In thermodynamics, the specific heat capacity (symbol c) of a substance is the amount of heat that must be added to one unit of mass of the substance in order to cause an increase of one unit in temperature. It is also referred to as massic heat capacity or as the specific heat. More formally it is the heat capacity of a sample of the substance divided by the mass of the sample. The SI unit of specific heat capacity is joule per kelvin per kilogram, J⋅kg−1⋅K−1. For example, the heat required to raise the temperature of 1 kg of water by 1 K is 4184 joules, so the specific heat capacity of water is 4184 J⋅kg−1⋅K−1. Specific heat capacity often varies with temperature, and is different for each state of matter. Liquid water has one of the highest specific heat capacities among common substances, about 4184 J⋅kg−1⋅K−1 at 20 °C, but that of ice, just below 0 °C, is only 2093 J⋅kg−1⋅K−1. The specific heat capacities of iron, granite, and hydrogen gas are about 449 J⋅kg−1⋅K−1, 790 J⋅kg−1⋅K−1, and 14300 J⋅kg−1⋅K−1, respectively. While the substance is undergoing a phase transition, such as melting or boiling, its specific heat capacity is technically undefined, because the heat goes into changing its state rather than raising its temperature. The specific heat capacity of a substance, especially a gas, may be significantly higher when it is allowed to expand as it is heated (specific heat capacity at constant pressure) than when it is heated in a closed vessel that prevents expansion (specific heat capacity at constant volume). These two values are usually denoted by c p {\displaystyle c_{p}} and c V {\displaystyle c_{V}} , respectively; their quotient γ = c p / c V {\displaystyle \gamma =c_{p}/c_{V}} is the heat capacity ratio. The term specific heat may also refer to the ratio between the specific heat capacities of a substance at a given temperature and of a reference substance at a reference temperature, such as water at 15 °C; much in the fashion of specific gravity. Specific heat capacity is also related to other intensive measures of heat capacity with other denominators. If the amount of substance is measured as a number of moles, one gets the molar heat capacity instead, whose SI unit is joule per kelvin per mole, J⋅mol−1⋅K−1. If the amount is taken to be the volume of the sample (as is sometimes done in engineering), one gets the volumetric heat capacity, whose SI unit is joule per kelvin per cubic meter, J⋅m−3⋅K−1.
History
Discovery of specific heat
One of the first scientists to use the concept was Joseph Black, an 18th-century medical doctor and professor of medicine at Glasgow University. He measured the specific heat capacities of many substances, using the term capacity for heat. In 1756 or soon thereafter, Black began an extensive study of heat. In 1760 he realized that when two different substances of equal mass but different temperatures are mixed, the changes in number of degrees in the two substances differ, though the heat gained by the cooler substance and lost by the hotter is the same. Black related an experiment conducted by Daniel Gabriel Fahrenheit on behalf of Dutch physician Herman Boerhaave. For clarity, he then described a hypothetical, but realistic variant of the experiment: If equal masses of 100 °F water and 150 °F mercury are mixed, the water temperature increases by 20 ° and the mercury temperature decreases by 30 ° (both arriving at 120 °F), even though the heat gained by the water and lost by the mercury is the same. This clarified the distinction between heat and temperature. It also introduced the concept of specific heat capacity, being different for different substances. Black wrote: "Quicksilver [mercury] ... has less capacity for the matter of heat than water."
Definition The specific heat capacity of a substance, usually denoted by c {\displaystyle c} or s {\displaystyle s} , is the heat capacity C {\displaystyle C} of a sample of the substance, divided by the mass M {\displaystyle M} of the sample:
c = C M = 1 M ⋅ d Q d T , {\displaystyle c={\frac {C}{M}}={\frac {1}{M}}\cdot {\frac {\mathrm {d} Q}{\mathrm {d} T}},}
where d Q {\displaystyle \mathrm {d} Q} represents the amount of heat needed to uniformly raise the temperature of the sample by a small increment d T {\displaystyle \mathrm {d} T} . Like the heat capacity of an object, the specific heat capacity of a substance may vary, sometimes substantially, depending on the starting temperature T {\displaystyle T} of the sample and the pressure p {\displaystyle p} applied to it. Therefore, it should be considered a function c ( p , T ) {\displaystyle c(p,T)} of those two variables. These parameters are usually specified when giving the specific heat capacity of a substance. For example, "Water (liquid): c p {\displaystyle c_{p}} = 4187 J⋅kg−1⋅K−1 (15 °C)." When not specified, published values of the specific heat capacity c {\displaystyle c} generally are valid for some standard conditions for temperature and pressure. However, the dependency of c {\displaystyle c} on starting temperature and pressure can often be ignored in practical contexts, e.g. when working in narrow ranges of those variables. In those contexts one usually omits the qualifier ( p , T ) {\displaystyle (p,T)} and approximates the specific heat capacity by a constant c {\displaystyle c} suitable for those ranges. Specific heat capacity is an intensive property of a substance, an intrinsic characteristic that does not depend on the size or shape of the amount in consideration. (The qualifier "specific" in front of an extensive property often indicates an intensive property derived from it.)
Variations The injection of heat energy into a substance, besides raising its temperature, usually causes an increase in its volume and/or its pressure, depending on how the sample is confined. The choice made about the latter affects the measured specific heat capacity, even for the same starting pressure p {\displaystyle p} and starting temperature T {\displaystyle T} . Two particular choices are widely used:
If the pressure is kept constant (for instance, at the ambient atmospheric pressure), and the sample is allowed to expand, the expansion generates work, as the force from the pressure displaces the enclosure or the surrounding fluid. That work must come from the heat energy provided. The specific heat capacity thus obtained is said to be measured at constant pressure (or isobaric) and is often denoted c p {\displaystyle c_{p}} . On the other hand, if the expansion is prevented – for example, by a sufficiently rigid enclosure or by increasing the external pressure to counteract the internal one – no work is generated, and the heat energy that would have gone into it must instead contribute to the internal energy of the sample, including raising its temperature by an extra amount. The specific heat capacity obtained this way is said to be measured at constant volume (or isochoric) and denoted c V {\displaystyle c_{V}} . The value of c V {\displaystyle c_{V}} is always less than the value of c p {\displaystyle c_{p}} for all fluids. This difference is particularly notable in gases where values under constant pressure are typically 30% to 66.7% greater than those at constant volume. Hence the heat capacity ratio of gases is typically between 1.3 and 1.67.
Applicability The specific heat capacity can be defined and measured for gases, liquids, and solids of fairly general composition and molecular structure. These include gas mixtures, solutions and alloys, or heterogenous materials such as milk, sand, granite, and concrete, if considered at a sufficiently large scale. The specific heat capacity can be defined also for materials that change state or composition as the temperature and pressure change, as long as the changes are reversible and gradual. Thus, for example, the concepts are definable for a gas or liquid that dissociates as the temperature increases, as long as the products of the dissociation promptly and completely recombine when it drops. The specific heat capacity is not meaningful if the substance undergoes irreversible chemical changes, or if there is a phase change, such as melting or boiling, at a sharp temperature within the range of temperatures spanned by the measurement.
Measurement The specific heat capacity of a substance is typically determined according to the definition; namely, by measuring the heat capacity of a sample of the substance, usually with a calorimeter, and dividing by the sample's mass. Several techniques can be applied for estimating the heat capacity of a substance, such as differential scanning calorimetry.
The specific heat capacities of gases can be measured at constant volume, by enclosing the sample in a rigid container. On the other hand, measuring the specific heat capacity at constant volume can be prohibitively difficult for liquids and solids, since one often would need impractical pressures in order to prevent the expansion that would be caused by even small increases in temperature. Instead, the common practice is to measure the specific heat capacity at constant pressure (allowing the material to expand or contract as it wishes), determine separately the coefficient of thermal expansion and the compressibility of the material, and compute the specific heat capacity at constant volume from these data according to the laws of thermodynamics.
Units
International system The SI unit for specific heat capacity is joule per kelvin per kilogram J/kg⋅K, J⋅K−1⋅kg−1. Since an increment of temperature of one degree Celsius is the same as an increment of one kelvin, that is the same as joule per degree Celsius per kilogram: J/(kg⋅°C). Sometimes the gram is used instead of kilogram for the unit of mass: 1 J⋅g−1⋅K−1 = 1000 J⋅kg−1⋅K−1. The specific heat capacity of a substance (per unit of mass) has dimension L2⋅Θ−1⋅T−2, or (L/T)2/Θ. Therefore, the SI unit J⋅kg−1⋅K−1 is equivalent to metre squared per second squared per kelvin (m2⋅K−1⋅s−2).
Imperial engineering units Professionals in construction, civil engineering, chemical engineering, and other technical disciplines, especially in the United States, may use English Engineering units including the pound (lb = 0.45359237 kg) as the unit of mass, the degree Fahrenheit or Rankine (°R = 5/9 K, about 0.555556 K) as the unit of temperature increment, and the British thermal unit (BTU ≈ 1055.056 J), as the unit of heat. In those contexts, the unit of specific heat capacity is BTU/lb⋅°R, or 1 BTU/lb⋅°R = 4186.68J/kg⋅K. The BTU was originally defined so that the average specific heat capacity of water would be 1 BTU/lb⋅°F. Note the value's similarity to that of the calorie - 4187 J/kg⋅°C ≈ 4184 J/kg⋅°C (~.07%) - as they are essentially measuring the same energy, using water as a basis reference, scaled to their systems' respective lbs and °F, or kg and °C.
Calories In chemistry, heat amounts were often measured in calories. Confusingly, there are two common units with that name, respectively denoted cal and Cal:
the small calorie (gram-calorie, cal) is 4.184 J exactly. It was originally defined so that the specific heat capacity of liquid water would be 1 cal/(°C⋅g). The grand calorie (kilocalorie, kilogram-calorie, food calorie, kcal, Cal) is 1000 small calories, 4184 J exactly. It was defined so that the specific heat capacity of water would be 1 Cal/(°C⋅kg). While these units are still used in some contexts (such as kilogram calorie in nutrition), their use is now deprecated in technical and scientific fields. When heat is measured in these units, the unit of specific heat capacity is usually:
Note that while cal is 1⁄1000 of a Cal or kcal, it is also per gram instead of kilogram: ergo, in either unit, the specific heat capacity of water is approximately 1.
Physical basis
The temperature of a sample of a substance reflects the average kinetic energy of its constituent particles (atoms or molecules) relative to its center of mass. However, not all energy provided to a sample of a substance will go into raising its temperature, exemplified via the equipartition theorem.
Monatomic gases Statistical mechanics predicts that at room temperature and ordinary pressures, an isolated atom in a gas cannot store any significant amount of energy except in the form of kinetic energy, unless multiple electronic states are accessible at room temperature (such is the case for atomic fluorine). Thus, the heat capacity per mole at room temperature is the same for all of the noble gases as well as for many other atomic vapors. More precisely, c V , m = 3 R / 2 ≈ 12.5 J ⋅ K − 1 ⋅ m o l − 1 {\displaystyle c_{V,\mathrm {m} }=3R/2\approx \mathrm {12.5\,J\cdot K^{-1}\cdot mol^{-1}} } and c P , m = 5 R / 2 ≈ 21 J ⋅ K − 1 ⋅ m o l − 1 {\displaystyle c_{P,\mathrm {m} }=5R/2\approx \mathrm {21\,J\cdot K^{-1}\cdot mol^{-1}} } , where R ≈ 8.31446 J ⋅ K − 1 ⋅ m o l − 1 {\displaystyle R\approx \mathrm {8.31446\,J\cdot K^{-1}\cdot mol^{-1}} } is the ideal gas unit (which is the product of Boltzmann conversion constant from kelvin microscopic energy unit to the macroscopic energy unit joule, and the Avogadro number). Therefore, the specific heat capacity (per gram, not per mole) of a monatomic gas will be inversely proportional to its (adimensional) atomic weight A {\displaystyle A} . That is, approximately,
c V ≈ 12470 J ⋅ K − 1 ⋅ k g − 1 / A c p ≈ 20785 J ⋅ K − 1 ⋅ k g − 1 / A {\displaystyle c_{V}\approx \mathrm {12470\,J\cdot K^{-1}\cdot kg^{-1}} /A\quad \quad \quad c_{p}\approx \mathrm {20785\,J\cdot K^{-1}\cdot kg^{-1}} /A}
For the noble gases, from helium to xenon, these computed values are
Polyatomic gases A polyatomic gas molecule can store energy in additional degrees of freedom. Its kinetic energy contributes to the heat capacity in the same way as monatomic gases, but there are also contributions from the rotations of the molecule and vibration of the atoms relative to each other (including internal potential energy). The heat capacity may also have contribution from excited electronic states for molecules with a sufficiently small energy gap between the ground state and the excited state, such as in NO. For a few systems, quantum spin statistics can also be important contributions to the heat capacity, even at room temperature. The analysis of the heat capacity of H2 due to ortho/para separation, which arises from nuclear spin statistics, has been referred to as "one of the great triumphs of post-quantum mechanical statistical mechanics." These extra degrees of freedom or "modes" contribute to the specific heat capacity of the substance. Namely, when energy is introduced into a gas with polyatomic molecules, only part of it will increase their kinetic energy, and hence the temperature; the rest will go into the other degrees of freedom. To achieve the same increase in temperature, more heat is needed for a gram of that substance than for a gram of a monatomic gas. Thus, the specific heat capacity per mole of a polyatomic gas depends both on the molecular mass and the number of degrees of freedom of the molecules. Quantum statistical mechanics predicts that each rotational or vibrational mode can only take or lose energy in certain discrete amounts (quanta), and that this affects the system's thermodynamic properties. Depending on the temperature, the average energy per molecule may be too small compared to the quanta needed to activate some of those degrees of freedom. Those modes are said to be "frozen out". In that case, the specific heat capacity of the substance increases with temperature, sometimes in a step-like fashion as mode becomes unfrozen and starts absorbing part of the input heat. For example, the molar heat capacity of nitrogen N2 at constant volume is c V , m = 20.6 J ⋅ K − 1 ⋅ m o l − 1 {\displaystyle c_{V,\mathrm {m} }=\mathrm {20.6\,J\cdot K^{-1}\cdot mol^{-1}} } (at 15 °C, 1 atm), which is 2.49 R {\displaystyle 2.49R} . That is the value expected from the Equipartition Theorem if each molecule had 5 kinetic degrees of freedom. These turn out to be three degrees of the molecule's velocity vector, plus two degrees from its rotation about an axis through the center of mass and perpendicular to the line of the two atoms. Because of those two extra degrees of freedom, the specific heat capacity c V {\displaystyle c_{V}} of N2 (736 J⋅K−1⋅kg−1) is greater than that of an hypothetical monatomic gas with the same molecular mass 28 (445 J⋅K−1⋅kg−1), by a factor of 5/3. The vibrational and electronic degrees of freedom do not contribute significantly to the heat capacity in this case, due to the relatively large energy level gaps for both vibrational and electronic excitation in this molecule. This value for the specific heat capacity of nitrogen is practically constant from below −150 °C to about 300 °C. In that temperature range, the two additional degrees of freedom that correspond to vibrations of the atoms, stretching and compressing the bond, are still "frozen out". At about that temperature, those modes begin to "un-freeze" as vibrationally excited states become accessible. As a result c V {\displaystyle c_{V}} starts to increase rapidly at first, then slower as it tends to another constant value. It is 35.5 J⋅K−1⋅mol−1 at 1500 °C, 36.9 at 2500 °C, and 37.5 at 3500 °C. The last value corresponds almost exactly to the value predicted by the Equipartition Theorem, since in the high-temperature limit the theorem predicts that the vibrational degree of freedom contributes twice as much to the heat capacity as any one of the translational or rotational degrees of freedom.
Derivations of heat capacity
Relation between specific heat capacities Starting from the fundamental thermodynamic relation one can show,
c p − c v = α 2 T ρ β T {\displaystyle c_{p}-c_{v}={\frac {\alpha ^{2}T}{\rho \beta _{T}}}}
where
α {\displaystyle \alpha } is the coefficient of thermal expansion,
β T {\displaystyle \beta _{T}} is the isothermal compressibility, and
ρ {\displaystyle \rho } is density. A derivation is discussed in the article Relations between specific heats. For an ideal gas, if ρ {\displaystyle \rho } is expressed as molar density in the above equation, this equation reduces simply to Mayer's relation,
C p , m − C v , m = R {\displaystyle C_{p,m}-C_{v,m}=R\!}
where C p , m {\displaystyle C_{p,m}} and C v , m {\displaystyle C_{v,m}} are intensive property heat capacities expressed on a per-mole basis at constant pressure and constant volume, respectively.
Specific heat capacity The specific heat capacity of a material on a per-mass basis is
c = ∂ C ∂ m , {\displaystyle c={\frac {\partial C}{\partial m}},}
which in the absence of phase transitions is equivalent to
c = E m = C m = C ρ V , {\displaystyle c=E_{m}={\frac {C}{m}}={\frac {C}{\rho V}},}
where
C {\displaystyle C} is the heat capacity of a body made of the material in question,
m {\displaystyle m} is the mass of the body,
V {\displaystyle V} is the volume of the body,
ρ = m V {\displaystyle \rho ={\frac {m}{V}}} is the density of the material. For gases, and also for other materials under high pressures, there is need to distinguish between different boundary conditions for the processes under consideration (since values differ significantly between different conditions). Typical processes for which a heat capacity may be defined include isobaric (constant pressure, d P = 0 {\displaystyle {\text{d}}P=0} ) or isochoric (constant volume, d V = 0 {\displaystyle {\text{d}}V=0} ) processes. The corresponding specific heat capacities are expressed as
c P = ( ∂ C ∂ m ) P , c V = ( ∂ C ∂ m ) V . {\displaystyle {\begin{aligned}c_{P}&=\left({\frac {\partial C}{\partial m}}\right)_{P},\\c_{V}&=\left({\frac {\partial C}{\partial m}}\right)_{V}.\end{aligned}}}
From the results of the previous section, dividing through by the mass gives the relation
c P − c V = α 2 T ρ β T . {\displaystyle c_{P}-c_{V}={\frac {\alpha ^{2}T}{\rho \beta _{T}}}.}
A related parameter to c {\displaystyle c} is C / V {\displaystyle C/V} , the volumetric heat capacity. In engineering practice, c V {\displaystyle c_{V}} for solids or liquids often signifies a volumetric heat capacity, rather than a constant-volume one. In such cases, the specific heat capacity is often explicitly written with the subscript m {\displaystyle m} , as c m {\displaystyle c_{m}} . Of course, from the above relationships, for solids one writes
c m = C m = c volumetric ρ . {\displaystyle c_{m}={\frac {C}{m}}={\frac {c_{\text{volumetric}}}{\rho }}.}
For pure homogeneous chemical compounds with established molecular or molar mass, or a molar quantity, heat capacity as an intensive property can be expressed on a per-mole basis instead of a per-mass basis by the following equations analogous to the per-mass equations:
C P , m = ( ∂ C ∂ n ) P = molar heat capacity at constant pressure, C V , m = ( ∂ C ∂ n ) V = molar heat capacity at constant volume, {\displaystyle {\begin{alignedat}{3}C_{P,m}&=\left({\frac {\partial C}{\partial n}}\right)_{P}&={\text{molar heat capacity at constant pressure,}}\\C_{V,m}&=\left({\frac {\partial C}{\partial n}}\right)_{V}&={\text{molar heat capacity at constant volume,}}\end{alignedat}}}
where n is the number of moles in the body or thermodynamic system. One may refer to such a per-mole quantity as molar heat capacity to distinguish it from specific heat capacity on a per-mass basis.
Polytropic heat capacity The polytropic heat capacity is calculated at processes if all the thermodynamic properties (pressure, volume, temperature) change:
C i , m = ( ∂ C ∂ n ) = molar heat capacity at polytropic process. {\displaystyle C_{i,m}=\left({\frac {\partial C}{\partial n}}\right)={\text{molar heat capacity at polytropic process.}}}
The most important polytropic processes run between the adiabatic and the isotherm functions, the polytropic index is between 1 and the adiabatic exponent (γ or κ).
Dimensionless heat capacity The dimensionless heat capacity of a material is
C ∗ = C n R = C N k B , {\displaystyle C^{*}={\frac {C}{nR}}={\frac {C}{Nk_{\text{B}}}},}
where
C {\displaystyle C} is the heat capacity of a body made of the material in question (J/K), n is the amount of substance in the body (mol), R is the gas constant (J/(K⋅mol)), N is the number of molecules in the body (dimensionless), kB is the Boltzmann constant (J/(K⋅molecule)). In the ideal gas article, dimensionless heat capacity C ∗ {\displaystyle C^{*}} is expressed as c ^ {\displaystyle {\hat {c}}} and is related there directly to half the number of degrees of freedom per particle. This holds true for quadratic degrees of freedom, a consequence of the equipartition theorem. More generally, the dimensionless heat capacity relates the logarithmic increase in temperature to the increase in the dimensionless entropy per particle S ∗ = S / N k B {\displaystyle S^{*}=S/Nk_{\text{B}}} , measured in nats.
C ∗ = d S ∗ d ( ln T ) . {\displaystyle C^{*}={\frac {{\text{d}}S^{*}}{{\text{d}}(\ln T)}}.}
Alternatively, using base-2 logarithms, C ∗ {\displaystyle C^{*}} relates the base-2 logarithmic increase in temperature to the increase in the dimensionless entropy measured in bits.
Heat capacity at absolute zero From the definition of entropy
T d S = δ Q , {\displaystyle T\,{\text{d}}S=\delta Q,}
the absolute entropy can be calculated by integrating from zero to the final temperature Tf:
S ( T f ) = ∫ T = 0 T f δ Q T = ∫ 0 T f δ Q d T d T T = ∫ 0 T f C ( T ) d T T . {\displaystyle S(T_{\text{f}})=\int _{T=0}^{T_{\text{f}}}{\frac {\delta Q}{T}}=\int _{0}^{T_{\text{f}}}{\frac {\delta Q}{{\text{d}}T}}{\frac {{\text{d}}T}{T}}=\int _{0}^{T_{\text{f}}}C(T)\,{\frac {{\text{d}}T}{T}}.}
The heat capacity must be zero at zero temperature in order for the above integral not to yield an infinite absolute entropy, thus violating the third law of thermodynamics. One of the strengths of the Debye model is that (unlike the preceding Einstein model) it predicts the proper mathematical form of the approach of heat capacity toward zero, as absolute zero temperature is approached.
Solid phase The theoretical maximum heat capacity for larger and larger multi-atomic gases at higher temperatures, also approaches the Dulong–Petit limit of 3R, so long as this is calculated per mole of atoms, not molecules. The reason is that gases with very large molecules, in theory have almost the same high-temperature heat capacity as solids, lacking only the (small) heat capacity contribution that comes from potential energy that cannot be stored between separate molecules in a gas. The Dulong–Petit limit results from the equipartition theorem, and as such is only valid in the classical limit of a microstate continuum, which is a high temperature limit. For light and non-metallic elements, as well as most of the common molecular solids based on carbon compounds at standard ambient temperature, quantum effects may also play an important role, as they do in multi-atomic gases. These effects usually combine to give heat capacities lower than 3R per mole of atoms in the solid, although in molecular solids, heat capacities calculated per mole of molecules in molecular solids may be more than 3R. For example, the heat capacity of water