Relativistic Cosmology
Applies general relativity to the universe and introduces the cosmological constant in a static cosmological model.
Follow Albert Einstein through 240 dated historical records for United States of America.
A chronological timeline drawn from matching World History Database records.
Applies general relativity to the universe and introduces the cosmological constant in a static cosmological model.
Einstein interprets the cosmological constant as a repulsive contribution capable of balancing ordinary gravitational attraction on the largest cosmic scales.
Becomes founding director of the Kaiser Wilhelm Institute for Physics.
Formulates stimulated emission in his quantum theory of radiation, a principle later fundamental to lasers.
Refines gravitational-wave theory and derives the quadrupole form for radiated energy.
Publishes a foundational discussion of general relativity in which he explicitly names Mach's principle and distinguishes it from the equivalence and relativity principles.
Derives the quadrupole formula for gravitational radiation, relating emitted wave power to changing mass distributions in accelerating systems.
Einstein derives the quadrupole formula for gravitational radiation, relating emitted wave power to the changing mass distribution of an accelerating source.
Returns to Zurich for guest lectures while continuing work on relativity and quantum theory.
British eclipse expeditions photograph stars near the Sun to test Einstein's predicted gravitational deflection.
The total solar eclipse provides observations designed to test the bending of starlight predicted by Einstein's general theory of relativity.
Royal Society and Royal Astronomical Society report eclipse results supporting Einstein's general relativity.
Publishes an accessible explanation of relativity in The Times, describing the conceptual differences between the special and general theories for a broad audience.
Becomes internationally famous after eclipse observations are widely reported as confirming general relativity.
Delivers the lecture Ether and the Theory of Relativity, redefining the concept in gravitational terms.
Delivers his Leiden inaugural lecture on ether and relativity, arguing that general relativity permits a physical spacetime structure without a mechanical luminiferous ether.
Publicly debates critics including Philipp Lenard at the German scientists' meeting in Bad Nauheim, defending the physical basis and interpretation of relativity.
Begins official duties as special professor at Leiden University.
Publicly confronts organized attacks on relativity amid growing political and antisemitic hostility.
Explains how geometry acquires physical meaning through measurement and discusses the relationship between mathematical geometry and the spacetime structure of general relativity.
Arrives in New York during his first visit to the United States, including lectures and fundraising.
Elected a Foreign Member of the Royal Society.
Receives an honorary Doctor of Science degree from the University of Manchester and lectures on relativity.
Publishes a proposed addition to the foundations of general relativity, continuing his effort to strengthen the conceptual and mathematical basis of gravitational field theory.
Uses his first American visit to support fundraising for the future Hebrew University of Jerusalem.
Awarded the 1921 Nobel Prize in Physics for theoretical physics, especially the law of the photoelectric effect.
Receives the Nobel Prize in Physics for contributions to theoretical physics, particularly his explanation of the law governing the photoelectric effect.
Delivers four Stafford Little Lectures explaining special and general relativity.
Debates Henri Bergson over the meaning of time, confronting philosophical objections to the operational treatment of simultaneity in special relativity.
Presents relativity to French scientific audiences during a highly publicised Paris visit, explaining both the special theory and the geometric theory of gravitation.
A total solar eclipse expedition at Wallal obtains measurements of gravitational light deflection that provide another observational test of Einstein's relativity prediction.
Explains how he developed the theory of relativity in a lecture at Kyoto University.
Begins sustained attempts to combine gravitation and electromagnetism within a single field framework.
Travels through Japan giving lectures and public talks on relativity and modern physics.
Publishes The Meaning of Relativity from his Princeton lectures, giving a systematic account of special relativity, tensor methods, gravitation and cosmological applications.
The Meaning of Relativity is published from the four lectures Einstein delivered at Princeton in May 1921.
Lectures in French on relativity during his visit to British Mandate Palestine.
Gives a second Jerusalem lecture on relativity, this time in German.
Begins his Spanish visit with lectures in Barcelona, presenting relativity to scientists and helping stimulate wider discussion of modern theoretical physics in Spain.
Becomes a corresponding member of the Royal Academy of Exact, Physical and Natural Sciences in Madrid.
These dates and descriptions come from the historical_events database. Exact duplicate records have been collapsed. Names are grouped by the country, Name 2 and Name 1 fields; records with missing Name 2 cannot be reliably assigned to an individual biography. Check the underlying sources before formal citation.