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  2. Schwinger effect - Wikipedia

    en.wikipedia.org/wiki/Schwinger_effect

    To understand this, note that electrons and positrons are each other's antiparticles, with identical properties except opposite electric charge. To conserve energy, the electric field loses energy when an electron–positron pair is created, by an amount equal to 2 m e c 2 {\displaystyle 2m_{\text{e}}c^{2}} , where m e {\displaystyle m_{\text{e ...

  3. Electron pair - Wikipedia

    en.wikipedia.org/wiki/Electron_pair

    Therefore, for two electrons to occupy the same orbital, and thereby have the same orbital quantum number, they must have different spin quantum numbers. This also limits the number of electrons in the same orbital to two. The pairing of spins is often energetically favorable, and electron pairs therefore play a large role in chemistry.

  4. Avalanche breakdown - Wikipedia

    en.wikipedia.org/wiki/Avalanche_breakdown

    There are two types of charge carriers in a semiconductor: free electrons (mobile electrons) and electron holes (mobile holes which are missing electrons from the normally-occupied electron states). A normally-bound electron (e.g., in a bond) in a reverse-biased diode may break loose due to a thermal fluctuation or excitation, creating a mobile ...

  5. Electron avalanche - Wikipedia

    en.wikipedia.org/wiki/Electron_avalanche

    However, free electrons are easily captured by neutral oxygen or water vapor molecules (so-called electronegative gases), forming negative ions. In air at STP, free electrons exist for only about 11 nanoseconds before being captured. Captured electrons are effectively removed from play — they can no longer contribute to the avalanche process.

  6. Intersystem crossing - Wikipedia

    en.wikipedia.org/wiki/Intersystem_crossing

    That is, the spin of the excited electron is still paired with the ground state electron (a pair of electrons in the same energy level must have opposite spins, per the Pauli exclusion principle). In a triplet state the excited electron is no longer paired with the ground state electron; that is, they are parallel (same spin). Since excitation ...

  7. Carrier generation and recombination - Wikipedia

    en.wikipedia.org/wiki/Carrier_generation_and...

    Trap emission is a multistep process wherein a carrier falls into defect-related wave states in the middle of the bandgap. A trap is a defect capable of holding a carrier. The trap emission process recombines electrons with holes and emits photons to conserve energy. Due to the multistep nature of trap emission, a phonon is also often emitted.

  8. Pair production - Wikipedia

    en.wikipedia.org/wiki/Pair_production

    As energy must be conserved, for pair production to occur, the incoming energy of the photon must be above a threshold of at least the total rest mass energy of the two particles created. (As the electron is the lightest, hence, lowest mass/energy, elementary particle, it requires the least energetic photons of all possible pair-production ...

  9. Pauli exclusion principle - Wikipedia

    en.wikipedia.org/wiki/Pauli_exclusion_principle

    In the case of electrons in atoms, the exclusion principle can be stated as follows: in a poly-electron atom it is impossible for any two electrons to have the same two values of all four of their quantum numbers, which are: n, the principal quantum number; ℓ, the azimuthal quantum number; m ℓ, the magnetic quantum number; and m s, the spin ...