Photochemistry

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Photochemical immersion well reactor (50 mL) with a mercury-vapor lamp.

Photochemistry is the branch of

visible (400–750 nm), or infrared radiation (750–2500 nm).[1]

In nature, photochemistry is of immense importance as it is the basis of photosynthesis, vision, and the formation of vitamin D with sunlight.[2] It is also responsible for the appearance of DNA mutations leading to skin cancers.[3]

Photochemical reactions proceed differently than temperature-driven reactions. Photochemical paths access high-energy intermediates that cannot be generated thermally, thereby overcoming large activation barriers in a short period of time, and allowing reactions otherwise inaccessible by thermal processes. Photochemistry can also be destructive, as illustrated by the photodegradation of plastics.

Concept

Grotthuss–Draper law and Stark–Einstein law

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.[4][5]

Fluorescence and phosphorescence

When a molecule or atom in the

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 would 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.

Jablonski diagram. 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 IC 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.[6]

Experimental setup

Photochemical immersion well reactor (750 mL) with a mercury-vapor lamp

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.

band
that can be efficiently used, as well as Rayonet lamps, to get approximately monochromatic beams.

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

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[when?], 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.[8][9]

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.[10]

Principles

In the case of photochemical reactions, light provides the activation energy. Simplistically, light is one mechanism for providing the activation energy required for many reactions. If laser light is employed, it is possible to selectively excite a molecule so as to produce a desired electronic and vibrational state.[11] Equally, the emission from a particular state may be selectively monitored, providing a measure of the population of that state. If the chemical system is at low pressure, this enables scientists to observe the energy distribution of the products of a chemical reaction before the differences in energy have been smeared out and averaged by repeated collisions.

The absorption of a photon by a reactant molecule may also permit a reaction to occur not just by bringing the molecule to the necessary activation energy, but also by changing the symmetry of the molecule's electronic configuration, enabling an otherwise-inaccessible reaction path, as described by the Woodward–Hoffmann selection rules. A [2+2] cycloaddition reaction is one example of a pericyclic reaction that can be analyzed using these rules or by the related frontier molecular orbital theory.

Some photochemical reactions are several orders of magnitude faster than thermal reactions; reactions as fast as 10−9 seconds and associated processes as fast as 10−15 seconds are often observed.

The photon can be absorbed directly by the reactant or by a photosensitizer, which absorbs the photon and transfers the energy to the reactant. The opposite process, when a photoexcited state is deactivated by a chemical reagent, is called quenching.

Most photochemical transformations occur through a series of simple steps known as primary photochemical processes. One common example of these processes is the excited state proton transfer.

Photochemical reactions

Examples of
photochemical reactions

Organic photochemistry

Examples of photochemical

photoisomerization, and Norrish reactions.[20][21]

Norrish type II reaction

transcription. The beneficial effects of sunlight are associated with the photochemically-induced retro-cyclization (decyclization) reaction of ergosterol to give vitamin D. In the DeMayo reaction, an alkene reacts with a 1,3-diketone reacts via its enol to yield a 1,5-diketone. Still another common photochemical reaction is Howard Zimmerman's di-π-methane rearrangement
.

In an industrial application, about 100,000 tonnes of benzyl chloride are prepared annually by the gas-phase photochemical reaction of toluene with chlorine.[22] The light is absorbed by chlorine molecules, the low energy of this transition being indicated by the yellowish color of the gas. The photon induces homolysis of the Cl-Cl bond, and the resulting chlorine radical converts toluene to the benzyl radical:

Cl2 + hν → 2 Cl·
C6H5CH3 + Cl· → C6H5CH2· + HCl
C6H5CH2· + Cl· → C6H5CH2Cl

olefins
.

Inorganic and organometallic photochemistry

THF solution of molybdenum hexacarbonyl
gives the THF complex, which is synthetically useful:

Mo(CO)6 + THF → Mo(CO)5(THF) + CO

In a related reaction, photolysis of iron pentacarbonyl affords diiron nonacarbonyl (see figure):

2 Fe(CO)5 → Fe2(CO)9 + CO

Select photoreactive coordination complexes can undergo oxidation-reduction processes via single electron transfer. This electron transfer can occur within the inner or outer coordination sphere of the metal.[23]

Types of photochemical reactions

Here are some different types of photochemical reactions-

  • Photo-dissociation: AB + hν → A* + B*
  • Photo induced rearrangements, isomerization: A + hν → B
  • Photo-addition: A + B + hν → AB + C
  • Photo-substitution: A + BC + hν → AB + C
  • Photo-redox reaction: A + B + hν → A− + B+

Historical

Although bleaching has long been practiced, the first photochemical reaction was described by Trommsdorff in 1834.[24] He observed that crystals of the compound α-santonin when exposed to sunlight turned yellow and burst. In a 2007 study the reaction was described as a succession of three steps taking place within a single crystal.[25]

Santonin Photochemical reaction.

The first step is a

dimerization in a Diels–Alder reaction (3), and the third one an intramolecular [2+2]cycloaddition
(4). The bursting effect is attributed to a large change in crystal volume on dimerization.

Specialized journals

Learned Societies

International conferences

The organization of these conferences is facilitated by the International Foundation for Photochemistry.[26]

See also

References

  1. .
  2. ^ J. Cadet and T. Douki Photochem. & Photobiol. Sci. 2018 (17) pp 1816-1841 DOI: 10.1039/c7pp00395a
  3. ^ Calvert, J. G.; Pitts, J. N. Photochemistry. Wiley & Sons: New York, US, 1966. Congress Catalog number: 65-24288
  4. ^ Photochemistry, website of William Reusch (Michigan State University), accessed 26 June 2016
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  12. , retrieved 2022-01-24
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  15. .
  16. ^ Peplow, Mark (17 April 2013). "Sanofi launches malaria drug production". Chemistry World.
  17. PMID 23575629
    .
  18. ^ CYCLOBUTANE- TYPE PYRIMIDINE DIMERS IN POLYNUCLEOTIDES, R. B. Setlow, Science 1966 Vol. 153, p. 379, DOI: 10.1126/science.153.3734.379
  19. .
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  25. ^ IUPAC Symposia on Photochemistry. A Brief History, S. Braslavsky, Chemistry International, March–April 2014.

Further reading