Alan Guth on new insights into the 'Big Bang' - 0 views
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Q: Can you explain the theory of cosmic inflation that you first put forth in 1980?
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describes the propulsion mechanism that drove the universe into the period of tremendous expansion that we call the Big Bang
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described how the universe was cooled by the expansion, and how the expansion was slowed by the attractive force of gravity
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According to Newton, gravity is a purely attractive force, but this changed with Einstein and the discovery of general relativity
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General relativity describes gravity as a distortion of spacetime, and allows for the possibility of repulsive gravity
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Modern particle theories strongly suggest that at very high energies, there should exist forms of matter that create repulsive gravity
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proposes that at least a very small patch of the early universe was filled with this repulsive-gravity material
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During the period of exponential expansion, any ordinary material would thin out, with the density diminishing to almost nothing
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The repulsive-gravity material actually maintains a constant density as it expands, no matter how much it expands
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But at the same time, more and more negative energy appears in the form of the gravitational field that is filling the region
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It is possible that the total energy of the entire universe is exactly zero, with the positive energy of matter completely canceled by the negative energy of gravity
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decays into ordinary particles, producing a very hot soup of particles that form the starting point of the conventional Big Bang
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point the repulsive gravity turns off, but the region continues to expand in a coasting pattern for billions of years to come
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inflation is a prequel to the era that cosmologists call the Big Bang, although it of course occurred after the origin of the universe, which is often also called the Big Bang.
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Q: What is the new result announced this week, and how does it provide critical support for your theory?
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The early universe, as we can see from the afterglow of the cosmic microwave background (CMB) radiation, was incredibly uniform,
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these nonuniformities—which later produce stars, galaxies, and all the structure of the universe—are attributed to quantum theory
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The temperature nonuniformities in the cosmic microwave background were first measured in 1992 by the COBE satellite
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have not generally been seen as proof of inflation, in part because it is not clear that inflation is the only possible way that these fluctuations could have been produced.
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The geometry of space also fluctuates on small scales, due to the physics of quantum theory, and inflation also stretches these fluctuations, producing gravity waves in the early universe.
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They do not see the gravity waves directly, but instead they have constructed a very detailed map of the polarization of the CMB in a patch of the sky.
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it determines the energy density of the universe at the time of inflation, which is something that previously had a wide range of possibilities.
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By determining the energy density of the universe at the time of inflation, the new result also tells us a lot about which detailed versions of inflation are still viable, and which are no longer viable
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The current result is not by itself conclusive, but it points in the direction of the very simplest inflationary models that can be constructed.