Judging from the quantities of scholarly activities, general relativity only entered the mainstream of research after the Second World War. [5] The advent of Space Age, marked by the launch of Sputnik , the world's first artificial satellite, in 1957; the rise of radio, X-ray, and gamma-ray astronomy; and the parallels between the physics of (nuclear) explosives and supernovae—shock waves, massive energy outputs, and the synthesis of heavy elements—fueled the growth of astronomy and astrophysics. [4] An increase in the number of researchers and funding in the postwar years also played a role. [5] The U.S. Air Force and Navy provided funding for some the early conferences, but stopped doing so after Congress passed the Mansfield Amendments, forbidding the use of the defense budget on basic research. The Texas Symposia were put in this category, despite the relevance of relativistic physics for missile guidance and the functioning of the Global Positioning System (GPS). [7] Over the years, some of the recurring topics of interest at the Texas Symposia have been astroparticle physics; the cosmic microwave background; extra-galactic gamma-ray bursts; gravitational waves; black holes, their thermodynamics, and Hawking radiation; pulsars; and X-ray astronomy. [7]
Twentieth century
The First Symposium, chiefly organized by Robinson, Alfred Schild, Engelbert Schücking, and Peter Bergmann, convened in Dallas, Texas, in December 16–18, 1963, shortly after the assassination of John F. Kennedy. [7] One of the major topic of discussion of the time was the optical and radio observations of quasi-stellar objects. [1] J. Robert Oppenheimer opened the first session on what would later be named "black holes" by John Archibald Wheeler. [1] Wheeler gave an extensive lecture on the gravitational collapse of stars, and expressed his enthusiasm for the Oppenheimer–Snyder model. [3] : 240 Another notable speaker was Roy Kerr, who gave a brief talk on his newfound exact solution to the Einstein field equations. With the notable exception of Achilles Papapetrou, most physicists did not grasp its significance. But they later realized that the Kerr metric described rotating black holes. [3] : 341–2 It was in fact the key to understanding quasars. [8] Hong-Yee Chiu used the word quasar for quasi-stellar radio sources (QSRS) in the proceedings of this conference, published in 1965, though it took some time to become standard. [7] The First Symposium attracted approximately 300 people from many different countries worldwide. However, against the backdrop of the Cold War, a number of physicists from the Soviet Union, such as Vitaly Ginzburg and Yakov Zeldovich, were not able to attend due to a ban from their own government or their inability to obtain a visa to visit the United States. [1] [7] The gathering was sponsored by Texas Instruments, the RAND Corporation, Lockheed, Boeing, among others. [7] In his after-dinner speech, Thomas Gold commented on the significance of this conference: "...the relativists with their sophisticated works are not only magnificent cultural ornaments but might actually be useful to science! Everyone is pleased: the relativists who feel they are being appreciated and are experts in a field they hardly knew existed, the astrophysicists for having enlarged their domain, their empire, by the annexation of another subject—general relativity." [3] : 341
The Second Symposium convened at the University of Texas at Austin in December 15–19, 1964. Discussions of quasars continued, now with astronomical observations at various portions of the electromagnetic spectrum, including X-rays and gamma-rays. Astronomers exhibited their discoveries on highly energetic cosmic rays, such as neutrinos. Robert Dicke presented his improved Eötvös experiment, verifying the principle of equivalence to one part in 1011. The Symposium concluded with a seminar on gravitational collapse, the energy released from such an event, and the relevance of relativistic hydrodynamics in the strong-field regime. [2]
At the Fifth Symposium in Austin, Texas, in 1970, participants discussed black holes, white holes, and the asymmetry between matter and antimatter. Stephen Hawking attended in his wheelchair. [7]
By the time of the Sixth Symposium in New York City, 1972, black holes had become a major topic of study. [9] Researchers presented their work on X-ray binaries, accretion disks, and Cygnus X-1, the first black-hole candidate. [7] This Symposium was one of the most popular of all time, attended by around 1,000 people. [7]
The Seventh Symposium, organized in Dallas, 1974, saw the first scheduled parallel sessions. [7] Some major topics of interest were the abundance of the chemical elements, gamma-ray bursts, supernovae, galaxies, compact objects, and gravitational waves. [10]
Jocelyn Bell Burnell, co-discoverer of pulsars, gave an after-dinner speech on her work at the Eighth Symposium in Boston, Massachusetts. [11] [7]
At the Ninth Symposium in Munich, Germany, in 1978, the newly discovered Hulse–Taylor pulsar, named after Russell Alan Hulse and Joseph Hooton Taylor Jr., attracted considerable attention as a test of general relativity outside of the solar system in the post-Newtonian limit. The observed orbital decay due to gravitational radiation and precession of the periastron were accurately predicted by general relativity. [12] This was the first Texas Symposium held in Europe. [7]
Gravitational waves were a major topic at the Fourteen Symposium in Chicago, Illinois, in 1986. [13] Kip Thorne shared his plans for what later became the Laser Interferometer Gravitational-Wave Observatory (LIGO). [3] : 498 Bernard Schultz examined how gravitational collapses, such as supernovae, as potential sources of gravitational waves and the prospects of detecting them by Weber bars (invented by Joseph Weber). [13] Other notable topics were active galactic nuclei; gravitational lenses and how they could be used to map the distribution of dark matter and to determine the Hubble constant; anisotropy in the cosmic microwave background and the upcoming Cosmic Background Explorer (COBE) satellite; and NASA's Great Observatories program. [13]
By the 1990s, a large public lecture in the evening has become a standard feature. Stephen Hawking gave this talk at the Fifteenth Symposium in Brighton, United Kingdom, 1990. [7]
Twenty-first century
The Twenty-Sixth Symposium took place in São Paulo, Brazil, in 2012. It was the first to be held in Latin America. [14]
The Twenty-Seventh Symposium returned to Dallas for the 50th anniversary of the First. This event featured a round table of the "veterans" of the original conference, co-chaired by Wolfgang Rindler. Other sessions discussed the evolution of galaxies, neutron stars, supermassive black holes, the implications of the Higgs boson for cosmology, plus updates from the Planck satellite and the Nuclear Spectroscopic Telescope Array (NuSTAR). [15]
The Twenty-Eighth Symposium met in Geneva, Switzerland, in 2015, commemorating the 100th anniversary of the completion of general relativity by Albert Einstein. Among the plenary speakers, Thanu Padmanabhan spoke of the first century of general relativity, Mustapha Ishak of the exact solutions to the Einstein field equations having applications in astrophysics, Alessandra Buonanno of gravitational waves emitted by binary systems, and Anna Watts of the equation of state for neutron stars. [16]
The Thirty-Second Symposium was held in Shanghai, China, at the Tsung-Dao Lee Institute of Shanghai Jiao Tong University in 2023. Shanghai is the first East Asian city to host the conference. It took place on the 60th anniversary of the First Symposium. Kip Thorne gave the opening speech online. [17] (See link below.)
At the Thirty-Third Symposium, organized by Arizona State University in Tempe, Arizona, in 2025, plenary talks focused on the imaging of black holes by the Event Horizon Telescope, gravitational-wave astronomy, observations by the James Webb Space Telescope , little red dots, and the Hubble tension. [18]
