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... * A long time ago, astronomers thought that the Earth was the centre of the Universe. This was called the geocentric model. The evidence for this model came from observations of the sky using the naked eye. After the telescope was invented, astronomers quickly gathered evidence which showed that the ...
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Word doc - UC-HiPACC - University of California, Santa Cruz

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Word version of Episode 704
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Subtle is the Gravity - The Institute of Mathematical Sciences
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Slide 1

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Kosovichev - Physics - New Jersey Institute of Technology
Kosovichev - Physics - New Jersey Institute of Technology

... Evaluate various Hertzsprung-Russell diagrams for different types of star clusters. Analyze the evolution of binary star systems. Describe Einstein’s model of the universe (both the special relativity and the general relativity theories). Describe the properties of the Milky Way galaxy. Analyze othe ...
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Flatness problem



The flatness problem (also known as the oldness problem) is a cosmological fine-tuning problem within the Big Bang model of the universe. Such problems arise from the observation that some of the initial conditions of the universe appear to be fine-tuned to very 'special' values, and that a small deviation from these values would have had massive effects on the nature of the universe at the current time.In the case of the flatness problem, the parameter which appears fine-tuned is the density of matter and energy in the universe. This value affects the curvature of space-time, with a very specific critical value being required for a flat universe. The current density of the universe is observed to be very close to this critical value. Since the total density departs rapidly from the critical value over cosmic time, the early universe must have had a density even closer to the critical density, departing from it by one part in 1062 or less. This leads cosmologists to question how the initial density came to be so closely fine-tuned to this 'special' value.The problem was first mentioned by Robert Dicke in 1969. The most commonly accepted solution among cosmologists is cosmic inflation, the idea that the universe went through a brief period of extremely rapid expansion in the first fraction of a second after the Big Bang; along with the monopole problem and the horizon problem, the flatness problem is one of the three primary motivations for inflationary theory.
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