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  2. Atomic orbital - Wikipedia

    en.wikipedia.org/wiki/Atomic_orbital

    In non-relativistic quantum mechanics, therefore, any atom with an atomic number greater than 137 would require its 1s electrons to be traveling faster than the speed of light. Even in the Dirac equation, which accounts for relativistic effects, the wave function of the electron for atoms with > is oscillatory and unbounded.

  3. Atom - Wikipedia

    en.wikipedia.org/wiki/Atom

    The amount of energy needed to remove or add an electron—the electron binding energy—is far less than the binding energy of nucleons. For example, it requires only 13.6 eV to strip a ground-state electron from a hydrogen atom, [54] compared to 2.23 million eV for splitting a deuterium nucleus. [55]

  4. Atomic electron transition - Wikipedia

    en.wikipedia.org/wiki/Atomic_electron_transition

    The energy of an electron is determined by its orbit around the atom, The n = 0 orbit, commonly referred to as the ground state, has the lowest energy of all states in the system. In atomic physics and chemistry , an atomic electron transition (also called an atomic transition, quantum jump, or quantum leap) is an electron changing from one ...

  5. Hydrogen atom - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_atom

    Depiction of a hydrogen atom showing the diameter as about twice the Bohr model radius. (Image not to scale) A hydrogen atom is an atom of the chemical element hydrogen.The electrically neutral hydrogen atom contains a single positively charged proton in the nucleus, and a single negatively charged electron bound to the nucleus by the Coulomb force.

  6. Bohr model - Wikipedia

    en.wikipedia.org/wiki/Bohr_model

    The Bohr model of the hydrogen atom (Z = 1) or a hydrogen-like ion (Z > 1), where the negatively charged electron confined to an atomic shell encircles a small, positively charged atomic nucleus and where an electron jumps between orbits, is accompanied by an emitted or absorbed amount of electromagnetic energy (hν). [1]

  7. The Vacuum of Space Won't Last Forever. In Fact, It ... - AOL

    www.aol.com/vacuum-space-wont-last-forever...

    One portion of that was calculated to be higher than it should be, the Slovenian physicists explain, which means the overall life of the vacuum in their opinion is 10 to the 790th power.

  8. Atomic energy - Wikipedia

    en.wikipedia.org/wiki/Atomic_energy

    Nuclear binding energy, the energy required to split a nucleus of an atom. Nuclear potential energy , the potential energy of the particles inside an atomic nucleus. Nuclear reaction , a process in which nuclei or nuclear particles interact, resulting in products different from the initial ones; see also nuclear fission and nuclear fusion .

  9. Are PFAS really 'forever chemicals'? It's complicated. Here's ...

    www.aol.com/pfas-really-forever-chemicals...

    Broadly speaking, all PFAS have a chain of carbon atoms bonded to fluorine atoms. Some substances have every carbon-hydrogen bond replaced by a fluorine atom (per-fluorinated) others have only ...