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A Jablonski diagram showing the excitation of molecule A to its singlet excited state (1 A*) followed by intersystem crossing to the triplet state (3 A) that relaxes to the ground state by phosphorescence. It was used to describe absorption and emission of light by fluorescents.
Atoms can be excited by heat, electricity, or light. The hydrogen atom provides a simple example of this concept.. The ground state of the hydrogen atom has the atom's single electron in the lowest possible orbital (that is, the spherically symmetric "1s" wave function, which, so far, has been demonstrated to have the lowest possible quantum numbers).
Excited states in nuclear, atomic, and molecule systems have distinct energy values, allowing external energy to be absorbed in the appropriate proportions. [ 6 ] In general, the excitation of electrons in atoms strongly varies from excitation in solids, due to the different nature of the electronic levels and the structural properties of some ...
If emission leaves a system in an excited state, additional transitions can occur, leading to atomic radiative cascade. For example, if calcium atoms a low pressure atomic beam are excited by ultraviolet light from their in the 4 1 S 0 ground state to the 6 1 P 1 state, they can decay in three steps, first to 6 1 S 0 then to 4 1 P 1 and finally ...
Rydberg states have energies converging on the energy of the ion. The ionization energy threshold is the energy required to completely liberate an electron from the ionic core of an atom or molecule. In practice, a Rydberg wave packet is created by a laser pulse on a hydrogenic atom and thus populates a superposition of Rydberg states. [3]
A corollary of Kasha's rule is the Vavilov rule, which states that the quantum yield of luminescence is generally independent of the excitation wavelength. [4] [7] This can be understood as a consequence of the tendency – implied by Kasha's rule – for molecules in upper states to relax to the lowest excited state non-radiatively.
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If atoms are in the excited state, spontaneous decay events to the ground state will occur at a rate proportional to N 2, the number of atoms in the excited state. The energy difference between the two states Δ E 21 is emitted from the atom as a photon of frequency ν 21 as given by the frequency-energy relation above.