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  2. Binding energy - Wikipedia

    en.wikipedia.org/wiki/Binding_energy

    The atomic binding energy derives from the electromagnetic interaction of the electrons with the nucleus, mediated by photons. For an atom of helium, with 2 electrons, the atomic binding energy is the sum of the energy of first ionization (24.587 eV) and the energy of second ionization (54.418 eV), for a total of 79.005 eV. Atomic level

  3. Alpha decay - Wikipedia

    en.wikipedia.org/wiki/Alpha_decay

    The nuclear force holding an atomic nucleus together is very strong, in general much stronger than the repulsive electromagnetic forces between the protons. However, the nuclear force is also short-range, dropping quickly in strength beyond about 3 femtometers, while the electromagnetic force has an unlimited range. The strength of the ...

  4. Ionic bonding - Wikipedia

    en.wikipedia.org/wiki/Ionic_bonding

    Atoms that lose electrons make positively charged ions (called cations). This transfer of electrons is known as electrovalence in contrast to covalence . In the simplest case, the cation is a metal atom and the anion is a nonmetal atom, but these ions can be more complex, e.g. molecular ions like NH +

  5. Chemical bond - Wikipedia

    en.wikipedia.org/wiki/Chemical_bond

    The bond results because the metal atoms become somewhat positively charged due to loss of their electrons while the electrons remain attracted to many atoms, without being part of any given atom. Metallic bonding may be seen as an extreme example of delocalization of electrons over a large system of covalent bonds, in which every atom ...

  6. Alpha particle - Wikipedia

    en.wikipedia.org/wiki/Alpha_particle

    Nobody knew exactly how many electrons were in an atom. Protons and neutrons had not yet been discovered. Rutherford decided the second explanation was the most plausible because it is the simplest and sizeable deposits of helium were commonly found underground next to deposits of radioactive elements.

  7. Ionization energy - Wikipedia

    en.wikipedia.org/wiki/Ionization_energy

    These electrons and ions will establish a current through the tube. The ionization energy will be the energy of photons hν i (h is the Planck constant) that caused a steep rise in the current: E i = hν i. When high-velocity electrons are used to ionize the atoms, they are produced by an electron gun inside a similar evacuated tube. The energy ...

  8. Radioactive decay - Wikipedia

    en.wikipedia.org/wiki/Radioactive_decay

    Radioactive decay is a random process at the level of single atoms. According to quantum theory, it is impossible to predict when a particular atom will decay, regardless of how long the atom has existed. [2] [3] [4] However, for a significant number of identical atoms, the overall decay rate can be expressed as a decay constant or as a half-life.

  9. Atom - Wikipedia

    en.wikipedia.org/wiki/Atom

    The electrons are negatively charged, and this opposing charge is what binds them to the nucleus. If the numbers of protons and electrons are equal, as they normally are, then the atom is electrically neutral as a whole. If an atom has more electrons than protons, then it has an overall negative charge, and is called a negative ion (or anion ...

  1. Related searches atoms that lose electrons become stronger than protons

    atoms that lose electrons become stronger than protons and neutrons