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.
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.
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.
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)
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
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)
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.
8
Q
Triple-Point
A
- The specific temperature and pressure where a substance exists as a solid, liquid, and gas simultaneously.
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
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
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)
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
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
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.
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