Thermodynamics Flashcards

(16 cards)

1
Q

Absolute zero

A

When the particles of a substance have zero kinetic energy, 0 Kelvin

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2
Q

Avogadro’s constant

A

The constant number of particles per mole of a substance

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3
Q

Black body radiation

A

A perfect emitter and absorber of all possible wavelengths of radiation

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4
Q

Boltzmann’s constant

A

A constant relating the average kinetic energy of the particle in a gas to the gas’ temperature

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5
Q

Boyle’s Law

A

As volume decreases, the pressure on a gas at a constant temperature increases

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6
Q

Charles’ Law

A

As temperature increases, the volume of a gas at a constant pressure increases

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7
Q

Ideal gas

A

A hypothetical gas that has molecules with no interactions and occupy negligible space so it obeys the ideal gas law

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8
Q

Ideal gas law

A

A combination of Boyle’s law, Charles’ law and the Pressure law that describes the relationship between pressure, volume and temperature of an ideal gas

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9
Q

Internal energy

A

The sum of all the randomly distributed potential and kinetic energy of the particles that make up a substance

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10
Q

Luminosity

A

Total power radiated by a light emitting source

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11
Q

Pressure Law

A

As temperature increases, the pressure of a gas at a constant volume increases

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12
Q

Specific heat capacity

A

The energy required to raise the temperature of 1kg of a substance by 1 Kelvin without changing its state

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13
Q

Specific latent heat

A

The energy required to change the state of 1kg of a substance without a change in temperature

Specific latent heat of fusion for solid to liquid and specific latent heat of vaporisation for liquid to gas

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14
Q

State changes

A

During a state change, a substance will not change kinetic energy and temperature will be constant but potential energy will change, bonds will be broken or formed

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15
Q

Stefan-Boltzmann Law

A

Luminosity of a black body radiation is directly proportional to its surface area and its absolute temperature to the fourth power

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16
Q

Wein’s Law

A

Peak wavelength of emitted radiation is inversely proportional to the absolute temperature of the black body