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Inflation theory was developed in the late 1970s and early 80s, with notable contributions by several theoretical physicists, including Alexei Starobinsky at Landau Institute for Theoretical Physics, Alan Guth at Cornell University, and Andrei Linde at Lebedev Physical Institute.
Alan Guth, the physicist who proposed the theory of cosmic inflation, discusses how it explains the origin, structure and evolution of our universe. He also explores emerging ideas about primordial black holes, the multiverse and the eternity of the universe.
Alan Harvey Guth ( / ɡuːθ /; born February 27, 1947) is an American theoretical physicist and cosmologist who is the Victor Weisskopf Professor of Physics at the Massachusetts Institute of Technology. Along with Alexei Starobinsky and Andrei Linde, he won the 2014 Kavli Prize "for pioneering the theory of cosmic inflation." [1]
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Mar 20, 2014 · MIT physicist Alan Guth explains how new results bolster his 1980 theory of cosmic inflation, which describes the propulsion mechanism that drove the universe into the period of tremendous expansion from a mere dot into a dense ball. He also discusses the significance of the new BICEP2 results, which measure the stretching effect of inflation on the geometry of space and the temperature nonuniformities of the cosmic microwave background.
Jan 8, 2021 · The most popular model for what preceded it is inflation. Alan Guth, who began developing the theory in 1979, wrote in his book The Inflationary Universe that “the standard Big Bang theory says ...
Jun 30, 2014 · June 30, 2014. • 20 min read. At the end of a quiet, carpeted hallway in MIT's physics department, a display case stands empty outside the office of physicist Alan Guth. Framed in blond wood and ...
ALAN H. GUTH Massachusetts Institute of Technology Abstract The basic workings of inflationary models are summarized, al ong with the arguments that strongly suggest that our universe is the product of inflatio n. I describe the quantum origin of density perturbations, giving a heuristic derivation of the scale invariance of the spectrum
