Temperature and Heat Flow: Heat transfers from hot to cold objects when they are in thermal contact, determined by their temperature difference.
Equilibrium: Objects reach thermal equilibrium when they have the same temperature.
Heat Definition: Heat is not a substance, but the transfer of thermal energy, often measured in calories or joules.
Temperature Scales: Common scales include Celsius (°C) and Kelvin (K). The relationship is T(K) = t(°C) + 273.
Pressure (P): Force exerted per unit area. SI units: Nm⁻² or Pascals (Pa).
Volume (V): Measured in m³ or cm³.
Temperature (t): Measured in °C or K.
Density (p): Calculated as p = m/V, where m is mass in kg and V is volume in m³.
Macroscopic: Looks at the system as a whole and how it interacts with its surroundings.
Microscopic: Examines interactions at the atomic and molecular levels.
An object gains or loses energy as its temperature changes, which can be in kinetic or potential forms.
Total internal energy (U) is the sum of kinetic and potential energy at the molecular level.
States of Matter:
Solids: Fixed volume and shape with particles vibrating in place.
Liquids: Fixed volume but changing shape, particles can move around each other.
Gases: No fixed volume or shape, particles move independently and collide.
Thermal Capacity (C): Energy required to raise temperature by 1 K; Specific Heat Capacity (c) is energy required to raise 1 kg of a substance by 1 K.
Methods for measuring include:
Electrical method (involving heat input & temperature changes).
Method of mixtures (using known heat capacities and temperature changes).
When a substance changes phase (e.g., melting, boiling), temperature remains constant, but thermal energy is absorbed or released.
Specific Latent Heat (L): Energy absorbed/released per unit mass during phase changes.
Methods involve calorimetry and calculations using energy balances during phase transitions.
Definition: Heat transfer through matter without any bulk movement.
Mechanism: Kinetic energy transfer through particle collisions.
Materials: Good conductors (metals) vs. insulators (wood, air).
Definition: Transfer of heat through liquid or gas movement due to density differences.
Example: Warm air rising and cool air sinking creates currents.
Definition: Transfer of energy through electromagnetic waves, doesn't require a medium.
Examples: Sun warming Earth, heat from a fire.
Most substances can be modeled with thermal concepts including specific heat, latent heat, and phase changes affecting interactions at the atomic level.
Inverse Square Law: Intensity of radiation drops with the square of the distance from the source, applies to all waves.
Newton’s Law of Gravitation: Describes how every mass attracts every other mass, F = G(m₁m₂)/r².
Defined as the force per unit mass (N/kg), varies by distance from mass.
Kepler’s Laws: Governs orbital motion, including relationships between the orbital period and radius.
Strong nuclear forces work at very short ranges to keep nucleons together. Weak forces engage with beta decay processes.
Isotopes stabilize differently; binding energy plays a crucial role in decay processes.
Charges produce electric fields; Coulomb's law defines their interactions.
Defined as force on a unit charge (N/C or V/m), represented with field lines indicating direction and intensity.
Defines energy per charge related to the electric field and is integral in determining work done in moving charges between points in the field.
Light and matter exhibit both particle-like and wave-like properties captured in phenomena such as the photoelectric effect and Compton scattering.
De Broglie's hypothesis equates the motion of particles with wave characteristics, influencing calculations for momentum and wavelength.
Radioactive decay emits alpha, beta, or gamma radiation, each possessing unique ionizing properties affecting biological structures.
Chain reactions are crucial in nuclear fission processes, often regulated to prevent uncontrolled reactions.
Applications in medical diagnostics, treatments, sterilization processes, and illumination of processes such as carbon dating.
Half-life calculations allow the determination of remaining quantities of radioactive materials, critical in understanding the longevity of isotopes.