Adiabatic process

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This article covers adiabatic processes in thermodynamics. For adiabatic processes in quantum mechanics, see adiabatic process (quantum mechanics). For atmospheric adiabatic processes, see adiabatic lapse rate.

In thermodynamics, an adiabatic process or an isocaloric process is a process in which no heat is transferred to or from working fluid. The term "adiabatic" literally means an absence of heat transfer; for example, an adiabatic boundary is a boundary that is impermeable to heat transfer and the system is said to be adiabatically (or thermally) insulated. An insulated wall approximates an adiabatic boundary. Another example is the adiabatic flame temperature, which is the temperature that would be achieved by a flame in the absence of heat loss to the surroundings. An adiabatic process which is also reversible is called an isentropic process.

The opposite extreme, in which the maximum heat transfer with its surroundings occurs, causing the temperature to remain constant, is known as an isothermal process. Since temperature is thermodynamically conjugate to entropy, the isothermal process is conjugate to the adiabatic process for reversible transformations.

A transformation of a thermodynamic system can be considered adiabatic when it is quick enough so that no significant heat transfer happens between the system and the outside. At the opposite, a transformation of a thermodynamic system can be considered isothermal if it is slow enough so that the system's temperature can be maintained by heat exchange with the outside.

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[edit] Adiabatic heating and cooling

Adiabatic heating and cooling are processes that commonly occur due to a change in the pressure of a gas. Adiabatic heating occurs when the pressure of a gas is increased. An example of this is what goes on in a bicycle pump. After using a bicycle pump to inflate a pneumatic tire or soccer ball the barrel of the pump is found to have heated up as a result of adiabatic heating. Diesel engines rely on adiabatic heating during their compression stroke to reach the high temperatures needed to ignite the fuel. Adiabatic heating also occurs in the Earth's atmosphere when an air mass descends, for example in a katabatic wind or Foehn wind flowing downhill.

Adiabatic cooling occurs when the pressure of a gas is decreased, such as when it expands into a larger volume. An example of this is when the air is released from a pneumatic tire; the outlet air will be noticeably cooler than the tire, and after all the air has escaped the valve stem will be cold to the touch. Adiabatic cooling does not have to involve a fluid. One technique used to reach very low temperatures (thousandths and even millionths of a degree above absolute zero) is adiabatic demagnetisation, where the change in magnetic field on a magnetic material is used to provide adiabatic cooling. Adiabatic cooling also occurs in the Earth's atmosphere with orographic lifting and lee waves, and this can form pileus or lenticular clouds if the air is cooled below the dew point.

Such temperature changes can be quantified using the ideal gas law, or the hydrostatic equation for atmospheric processes.

[edit] Ideal gas

For a simple substance, during an adiabatic process in which the volume increases, the internal energy of the working substance must necessarily decrease
Enlarge
For a simple substance, during an adiabatic process in which the volume increases, the internal energy of the working substance must necessarily decrease

The mathematical equation for an ideal fluid undergoing an adiabatic process is

P V^{\gamma} = \operatorname{constant} \qquad

where P is pressure, V is volume, and

\gamma = {C_{P} \over C_{V}} = \frac{\alpha + 1}{\alpha},

CP being the molar specific heat for constant pressure and CV being the molar specific heat for constant volume. α comes from the number of degrees of freedom divided by 2 (3/2 for monatomic gas, 5/2 for diatomic gas). For a monatomic ideal gas, γ = 5 / 3, and for a diatomic gas (such as nitrogen and oxygen, the main components of air) γ = 7 / 5. Note that the above formula is only applicable to classical ideal gases and not Bose-Einstein or Fermi gases.

For adiabatic processes, it is also true that

VT^\alpha = \operatorname{constant}

T is temperature in kelvins. This can also be written as

TV^{\gamma - 1} = \operatorname{constant}

[edit] Derivation of formula

The definition of an adiabatic process is that heat transfer to the system is zero, δQ = 0. Then, according to the first law of thermodynamics,

d U + \delta W = \delta Q = 0 \qquad \qquad \qquad (1)

where dU is the change in the internal energy of the system and δW is work done by the system. Any work (δW) done must be done at the expense of internal energy U, since no heat δQ is being supplied from the surroundings. Pressure-volume work δW done by the system is defined as

\delta W = P dV. \qquad \qquad \qquad (2)

However, P does not remain constant during an adiabatic process but instead changes along with V.

It is desired to know how the values of dP and dV relate to each other as the adiabatic process proceeds. For an ideal gas the internal energy is given by

U = \alpha n R T \qquad \qquad \qquad (3)

where R is the universal gas constant and n is the number of moles in the system (a constant).

Differentiating equation (3) and use of the ideal gas law yields

d U = \alpha n R d T = \alpha d (P V) = \alpha (P d V + V d P). \qquad (4)

Equation (4) is often expressed as dU = nCVdT because CV = αR.

Now substitute equations (2), (3), and (4) into equation (1) to obtain

-P d V = \alpha P d V + \alpha V d P \,

simplify,

- (\alpha + 1) P d V = \alpha V d P \,

divide both sides by PV,

-(\alpha + 1) {d V \over V} = \alpha {d P \over P}.

From the differential calculus it is then known that

-(\alpha + 1) d (\ln V) = \alpha d (\ln P) \,

which can be expressed as

{\ln P - \ln P_0 \over \ln V - \ln V_0 } = -{\alpha + 1 \over \alpha}

for certain constants P0 and V0 of the initial state. Then

{\ln (P/P_0) \over \ln (V/V_0)} = -{\alpha + 1 \over \alpha},
\ln \left( {P \over P_0} \right) = {-{\alpha + 1 \over \alpha}} \ln \left( {V \over V_0} \right).

Exponentiate both sides,

\left( {P \over P_0} \right) = \left( {V \over V_0} \right)^{-{\alpha + 1 \over \alpha}},

eliminate the negative sign,

\left( {P \over P_0} \right) = \left( {V_0 \over V} \right)^{\alpha + 1 \over \alpha}.

Therefore

\left( {P \over P_0} \right) \left( {V \over V_0} \right)^{\alpha+1 \over \alpha} = 1

and

P V^{\alpha+1 \over \alpha} = P_0 V_0^{\alpha+1 \over \alpha} = P V^\gamma = \operatorname{constant}.

[edit] Graphing adiabats

An adiabat is a curve of constant entropy on the P-V diagram. Properties of adiabats on a P-V diagram are:

  1. Every adiabat asymptotically approaches both the V axis and the P axis (just like isotherms).
  2. Each adiabat intersects each isotherm exactly once.
  3. An adiabat looks similar to an isotherm, except that during an expansion, an adiabat loses more pressure than an isotherm, so it has a steeper inclination (more vertical).
  4. If isotherms are concave towards the "north-east" direction (45 °), then adiabats are concave towards the "east north-east" (31 °).
  5. If adiabats and isotherms are graphed severally at regular changes of entropy and temperature, respectively (like altitude on a contour map), then as the eye moves towards the axes (towards the south-west), it sees the density of isotherms stay constant, but it sees the density of adiabats grow. The exception is very near absolute zero, where the density of adiabats drops sharply and they become rare (see Nernst's theorem).

The following diagram is a P-V diagram with a superposition of adiabats and isotherms:

Image:Entropyandtemp.PNG

The isotherms are the red curves and the adiabats are the black curves. The adiabats are isentropic. Volume is the abscissa (x-axis) and pressure is the ordinate (y-axis).

[edit] See also

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