Compressibility

The specification above is incomplete, because for any object or system the magnitude of the compressibility depends strongly on whether the process is isentropic or isothermal. Accordingly, isothermal compressibility is defined:

${\displaystyle \beta _{T}=-{\frac {1}{V}}\left({\frac {\partial V}{\partial p}}\right)_{T},}$

where the subscript T indicates that the partial differential is to be taken at constant temperature.

Isentropic compressibility is defined:

${\displaystyle \beta _{S}=-{\frac {1}{V}}\left({\frac {\partial V}{\partial p}}\right)_{S},}$

where S is entropy. For a solid, the distinction between the two is usually negligible.

Since the density ρ of a material is inversely proportional to its volume, it can be shown that in both cases

${\displaystyle \beta ={\frac {1}{\rho }}\left({\frac {\partial \rho }{\partial p}}\right).}$

The isothermal compressibility is generally related to the isentropic (or adiabatic) compressibility by a few relations:[3]

${\displaystyle {\frac {\beta _{T}}{\beta _{S}}}={\frac {c_{p}}{c_{v}}}=\gamma ,}$

${\displaystyle \beta _{S}=\beta _{T}-{\frac {\alpha ^{2}T}{\rho c_{p}}},}$

${\displaystyle {\frac {1}{\beta _{S}}}={\frac {1}{\beta _{T}}}+{\frac {\Lambda ^{2}T}{\rho c_{v}}},}$

where γ is the heat capacity ratio, α is the volumetric coefficient of thermal expansion, ρ = N/V is the particle density, and ${\displaystyle \Lambda =(\partial P/\partial T)_{V}}$ is the thermal pressure coefficient.

In an extensive thermodynamic system, the application of statistical mechanics shows that the isothermal compressibility is also related to the relative size of fluctuations in particle density:[3]

${\displaystyle \beta _{T}={\frac {(\partial \rho /\partial \mu )_{V,T}}{\rho ^{2}}}={\frac {\langle (\Delta N)^{2}\rangle /V}{k_{\rm {B}}T\rho ^{2}}},}$

where μ is the chemical potential.

The term "compressibility" is also used in thermodynamics to describe deviations of the thermodynamic properties of a real gas from those expected from an ideal gas.

The compressibility factor is defined as

${\displaystyle Z={\frac {pV_{m}}{RT}}}$

where p is the pressure of the gas, T is its temperature, and ${\displaystyle V_{m}}$ is its molar volume, all measured independently of one another. In the case of an ideal gas, the compressibility factor Z is equal to unity, and the familiar ideal gas law is recovered:

${\displaystyle p={\frac {RT}{V_{m}}}}$

Z can, in general, be either greater or less than unity for a real gas.

The deviation from ideal gas behavior tends to become particularly significant (or, equivalently, the compressibility factor strays far from unity) near the critical point, or in the case of high pressure or low temperature. In these cases, a generalized compressibility chart or an alternative equation of state better suited to the problem must be utilized to produce accurate results.

Vertical, drained compressibilities[4]

Material	${\displaystyle \beta _{T}}$ (m2/N or Pa−1)
Plastic clay	2×10−6 – 2.6×10−7
Stiff clay	2.6×10−7 – 1.3×10−7
Medium-hard clay	1.3×10−7 – 6.9×10−8
Loose sand	1×10−7 – 5.2×10−8
Dense sand	2×10−8 – 1.3×10−8
Dense, sandy gravel	1×10−8 – 5.2×10−9
Ethyl alcohol[5]	1.1×10−9
Carbon disulfide[5]	9.3×10−10
Rock, fissured	6.9×10−10 – 3.3×10−10
Water at 25 °C (undrained)[5][6]	4.6×10–10
Rock, sound	< 3.3×10−10
Glycerine[5]	2.1×10−10
Mercury[5]	3.7×10−11

The Earth sciences use compressibility to quantify the ability of a soil or rock to reduce in volume under applied pressure. This concept is important for specific storage, when estimating groundwater reserves in confined aquifers. Geologic materials are made up of two portions: solids and voids (or same as porosity). The void space can be full of liquid or gas. Geologic materials reduce in volume only when the void spaces are reduced, which expel the liquid or gas from the voids. This can happen over a period of time, resulting in settlement.

It is an important concept in geotechnical engineering in the design of certain structural foundations. For example, the construction of high-rise structures over underlying layers of highly compressible bay mud poses a considerable design constraint, and often leads to use of driven piles or other innovative techniques.

The degree of compressibility of a fluid has strong implications for its dynamics. Most notably, the propagation of sound is dependent on the compressibility of the medium.

Compressibility is an important factor in aerodynamics. At low speeds, the compressibility of air is not significant in relation to aircraft design, but as the airflow nears and exceeds the speed of sound, a host of new aerodynamic effects become important in the design of aircraft. These effects, often several of them at a time, made it very difficult for World War II era aircraft to reach speeds much beyond 800 km/h (500 mph).

Many effects are often mentioned in conjunction with the term "compressibility", but regularly have little to do with the compressible nature of air. From a strictly aerodynamic point of view, the term should refer only to those side-effects arising as a result of the changes in airflow from an incompressible fluid (similar in effect to water) to a compressible fluid (acting as a gas) as the speed of sound is approached. There are two effects in particular, wave drag and critical mach.

One complication occurs in hypersonic aerodynamics, where dissociation causes an increase in the “notional” molar volume because a mole of oxygen, as O₂, becomes 2 moles of monatomic oxygen and N₂ similarly dissociates to 2 N. Since this occurs dynamically as air flows over the aerospace object, it is convenient to alter the compressibility factor Z, defined for an initial 30 gram moles of air, rather than track the varying mean molecular weight, millisecond by millisecond. This pressure dependent transition occurs for atmospheric oxygen in the 2,500–4,000 K temperature range, and in the 5,000–10,000 K range for nitrogen.[7]

In transition regions, where this pressure dependent dissociation is incomplete, both beta (the volume/pressure differential ratio) and the differential, constant pressure heat capacity greatly increases. For moderate pressures, above 10,000 K the gas further dissociates into free electrons and ions. Z for the resulting plasma can similarly be computed for a mole of initial air, producing values between 2 and 4 for partially or singly ionized gas. Each dissociation absorbs a great deal of energy in a reversible process and this greatly reduces the thermodynamic temperature of hypersonic gas decelerated near the aerospace object. Ions or free radicals transported to the object surface by diffusion may release this extra (nonthermal) energy if the surface catalyzes the slower recombination process.

For ordinary materials, the bulk compressibility (sum of the linear compressibilities on the three axes) is positive, that is, an increase in pressure squeezes the material to a smaller volume. This condition is required for mechanical stability.[8] However, under very specific conditions, materials can exhibit a compressibility that can be negative.[9][10][11][12]

• Mach number
• Mach tuck
• Poisson ratio
• Prandtl–Glauert singularity, associated with supersonic flight
• Shear strength