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Physical chemistry is the part of chemistry that seeks to account for the properties and transformations of matter in terms of concepts, principles, and laws drawn from physics. This glossary is a compilation of definitions, descriptions, formulae, and illustrations of concepts that are encountered throughout the subject. This section describes the concepts that begin with the letter P; where appropriate, the entries also describe subsidiary but related concepts. Refer to the Directory for a full list of all the concepts treated.

A p orbital is an atomic orbital with l = 1. There are three p orbitals in each subshell (ml = −1, 0, +1). Real linear combinations are denoted px, py, pz according to their orientation with respect to the three Cartesian axes, each one having one angular nodal plane perpendicular to its axis and passing through the nucleus (Figure P.1). A p orbital has zero amplitude at r = 0, and in a shell with quantum number n has n – 2 radial nodes at r > 0.

Figure P.1

The three orthogonal p orbitals.

Figure P.1

The three orthogonal p orbitals.

Close modal

In molecular orbital theory, a π orbital is a molecular orbital with a nodal plane lying along the internuclear distance (Figure P.2). When occupied by one or two electrons it represents a π bond. In valence bond theory a π bond consists of two paired electrons in overlapping p orbitals, also with a nodal plane that contains the internuclear distance. In a linear molecule, degenerate π orbitals occur in pairs, with angular momentum of magnitude ħ in opposite directions around the internuclear axis. When occupied, the electron density of the pair of orbitals has cylindrical symmetry. In nonlinear molecules, a π bond supplies torsional rigidity to a double bond because rotation around the bond decreases the overlap of the p orbitals and thereby weakens the bond they form.

Figure P.2

(a) Bonding and (b) antibonding π orbitals.

Figure P.2

(a) Bonding and (b) antibonding π orbitals.

Close modal

Two electron spins are said to be paired if the total spin angular momentum is zero. Paired spins are denoted ↑↓. Specifically, the spin wavefunction for two paired spins is (1/2)1/2{α(1)β(2) − β(1)α(2)} and is antisymmetric under particle exchange. This combination corresponds to S = 0, MS = 0 (see vector model). According to the Pauli exclusion principle, two electrons must have paired spins if they occupy the same orbital.

A parabolic potential energy is one that varies with distance as x 2, where x is the displacement from equilibrium. See harmonic oscillator.

A parallel band in infrared spectroscopy is a series of lines that arise from a vibrational transition in which the dipole moment of the molecule changes parallel to the axis of symmetry, as in the antisymmetric stretch of CO2.

A paramagnetic material is one with a positive magnetic susceptibility (see magnetic susceptibility); it tends to move into a magnetic field. The magnetic flux density is greater inside a paramagnetic sample than in a vacuum. Paramagnetism is normally due to the presence of unpaired electron spins. In some instances it can arise from the presence of low-lying excited orbital states and is due to orbital magnetism. In the latter case it is known as temperature-independent paramagnetism (TIP).

Parity is the behaviour of an entity under the operation of inversion. See centre of inversion and g and u.

Two liquids are classified as partially miscible if the temperature–composition phase diagram possesses a region in which the system forms two liquid phases (Figure P.3). The relative composition of the phases in equilibrium is given by the lever rule.

Figure P.3

The phase diagram of two partially miscible liquids.

Figure P.3

The phase diagram of two partially miscible liquids.

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A partial molar property, XJ or J, is defined as
The constraint n′ implies that the abundances of all components of the mixture other than J are held constant. The partial molar volumes of water and ethanol are depicted in Figure P.4. The partial molar Gibbs energy, GJ, is called the chemical potential and is denoted μJ.
Figure P.4

The partial molar volumes of water and ethanol at 298 K.

Figure P.4

The partial molar volumes of water and ethanol at 298 K.

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Partial molar properties are found by fitting a polynomial to the observed variation of a property X with composition and then differentiating this function. A partial molar property can be interpreted as the contribution per mole of substance made by the specified component to the total value of the property. The total value of a property is the weighted sum of the related partial molar properties of all the components:
Variations in partial molar properties obey the Gibbs–Duhem equation:
A special case of this equation for a binary mixture of consisting of A and B is
This relation implies that in a binary mixture when one partial molar quantity increases the other must decrease.
The partial pressure of a gas (real or perfect), pJ, is defined as
where xJ is the mole fraction of J in the mixture and p is the total pressure (Figure P.5). If all the gases in the mixture are perfect, then the partial pressure is the pressure that each gas would exert if it occupied the container alone. According to Dalton’s law, the total pressure of a gaseous mixture is the sum of the partial pressures of the components of the mixture. This law is exact for the formal definition of partial pressure given above but is a limiting law if partial pressures are interpreted as contributing pressures.
Figure P.5

Partial pressure and total pressure.

Figure P.5

Partial pressure and total pressure.

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The particle in a box (PIB) model consists of a particle of mass m in in a one-dimensional region of space of length L in which the potential energy is zero within the box and is infinite elsewhere. It is an elementary problem in quantum mechanics often used to display how the boundary conditions that a wavefunction must satisfy lead to the quantization of energy. Thus, the boundary conditions ψ(0) = 0 and ψ(L) = 0 lead to the following solutions for the energies and wavefunctions (Figures P.6 and P.7):
Note that there is a zero-point energy (at n = 1) of magnitude h 2/mL 2. All the levels are nondegenerate. The separation of neighbouring levels and the transition dipole moment between them are
The separation decreases with increasing mass of the particle and the length of the box. The solutions are readily extended to higher numbers of dimensions. Thus, the energies in a d-dimensional box are
Degeneracies, both accidental and symmetry-related, may be present for d > 1, depending on the relative lengths of the sides of the box.
Figure P.6

The energy levels of a particle in a box.

Figure P.6

The energy levels of a particle in a box.

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Figure P.7

The first five wavefunctions of a particle in a box.

Figure P.7

The first five wavefunctions of a particle in a box.

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The molecular partition function, q , of an isolated molecule is the following sum over its states:
where εi is the energy of the state i measured from the lowest state. If a level J is gJ-fold degenerate, then the sum over states can be replaced by the following sum over levels:
The molecular partition functions for various modes of motion at high temperature (when many states are occupied) are as follows:
σ is the symmetry number for the molecule; the are the rotational constants (as wavenumbers).

The numerical value of a molecular partition function is an indication of the number of states that are thermally accessible at the temperature of interest; typically q = 1 at T = 0, when only the nondegenerate ground state is accessible, and q rises towards the total number of states in the molecule (which is typically infinite) as T rises to infinity (Figure P.8).

Figure P.8

The temperature dependence of the partition functions for systems that have 2, 4, 6, and 8 nondegenerate states.

Figure P.8

The temperature dependence of the partition functions for systems that have 2, 4, 6, and 8 nondegenerate states.

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The molecular partition function summarizes the distribution of populations of the available molecular states and therefore contains information about all the thermodynamic properties of a system composed of independent molecules. Three important relations are
where q m = q / n is the molar partition function.
The canonical partition function, Q, is the analogue of the molecular partition function for a system composed of molecules that may interact. It summarizes the distribution of populations over the states of the entire system. The thermodynamic properties of a system composed of interacting molecules are related to it by
The molecular and canonical partition functions of N noninteracting molecules are related by expressions that depend on whether the molecules are indistinguishable (as in a gas) or distinguishable (as in a solid, where, although chemically identical, they can be identified by their locations):

The pascal (Pa) is the SI unit of pressure, with 1 Pa = 1 N m−2. A convenient related unit is 1 bar = 105 Pa.

Pascal’s triangle is an array of numbers formed from the coefficients in the binomial expansion of (1 + x)n . The first 10 rows are as follows:

graphic
Note that the number in any location is the sum of the two numbers diagonally above it. The number in the rth location (with r = 1 on the far left and r = n on the far right) of the nth row (with n = 1 at the top) is (n – 1)!/(r – 1)!(nr)! (note: 0! = 1).

The Paschen series is a set of lines in the spectrum of atomic hydrogen arising from the transitions between n = 4, 5,… and n = 3. All the lines lie in the infrared.

Passivation is the protection of a surface of a metal by an adhering, impervious, stable film, usually an oxide.

A Patterson synthesis is a technique of data analysis in X-ray crystallography in which the function P( r ) is formed by calculating the Fourier transform of the squares of the structure factors (which are proportional to the diffraction intensities):
The outcome is a map of the separations of the atoms in the unit cell of the crystal, as shown in Figure P.9. If some atoms are heavy, perhaps because they have been introduced by isomorphous replacement, they dominate P( r ) and their locations can be deduced quite simply and used in the determination of the location of lighter atoms.
Figure P.9

Actual and Patterson patterns.

Figure P.9

Actual and Patterson patterns.

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The Pauli exclusion principle states that no more than two electrons can occupy a single orbital, and if two electrons do occupy it, then their spins must be paired. The principle is a consequence of the more general Pauli principle and is at the heart of the building-up principle for the explanation of the electron configurations of atoms (and molecules) and therefore of the periodic table.

The Pauli principle states that the overall wavefunction of a system must change sign when the labels of any two identical fermions are interchanged but must remain unchanged when any two identical bosons are interchanged. Formally:
where the negative sign applies if A and B are identical fermions and the positive sign applies if they are identical bosons. There are numerous important consequences of this principle. It implies, for instance, the Pauli exclusion principle for fermions and for electrons in particular. It also implies that there is no restriction on the number of bosons that may in a given state, so allowing for the formation of rays of intense (multiphoton) monochromatic light. Other consequences include nuclear statistics. The repulsive interaction between closed-shell molecules, and therefore the existence of bulk matter, is essentially a consequence of the principle.

Penetration is the ability of an outer electron to be found inside the inner shells of atoms and hence to experience the full Coulombic attraction of the nucleus. The most penetrating electrons are those in s orbitals, which have nonzero probability density at the nucleus. They penetrate more than other electrons of the same shell, which due to their orbital angular momentum have amplitudes that vary as r l close to the nucleus (Figure P.10); consequently they experience a less shielded nuclear charge and therefore lie lower in energy than the p and d electrons of the same shell. This lowering of the energy is used in the building-up principle to account for the structure of the periodic table.

Figure P.10

Hydrogenic radial distribution functions close to the nucleus.

Figure P.10

Hydrogenic radial distribution functions close to the nucleus.

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A perfect gas (or ideal gas) is a fluid that is described by the equation of state
where p is the pressure, V the volume, T the temperature, n the amount of substance, and R is the gas constant (R = NAk). The isotherms are hyperbolas (Figure P.11).
Figure P.11

Perfect gas isotherms.

Figure P.11

Perfect gas isotherms.

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The perfect gas equation is a limiting law in the sense that the equations of state of all real gases approach it as p → 0. Perfect gas behaviour stems from the absence of intermolecular forces, with the implication that
Two consequences of this relation are
and
where μJT is the Joule–Thomson coefficient. The properties of a perfect gas are captured by the kinetic model, where the internal energy (at T > 0) is ascribed solely to the kinetic energy of the molecules, which are pictured as undergoing ceaseless, chaotic motion characterized in space by the mean free path and in time by the collision frequency. Those parameters can be adapted to account for the transport properties of the gas.
The permeability, μ, of a material is the ratio of the magnetic flux density, B , to the strength, H , of an applied magnetic field:
It is related to the magnetic susceptibility, χ, by
where μ0 is the magnetic constant (formerly: vacuum permeability and also formerly, but no longer, a defined quantity with the value 4π × 10−7 N A−2). Its determined value is
The permittivity, ε, of a material modifies the Coulomb potential in a medium from Q/4πε0r to Q/4πεr, where ε0 is the electric constant (formerly, the vacuum permittivity). The latter is related to the magnetic constant by
and has the experimentally determined value
The relative permittivity (formerly, dielectric constant), εr, of a medium is

A perpendicular band in infrared spectroscopy is an absorption arising from a transition in which the electric dipole moment of the molecule changes in a direction perpendicular to the principal axis of the molecule. An example is the bending mode of CO2. The perpendicular band of a linear molecule may also show a Q-branch of rotational structure.

The formal definition of the pH of a solution is
where a(H+) is the activity of hydrogen ions in the solution. The pH of pure water is 7.0 at 25 °C, and this value corresponds to a neutral solution at this temperature. A pH > 7 signifies a basic solution and a pH < 7 signifies an acidic solution. More generally, because
where pOH = −log a(OH), for a neutral solution pH = pOH and therefore,
The pH of solutions of weak acids and bases may be estimated by consideration of acidity constants. For dilute solutions of nominal molar concentration c with low degrees of deprotonation
The pH of a solution of an acid and its salt (so the acid and the anion of the salt are conjugate pairs) may be estimated from the HendersonHasselbalch equation:
Typical pH curves showing how that pH changes in the course of titration of a weak acid with a strong base are shown in Figure P.12. See also buffer solution.
Figure P.12

pH curves for the titration of weak acids with a strong base.

Figure P.12

pH curves for the titration of weak acids with a strong base.

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A phase diagram is a map showing the regions of the intensive variables (commonly pressure and temperature or relative composition and temperature) where each phase of a system is thermodynamically the most stable. The coexistence curves (or phase boundaries), the lines separating the regions, show the conditions under which the two phases separated by the line are in equilibrium. The locations of the coexistence curves can be discussed in terms of the Clapeyron equation and the related Clausius–Clapeyron equation. A triple point is a point in a phase diagram showing the conditions under which three phases are mutually in equilibrium. Three examples of phase diagrams and their interpretation are shown in Figures P.13P.15.

Figure P.13

A single-component phase diagram.

Figure P.13

A single-component phase diagram.

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Figure P.14

A phase diagram for two partially miscible solids.

Figure P.14

A phase diagram for two partially miscible solids.

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Figure P.15

A phase diagram for solids that form a compound AB2 that does not survive melting.

Figure P.15

A phase diagram for solids that form a compound AB2 that does not survive melting.

Close modal
The phase problem arises in connection with the Fourier synthesis of the electron density from X-ray diffraction intensities. Thus, to form
it is necessary to know the sign of the structure factors Fhkl. However, because the diffraction intensities are proportional to the square modulus of the structure factors, |Fhkl|2, the intensities do not provide information on the sign. For noncentrosymmetric crystals the structure factors may be complex and of the form |Fhkl|eiα , with the phase α indeterminate from the intensity data. The phase problem can be evaded by the use of a Patterson synthesis or tackled directly by using so-called direct methods of phase allocation.
The (Gibbs) phase rule states that the number of phases, P, the number of components, C, and the variance, F, of a system in equilibrium are related by
A phase is a form of matter that is uniform throughout in both chemical composition and physical state. A component is a chemically independent constituent of a system; a constituent is any species present. The number of components is the number of constituents that are necessary to define the composition of all the phases present in the system, taking into account any necessary relations between their concentrations (such as charge neutrality). The variance is the number of intensive variables that can be changed independently without disturbing the number of phases in equilibrium. A single component system (C = 1) for which F = 0 and therefore P = 3 with three phases in mutual equilibrium is said to be invariant and is represented on the phase diagram by a point, the triple point.

Empirically, phosphorescence is the emission of visible light when the substance is illuminated with higher energy electromagnetic radiation and which persists for at least short times after the source of illumination is removed. Mechanistically, it is the emission of visible light after excitation and steps that include intersystem crossing, commonly from a singlet to a triplet state.

In more detail, the mechanism of phosphorescence is as follows (Figure P.16). First, a molecule is excited electronically into a vibrationally excited state of an upper electronic state. Then, as radiationless decay of the vibrational excitation occurs, the excited electronic state undergoes intersystem crossing under the influence of spin–orbit coupling and turns into an excited state with a different multiplicity, commonly a triplet (S = 1). Radiationless decay of the vibrational excitation now continues in the new electronic state until the molecule reaches the vibrational ground state of that state. There is then a delay as the state undergoes a spin-forbidden emission transition to the ground singlet state.

Figure P.16

The mechanism of phosphorescence.

Figure P.16

The mechanism of phosphorescence.

Close modal

Intersystem crossing depends on the presence of spin–orbit coupling, so the phosphorescence may be enhanced by the presence of atoms of a heavy element (such as sulfur). Phosphorescent radiation has a lower frequency than the incident radiation because vibrational energy has been discarded and because the intersystem crossing generally takes place to a lower lying electronic state than the initially excited state.

The photoelectric effect is the ejection of electrons from a solid, usually a metal, when it is illuminated with high energy electromagnetic radiation, typically in the ultraviolet region. The following characteristics are observed:

  1. No electrons are ejected, regardless of the intensity of the radiation, unless the frequency exceeds a threshold value characteristic of the solid.

  2. The kinetic energy of the ejected electrons varies linearly with the frequency of the incident radiation but is independent of its intensity.

  3. Even at low light intensities electrons are rejected immediately if the frequency is above threshold.

The effect is explained in terms of the collision of a photon of frequency ν and energy h ν with an electron that can be removed from the solid only if it is supplied with at least an energy Φ, for the conservation of energy demands that the kinetic energy, Ek, of the ejected electron will be
The quantity Φ is called the photoelectric work function of the solid.
Photoelectron spectroscopy (or photoemission spectroscopy, PES and PS) is the observation of the kinetic energies of electrons ejected by the absorption of high frequency monochromatic electromagnetic radiation. The technique is designated UV-PES if the incident radiation is in the ultraviolet region and XPS or ESCA (electron spectroscopy for chemical analysis) if X-rays are used. The basis of the technique is the conservation of energy and the fact that a photon of frequency ν has energy h ν and the kinetic energy of the ejected electron is
where Ii is the ionization energy of the target in which the electron occupied the orbital i. According to Koopmans’ theorem, that ionization energy is equal to the one-electron energy of the occupied orbital, Ii = −εi.

The ultraviolet technique yields information about the valence shells of molecules. The X-ray technique allows inner electrons to be studied. These electrons are largely but not entirely independent of the state of bonding of the atom, so the kinetic energy of the photoejected electron can be used to identify the element present in the sample (hence the name ESCA). The ultraviolet technique is enriched by the observation of vibrational structure in the spectrum because some of the energy of the incident photon is left in an excited state of vibration of the cation formed by ionization.

A photon is a quantum of electromagnetic radiation. More generally, a photon is a boson responsible for conveying the electromagnetic force between electrically charged particles. A photon of radiation of frequency ν has an energy h ν ; it is massless and is a spin-1 boson. The component of spin angular momentum around its direction of travel is designated by its helicity, σ, which may be ±1, corresponding to left and right circularly polarized radiation, respectively. In a vacuum, photons travel at the speed of light, c, which has the exact, defined value c = 299 792 458 m s−1.

A plait point is a critical point on a triangular phase diagram at which two phases in equilibrium have the same composition (Figure P.17).

Figure P.17

A plait point.

Figure P.17

A plait point.

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Planck’s constant, h, is the fundamental constant introduced at the inception of quantum theory and occurs whenever quantum phenomena are important. Its exact, defined value is h = 6.626 070 15 × 10−34 J s. A closely related quantity, which is particularly useful for the discussion of the of angular momenta and circular motion in general, is the reduced Planck’s constant, ħ = h/2π. Its value is ħ ≈ 1.054 571 817 × 10−34 J s.

Poiseuille’s formula gives the rate of flow of an incompressible fluid of viscosity η through a tube of radius r and length L when the pressures are p1 and p2 at either end:
where p0 is the pressure at which the volume V is measured.
Poisson’s equation relates the electric potential, ϕ, to the charge density, ρ. Its general form is
where ε is the permittivity of the medium. For a spherically symmetrical charge distribution it becomes either of the two equivalent forms

A polar molecule is a molecule with a permanent electric dipole moment. For a molecule to be polar it must belong to one of the groups Cn; in which case the dipole moment lies parallel to the symmetry axis.

The polarizability, α, of a molecule is the constant of proportionality between the strength of the applied field, E , and the magnitude of the resulting induced electric dipole moment, μ:
For a general orientation of a nonspherical molecule the induced moment is not necessarily parallel to the direction of the applied field, in which case this expression becomes
Polarizabilities are commonly reported as a polarizability volume, α′, where
Polarizability volumes have the dimensions of volume and numerical values comparable to the volume of the molecule. In general, a molecule has a high polarizability if it has many electrons, has low lying excited states, and is large.

The polarizability of a molecule varies with frequency of the applied field (Figure P.18). At low frequencies and if the molecule is polar, the polarizability includes a contribution from orientation distortion, the alignment of the entire molecules in the applied field. This contribution is lost when the frequency is greater than the rotational frequency of the molecule. The next contribution to disappear is the distortion polarization, the polarization that stems from the distortion of the shape of the molecule. This contribution disappears when the frequency exceeds the vibrational frequency of the molecule. At optical frequencies, only the electronic polarization, the polarization stemming from the shift in positions of electrons, survives.

Figure P.18

The variation of polarizability with freequency.

Figure P.18

The variation of polarizability with freequency.

Close modal
The polarization of an electrode is the change in its kinetic behaviour due to modification of the composition of the electrolyte in its vicinity. One source of polarization is the depletion of the electroactive species as a result of a high current density. A higher overpotential is then needed to produce a given current. This contribution to the overpotential is called the polarization overpotential, η′. If it is supposed that there is a Nernst diffusion layer of thickness δ at the electrode, then the polarization overpotential when the current density is j is
where z is the charge number of the ions in solution at a molar concentration c and D is the diffusion coefficient. The limiting current density, jmax, the maximum current density for a given molar concentration and thickness of layer, is

The polarization mechanism is a means of coupling the magnetic moments of nuclei and electrons through the bonds that link them. It is responsible for aspects of the hyperfine structure of EPR spectra and the fine structure of NMR spectra.

The mechanism of the interaction between the two protons in an H–C–H group is as follows (Figure P.19). Suppose the spin of one proton is α. There is a slight advantage, due to the Fermi contact interaction, for the electron in the bond to it to be α too. Therefore, the other electron in the bond must be β, and will be close to the C atom. Hund’s rule favours parallel spins in orthogonal orbitals on atoms, so there will be a slight advantage in the electron close to the C atom in the second bond to be β too. Therefore, the second electron of the second bond will be α and close to the second proton. That proton interacts with it by another Fermi contact interaction, and has a lower energy if it too is α and a higher energy if it is β. Thus, there is a coupling between the two protons. A similar line of reasoning applies to the hyperfine coupling of a π electron in a C–H fragment as expressed by the McConnell equation.

Figure P.19

The polarization mechanism.

Figure P.19

The polarization mechanism.

Close modal

Light is plane polarized if its electric field oscillates in a single plane (and its magnetic component oscillates in a perpendicular plane). It is circularly polarized when the electric vector rotates around the direction of propagation (Figure P.20). Left-circularly polarized light rotates in a counterclockwise direction as perceived by a viewer facing the oncoming ray (and consists of photons of helicity σ = +1). Right-circularly polarized light rotates in a clockwise direction from the same viewpoint (and consists of photons of helicity σ = −1). Plane polarized light can be regarded as a superposition of two counter-rotating circularly polarized rays with the same amplitude. Elliptically polarized light is obtained when the superimposed circular components have different amplitudes.

Figure P.20

Linearly and circularly polarized light.

Figure P.20

Linearly and circularly polarized light.

Close modal
There are two principal modes of polymerization. In chain polymerization an activated monomer M attacks another monomer, links to it, and then that unit attacks another monomer, and so on. High polymers are formed rapidly and only the yield and not the molar mass of the polymer is increased by allowing long reaction times. The rate of reaction is proportional to the square root of the initiator concentration:
In stepwise polymerization any two monomers present in the reaction mixture can link together at any time and growth is not confined to the chains that have already started. The molar mass of the product grows with time:
where [A]0 is the initial molar concentration of monomers and 〈n〉 is the average number of monomer units in a chain.

Positronium, Ps, is a hydrogenic species consisting of an electron, e, and its antiparticle, a positron, e+. The ground state is para-positronium (p-Ps), with paired spins (S = 0, MS = 0); its lifetime is 0.12 ns and decays with the emission of two γ-ray photons. ortho-Positronium (o-Ps), with S = 1, MS = 0, ±1, lies 1 meV above the singlet, lives for 142 ns, and decays into three γ-ray photons.

A potential energy surface is a plot of the potential energy of a collection of atoms as their relative coordinates are allowed to range over all positions. It is common for visual portrayals to exhibit slices through the full surface; the slices correspond to a variety of constraints applied to the atoms. Thus, in the discussion of a triatomic system the three atoms may be constrained to be collinear (Figure P.21). The trajectory of least potential energy through a surface is identified with the reaction coordinate and the energy requirements and optimum mode of motion, including the value of the activation energy, are assessed on the basis of trajectories over the surface. For a correct mechanistic portrayal of the behaviour of a point on the surface, the axes are slanted (at 60° for a homonuclear triatomic system), for otherwise the effective mass of the system would depend on the direction in which it was travelling. For the classification of surfaces as attractive and repulsive, see that entry.

Figure P.21

A potential energy surface for a linear triatomic system and the slanted version.

Figure P.21

A potential energy surface for a linear triatomic system and the slanted version.

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The powder method of X-ray diffraction makes use of a monochromatic beam of X-rays and a powder sample. The technique is used to recognize the composition of samples from their characteristic diffraction patterns and to determine the symmetry and dimensions of the unit cell.

Power, P, is the rate at which energy is supplied. It is measured in watts, W, with 1 W = 1 J s−1.

Precession is the migration of the axis of rotation of a body on a cone around a fixed axis (Figure P.22). Classically, a magnetic dipole precesses around the direction of an applied magnetic field. In quantum mechanics the concept of precession is preserved in the vector model of angular momentum. In this model, an angular momentum is represented by a vector with a length proportional to the magnitude of the momentum, {j(j + 1)}1/2, and a component on the z-axis proportional to the quantum number mj. In the absence of a magnetic field the vector lies stationary at an unspecified angle on a cone. In the presence of a magnetic field, it is supposed to process on this cone at its Larmor frequency. The stronger the field, the faster is the procession.

Figure P.22

Precessional motion.

Figure P.22

Precessional motion.

Close modal

In the phenomenon of predissociation it is found that the sharp vibrational structure of an electronic transition gives way to a broad featureless structure before the sharp structure resumes and the continuum characteristic of dissociation is reached. The explanation is that the upper electronic molecular potential energy curve is crossed by a dissociative state (Figure P.23). An internal conversion occurs at the intersection, and the upper state takes on a dissociative character at energies that correspond to the crossing. That dissociative character shortens the lifetime of vibrational states, and as a result of lifetime broadening transitions to these states become blurred.

Figure P.23

Predissociation at the intersection of curves.

Figure P.23

Predissociation at the intersection of curves.

Close modal
A pre-equilibrium in a reaction mechanism is an elementary reaction and its reverse that are assumed to occur so rapidly that the reactants and the products of that step (which is an intermediate in the overall scheme) are in dynamic equilibrium. The concentration of the intermediate can be expressed in terms of an equilibrium constant for the step, as in
Pressure, p, is force, F, divided by the area, A, to which the force is applied: p = F/A. It is normally reported in pascals, Pa, where 1 Pa = 1 N m−2. Other common units are 1 bar = 105 Pa and 1 atm =101.325 kPa exactly. The pressure of a gas is detected by the impact of its molecules on the walls of the vessel or some interior surface. The pressure at the base of a column of incompressible fluid is due to the weight of the overlying fluid. The following equations express the pressure in a variety of systems:
where M is the molar mass, n the amount, A the Helmholtz energy, Q the canonical partition function, ρ the mass density, m the mass, and σ the area on which that mass rests. See also equation of state.

The principal axis is the axis of symmetry of highest order; the Cn axis with the highest value of n.

The principal quantum number, n, is the quantum number that specifies the (bound state) energy of electron in a hydrogenic atom and governs the ranges of the quantum numbers l and ml of its wavefunctions:
where μ is the reduced mass. It is the label of the shells of an atom, with n also the number of subshells of the shell and n 2 the total number of orbitals in the shell. A wavefunction of the atom has n−1 nodes, of which nl−1 are radial nodes and the remaining l are angular nodes.

Promotion is a concept employed in valence bond theory to account for the number of bonds that an atom can form. It is supposed that the overall lowering of energy on bond formation involves an investment in energy in which one or more electrons are transferred from filled valence-shell orbitals into empty valence-shell orbitals, so making more unpaired electrons available for bond formation. Thus, the ground state configuration of carbon, which being [ He ] 2 s 2 2 p x 1 2 p y 1 can form only two bonds, is regarded as promoted to [ He ] 2 s 1 2 p x 1 2 p y 1 2 p z 1 , which can form four bonds. The notional investment of energy is recovered from the energy released by the formation of more bonds.

Proton decoupling is a technique used in NMR to simplify the appearance of carbon-13 spectra. The fine structure of the carbon-13 resonance due to their spin-coupling to protons is effectively eliminated by irradiating the latter at their resonance frequencies so that they undergo a rapid spin reorientation. As a result, the coupling to them is averaged to zero.

A pVT surface is a graphical depiction of the equation of state in which one variable is plotted against the other two. The only states in which the substance can exist correspond to points on the surface. The surfaces shown in Figures P.24 and P.25 are for a perfect gas and a van der Waals gas (the labels on the latter are reduced temperatures).

Figure P.24

The pVT surface of a perfect gas.

Figure P.24

The pVT surface of a perfect gas.

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Figure P.25

The pVT surface of a van der Waals gas.

Figure P.25

The pVT surface of a van der Waals gas.

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