Thermal Flashcards

1
Q

Phases of matter

A
  • Solid
    • Particles in solids are closely packed in a fixed lattice structure and held by strong intermolecular forces.
    • Particles can only vibrate about fixed positions and have low energy compared to liquids and gases.
    • Solids have high density and are incompressible.
  • Liquid
    • Particles in liquids are closely packed, randomly arranged, and held by weaker intermolecular forces than solids.
    • Particles can flow past each other and have higher energy than solids but lower than gases.
    • Liquids have a fixed volume, take the shape of their container, and are difficult to compress.
  • Gas
    • Particles in gases have negligible intermolecular forces, are randomly arranged, and are far apart compared to solids and liquids.
    • Particles move freely in all directions at various speeds and have higher energy than those in solids and liquids.
    • Gases take the shape of their container, have no fixed volume, are compressible, and have the lowest densities.
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2
Q

Brownian motion

A
  • Brownian motion is the random movement of small particles suspended in a liquid or gas, caused by collisions with faster-moving atoms or molecules.
  • This phenomenon supports the idea of molecular motion and explains the concept of pressure in gases.
  • Smaller molecules affect larger particles due to their high speeds and momentum transfer during collisions.
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3
Q

Energy during change of phase

A
  • During phase changes, energy increases or decreases electrostatic potential energy instead of kinetic energy, so temperature remains constant.
  • In melting or boiling, energy breaks intermolecular bonds, increasing electrostatic potential energy and moving molecules further apart.
  • In freezing or condensation, energy forms bonds, decreasing electrostatic potential energy and moving molecules closer together.
  • Kinetic energy stays constant, indicating no temperature change during a phase transition.
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4
Q

Specific heat capacity

A
  • Amount of energy needed to raise the temperature of unit mass (1 kg) of a substance by 1 K (unit temp)
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5
Q

Internal energy

A
  • The sum of the randomly distributed kinetic and potential energies of atoms or molecules within a substance
  • ΔU ∝ ΔT
  • Stronger intermolecular forces mean higher potential energy
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6
Q

Thermal equilibrium

A
  • Heat flows (thermal energy) from a hotter object to a colder one until both objects reach the same temperature, known as thermal equilibrium.
  • Thermal equilibrium occurs when two substances in contact no longer exchange heat energy and both reach the same temperature.
  • The final temperature in thermal equilibrium depends on the initial temperature difference between the two objects. An example is ice cubes melting in room temperature water.
  • Energy lost by hotter object = Energy gained by colder object
  • (Ice)
    Energy gained = ml + mc (T-T1)
    Equal to
  • Hot drink
    Energy lost = mc (T2-T)
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7
Q

Specific Latent Heat

A
  • Specific Latent Heat of Fusion:
    • Energy required to convert 1 kg of solid (unit mass) to liquid with no temperature change.
  • Specific Latent Heat of Vaporisation:
    • Energy required to convert 1 kg of liquid to gas with no temperature change.
  • Evaporating 1 kg of water requires seven times more energy than melting 1 kg of ice.
  • Ice melting increases molecular separation, while boiling water fully separates molecules, breaking all intermolecular forces.
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8
Q

Triple-Point

A
  • The specific temperature and pressure where a substance exists as a solid, liquid, and gas simultaneously.
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9
Q

Gas Laws

A

-Boyle’s Law
- p ∝ V-1 (at constant temperature)
- If the temperature increases, the graph is further from the origin and vice versa
- area under graph is energy
-Pressure Law
- p ∝ T
-Charle’s Law
- V ∝ T

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10
Q

Avogadro Constant

A
  • Mole: The SI base unit for the amount of substance, defined as the amount containing as many particles (e.g., atoms or molecules) as there are in 12 g of carbon-12.
  • Avogadro’s Constant (Na): The number of atoms in 12 g of carbon-12.
  • Equation:
    Number of particles (N)= n * Na

    Where:
    • n: Number of moles
    • Na: Avogadro’s constant
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11
Q

Molar mass

A
  • Molar Mass: The mass of one mole of a substance, measured in grams per mole (g mol⁻¹).
  • Equation:
    n = m * M⁻¹
    Where:
    • n: Number of moles
    • m: Mass of the substance (g)
    • M: Molar mass (g mol⁻¹)
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12
Q

molar gas constant

A
  • pVT-1= constant depends on the amount of gas used, which can be measured in moles (n)
  • This constant is known as the molar gas constant (R).
  • constant=nR
  • relates the energy to temperature in thermal physics, when a mole of particles at the state temperature is considered
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13
Q

Boltzmann’s constant

A
  • Boltzmann constant (kB) links the average kinetic energy of particles in a gas to its temperature.
    • kB = R / Nₐ
  • Derivation of nR = NkB:
    • kB = R / Nₐ
    • R / (N/n) = kB
    • nR/N = kB
    • nR= NkB
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14
Q

Kinetic theory of an ideal gas assumptions

A
  • R | RANDOM:
    Large number of Gas particles move randomly and in straight lines until they collide with each other or the container walls.
  • A | ATTRACTION:
    No intermolecular forces between particles except during collisions.
  • V | VOLUME:
    Negligible volume of particles compared to the volume of the gas.
  • E | ELASTIC:
    Elastic collisions: collisions between particles and with container walls are perfectly elastic.
  • D | DURATION:
    Negligible time spent on each collision compared to time between collisions.
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15
Q

Pressure in terms of the kinetic theory of gases and Newtonian thoery

A
  • Gas particles move randomly with constant velocities and no intermolecular forces, following Newton’s 1st law (objects in motion stay in motion unless acted upon).
  • When particles collide with the walls of the container, they exert a force on the wall, and the wall exerts an equal and opposite force on the particle (Newton’s 3rd law).
  • The force on the wall is calculated using Newton’s 2nd law (force = rate of change of momentum). The momentum change during a collision (from mu to -mu) results in a force proportional to the particle’s mass and velocity.
  • Although each particle exerts a tiny force, with billions of particles in the container, the combined force is much larger, leading to a steady, uniform pressure on the walls.
  • Pressure is the result of many collisions between particles and the container walls, leading to the equation for pressure in an ideal gas.
  • (Rate of momentum ÷ area) * number of particles
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16
Q

Root Mean Square

A
  • Gas particles move in random directions, resulting in a net velocity of zero; squaring the velocities ensures all values are positive, avoiding cancellation.
  • The root-mean-square speed (rms), calculated as crms =√mean2, provides the average speed of particles by taking the square root of the mean square speed.
17
Q

Maxwell-Boltzmann distribution

A
  • The Maxwell-Boltzmann distribution shows the range of kinetic energies of gas particles, with most particles moving at moderate speeds, fewer at very high or low speeds.
  • The curve starts at (0, 0) because no molecules have zero energy, and it peaks at the most-probable energy/speed.
  • Kinetic energy is proportional to the square of speed, so the distribution can also represent particle speeds.
  • As temperature increases, the average speed, most-probable speed, and maximum speed all increase, and the curve becomes broader and flatter.
  • Collisions between particles redistribute momentum and energy, creating a skewed bell-shaped curve while maintaining the gas’s total energy.
18
Q

Kinetic energy of a molecule

A
  • Kinetic theory of gases connects the microscopic properties of gas particles, such as mass and speed, to their macroscopic properties like pressure and volume.
  • 1/3N mc2 = N kbT
    m is mass of 1 molecule
    pressure=1/3(density)c2 as Nm/V = density
  • which can rearrange to give energy
19
Q

Internal energy of an ideal gas

A
  • Internal energy of an ideal gas is entirely due to the kinetic energy of its particles.
  • Electrostatic forces between particles in an ideal gas are negligible except during collisions, meaning there is no electrostatic potential energy.
  • When the container is heated, gas molecules move faster, resulting in higher kinetic energy and increased internal energy.
  • Change in internal energy ∆U is equal to the total kinetic energy Ek of all the particles.
20
Q

Kinetic theory equation derivation

A
  • F = -2mv / t
  • t = distance (2L) ÷ velocity
  • p = F / Volume