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Kinetic Theory Kinetic Theory of Gases of Gases CM2004 CM2004 States of Matter: States of Matter: Gases Gases

Kinetic Theory of Gases CM2004 States of Matter: Gases

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Page 1: Kinetic Theory of Gases CM2004 States of Matter: Gases

Kinetic Theory of Kinetic Theory of Gases Gases

CM2004 CM2004 States of Matter: States of Matter: Gases Gases

Page 2: Kinetic Theory of Gases CM2004 States of Matter: Gases

A Theory for 10A Theory for 102323 Particles Particles• In classical theory a

particle’s next move depends upon (equated to) its position, velocity and force acting on it

• Trying to solve such equations for a mole of gas with 1023 particles each with x,y,z coordinates and different speeds is almost impossible

So we theoretically describe the kinetic system on average in terms of a large set of no-volume “points”, which do not attract or repel each other

Page 3: Kinetic Theory of Gases CM2004 States of Matter: Gases

Pressures on AveragePressures on Average

On average the speed term is best represented by <v> as given in the Maxwell-Boltzmann distribution.

Furthermore a particle is equally likely to hit any one of the 6 available walls of the box. Hence:

“Mean-square speed”

Page 4: Kinetic Theory of Gases CM2004 States of Matter: Gases

Microscopic EnergiesMicroscopic Energies

Can be reformulated as:

<k> is called the average kinetic energy per particle

Page 5: Kinetic Theory of Gases CM2004 States of Matter: Gases

Macroscopic Energies and Macroscopic Energies and Boyle’s LawBoyle’s Law

N0<k> is the Total Kinetic Energy of one mole and is called Ek, the macroscopic energy:

PV=nRT

So TEMPERATURE is a direct measure of the INTERNAL

ENERGY of moving gas particles

Page 6: Kinetic Theory of Gases CM2004 States of Matter: Gases

Internal EnergiesInternal Energies

T2>T1

COLD HOT

Each particle moves with an average kinetic energy of:

Page 7: Kinetic Theory of Gases CM2004 States of Matter: Gases

Root Mean Square Speeds Root Mean Square Speeds These (vRMS)represent a single chosen speed to associate with every gas particle, as if they were all moving at this rate.

START END

Molar Mass

Page 8: Kinetic Theory of Gases CM2004 States of Matter: Gases

Thermal Energy: Energy Thermal Energy: Energy at a Definite Temperatureat a Definite Temperature

Kinetic Energy of 1 mole is:

Define Boltzmann’s constant:

Because:

Then Kinetic Energy of 1 particle is:

Page 9: Kinetic Theory of Gases CM2004 States of Matter: Gases

Equipartition of EnergyEquipartition of Energy

The EQUIPARTITION theorem states that a molecule gains ½ kBT of thermal energy for each DEGREE OF FREEDOM (i.e. x,y, z directions). So the total is ³/2 kBT

Page 10: Kinetic Theory of Gases CM2004 States of Matter: Gases

Quantifying Collision RatesQuantifying Collision Rates

Collision Rate (Z*) per face of

cubep = 2mv x Z/6A

Z = 6pvA/ 2mv2

Z = pvA/(kBT)

A is termed, , the collision cross-section

v is termed crel the relative mean speed

NOTE:

But, mv2 = 3kBTTOTAL pressure in the cube volume, where

Z=6Z*

Page 11: Kinetic Theory of Gases CM2004 States of Matter: Gases

Relative Mean Speeds, cRelative Mean Speeds, crelrel

Same Direction

Direct Approach

Typical “on average”

approach

Page 12: Kinetic Theory of Gases CM2004 States of Matter: Gases

Mean Free Path,Mean Free Path,The average distance between collisions is called the

MEAN FREE PATH,

Hence if a molecule collides with a frequency, Z, it spends a time, 1/Z in free flight between collisions and therefore travels a distance of [(1/Z) x c]

= c/Z Z = p crel /(kBT)

= c kB T/p crel

crel = 2½ c

Therefore:

and

= kB T/2½p

=d/2)2

d is the

collision

diameter

Page 13: Kinetic Theory of Gases CM2004 States of Matter: Gases

Maxwell-Boltzmann and vMaxwell-Boltzmann and vRMSRMS

Probability that particle has specific energy,

INCREASING TEMPERATURE

MORE PARTICLES MOVE FASTER

Page 14: Kinetic Theory of Gases CM2004 States of Matter: Gases

PopulationsPopulations

We shall return to the importance of Maxwell-Boltzmann Distributions in CM3006 next year

Molecules and atoms consist of many “micro” states and the higher the temperature the higher the probability

that “excited” states become populated

Page 15: Kinetic Theory of Gases CM2004 States of Matter: Gases

Important Equations (1)Important Equations (1)

Page 16: Kinetic Theory of Gases CM2004 States of Matter: Gases

Important Equations (2)Important Equations (2)

Z = p crel /(kBT) = kB T/ 2½ p