Light can change things. 
Light can change how things work. 
Light helps plants make food. Sunlight helps our bodies make vitamin D. It even helps us see! 
But light can also break things. It can make plastic fall apart. It can even change our DNA. Light is a very busy force in our world.
Photochemistry is a branch of chemistry. It studies how light causes changes in things. This happens when a substance soaks up light. The light can be ultraviolet, visible, or infrared radiation. 
There are rules for how this works. The Grotthuss–Draper law says a substance must soak up light to react. The Stark–Einstein law says one photon of light can only activate one molecule. This process starts with photoexcitation. This is when a part of a molecule moves to a higher energy state. This state is called an excited state.
When things are in an excited state, they can act in different ways. They might give off light through fluorescence. They might also give off light through phosphorescence, which is much slower. Scientists use a Jablonski diagram to show these paths. 
Light is very important in nature. It helps plants make food through photosynthesis. It helps humans make vitamin D from sunlight. It even helps us see. 
Photochemistry is a special branch of chemistry. It focuses on the chemical effects of light. This field studies how light causes changes in matter. Light can come in different forms like ultraviolet, visible, or infrared radiation. 
To understand how it works, we look at the first step called photoexcitation. This is when a molecule soaks up light and moves to a higher energy state. This new state is called an excited state. There are two main rules for this process. The Grotthuss–Draper law says a substance must absorb light to react. The Stark–Einstein law says one photon of light activates no more than one molecule. 
Scientists have studied these light paths for a long time. They use a special chart called a Jablonski diagram to map them. This diagram shows how molecules move between different energy levels. Researchers like Theodor Grotthuss and John W. Draper helped define the first law. Physicists Johannes Stark and Albert Einstein helped define the second law. 
There are many important facts about how light interacts with different materials. For example, Pyrex glass absorbs light shorter than 275 nm. Because of this, scientists often use quartz for their reactors instead. The type of liquid used in an experiment is also very important. Some liquids, like acetone, can block certain types of light.
Photochemistry connects to many things you see every day. It is the reason plants can make food through photosynthesis. It is also how your body makes vitamin D from sunlight. Even your eyes use a photochemical reaction to help you see. 
Photochemistry is the branch of chemistry that studies the chemical effects of light. It explores how light energy causes matter to undergo chemical changes. This field is essential because light can drive reactions that heat alone cannot achieve. While temperature-driven reactions rely on thermal energy, photochemical reactions access high-energy intermediates. These intermediates allow molecules to overcome large activation barriers in very short periods. This capability makes certain chemical pathways accessible that would otherwise be impossible through thermal processes alone. 
The process begins with photoexcitation. This is the first step where a reactant absorbs light and is elevated to a higher energy state called an excited state. This process is governed by two fundamental principles. The Grotthuss–Draper law states that a substance must absorb light to undergo a photochemical reaction. The Stark–Einstein law adds that for every photon of light absorbed, no more than one molecule is activated. This relationship is often defined by the quantum yield of the reaction. 
When a molecule in its ground state (S0) absorbs light, an electron is excited to a higher orbital. This electron maintains its spin, following the spin selection rule. This excitation can move an electron from the Highest Occupied Molecular Orbital (HOMO) to the Lowest Unoccupied Molecular Orbital (LUMO). Molecules can reach various singlet excited states, labeled S1, S2, and so on. According to Kasha's rule, higher singlet states quickly relax to the S1 state through radiationless decay or internal conversion (IC). From S1, the molecule can return to the ground state by emitting a photon, a process known as fluorescence. 
Alternatively, a molecule may undergo a different path called intersystem crossing (ISC). During ISC, the molecule undergoes spin inversion to create a triplet excited state (T1). In this state, two unpaired electrons have the same spin. According to Hund's rule of maximum multiplicity, the T1 state is more stable than the S1 state. This triplet state can relax to the ground state through radiation called phosphorescence. Because this process requires a change in electronic spin, phosphorescence is much slower than fluorescence. These various energy transitions are mapped using a Jablonski diagram, which serves as the paradigm of molecular photochemistry.
To study these reactions, scientists use specific light sources and equipment. In nature, sunlight is a common polychromatic source. In laboratories, mercury-vapor lamps are frequently used because they emit specific wavelengths, such as 254 nm. Researchers may also use lasers for monochromatic light or LEDs for narrow bands. The choice of container is critical because different materials absorb different wavelengths. For example, Pyrex glass absorbs wavelengths shorter than 275 nm. Therefore, many photochemical reactors are made of quartz to ensure the light reaches the target.
The solvent used in an experiment is another vital parameter. Solvents can act as reactants or block light from reaching the substrate. Chlorinated solvents are often avoided because the C–Cl bond can lead to unwanted chlorination. Hydrocarbon solvents are preferred for high-energy photon experiments because they only absorb short wavelengths. Some solvents, like acetone, have a "cut off" point where they absorb strongly, such as at wavelengths shorter than 330 nm. Scientists often select wavelengths based on the absorption maximum of the reactive species to maximize efficiency. 
Photochemistry has massive industrial and biological significance. In industry, about 100,000 tonnes of benzyl chloride are produced annually via a gas-phase photochemical reaction of toluene with chlorine. In biology, photochemistry is the foundation of photosynthesis, where plants convert carbon dioxide and water into glucose and oxygen. It also enables human vision through the reaction of rhodopsin and helps the body form vitamin D from sunlight. However, it can also be destructive, such as the photodegradation of plastics or DNA mutations that lead to skin cancers. 
Beyond simple reactions, photochemistry connects to advanced medical and technological fields. Photodynamic therapy uses light to destroy tumors by generating singlet oxygen through photosensitized reactions. In technology, photoresist technology is used to produce microelectronic components. Furthermore, continuous-flow photochemistry offers advantages over traditional batch methods. By using microreactors, scientists can maximize illumination through a large surface-area-to-volume ratio. This setup also allows for efficient cooling, which helps decrease the formation of unwanted thermal side products.
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