The Recombination Epoch marks the era in the early universe when electrons combined with protons to form neutral hydrogen atoms, leading to the decoupling of matter and radiation. This pivotal event allowed photons to travel freely, resulting in the Cosmic Microwave Background radiation that we observe today as a snapshot of the universe at that time.

Recombination Epoch

The early universe refers to the period immediately following the Big Bang, characterized by rapid expansion and cooling that led to the formation of fundamental particles and eventually atoms. This era set the stage for the development of cosmic structures such as galaxies, stars, and planets through processes governed by fundamental forces and cosmic inflation.

early universe

electrons combined with protons

neutral hydrogen atoms

The decoupling of matter and radiation refers to the epoch in the universe's history when photons ceased to interact frequently with matter, allowing light to travel freely through space. This event, occurring approximately 380,000 years after the Big Bang, marks the transition from an opaque, hot plasma to a transparent universe, enabling the formation of the cosmic microwave background radiation.

decoupling of matter and radiation

pivotal event

Photons travel freely

Cosmic microwave background radiation is the thermal remnant from the Big Bang, providing a snapshot of the universe when it was just 380,000 years old. It is a nearly uniform background of microwave radiation that fills the universe and is a critical piece of evidence for the Big Bang theory, offering insights into the early conditions and subsequent evolution of the cosmos.

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