Copolymer
Fundamentals
Definition and Nomenclature
A copolymer is a polymer derived from more than one species of monomer. In contrast, a homopolymer is derived from only one species of monomer. Copolymers from two monomer species are sometimes called bipolymers, from three terpolymers, and from four quaterpolymers.[4] The composition of a copolymer refers to the relative proportions of the different monomer units, typically expressed as mole fractions or mole percentages. The sequence distribution describes the manner in which these monomer units are arranged along the polymer chain, which can vary from random to more ordered patterns. Mole fractions are indicated in copolymer nomenclature by placing them in parentheses after the name, such as poly(A-co-B) (0.70:0.30 mol/mol), denoting 70 mol% A and 30 mol% B. The specific sequence distribution is influenced by reactivity ratios, which affect the likelihood of one monomer adding to the growing chain relative to another.[5][6] IUPAC nomenclature for copolymers employs source-based naming, where the prefix "poly" is followed by the monomer names connected by italicized qualifiers that indicate the arrangement. For unspecified sequence, "-co-" is used, as in poly(styrene-co-acrylonitrile); for random, "-ran-"; for block, "-block-"; and for graft, "-graft-". Monomer names are alphabetized within the name unless a specific sequence must be preserved.[7] The first major synthetic copolymer, styrene-butadiene rubber (Buna S), was developed in Germany in 1929 through emulsion copolymerization as a substitute for natural rubber during shortages. A common example is styrene-acrylonitrile copolymer (SAN), a transparent thermoplastic typically containing 70-75% styrene and 25-30% acrylonitrile, valued for its rigidity and chemical resistance in applications like housings and appliances.[8][9]Copolymerization Mechanisms
Copolymerization primarily occurs through two broad classes of mechanisms: chain-growth and step-growth polymerization. In chain-growth copolymerization, the process involves the sequential addition of monomers to an active chain end, typically initiated by species that generate reactive centers on the monomers. This mechanism is widely used for synthesizing copolymers from vinyl or olefinic monomers and proceeds via free radical, anionic, cationic, or coordination pathways.[10][11] Free radical chain-growth copolymerization is one of the most common methods, initiated by thermal or photochemical decomposition of initiators such as peroxides to form radicals that add to the double bond of a monomer, creating a propagating radical chain end. Propagation occurs through rapid addition of subsequent monomers, with the rate governed by the equation for monomer 1 consumption:
where is the propagation rate constant, is the concentration of monomer 1, and is the concentration of the propagating radical; this extends analogously to the second monomer and cross-additions in copolymerization.[12][10] Anionic copolymerization, suitable for monomers with electron-withdrawing groups like styrene or acrylonitrile, begins with nucleophilic initiators such as organolithium compounds that deprotonate or add to the monomer, forming a carbanion that propagates by attacking additional monomers. Cationic copolymerization, employed for monomers stabilizing carbocations such as isobutylene, uses initiators like proton acids (e.g., BF₃ with water co-initiator) to generate a carbocation chain end that adds monomers sequentially. Coordination copolymerization, often for olefins like ethylene and propylene, relies on transition metal catalysts such as Ziegler-Natta systems (e.g., TiCl₄ with AlR₃), where monomers coordinate to the metal center before insertion into the growing chain, enabling stereoregular copolymers under controlled temperature and pressure conditions.[10][11][13]
Step-growth copolymerization, in contrast, involves the reaction of bifunctional monomers to form covalent bonds between functional groups, typically through condensation with elimination of small molecules like water. This mechanism is prevalent for producing condensation copolymers such as polyesters from diols and diacids (e.g., polyethylene terephthalate from ethylene glycol and terephthalic acid) or polyamides from diamines and diacids (e.g., nylon 6,6 from hexamethylenediamine and adipic acid). The process requires stoichiometric balance of monomers and often elevated temperatures (e.g., 200–300°C) under reduced pressure to drive equilibrium toward high molecular weight, with catalysts like acids or bases accelerating the nucleophilic acyl substitution steps.[14][11]
In both mechanisms, the incorporation of monomers into the copolymer is influenced by factors such as differences in monomer reactivity, which determine the preference for homopropagation versus cross-propagation, and solubility, which affects monomer availability in the reaction medium— for instance, poor solubility of one monomer can lead to heterogeneous incorporation and phase-separated domains in the resulting copolymer.[15][16]
Reactivity Ratios
Reactivity ratios are fundamental kinetic parameters in copolymerization that govern the relative rates at which different monomers are incorporated into the growing polymer chain, thereby influencing the sequence distribution. The reactivity ratio for monomer 1, denoted $ r_1 k_{11} k_{12} $), expressed as $ r_1 = \frac{k_{11}}{k_{12}} $. Similarly, the reactivity ratio for monomer 2 is $ r_2 = \frac{k_{22}}{k_{21}} $, where $ k_{21} $ and $ k_{22} $ are the corresponding rate constants for the chain-end radical derived from monomer 2.[17] The Mayo-Lewis equation relates the instantaneous mole fraction of monomer 1 incorporated into the copolymer ($ F_1 f_1 $ and $ f_2 = 1 - f_1 $) through the reactivity ratios:
This equation, derived from steady-state assumptions in free radical copolymerization, predicts composition drift as polymerization proceeds if $ r_1 \neq r_2 $.[17]
The magnitudes of $ r_1 $ and $ r_2 $ interpret the copolymerization behavior: when both equal 1, the system exhibits ideal random incorporation, with copolymer composition matching the feed. Values where $ r_1 > 1 $ and $ r_2 < 1 $ (or vice versa) indicate that each radical preferentially adds its own monomer, promoting gradient or block-like sequences. Conversely, both $ r_1 < 1 $ and $ r_2 < 1 $ signify a preference for cross-addition, favoring alternating structures.[18]
Experimental determination of reactivity ratios typically involves copolymerizations at low monomer conversions (<10%) to ensure the instantaneous composition approximates the feed, followed by analysis of copolymer composition via techniques such as nuclear magnetic resonance (NMR) spectroscopy for sequence assignment or gravimetric/elemental methods for overall monomer content. Data from multiple feed compositions are then fitted to the Mayo-Lewis equation using nonlinear least-squares optimization to yield $ r_1 $ and $ r_2 $; for processes at higher conversions, numerical integration of the differential copolymer equation accounts for evolving feed composition.[19]
Illustrative examples highlight diverse behaviors: in the free radical copolymerization of styrene (monomer 1) and methyl methacrylate (monomer 2) at 60°C, $ r_1 \approx 0.52 $ and $ r_2 \approx 0.46 $, reflecting nearly ideal random copolymerization with mild alternation tendency. By contrast, the butadiene (monomer 1)-styrene (monomer 2) system in certain anionic conditions yields $ r_1 \approx 0.1 $ and $ r_2 \approx 5 $, exhibiting strong block-forming propensity due to the butadienyl radical's high self-preference.[17][20]