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  2. Atomic Age - Wikipedia

    en.wikipedia.org/wiki/Atomic_Age

    In the 21st century, the label of the "Atomic Age" connotes either a sense of nostalgia or naïveté and is considered by many to have ended with the fall of the Soviet Union in 1991, though the term continues to be used by many historians to describe the era following the conclusion of the Second World War. Atomic energy and weapons continue ...

  3. Recombination (cosmology) - Wikipedia

    en.wikipedia.org/wiki/Recombination_(cosmology)

    The thermal energy at the peak of the blackbody spectrum is the Boltzmann constant, k B, times the temperature, () but simply comparing this to the ionization energy of hydrogen atoms will not consider the spectrum of energies. A better estimate evaluates the thermal equilibrium between matter (atoms) and radiation.

  4. Chronology of the universe - Wikipedia

    en.wikipedia.org/wiki/Chronology_of_the_universe

    Recombination describes the ionized particles combining to form the first neutral atoms, and decoupling refers to the photons released ("decoupled") as the newly formed atoms settle into more stable energy states. Just before recombination, the baryonic matter in the universe was at a temperature where it formed a hot ionized plasma. Most of ...

  5. Atomism - Wikipedia

    en.wikipedia.org/wiki/Atomism

    Ajivika is a "Nastika" school of thought whose metaphysics included a theory of atoms or atomism which was later adapted in the Vaiśeṣika school, which postulated that all objects in the physical universe are reducible to paramāṇu , and one's experiences are derived from the interplay of substance (a function of atoms, their number and ...

  6. Reionization - Wikipedia

    en.wikipedia.org/wiki/Reionization

    In the fields of Big Bang theory and cosmology, reionization is the process that caused electrically neutral atoms in the universe to reionize after the lapse of the "dark ages". Detecting and studying the reionization process is challenging but multiple avenues have been pursued.

  7. Future of an expanding universe - Wikipedia

    en.wikipedia.org/wiki/Future_of_an_expanding...

    The second, the Stelliferous Era, includes the present day and all of the stars and galaxies now seen. It is the time during which stars form from collapsing clouds of gas. In the subsequent Degenerate Era, the stars will have burnt out, leaving all stellar-mass objects as stellar remnants—white dwarfs, neutron stars, and black holes.

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  9. Atomic Age (design) - Wikipedia

    en.wikipedia.org/wiki/Atomic_Age_(design)

    Atomic power was a paradox during the era. It held great promise of technological solutions for the problems facing an increasingly complex world; at the same time, people were fearful of a nuclear armageddon, after the use of atomic weapons at the end of World War II. People were ever-aware of the potential good, and lurking menace, in technology.