Big Bang

The Big Bang is the prevailing cosmological model explaining the origin of the universe approximately 13.8 billion years ago, when all matter and energy expanded from an infinitely dense and hot initial state.

Origins of the Universe

The Big Bang represents the theoretical beginning point of our observable universe, marking the start of space-time itself. Unlike a conventional explosion, the Big Bang describes the rapid expansion of space itself from an initial state of extreme density and temperature.

Key Characteristics

  • Initial conditions included infinite density at a singularity
  • Occurred approximately 13.8 billion years ago
  • Represents the beginning of measurable physical laws
  • Temperature at earliest measurable moment: ~10^32 degrees Kelvin

Evidence Supporting the Theory

Cosmic Microwave Background

The discovery of cosmic microwave background radiation in 1964 provided crucial evidence for the Big Bang theory. This ambient radiation represents the "afterglow" of the early universe, showing remarkable uniformity across all directions.

Element Abundance

The theory accurately predicts the observed ratios of light elements in the universe through nucleosynthesis:

  • Hydrogen: ~75%
  • Helium: ~25%
  • Trace amounts of lithium and other elements

Timeline of Early Universe

  1. Planck Epoch (10^-43 seconds)

  2. Grand Unification Epoch (10^-43 to 10^-36 seconds)

  3. Inflationary Period (10^-36 to 10^-32 seconds)

    • Exponential expansion of space
    • Universe grows by factor of 10^78
  4. Particle Era (10^-32 seconds to 380,000 years)

Ongoing Research

Modern cosmologists continue investigating several mysteries related to the Big Bang:

Cultural Impact

The Big Bang theory has profoundly influenced human understanding of our cosmic origins, sparking philosophical debates about:

Alternative Theories

While the Big Bang theory is widely accepted, some scientists propose alternative models:

The Big Bang remains our best explanation for cosmic origins, supported by multiple lines of observational evidence and theoretical frameworks in modern physics.