Odtnhj

Thermodynamics
The classical Carnot heat engine
Branches Classical Statistical Chemical Quantum thermodynamics Equilibrium / Non-equilibrium
Laws Zeroth First Second Third
Systems State Equation of state Ideal gas Real gas State of matter Equilibrium Control volume Instruments Processes Isobaric Isochoric Isothermal Adiabatic Isentropic Isenthalpic Quasistatic Polytropic Free expansion Reversibility Irreversibility Endoreversibility Cycles Heat engines Heat pumps Thermal efficiency
System properties Note: Conjugate variables in italics Property diagrams Intensive and extensive properties Process functions Work Heat Functions of state Temperature / Entropy (introduction) Pressure / Volume Chemical potential / Particle number Vapor quality Reduced properties
Material properties Property databases Specific heat capacity  c=displaystyle c= Tdisplaystyle T ∂Sdisplaystyle partial S Ndisplaystyle N ∂Tdisplaystyle partial T Compressibility  β=−displaystyle beta =- 1displaystyle 1 ∂Vdisplaystyle partial V Vdisplaystyle V ∂pdisplaystyle partial p Thermal expansion  α=displaystyle alpha = 1displaystyle 1 ∂Vdisplaystyle partial V Vdisplaystyle V ∂Tdisplaystyle partial T
Equations Carnot's theorem Clausius theorem Fundamental relation Ideal gas law Maxwell relations Onsager reciprocal relations Bridgman's equations Table of thermodynamic equations
Potentials Free energy Free entropy Internal energy U(S,V)displaystyle U(S,V) Enthalpy H(S,p)=U+pVdisplaystyle H(S,p)=U+pV Helmholtz free energy A(T,V)=U−TSdisplaystyle A(T,V)=U-TS Gibbs free energy G(T,p)=H−TSdisplaystyle G(T,p)=H-TS
History Culture History General Heat Entropy Gas laws "Perpetual motion" machines Philosophy Entropy and time Entropy and life Brownian ratchet Maxwell's demon Heat death paradox Loschmidt's paradox Synergetics Theories Caloric theory Theory of heat Vis viva ("living force") Mechanical equivalent of heat Motive power Key publications "An Experimental Enquiry Concerning ... Heat" "On the Equilibrium of Heterogeneous Substances" "Reflections on the Motive Power of Fire" Timelines Thermodynamics Heat engines Art Education Maxwell's thermodynamic surface Entropy as energy dispersal
Scientists Bernoulli Boltzmann Carnot Clapeyron Clausius Carathéodory Duhem Gibbs von Helmholtz Joule Maxwell von Mayer Onsager Rankine Smeaton Stahl Thompson Thomson van der Waals Waterston
Book Category Thermodynamics Portal
v t e

Enthalpy /ˈɛnθəlpi/ (listen), a property of a thermodynamic system, is equal to the system's internal energy plus the product of its pressure and volume.^[1][2] In a system enclosed so as to prevent matter transfer, for processes at constant pressure, the heat absorbed or released equals the change in enthalpy.

The unit of measurement for enthalpy in the International System of Units (SI) is the joule. Other historical conventional units still in use include the British thermal unit (BTU) and the calorie.

Enthalpy comprises a system's internal energy, which is the energy required to create the system, plus the amount of work required to make room for it by displacing its environment and establishing its volume and pressure.^[3]

Enthalpy is defined as a state function that depends only on the prevailing equilibrium state identified by the system's internal energy, pressure, and volume. It is an extensive quantity.

Enthalpy is the preferred expression of system energy changes in many chemical, biological, and physical measurements at constant pressure, because it simplifies the description of energy transfer. In a system enclosed so as to prevent matter transfer, at constant pressure, the enthalpy change equals the energy transferred from the environment through heat transfer or work other than expansion work.

The total enthalpy, H, of a system cannot be measured directly. The same situation exists in classical mechanics: only a change or difference in energy carries physical meaning. Enthalpy itself is a thermodynamic potential, so in order to measure the enthalpy of a system, we must refer to a defined reference point; therefore what we measure is the change in enthalpy, ΔH. The ΔH is a positive change in endothermic reactions, and negative in heat-releasing exothermic processes.

For processes under constant pressure, ΔH is equal to the change in the internal energy of the system, plus the pressure-volume work p ΔV done by the system on its surroundings (which is > 0 for an expansion and < 0 for a contraction).^[4] This means that the change in enthalpy under such conditions is the heat absorbed or released by the system through a chemical reaction or by external heat transfer. Enthalpies for chemical substances at constant pressure usually refer to standard state: most commonly 1 bar pressure. Standard state does not, strictly speaking, specify a temperature (see standard state), but expressions for enthalpy generally reference the standard heat of formation at 25 °C.

Enthalpy of ideal gases and incompressible solids and liquids does not depend on pressure, unlike entropy and Gibbs energy. Real materials at common temperatures and pressures usually closely approximate this behavior, which greatly simplifies enthalpy calculation and use in practical designs and analyses.

History

The word enthalpy was coined relatively late, in the early 20th century, in analogy with the 19th-century terms energy (introduced in its modern sense by Thomas Young in 1802) and entropy (coined in analogy to energy by Rudolf Clausius in 1865).
It uses the root of Greek θάλπος "warmth, heat"^[5]
where energy has ἔργον "work" and entropy τροπή "transformation", by analogy expressing the idea of "heat-content" where energy refers to "work-content" and entropy to "transformation-content".
The term does in fact stand in for the older term "heat content",^[6]
a term which is now mostly deprecated as misleading, as dH refers to the amount of heat absorbed in a process at constant pressure only,^[7]
but not in the general case (when pressure is variable).^[8]Josiah Willard Gibbs used the term "a heat function for constant pressure" for clarity.^{[note 1]}

Introduction of the concept of "heat content" H is associated with Benoît Paul Émile Clapeyron and Rudolf Clausius (Clausius–Clapeyron relation, 1850).

The term enthalpy first appeared in print in 1909.^[9] It is attributed to Heike Kamerlingh Onnes, who most likely introduced it orally the year before, at the first meeting of the Institute of Refrigeration in Paris.^[10]
It gained currency only in the 1920s, notably with the Mollier Steam Tables and Diagrams, published in 1927.

Until the 1920s, the symbol H was used, somewhat inconsistently, for "heat" in general.
The definition of H as strictly limited to enthalpy or "heat content at constant pressure" was formally proposed by Alfred W. Porter in 1922.^[11]

Formal definition

The enthalpy of a thermodynamic system is defined as^[12][13]

H=U+pV,displaystyle H=U+pV,

where

H is the enthalpy of the system,

U is the internal energy of the system,

p is the pressure of the system,

V is the volume of the system.

Enthalpy is an extensive property. This means that, for homogeneous systems, the enthalpy is proportional to the size of the system. It is convenient to introduce the specific enthalpy h = H/m, where m is the mass of the system, or the molar enthalpy H_m = H/n, where n is the number of moles (h and H_m are intensive properties). For inhomogeneous systems the enthalpy is the sum of the enthalpies of the composing subsystems:

H=∑kHk,displaystyle H=sum _kH_k,

where the label k refers to the various subsystems. In case of continuously varying p, T or composition, the summation becomes an integral:

H=∫ρhdV,displaystyle H=int rho h,dV,

where ρ is the density.

The enthalpy of homogeneous systems can be viewed as function H(S,p) of the entropy S and the pressure p, and a differential relation for it can be derived as follows. We start from the first law of thermodynamics for closed systems for an infinitesimal process:

dU=δQ−δW.displaystyle dU=delta Q-delta W.

Here, δQ is a small amount of heat added to the system, and δW a small amount of work performed by the system. In a homogeneous system only reversible processes can take place, so the second law of thermodynamics gives δQ = T dS, with T the absolute temperature of the system. Furthermore, if only pV work is done, δW = p dV. As a result,

dU=TdS−pdV.displaystyle dU=T,dS-p,dV.

Adding d(pV) to both sides of this expression gives

dU+d(pV)=TdS−pdV+d(pV),displaystyle dU+d(pV)=T,dS-p,dV+d(pV),

or

d(U+pV)=TdS+Vdp.displaystyle d(U+pV)=T,dS+V,dp.

So

dH(S,p)=TdS+Vdp.displaystyle dH(S,p)=T,dS+V,dp.

Other expressions

The above expression of dH in terms of entropy and pressure may be unfamiliar to some readers. However, there are expressions in terms of more familiar variables such as temperature and pressure:^[12]:88[14]

dH=CpdT+V(1−αT)dp.displaystyle dH=C_p,dT+V(1-alpha T),dp.

Here C_p is the heat capacity at constant pressure and α is the coefficient of (cubic) thermal expansion:

α=1V(∂V∂T)p.displaystyle alpha =frac 1Vleft(frac partial Vpartial Tright)_p.

With this expression one can, in principle, determine the enthalpy if C_p and V are known as functions of p and T.

Note that for an ideal gas, αT = 1,^{[note 2]} so that

dH=CpdT.displaystyle dH=C_p,dT.

In a more general form, the first law describes the internal energy with additional terms involving the chemical potential and the number of particles of various types. The differential statement for dH then becomes

dH=TdS+Vdp+∑iμidNi,displaystyle dH=T,dS+V,dp+sum _imu _i,dN_i,

where μ_i is the chemical potential per particle for an i-type particle, and N_i is the number of such particles. The last term can also be written as μ_i dn_i (with dn_i the number of moles of component i added to the system and, in this case, μ_i the molar chemical potential) or as μ_i dm_i (with dm_i the mass of component i added to the system and, in this case, μ_i the specific chemical potential).

Cardinal functions

The enthalpy, H(S[p],p,N_i), expresses the thermodynamics of a system in the energy-language, or in the energy representation. As a function of state, its arguments include both one intensive and several extensive state variables. The state variables S[p], p, and N_i are said to be the natural state variables in this representation. They are suitable for describing processes in which they are experimentally controlled. For example, in an idealized process, S[p] and p can be controlled by preventing heat and matter transfer by enclosing the system with a wall that is adiathermal and impermeable to matter, and by making the process infinitely slow, and by varying only the external pressure on the piston that controls the volume of the system. This is the basis of the so-called adiabatic approximation that is used in meteorology.^[15]

Alongside the enthalpy, with these arguments, the other cardinal function of state of a thermodynamic system is its entropy, as a function, S[p](H,p,N_i), of the same list of variables of state, except that the entropy, S[p], is replaced in the list by the enthalpy, H. It expresses the entropy representation. The state variables H, p, and N_i are said to be the natural state variables in this representation. They are suitable for describing processes in which they are experimentally controlled. For example, H and p can be controlled by allowing heat transfer, and by varying only the external pressure on the piston that sets the volume of the system.^[16][17][18]

Physical interpretation

The U term can be interpreted as the energy required to create the system, and the pV term as the work that would be required to "make room" for the system if the pressure of the environment remained constant. When a system, for example, n moles of a gas of volume V at pressure p and temperature T, is created or brought to its present state from absolute zero, energy must be supplied equal to its internal energy U plus pV, where pV is the work done in pushing against the ambient (atmospheric) pressure.

In basic physics and statistical mechanics it may be more interesting to study the internal properties of the system and therefore the internal energy is used.^[19][20] In basic chemistry, experiments are often conducted at constant atmospheric pressure, and the pressure-volume work represents an energy exchange with the atmosphere that cannot be accessed or controlled, so that ΔH is the expression chosen for the heat of reaction.

For a heat engine a change in its internal energy is the difference between the heat input and the pressure-volume work done by the working substance while a change in its enthalpy is the difference between the heat input and the work done by the engine:^[21]

dH=δQ−δWdisplaystyle dH=delta Q-delta W

where the work W done by the engine is:

W=−∮⁡pdVdisplaystyle W=-oint pdV

Relationship to heat

In order to discuss the relation between the enthalpy increase and heat supply, we return to the first law for closed systems, with the physics sign convention: dU = δQ − δW, where the heat δQ is supplied by conduction, radiation, and Joule heating. We apply it to the special case with a constant pressure at the surface. In this case the work term can be split into two contributions, the so-called pV work, given by p dV (where here p is the pressure at the surface, dV is the increase of the volume of the system), and the so-called isochoric mechanical work δW′, such as stirring by a shaft with paddles. Cases of long range electromagnetic interaction require further state variables in their formulation, and are not considered here. So we write δW = p dV + δW′. In this case the first law reads:

dU=δQ−pdV−δW′.displaystyle dU=delta Q-p,dV-delta W'.

Now,

dH=dU+d(pV).displaystyle dH=dU+d(pV).

So

dH=δQ+Vdp+pdV−pdV−δW′displaystyle dH=delta Q+V,dp+p,dV-p,dV-delta W'

=δQ+Vdp−δW′.displaystyle ,,=delta Q+V,dp-delta W'.

With sign convention of physics, δW' < 0, because isochoric shaft work done by an external device on the system adds energy to the system, and may be viewed as virtually adding heat. The only thermodynamic mechanical work done by the system is expansion work, p dV.^[22]

The system is under constant pressure (dp = 0). Consequently, the increase in enthalpy of the system is equal to the added heat and virtual heat:

dH=δQ−δW′.displaystyle dH=delta Q-delta W'.

This is why the now obsolete term heat content was used in the nineteenth century.

Applications

In thermodynamics, one can calculate enthalpy by determining the requirements for creating a system from "nothingness"; the mechanical work required, pV, differs based upon the conditions that obtain during the creation of the thermodynamic system.

Energy must be supplied to remove particles from the surroundings to make space for the creation of the system, assuming that the pressure p remains constant; this is the pV term. The supplied energy must also provide the change in internal energy, U, which includes activation energies, ionization energies, mixing energies, vaporization energies, chemical bond energies, and so forth. Together, these constitute the change in the enthalpy U + pV. For systems at constant pressure, with no external work done other than the pV work, the change in enthalpy is the heat received by the system.

For a simple system, with a constant number of particles, the difference in enthalpy is the maximum amount of thermal energy derivable from a thermodynamic process in which the pressure is held constant.^[23]

Heat of reaction

The total enthalpy of a system cannot be measured directly, the enthalpy change of a system is measured instead. Enthalpy change is defined by the following equation:

ΔH=Hf−Hi,displaystyle Delta H=H_mathrm f -H_mathrm i ,

where

ΔH is the "enthalpy change",

H_f is the final enthalpy of the system (in a chemical reaction, the enthalpy of the products),

H_i is the initial enthalpy of the system (in a chemical reaction, the enthalpy of the reactants).

For an exothermic reaction at constant pressure, the system's change in enthalpy equals the energy released in the reaction, including the energy retained in the system and lost through expansion against its surroundings. In a similar manner, for an endothermic reaction, the system's change in enthalpy is equal to the energy absorbed in the reaction, including the energy lost by the system and gained from compression from its surroundings. If ΔH is positive, the reaction is endothermic, that is heat is absorbed by the system due to the products of the reaction having a greater enthalpy than the reactants. On the other hand, if ΔH is negative, the reaction is exothermic, that is the overall decrease in enthalpy is achieved by the generation of heat.^[24]

From the definition of enthalpy as H=U+pV,displaystyle H=U+pV, the enthalpy change at constant pressure ΔH=ΔU+pΔV.displaystyle Delta H=Delta U+pDelta V. However for most chemical reactions, the work term pΔVdisplaystyle pDelta V is much smaller than the internal energy change ΔUdisplaystyle Delta U which is approximately equal to ΔH.displaystyle Delta H. As an example, for the combustion of carbon monoxide 2 CO(g) + O₂(g) → 2 CO₂(g), ΔHdisplaystyle Delta H = –566.0 kJ and ΔUdisplaystyle Delta U = –563.5 kJ.^[25] Since the differences are so small, reaction enthalpies are often loosely described as reaction energies and analyzed in terms of bond energies.

Specific enthalpy

The specific enthalpy of a uniform system is defined as h = H/m where m is the mass of the system. The SI unit for specific enthalpy is joule per kilogram. It can be expressed in other specific quantities by h = u + pv, where u is the specific internal energy, p is the pressure, and v is specific volume, which is equal to 1/ρ, where ρ is the density.

Enthalpy changes

An enthalpy change describes the change in enthalpy observed in the constituents of a thermodynamic system when undergoing a transformation or chemical reaction. It is the difference between the enthalpy after the process has completed, i.e. the enthalpy of the products, and the initial enthalpy of the system, i.e. the reactants. These processes are reversible^[why?] and the enthalpy for the reverse process is the negative value of the forward change.

A common standard enthalpy change is the enthalpy of formation, which has been determined for a large number of substances. Enthalpy changes are routinely measured and compiled in chemical and physical reference works, such as the CRC Handbook of Chemistry and Physics. The following is a selection of enthalpy changes commonly recognized in thermodynamics.

When used in these recognized terms the qualifier change is usually dropped and the property is simply termed enthalpy of 'process'. Since these properties are often used as reference values it is very common to quote them for a standardized set of environmental parameters, or standard conditions, including:

• A temperature of 25 °C or 298.15 K,


• A pressure of one atmosphere (1 atm or 101.325 kPa),


• A concentration of 1.0 M when the element or compound is present in solution,


• Elements or compounds in their normal physical states, i.e. standard state.

For such standardized values the name of the enthalpy is commonly prefixed with the term standard, e.g. standard enthalpy of formation.

Chemical properties:

• 
  Enthalpy of reaction, defined as the enthalpy change observed in a constituent of a thermodynamic system when one mole of substance reacts completely.


• 
  Enthalpy of formation, defined as the enthalpy change observed in a constituent of a thermodynamic system when one mole of a compound is formed from its elementary antecedents.


• 
  Enthalpy of combustion, defined as the enthalpy change observed in a constituent of a thermodynamic system when one mole of a substance burns completely with oxygen.


• 
  Enthalpy of hydrogenation, defined as the enthalpy change observed in a constituent of a thermodynamic system when one mole of an unsaturated compound reacts completely with an excess of hydrogen to form a saturated compound.


• 
  Enthalpy of atomization, defined as the enthalpy change required to atomize one mole of compound completely.


• 
  Enthalpy of neutralization, defined as the enthalpy change observed in a constituent of a thermodynamic system when one mole of water is formed when an acid and a base react.


• Standard Enthalpy of solution, defined as the enthalpy change observed in a constituent of a thermodynamic system when one mole of a solute is dissolved completely in an excess of solvent, so that the solution is at infinite dilution.


• Standard enthalpy of Denaturation (biochemistry), defined as the enthalpy change required to denature one mole of compound.


• 
  Enthalpy of hydration, defined as the enthalpy change observed when one mole of gaseous ions are completely dissolved in water forming one mole of aqueous ions.

Physical properties:

• 
  Enthalpy of fusion, defined as the enthalpy change required to completely change the state of one mole of substance between solid and liquid states.


• 
  Enthalpy of vaporization, defined as the enthalpy change required to completely change the state of one mole of substance between liquid and gaseous states.


• 
  Enthalpy of sublimation, defined as the enthalpy change required to completely change the state of one mole of substance between solid and gaseous states.


• 
  Lattice enthalpy, defined as the energy required to separate one mole of an ionic compound into separated gaseous ions to an infinite distance apart (meaning no force of attraction).


• 
  Enthalpy of mixing, defined as the enthalpy change upon mixing of two (non-reacting) chemical substances.

Open systems

In thermodynamic open systems, matter may flow in and out of the system boundaries. The first law of thermodynamics for open systems states: The increase in the internal energy of a system is equal to the amount of energy added to the system by matter flowing in and by heating, minus the amount lost by matter flowing out and in the form of work done by the system:

dU=δQ+dUin−dUout−δW,displaystyle dU=delta Q+dU_textin-dU_textout-delta W,

where U_in is the average internal energy entering the system, and U_out is the average internal energy leaving the system.

During steady, continuous operation, an energy balance applied to an open system equates shaft work performed by the system to heat added plus net enthalpy added

The region of space enclosed by the boundaries of the open system is usually called a control volume, and it may or may not correspond to physical walls. If we choose the shape of the control volume such that all flow in or out occurs perpendicular to its surface, then the flow of matter into the system performs work as if it were a piston of fluid pushing mass into the system, and the system performs work on the flow of matter out as if it were driving a piston of fluid. There are then two types of work performed: flow work described above, which is performed on the fluid (this is also often called pV work), and shaft work, which may be performed on some mechanical device.

These two types of work are expressed in the equation

δW=d(poutVout)−d(pinVin)+δWshaft.displaystyle delta W=d(p_textoutV_textout)-d(p_textinV_textin)+delta W_textshaft.

Substitution into the equation above for the control volume (cv) yields:

dUcv=δQ+dUin+d(pinVin)−dUout−d(poutVout)−δWshaft.displaystyle dU_textcv=delta Q+dU_textin+d(p_textinV_textin)-dU_textout-d(p_textoutV_textout)-delta W_textshaft.

The definition of enthalpy, H, permits us to use this thermodynamic potential to account for both internal energy and pV work in fluids for open systems:

dUcv=δQ+dHin−dHout−δWshaft.displaystyle dU_textcv=delta Q+dH_textin-dH_textout-delta W_textshaft.

If we allow also the system boundary to move (e.g. due to moving pistons), we get a rather general form of the first law for open systems.^[26] In terms of time derivatives it reads:

dUdt=∑kQ˙k+∑kH˙k−∑kpkdVkdt−P,displaystyle frac dUdt=sum _kdot Q_k+sum _kdot H_k-sum _kp_kfrac dV_kdt-P,

with sums over the various places k where heat is supplied, matter flows into the system, and boundaries are moving. The Ḣ_k terms represent enthalpy flows, which can be written as

H˙k=hkm˙k=Hmn˙k,displaystyle dot H_k=h_kdot m_k=H_mdot n_k,

with ṁ_k the mass flow and ṅ_k the molar flow at position k respectively. The term dV_k/dt represents the rate of change of the system volume at position k that results in pV power done by the system. The parameter P represents all other forms of power done by the system such as shaft power, but it can also be e.g. electric power produced by an electrical power plant.

Note that the previous expression holds true only if the kinetic energy flow rate is conserved between system inlet and outlet.^{[clarification needed]} Otherwise, it has to be included in the enthalpy balance. During steady-state operation of a device (see turbine, pump, and engine), the average dU/dt may be set equal to zero. This yields a useful expression for the average power generation for these devices in the absence of chemical reactions:

P=∑k⟨Q˙k⟩+∑k⟨H˙k⟩−∑k⟨pkdVkdt⟩,displaystyle P=sum _kleftlangle dot Q_krightrangle +sum _kleftlangle dot H_krightrangle -sum _kleftlangle p_kfrac dV_kdtrightrangle ,

where the angle brackets denote time averages. The technical importance of the enthalpy is directly related to its presence in the first law for open systems, as formulated above.

Diagrams

T–s diagram of nitrogen.^[27] The red curve at the left is the melting curve. The red dome represents the two-phase region with the low-entropy side the saturated liquid and the high-entropy side the saturated gas. The black curves give the T–s relation along isobars. The pressures are indicated in bar. The blue curves are isenthalps (curves of constant enthalpy). The values are indicated in blue in kJ/kg. The specific points a, b, etc., are treated in the main text.

The enthalpy values of important substances can be obtained using commercial software. Practically all relevant material properties can be obtained either in tabular or in graphical form. There are many types of diagrams, such as h–T diagrams, which give the specific enthalpy as function of temperature for various pressures, and h–p diagrams, which give h as function of p for various T. One of the most common diagrams is the temperature–specific entropy diagram (T–s-diagram). It gives the melting curve and saturated liquid and vapor values together with isobars and isenthalps. These diagrams are powerful tools in the hands of the thermal engineer.

Some basic applications

The points a through h in the figure play a role in the discussion in this section.

a: T = 300 K, p = 1 bar, s = 6.85 kJ/(kg K), h = 461 kJ/kg;

b: T = 380 K, p = 2 bar, s = 6.85 kJ/(kg K), h = 530 kJ/kg;

c: T = 300 K, p = 200 bar, s = 5.16 kJ/(kg K), h = 430 kJ/kg;

d: T = 270 K, p = 1 bar, s = 6.79 kJ/(kg K), h = 430 kJ/kg;

e: T = 108 K, p = 13 bar, s = 3.55 kJ/(kg K), h = 100 kJ/kg (saturated liquid at 13 bar);

f: T = 77.2 K, p = 1 bar, s = 3.75 kJ/(kg K), h = 100 kJ/kg;

g: T = 77.2 K, p = 1 bar, s = 2.83 kJ/(kg K), h = 28 kJ/kg (saturated liquid at 1 bar);

h: T = 77.2 K, p = 1 bar, s = 5.41 kJ/(kg K), h = 230 kJ/kg (saturated gas at 1 bar);

Throttling

Schematic diagram of a throttling in the steady state. Fluid enters the system (dotted rectangle) at point 1 and leaves it at point 2. The mass flow is ṁ.

One of the simple applications of the concept of enthalpy is the so-called throttling process, also known as Joule-Thomson expansion. It concerns a steady adiabatic flow of a fluid through a flow resistance (valve, porous plug, or any other type of flow resistance) as shown in the figure. This process is very important, since it is at the heart of domestic refrigerators, where it is responsible for the temperature drop between ambient temperature and the interior of the refrigerator. It is also the final stage in many types of liquefiers.

For a steady state flow regime, the enthalpy of the system (dotted rectangle) has to be constant. Hence

0=m˙h1−m˙h2.displaystyle 0=dot mh_1-dot mh_2.

Since the mass flow is constant, the specific enthalpies at the two sides of the flow resistance are the same:

h1=h2,displaystyle h_1=h_2,

that is, the enthalpy per unit mass does not change during the throttling. The consequences of this relation can be demonstrated using the T–s diagram above. Point c is at 200 bar and room temperature (300 K). A Joule–Thomson expansion from 200 bar to 1 bar follows a curve of constant enthalpy of roughly 425 kJ/kg (not shown in the diagram) lying between the 400 and 450 kJ/kg isenthalps and ends in point d, which is at a temperature of about 270 K. Hence the expansion from 200 bar to 1 bar cools nitrogen from 300 K to 270 K. In the valve, there is a lot of friction, and a lot of entropy is produced, but still the final temperature is below the starting value!

Point e is chosen so that it is on the saturated liquid line with h = 100 kJ/kg. It corresponds roughly with p = 13 bar and T = 108 K. Throttling from this point to a pressure of 1 bar ends in the two-phase region (point f). This means that a mixture of gas and liquid leaves the throttling valve. Since the enthalpy is an extensive parameter, the enthalpy in f (h_f) is equal to the enthalpy in g (h_g) multiplied by the liquid fraction in f (x_f) plus the enthalpy in h (h_h) multiplied by the gas fraction in f (1 − x_f). So

hf=xfhg+(1−xf)hh.displaystyle h_mathbf f =x_mathbf f h_mathbf g +(1-x_mathbf f )h_mathbf h .

With numbers: 100 = x_f × 28 + (1 − x_f) × 230, so x_f = 0.64. This means that the mass fraction of the liquid in the liquid–gas mixture that leaves the throttling valve is 64%.

Compressors

Schematic diagram of a compressor in the steady state. Fluid enters the system (dotted rectangle) at point 1 and leaves it at point 2. The mass flow is ṁ. A power P is applied and a heat flow Q̇ is released to the surroundings at ambient temperature T_a.

A power P is applied e.g. as electrical power. If the compression is adiabatic, the gas temperature goes up. In the reversible case it would be at constant entropy, which corresponds with a vertical line in the T–s diagram. For example, compressing nitrogen from 1 bar (point a) to 2 bar (point b) would result in a temperature increase from 300 K to 380 K. In order to let the compressed gas exit at ambient temperature T_a, heat exchange, e.g. by cooling water, is necessary. In the ideal case the compression is isothermal. The average heat flow to the surroundings is Q̇. Since the system is in the steady state the first law gives

0=−Q˙+m˙h1−m˙h2+P.displaystyle 0=-dot Q+dot mh_1-dot mh_2+P.

The minimal power needed for the compression is realized if the compression is reversible. In that case the second law of thermodynamics for open systems gives

0=−Q˙Ta+m˙s1−m˙s2.displaystyle 0=-frac dot QT_mathrm a +dot ms_1-dot ms_2.

Eliminating Q̇ gives for the minimal power

Pminm˙=h2−h1−Ta(s2−s1).displaystyle frac P_textmindot m=h_2-h_1-T_mathrm a (s_2-s_1).

For example, compressing 1 kg of nitrogen from 1 bar to 200 bar costs at least (h_c − h_a) − T_a(s_c − s_a). With the data, obtained with the T–s diagram, we find a value of (430 − 461) − 300 × (5.16 − 6.85) = 476 kJ/kg.

The relation for the power can be further simplified by writing it as

Pminm˙=∫12(dh−Tads).displaystyle frac P_textmindot m=int _1^2(dh-T_mathrm a ,ds).

With dh = T ds + v dp, this results in the final relation

Pminm˙=∫12vdp.displaystyle frac P_textmindot m=int _1^2v,dp.

See also

• Standard enthalpy change of formation (data table)


• Calorimetry


• Calorimeter


• Departure function


• Hess's law


• Isenthalpic process


• Stagnation enthalpy


• Thermodynamic databases for pure substances

Notes

References

Bibliography

• 
  Dalton, J.P. (1909). "Researches on the Joule–Kelvin effect, especially at low temperatures. I. Calculations for hydrogen" (PDF). KNAW Proceedings. 11: 863–873. Bibcode:1908KNAB...11..863D.
  


• 
  Haase, R. (1971). Jost, W., ed. Physical Chemistry: An Advanced Treatise. New York, NY: Academic. p. 29.
  


• 
  Gibbs, J. W. The Collected Works of J. Willard Gibbs, Vol. I (1948 ed.). New Haven, CT: Yale University Press. p. 88..


• 
  Howard, I. K. (2002). "H Is for Enthalpy, Thanks to Heike Kamerlingh Onnes and Alfred W. Porter". J. Chem. Educ. 79 (6): 697–698. Bibcode:2002JChEd..79..697H. doi:10.1021/ed079p697.
  


• 
  Laidler, K. (1995). The World of Physical Chemistry. Oxford: Oxford University Press. p. 110.
  


• 
  Kittel, C.; Kroemer, H. (1980). Thermal Physics. New York, NY: S. R. Furphy & Co. p. 246.
  


• 
  DeHoff, R. (2006). "Thermodynamics in Materials Science". Entropy (2nd ed.). 20 (7): 532. Bibcode:2018Entrp..20..532G. doi:10.3390/e20070532.
  

External links

• 
  Enthalpy - Eric Weisstein's World of Physics


• 
  Enthalpy - Georgia State University


• 
  Enthalpy example calculations - Texas A&M University Chemistry Department