Photoexcitation is the first step in a photochemical process: the reactant is elevated to a state of higher energy, an
excited state.
Grotthuss–Draper law and Stark–Einstein law The first law of photochemistry, known as the
Grotthuss–Draper law (for chemists
Theodor Grotthuss and
John W. Draper), states that light must be
absorbed by a chemical substance in order for a
photochemical reaction to take place. According to the second law of photochemistry, known as the
Stark–Einstein law (for physicists
Johannes Stark and
Albert Einstein), for each photon of light absorbed by a chemical system, no more than one molecule is activated for a photochemical reaction, as defined by the
quantum yield.
Fluorescence and phosphorescence When a substance in its
ground state (S0) absorbs light, one electron is excited. This electron maintains its
spin. According to the spin selection rule; other transitions would violate the law of
conservation of angular momentum. The excitation to a higher
singlet state can be from
HOMO to
LUMO or to a higher orbital, so that singlet excitation states S1, S2, S3... at different energies are possible.
Kasha's rule stipulates that higher singlet states quickly relax by radiationless decay or
internal conversion (IC) to S1. Thus, S1 is usually, but not always, the only relevant singlet excited state. This excited state S1 can further relax to S0 by IC, but also by an allowed radiative transition from S1 to S0 that emits a photon; this process is called
fluorescence. . Radiative paths are represented by straight arrows and non-radiative paths by curly lines. Alternatively, it is possible for the excited state S1 to undergo spin inversion and to generate a
triplet excited state T1 having two unpaired electrons with the same spin. This violation of the spin selection rule is possible by
intersystem crossing (ISC) of the vibrational and electronic levels of S1 and T1. According to
Hund's rule of maximum multiplicity, this T1 state would be somewhat more stable than S1. This triplet state can relax to the ground state S0 by radiationless ISC or by a radiation pathway called
phosphorescence. This process implies a change of electronic spin, which is forbidden by spin selection rules, making phosphorescence (from T1 to S0) much slower than fluorescence (from S1 to S0). Thus, triplet states generally have longer lifetimes than singlet states. These transitions are usually summarized in a state energy diagram or
Jablonski diagram, the paradigm of molecular photochemistry. These excited species, either S1 or T1, have a half-empty low-energy orbital, and are consequently more
oxidizing than the ground state. But at the same time, they have an electron in a high-energy orbital, and are thus more
reducing. In general, excited species are prone to participate in electron transfer processes.
Experimental setup Photochemical reactions require a light source that emits wavelengths corresponding to an electronic transition in the reactant. In the early experiments (and in everyday life), sunlight was the light source, although it is polychromatic.
Mercury-vapor lamps are more common in the laboratory. Low-pressure mercury-vapor lamps mainly emit at 254 nm. For polychromatic sources, wavelength ranges can be selected using filters. Alternatively, laser beams are usually monochromatic (although two or more wavelengths can be obtained using
nonlinear optics), and
LEDs have a relatively narrow
band that can be efficiently used, as well as Rayonet lamps, to get approximately monochromatic beams. containing slurry of orange crystals of
Fe2(CO)9 in
acetic acid after its photochemical synthesis from
Fe(CO)5. The
mercury lamp (connected to white power cords) can be seen on the left, set inside a water-jacketed quartz tube. The emitted light must reach the targeted
functional group without being blocked by the reactor, medium, or other
functional groups present. For many applications,
quartz is used for the reactors as well as to contain the lamp.
Pyrex absorbs at wavelengths shorter than 275 nm. The
solvent is an important experimental parameter. Solvents are potential reactants, and for this reason,
chlorinated solvents are avoided because the C–Cl bond can lead to
chlorination of the substrate. Strongly-absorbing solvents prevent photons from reaching the substrate.
Hydrocarbon solvents absorb only at short wavelengths and are thus preferred for photochemical experiments requiring high-energy photons. Solvents containing
unsaturation absorb at longer wavelengths and can usefully filter out short wavelengths. For example,
cyclohexane and
acetone "cut off" (absorb strongly) at wavelengths shorter than 215 and 330 nm, respectively. Typically, the wavelength employed to induce a photochemical process is selected based on the
absorption spectrum of the reactive species, most often the absorption maximum. Over the last years, however, it has been demonstrated that, in the majority of bond-forming reactions, the absorption spectrum does not allow selecting the optimum wavelength to achieve the highest reaction yield based on absorptivity. This fundamental mismatch between absorptivity and reactivity has been elucidated with so-called
photochemical action plots.
Photochemistry in combination with flow chemistry Continuous-flow photochemistry offers multiple advantages over batch photochemistry. Photochemical reactions are driven by the number of photons that are able to activate molecules causing the desired reaction. The large
surface-area-to-volume ratio of a microreactor maximizes the illumination, and at the same time allows for efficient cooling, which decreases the thermal side products. ==Photochemical reactions==