Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

18
Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11
  • date post

    21-Dec-2015
  • Category

    Documents

  • view

    218
  • download

    1

Transcript of Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Page 1: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Kinetic Theory of Gases

Physics 313Professor Lee

CarknerLecture 11

Page 2: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Exercise #10 Ideal Gas 8 kmol of ideal gas

Compressibility factors

Zm = yiZi

yCO2 = 6/8 = 0.75 V = ZnRT/P = (0.48)(1.33) = 0.638 m3

Error from experimental V = 0.648 m3

Compressibility factors: 1.5% Most of the deviation comes from CO2

Page 3: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Ideal Gas At low pressure all gases approach an ideal

state

The internal energy of an ideal gas depends only on the temperature:

The first law can be written in terms of the

heat capacities:dQ = CVdT +PdV dQ = CPdT -VdP

Page 4: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Heat Capacities Heat capacities defined as:

CV = (dQ/dT)V = (dU/dT)V

Heat capacities are a function of T only for

ideal gases: Monatomic gas

Diatomic gas

= cP/cV

Page 5: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Adiabatic Process

For adiabatic processes, no heat enters of leaves system

For isothermal, isobaric and isochoric processes, something remains constant

Page 6: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Adiabatic Relations

dQ = CVdT + PdV

VdP =CPdT

(dP/P) = - (dV/V)

. Can use with initial and final P and V of

adiabatic process

Page 7: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Adiabats Plotted on a PV diagram adibats have a

steeper slope than isotherms

If different gases undergo the same

adiabatic process, what determines the final properties?

Page 8: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.
Page 9: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Ruchhardt’s Method

How can be found experimentally?

Ruchhardt used a jar with a small oscillating ball suspended in a tube

Page 10: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.
Page 11: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Finding

Also related to PV and Hooke’s law

Modern method uses a magnetically

suspended piston (very low friction)

Page 12: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.
Page 13: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Microscopic View

Classical thermodynamics deals with macroscopic properties

The microscopic properties of a gas

are described by the kinetic theory of gases

Page 14: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Kinetic Theory of Gases The macroscopic properties of a gas are

caused by the motion of atoms (or molecules)

Pressure is the momentum transferred by atoms colliding with a container

Page 15: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Assumptions Any sample has

large number of particles (N)

Atoms have no internal structure

No forces except collision

Atoms distributed randomly in space and velocity direction

Atoms have speed distribution

Page 16: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Particle Motions

The pressure a gas exerts is due to the momentum change of particles striking the container wall

We can rewrite this in similar form to the ideal equation of state:

PV = (Nm/3) v2

Page 17: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Applications of Kinetic Theory

We then use the ideal gas law to find T:PV = nRT

T = (N/3nR)mv2

We can also solve for the velocity:

For a given sample of gas v depends only on the temperature

Page 18: Kinetic Theory of Gases Physics 313 Professor Lee Carkner Lecture 11.

Kinetic Energy

Since kinetic energy = ½mv2, K.E. per particle is:

where NA is Avogadro’s number

and k is the Boltzmann constant