THERMO1 Flashcards

(32 cards)

1
Q

0th Law of Thermodynamics

A

Defines temperature

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2
Q

1st Law of Thermodynamics

A

Conservation of energy

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3
Q

2nd Law of Thermodynamics

A

The entropy of an isolated system can never decrease

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4
Q

3rd Law of Thermodynamics

A

The entropy of a perfect crystal tends to zero at absolute zero

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5
Q

Zeroth Law of Thermodynamics

A

If two objects are in thermal equilibrium with a third, then the two objects are also on thermal equilibrium with each other

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6
Q

What is thermal equilibrium?

A

When heat flow ceases

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7
Q

What is heat?

A

Flow of energy caused by a difference in temperature

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8
Q

What is temperature?

A

A measure of the average translational kinetic energy per molecule

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9
Q

What happens when an object absorbs heat?

A

It increases its internal energy

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10
Q

What is a thermal reservoir?

A

An object with such a large specific heat capacity that any transfer of heat will not change its temperature

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11
Q

What does the amount of heat flow depend on?

A

Mass
Specific heat capacity
Temperature difference

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12
Q

Bose-Einstein Condensate

A

When the de Broglie wavelength of atoms becomes bigger than the atomic spacing
Occurs when a solid is cooled to a very low temperature

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13
Q

Cooling to Lower than the Surroundings

Magnetic Cooling

A
  • atoms with magnetic dipoles can be aligned with a magnetic field
  • if the magnetic field is slowly decreased then the dipoles can overcome the field and become randomly orientated by taking thermal energy from their motion
  • this leads to sample cooling as the average translational kinetic energy per molecule is decreasing
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14
Q

Cooling to Lower than the Surroundings

Laser Cooling

A
  • a laser photon of momentum p = hf is fired at the sample
  • the frequency of each photon is slightly less than the frequency corresponding to the transition energy of the atoms
  • this means that it can only be absorbed by atoms travelling towards it by the Doppler shift effect
  • this collision reduces the velocity of the atom
  • average kinetic energy and therefore temperature are reduced
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15
Q

Cooling to Lower than the Surroundings

Evaporative Cooling

A
  • atoms are held in a magnetic trap
  • only atoms with the highest velocity are able to escape
  • as these high energy atoms leave the average kinetic energy of the atoms in the magnetic trap decreases
  • the magnetic field is decreased so that atoms can continue to escape
  • this continues until there are far fewer but much colder atoms remaining
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16
Q

What kinetic energy do atoms have at absolute zero?

A

Zero translational kinetic energy

17
Q

What is the lowest temperature ever achieved?

18
Q

Cooling to Absolute Zero

A
  • removing all possible energy would require an infinite amount of time
  • it would contradict the Heisenberg Uncertainty Principle which doesn’t allow no motion as then it would be possible to specify both position and momentum precisely
  • zero-point energy remains
19
Q

Thermal Expansion

Linear Expansion

A

ΔL = LαΔT

L = initial length 
α = coefficient of linear expansion
20
Q

Coefficient of Linear Expansion

A

α = (ΔT->0)lim 1/L * dL/dT

21
Q

Thermal Expansion

Volume Expansion

A

ΔV = VβΔT

V = initial volume
β = coefficient of volume expansion
22
Q

What is the relationship between the coefficient of linear expansion and the coefficient of volume expansion?

23
Q

At what temperature does water have maximum density?

24
Q

Thermal Current

A

I = ΔQ/Δt = kA * ΔT/Δx

25
Thermal Conduction | V=IR
ΔT = IR = I*Δx/kA
26
Thermal Resistance
R = ΔX/kA
27
Thermal Resistors | Series
Rt = R1 + R2 + R3 + ... E.g. double glazing
28
Thermal Resistors | Parallel
1/Rt = 1/R1 + 1/R2 + 1/R3 + ...
29
What is convection?
The transfer of thermal energy by direct mass transport
30
What is radiation?
The transfer of thermal energy in the form of electromagnetic radiation No medium is necessary
31
Stefan-Boltzmann Law
Pnet = eσA (T⁴ - T0⁴)
32
Wien's Displacement Law
λmax = 2.898mmK / T