Presenter: Izza Nadia binti Mohd Maulana
Course Code: RXD12402
Overview of the course content aimed at supporting radiographers' understanding of fundamental physics concepts.
Introduction to Physics
Work, Energy, and Power
Properties of Electrical Charges
Law of Conservation of Energy
Heat and Temperature
Heat Transfer
Heat Energy in X-ray Tube
At the end of the topics, students should:
Describe work, energy (potential and kinetic energy), and power.
Understand the law of conservation of energy.
Explain electrical charges and Coulomb’s Law.
Describe heat and temperature.
Explain the processes of heat transfer: conduction, convection, and radiation.
Definition: Physics involves the study of interactions between energy, matter, space, and time.
Goal: To provide explanations for various phenomena, from subatomic particles to large-scale movements (e.g., cars, rockets).
Structural stability
Lighting
Acoustics
Electricity
Heating
Cooling
Radioactive dating of rocks
Earthquake analysis
Air quality assessment
Defined through measurement methods or calculations.
Example: Distance and time are measured; speed is derived from these measurements.
Importance of Standardized Units: Essential for meaningful comparisons of measurements.
Base Quantity: Not derived from other quantities (e.g., mass, length, time).
Derived Quantity: Resulting from combinations of base quantities (e.g., speed).
Metric systems simplify unit conversion using powers of 10.
Convert between units easily using metric prefixes (e.g., kilo, mega, nano).
Displacement: Change in position has both direction and magnitude.
Distance: The total length of the path traveled, a scalar quantity.
Example calculations provided for better understanding.
Work (W): Product of force and distance in the direction of the force; expressed as:
( W = F imes d imes \cos(θ) )
Energy Types:
Potential Energy (PE): Energy stored due to position, calculated as ( PE = mgh ).
Kinetic Energy (KE): Energy of motion, calculated as ( KE = \frac{1}{2} mv^2 ).
Explanation of conservation of energy through examples and equations.
The total energy in a closed system remains constant.
Example: Kinetic energy + Potential energy at various positions.
Work-Energy Theorem connection to non-conservative forces.
Definition: Rate at which work is done or energy is transferred.
Calculated as:
( Power = \frac{Work}{Time} )
Unit of Power: Watt (1 W = 1 J/s).
Fundamental property of subatomic particles, associated with forces in electric and magnetic fields.
Types: Positive (e.g., protons) and negative (e.g., electrons).
Unit: Coulomb (C).
Additivity: Charges combine to form net charge.
Conservation: Total charge is conserved in isolated systems.
Quantization: Electric charge exists in discrete units, defined as the elementary charge.
Explains the electrostatic force between charges.
Formula:
( F = k \frac{q_1 \cdot q_2}{r^2} )
Describes relationship among charge magnitudes and distance.
Heat: Form of energy flowing from hotter to cooler areas, measured in Joules.
Temperature: Degree of hotness/coldness, measured in Kelvin (K) or Celsius (°C).
Differences in the definitions and properties of heat and temperature explained.
Defined as the heat required to raise 1 kg of a substance by 1 °C.
Equation: ( Q = mcΔT ) for heat absorbed or lost.
Specific heat capacities of various substances provided for reference.
Exchange of thermal energy occurs from hot to cold areas.
Methods of Transfer:
Conduction: Heat transfer through materials (e.g., iron to clothes).
Convection: Movement of fluids to transfer heat (e.g., boiling water).
Radiation: Heat transfer via electromagnetic waves (e.g., heat from the sun).
X-ray production involves conversion of kinetic energy of electrons into thermal energy.
Most kinetic energy becomes heat; less than 1% is converted to x-rays.
Cooling methods utilize radiation, conduction, and convection.
Heat unit calculation: ( HU = kVp \times mA \times time(s) ).