Unraveling the Mystery of the Universe's Age: The Big Bang Theory Explained

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SUMMARY

The age of the universe has been calculated to be approximately 13.7 billion years, primarily using the Friedmann equations derived from general relativity. These equations relate the universe's expansion to current measurements of matter density, vacuum energy, and the Hubble constant. By inputting these quantifiable parameters into the equations, scientists arrive at the estimated age. Observations are limited by the Cosmic Microwave Background, which prevents direct observation of the universe's earliest moments.

PREREQUISITES
  • Understanding of general relativity
  • Familiarity with Friedmann equations
  • Knowledge of Hubble constant and its significance
  • Basic concepts of cosmic microwave background radiation
NEXT STEPS
  • Research the implications of the Friedmann equations in cosmology
  • Study the methods for measuring the Hubble constant
  • Explore the significance of cosmic microwave background radiation in understanding the universe's history
  • Investigate alternative theories of the universe's origin and age
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Astronomers, physicists, cosmologists, and anyone interested in the scientific understanding of the universe's age and the Big Bang theory.

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How has it been calculated that the universe really began 13.7 billion years ago with the big bang? Carbon dating or some other method? How exactly did they arrive at this conclusion ?
 
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If you apply general relativity, you get the Friedmann equations, which govern the expansion of the universe. http://en.wikipedia.org/wiki/Friedmann_equations

Using the equation, you can find an expression for the age of the universe that depends on the current day density of matter, vacuum energy, and rate of expansion (Hubble constant). These quantities can all, in principle, be measured in a number of ways. Plug them into the equation, and it gives you 13.7 billion years.
 
land_of_ice said:
How has it been calculated that the universe really began 13.7 billion years ago with the big bang? Carbon dating or some other method? How exactly did they arrive at this conclusion ?

Simply put the Friedmann equations tell us when the size of the Universe goes to zero. Problems arise before then, but not before the Universe is scrunched up into a tiny volume. Observations can't go all the way back to that point in time - the Cosmic Microwave Background is the heat-glow of opaque plasma that we can't see past - so we can't say for sure just how old the Universe really is, just how far back in time it is until the Universe is scrunched up and very hot.
 

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