Big Bang and Cosmic Microwave Background Radiation

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These flashcards cover important vocabulary and definitions related to the Big Bang theory, the early universe, cosmic radiation, and fundamental concepts in cosmology.

Last updated 9:30 PM on 4/10/26
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16 Terms

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Big Bang

The event that marks the beginning of the Universe, characterized by extreme heat and density.

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Primordial Nucleosynthesis

The process that occurred during the Big Bang leading to the formation of light elements such as hydrogen and helium.

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Cosmic Microwave Background Radiation (CMB)

The relic radiation from the Big Bang, now redshifted to a microwave frequency and observed uniformly across the universe.

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Hubble’s Law

The observation that the farther away galaxies are, the faster they appear to be moving away from us, indicating that the universe is expanding.

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George Gamow

A physicist who contributed to the Big Bang theory and the concept of primordial nucleosynthesis.

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Density of the Universe

The amount of matter in a region of the Universe, which influences its expansion and structure.

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General Theory of Relativity

Einstein's theory that describes gravity as the curvature of spacetime caused by mass, fundamental to understanding cosmology.

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Deuterium

An isotope of hydrogen consisting of one proton and one neutron, formed during the early minutes of the Universe.

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Stable Atoms Formation

The process that occurred when temperature dropped sufficiently for electrons to combine with protons, resulting in neutral atoms.

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Blackbody Radiation

The idealized spectrum of radiation emitted by an object in thermal equilibrium, relevant to the CMB.

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Redshift

The phenomenon where light from an object is shifted to longer wavelengths, indicative of the expansion of the Universe.

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Quasar

A massive and distant celestial object that emits exceptionally large amounts of energy, often used to measure early Universe conditions.

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Flat Universe

A model of the universe in which parallel lines remain parallel and the geometry is Euclidean, indicated by the distribution of galaxies.

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Closed Universe

A model of the universe where space curves back on itself; it has a finite volume with no boundaries.

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Open Universe

A model of the universe that continues to expand forever and has no boundaries, highlighting its infinite nature.

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Nucleosynthesis

The process of formation of new atomic nuclei from pre-existing nucleons, significant in the early stages of the Universe.