talks given at the conference “A Century of General Relativity.” Go to Media Library

In the context of the centenary of the General Theory of Relativity, the MPIWG received a wide attention in the media. Read more

“Albert Einstein - Genie und Grenzgänger,” a podcast-series with Alexander Blum about the Theory of Relativity. Podcast Oct 29/ Nov 06, 2015

A chronology of the milestones of the theory of general relativity. Download

On the occasion of the anniversary, a joint conference of physicists and historians of science takes place in Berlin from 30.11.–05.12.2015. To Conference Website

In occasion of the 100th anniversary of Einstein's formulation of general relativity in Berlin, the Max Planck Institute for the History of Science promotes a conference from 02.12.–05.12.2015. Go to Conference Website

The MPIWG commissioned the play " Transcendence " by Marc Robert Friedman about Einstein and the theory of relativity. It is performed from 20.11.–1.12. at the English Theatre Berlin. Go to Website

15th Einstein Lecture Dahlem: K.S. Thorne is giving a lecture titled “A Century of Einstein’s Relativity: From the Big Bang to Black Holes and “Interstellar”” (in English) on 25.11.2015. The Einstein Lectures Dahlem are organized by the FU Berlin and the MPG. Go to Website

Blum, Alexander S.: QED and the man who didn’t make it: Sidney Dancoff and the infrared divergence. – In: Studies in History and Philosophy of Modern Physics. – 50 (2015), p. 70–94. Go to Article

Hanoch Gutfreund and Jürgen Renn have recently published two new books on Einstein. The Road to Relativity and Relativity: The Special and the General Theory

Princeton University Press provides a database of The Collected Papers of Albert Einstein. Go to Database

See a selection of articles and interviews published in the context of the anniversary. Go to Media & Press

German version of this research topic

Download print version of this research topic

Research Topics Archive

Bathymetry model of the Strait of Gibraltar ca. 1932, Instituto Español de Oceanografía.
50: The Strait in the Cold War—Deep Science and Global Geopolitics in the Mediterranean
Andreas Ryff, Münz- und Mineralienbuch, 1594. Autograph in possession of the Basel University Library (A lambda II 46a).
49: Mountain Clamor! Resource Flows and Metal Culture in Early Modern Mining
Parades of Miners, Craftsmen, and Officials Marking the Marriage of Friedrich August II, Elector of Saxony, and Maria Josepha, Archduchess of Austria in 1719. Bergakademie Freiberg.
48: Data and Decisions in Early Modern Mines
Transcript of a Bobolink song by Ferdinand S. Mathews (1904), Field Book of Wild Birds and Their Music: A Description of the Character and Music of Birds.
47: Scientific Scores and Musical Ears: Sound Diagrams in Field Recording
School of Athens
46: Early Modern Adaptation of the Aristotelian Mechanics
better shelter
45: Refugee Housing
44: Mapping Climatology
Black Hole Merger
43: One Hundred Years of Gravitational Waves
42: How High Is the Sea?
41: The Renewal of Einstein's Theory of Relativity in the Post-War Era
40: Do Data Have Politics?
39: From Sound to Knowledge
38: Colours and Their Context
37: Is Bigger Better
36: Rooting Language Family Trees
35: Making Genetics Human
34: Galileo's Laboratory of Ideas
33: Historicizing Big Data
32: Ancient Balances at the Nexus of Innovation and Knowledge
31: Looking at Diversity
30: How Recipes Created Knowledge in Early Modern Households
29: Metallurgy, Ballistics and Epistemic Instruments
28: Science under Scrutiny
27: The Globalization of Knowledge and its Consequences
26: Parts Unknown: Making the Familiar Strange
25: Apprehending Human Difference and Population Size
24: Endangerment and Its Consequences
23: The Equilibrium Controversy
22: Art and Knowledge in Pre-Modern Europe
21: Knowledgescapes
20: Baby Science in fin-de-siècle America
19: Let him reconquer language
18: Histories of Scientific Observation
17: On Historicizing Epistemology : an essay
16: Johann Lambert's Conversion to a Geometry of Space
15: The Uncertain Boundaries between Light and Matter
14: Every move will be recorded
13: Courting the Crafts in Qing China
12: The Concepts of Immanuel Kant's Natural Philosophy
11: Jean Piaget and the Child's Spontaneous Geometry
10: Galileo and the Others
9: Historicizing Knowledge about Human Biodiversity
8: Dreaming in and of Neurophilosophy
7: Who Were Einstein's Opponents?
6: Physiology of the piano
5: Numbering Bees
4: New Ways of Using Digital Images
3: Telling Instruments
2: Microscope Slides: An Object of the History of Science?
1: What (Good) is Historical Epistemology?