General Principles of Gas Physics

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General Principles of Gas Physics

Basic Units and Relationships

Mass: The ability of matter to occupy space, and if in motion to remain in motion, and if at rest to remain at rest.

Weight: The quantification of the mass of an object; the effect of gravitational attraction on an object.

Velocity: The speed that an object moves between two points; expressed in miles per hour or centimeters per second.

Acceleration: The rate at which the velocity of an object increases. The units of acceleration are cm/sec2 or miles/hour2.

Work: The force needed to move an object multiplied by the specific distance the object is moved.

< ?xml:namespace prefix = "mml" />1cubic ft=28.3L1cubic ft28.3L=x3.5×106Lx=1.3×105cubic ft (1)

Work = Force × Distance (1)

Energy is defined as the ability to do work.

Pressure is the force applied per unit area. The units of pressure are:

II States of Matter

All matter exists in one of three basic states (Figure 2-1):

The state of a substance is determined by the relationship of two forces.

The KE of a substance is directly related to temperature.

Intermolecular attractive forces oppose the KE of molecules and tend to force them to exist in less free (solid or liquid) states. Basically there are three types of intermolecular attractive forces: dipole, hydrogen bonding, and dispersion.

1. Dipole forces: Forces that exist between molecules that have electrostatic polarity; the negative aspect of one molecule is lined up and attracted to the positive aspect of another molecule, as seen with NaCl. These substances frequently form crystals.

2. Hydrogen bonding: A force that exists between molecules formed by hydrogen reacting with fluorine, oxygen, or nitrogen.

3. Dispersion forces (London or van der Waals forces): Forces between molecules of relatively nonpolar substances.

Heat

1. The first law of thermodynamics states that energy (heat) is neither created nor lost but simply transformed from one form to another.

2. That is, any energy a substance gains must be lost by its surrounding environment.

3. Heat (energy) always moves from the hotter object to the cooler object until there is thermal equilibrium between the two objects.

4. Heat transfer occurs in four ways:

a. Conduction: Transfer of heat by direct contact between objects. Thermal conductivity is a measure of a substance’s ability to absorb heat.

b. Convection: Heating by the mixing of two fluids (liquids or gases). Heat is allowed to freely transfer in the mixture. Fluid currents carrying heat energy are called convection currents.

c. Radiation: Heating without direct contact, heat energy in the visible and infrared light ranges transferred to the objects they encounter—heating by the sun.

d. Vaporization/condensation: Heating by the transfer of energy as water changes from one state to another.

5. Heat and moisture exchangers function by the process of vaporization and condensation. Water is condensed, and heat is transferred to the device during exhalation. During inspiration the inhaled gas picks up water vapor by vaporization, and heat as a result is transferred to the inhaled gas (see Chapter 35).

6. Calorie: Unit of heat in the metric system. Essentially it is the amount of heat necessary to cause a 1° C increase in the temperature of 1 g of water.

7. British thermal unit (BTU): Unit of heat in the British system. Essentially it is the amount of heat necessary to cause a 1° F increase in the temperature of 1 lb of water.

8. One BTU is equal to 252 calories of heat.

9. Heat capacity: Number of calories needed to raise the temperature of 1 g of a substance 1° C.

10. Specific heat: Ratio of the heat capacity of a substance compared with the heat capacity of water.

Change of state

1. A specific defined amount of heat is needed to cause the molecules of a substance to change their state of matter without a change in temperature.

2. Latent heat of fusion is the amount of heat necessary to change 1 g of a substance at its melting point from a solid to a liquid without causing a change in temperature.

3. The latent heat of vaporization is the amount of heat necessary to change 1 g of a substance at its boiling point from a liquid to a gas without causing a change in temperature.

a. Boiling point is the temperature at 1 atm of pressure at which a substance changes from a liquid to a gas.

b. The total volume of a substance must change from a liquid to a gas before its temperature changes.

c. Latent heats of vaporization are generally much greater than latent heats of fusion.

d. Latent heats of vaporization and boiling points for various substances:

Substance Heat of vaporization (calories/g) Boiling point (° C)
Water 540 100
Hydrogen 40 − 252.5
Carbon dioxide 83 − 78.5
Nitrogen − 196
Oxygen 50 − 183

image

Effects of pressure on melting and boiling points

Triple point: Specific combination of temperature and pressure in which a substance can exist in all three states of matter in dynamic equilibrium.

Sublimation: Transition of a substance from a solid directly to a gas without existence in a liquid state. The heat of sublimation equals the heat of fusion plus the heat of vaporization.

III Properties of Liquids

Liquids flow and assume the shape of their containers.

Liquids exert pressure that varies with the depth of the liquid and its density.

According to Pascal’s principle the shape or volume of a container does not affect the pressure of a liquid; pressure is only affected by the liquid’s height and density.

Variations in liquid pressure in a column produce an upward force referred to as buoyancy.

As a result of buoyancy, objects in water appear to weigh less in water than in air.

Liquids exert a buoyancy force because the pressure below a submerged object always exceeds the pressure above the object.

According to Archimedes principle, the buoyancy force must equal the weight of the fluid displaced by the object.

If the weight of the object exceeds the weight of the displaced water, it sinks, but if it weighs less than the displaced water, it floats.

Archimedes principle is used to determine the specific gravity of liquids such as urine.

IV Kinetic Theory of Gases

The kinetic theory of gases normally is applied to relatively dilute gas volumes.

Principles of the kinetic theory of gases are:

1. Gases are composed of molecules that are in rapid continuous random motion.

2. The molecules undergo near collisions with each other and collide with the walls of their container.

3. All molecular collisions are elastic, and as long as the container is properly insulated, the temperature of the gas remains constant.

4. The KE of molecules of a gas is directly proportional to the absolute temperature.

Avogadro’s Law

VI Density

Density (D) is the mass of an object per unit volume (V) and usually is expressed as g/L:

D=MV (7)

image (7)

On the surface of the earth, mass in equation 7 may be replaced by weight.

Calculation of densities of solids and liquids is straightforward because their volumes are relatively stable at various temperatures and pressures.

The volumes of gases, on the other hand, are severely affected by temperature and pressure.

For this reason, the standard density of all gases is determined at STP (0° C and 760 mm Hg pressure) conditions where the volume used is 22.4 L and the weight used is the GMW of the particular gas:

Standard densities of various substances:

The density of a mixture of gases is determined by the following equation:

Specific gravity: Ratio of the density of a substance to the density of a standard. The specific gravity of solids and liquids is determined using water as the (density, 1 kg/L) standard; for gases, oxygen is used as the standard. When it is stated that the specific gravity of urine is 1.10, it means the urine is 1.10 times heavier than H2O because of the dissolved substances in the urine.

VII Gas Pressure

Pressure (P) in any sense is equal to force per unit area:

The pressure of a gas is directly related to the KE of the gas (see Section II, States of Matter) and to the gravitational attraction of the earth.

With an increase in altitude, the gravitational attraction of the earth on the molecules of gas in the atmosphere decreases.

The barometric pressure (Pb) of the atmosphere is equal to the height of a column of fluid times the fluid’s density (Figure 2-2):

P=gcm2;P=lbin˙2 (11)

Pb = (height of column of fluid)(fluid’s density) (11)

If the fluid used is mercury, normal atmospheric pressure is equal to psi:

P=gcm2;P=lbin˙2

14.7 psi = (29.9 in. Hg)(0.491 lb/in.3)

Mercury’s density in the metric system is 13.6 g/ml; in the British system it is 0.491 lb/in.3.

Gas pressure is frequently expressed as the height of a substance (i.e., mm Hg, cm H2O). These are not true pressure expressions, but they may be easily converted to the proper pressure notation by use of equation 11 if necessary.

Atmospheric pressure can be determined by a number of pressure-measuring devices (Figure 2-3).

Equivalent expressions of normal atmospheric pressure:

VIII Humidity

Water vapor content of the air under atmospheric conditions is variable. Temperature is the factor that most significantly affects water vapor content in the atmosphere.

At a particular temperature, there is a maximum amount of water that a gas can hold, capacity for water vapor.

Because the boiling point of water (100°C) is considerably higher than the normal temperature of the atmosphere, the maximum water vapor content of the atmosphere varies with temperature.

Expressions of water vapor content