Thermodynamics Flashcards

1
Q

One Mole

A

One mole of a substance has the same number of particles as 12 grams of carbon-12 atoms.

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2
Q

Boyle’s Law

A

The pressure exerted by a fixed mass of gas is inversely proportional to its volume, provided the temperature of the gas remains constant.

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3
Q

Charles’ Law

A

The volume occupied by a gas at constant pressure is directly proportional to its thermodynamic, absolute (i.e. in K) temperature.

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4
Q

Pressure Law

A

The pressure exerted by a fixed mass of gas in a fixed volume is directly proportional to its thermodynamic, absolute (i.e. in K) temperature.

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5
Q

Brownian motion and the 3 conclusions from it

A

Smoke/pollen particles suspended in air/water have random, unpredictable movement. This suggests that the visible particles are constantly bombarded by particles that are:

  1. Too small to be resolved.
  2. Considerably lighter than the visible particles.
  3. Travelling much faster, with a random distribution of velocities.
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6
Q

Explanation of Pressure of Gases

A

When a particle collides elastically with a wall, the wall exerts a force on the particle that reverses its momentum. By Newton’s third law, the particle exerts an equal an opposite force on the wall. The sum of all these forces over the area of the wall is equal to the pressure.

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7
Q

5 Ideal Gas Assumptions

A
  1. There are no forces between molecules (except those in collisions)
  2. The particles can be considered as point particles (occupy negligible volume)
  3. All collisions are perfectly elastic
  4. The duration of each collision is negligible compared to the time between collisions.
  5. Molecues have a random distribution of velocities
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8
Q

What happens to an ideal gas at low temperatures/high pressures? (2 points)

A
  1. The gas particles get much closer together so their finite volume becomes significant.
  2. As they are closer together the intermolecular forces cannot be ignored - they could cause a change in state.
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9
Q

What happens to an ideal gas at very high temperatures?

A

Collisions are no longer elastic as energy can be used to excite electrons to higher energy levels or to weaken bonds within other molecules (or to create plasma).

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10
Q

3 Applications of Boltzmann Factor and what the corresponding threshold energy represents.

A
  1. Rate of reaction (Arrenhius equation) - E_a is activation energy. Catalysts lower E_a and thus increase rate.
  2. Current in semiconductors - E_g is the band gap energy (energy between valence and conduction bands). Doping lowers E_g (by either extending the bands or introducing an intermediate energy level).
  3. Creep of polymers - Q is the activation energy, i.e. the energy needed to activate the diffusion of atoms/vacancies within crystals or the movement of dislocations.
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11
Q

Internal Energy

A

The sum of the random distribution of kinetic and potential energies in an ensemble.

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12
Q

First Law of Thermodynamics (in words)

A

The increase in internal energy of a system is equal to the work done on the system plus the heat supplied to the system.

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13
Q

Isovolumetric (meaning + effect on QWU for increase in p)

A
Constant volume
dW=0
For increase in p:
T increases therefore dU>0
Therefore dQ>0
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14
Q

Isobaric (meaning + effect on QWU for increase in V)

A
Constant pressure
For increase in V:
dW<0 (done by gas)
T increases therefore dU>0
Therefore dQ>0
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15
Q

Isothermal (meaning + effect on QWU for increase in V)

A
Constant temperature
dU=0
For increase in V:
dW<0 (done by gas)
Therefore dQ>0
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16
Q

Adiabatic (meaning + effect on QWU for increase in V)

A
No heat transfer with surroundings.
dQ=0
For increase in V:
dW<0 (done by gas)
Therefore dU<0
17
Q

What is a thermodynamic cycle?

A

A thermodynamic process which starts and ends at the same values of p and V.

18
Q

Heat engine definition (heat pump is opposite of heat engine)

A

A device that is supplied with thermal energy and converts some of this energy into useful work.

19
Q

Carnot Cycle

A

The most efficient thermodynamic cycle for a heat engine (consists of two isothermal and two adiabatic processes)

20
Q

Microstates and Macrostates (optional)

A

Microstates are every different possible arrangement of energy in a system. Macrostates are the more general results of a number of different microstates. The macrostates are things we observe, such as pressure or temperature.

21
Q

Entropy definition

A

Entropy is a measure of the number of ways of distributing energy (or particles) (i.e. the number of microstates) in a system (i.e. amongst the available macrostates).

22
Q

Second Law of Thermodynamics

A

The entropy of the universe tends to a maximum.

23
Q

Two cases where the entropy change of the universe can be 0

A
  1. Temperature is 0 K

2. A process which is isothermal and perfectly reversible

24
Q

Thermodynamic Arrow of Time

A

Irreversible processes separate the past from the future. Therefore since entropy doesn’t decrease (technically it could but yeah) a point where the universe has higher entropy must come after a point with lower entropy in time, as defined by this arrow.

25
Q

2 cosmological Implications of the Second Law

A
  1. The universe had a very low entropy to begin with, meaning it was in a very improbable state.
  2. One way in which the universe could end is a heat death (aka big freeze) where the entropy of the universe reaches a maximum value and so no further useful work can be done.