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The AQA A-level Physics Data and Formulae booklet

 The AQA A-level Physics Data and Formulae booklet

AQA  A-Level Physics Data Sheet


Here is an enhanced version of the AQA  A-Level Physics Data Sheet with context provided for each section and formula to help students understand where and how they are applied.

AQA A-Level Physics Data Sheet 

Fundamental Constants

These constants are universal values used across various topics in physics.

  • Speed of light (cc): 3.00×108m/s3.00 \times 10^8 \, \text{m/s}
    Used in wave equations, especially in electromagnetic wave problems.
  • Gravitational constant (GG): 6.67×1011N m2/kg26.67 \times 10^{-11} \, \text{N m}^2/\text{kg}^2
    Crucial for gravitational force and field strength calculations.
  • Planck constant (hh): 6.63×1034J s6.63 \times 10^{-34} \, \text{J s}
    Used in quantum physics to relate energy and frequency of photons.
  • Elementary charge (ee): 1.60×1019C1.60 \times 10^{-19} \, \text{C}
    Represents the charge of a single proton or electron, often used in particle physics.
  • Mass of proton (mpm_p): 1.67×1027kg
  • Mass of neutron (mnm_n): 1.67×1027kg1.67 \times 10^{-27} \, \text{kg}
  • Mass of electron (mem_e): 9.11×1031kg9.11 \times 10^{-31} \, \text{kg}
    These masses are used in atomic physics and calculations involving particles.
  • Avogadro constant (NAN_A): 6.02×1023mol16.02 \times 10^{23} \, \text{mol}^{-1}
    Links the microscopic world (atoms, molecules) to macroscopic quantities.
  • Boltzmann constant (kk): 1.38×1023J/K1.38 \times 10^{-23} \, \text{J/K}
    Relates temperature to the kinetic energy of particles in thermal physics.

Mechanics

Mechanics is the study of motion and forces acting on objects.

  • Equations of motion: Used for objects moving with constant acceleration.
    • v=u+atv = u + at: Final velocity.
    • s=ut+12at2s = ut + \frac{1}{2}at^2: Displacement over time.
    • v2=u2+2asv^2 = u^2 + 2as: Relation between velocity, acceleration, and displacement.
  • Kinetic energy (EkE_k): 12mv2\frac{1}{2}mv^2
    Energy of a moving object.
  • Potential energy (EpE_p): mghmgh
    Energy stored in an object due to height in a gravitational field.
  • Force (FF): mama
    Newton's second law, used to relate mass, acceleration, and force.
  • Work done (WW): FdcosθFd \cos\theta
    Work is the transfer of energy when a force is applied over a distance.
  • Power (PP): Wt=Fv\frac{W}{t} = Fv
    Rate of doing work or energy transfer.

Waves

Waves describe the transfer of energy without the transfer of matter.

  • Wave equation: v=fλv = f\lambda
    Relates wave speed, frequency, and wavelength.
  • Intensity: I=P4πr2I = \frac{P}{4\pi r^2}
    Describes energy transfer per unit area, often used in light or sound.
  • Refractive index (nn): n=sinisinr=cvn = \frac{\sin i}{\sin r} = \frac{c}{v}
    Used in refraction problems to compare wave speeds in different media.

Electricity

Electricity involves the study of charges, currents, and their effects.

  • Ohm’s law: V=IRV = IR
    Relationship between voltage, current, and resistance in a circuit.
  • Resistance (RR): R=ρLAR = \rho \frac{L}{A}
    Resistance depends on material properties and geometry.
  • Power (PP): P=VI=I2R=V2RP = VI = I^2R = \frac{V^2}{R}
    Describes energy transfer in electrical systems.
  • Capacitance (CC): C=QVC = \frac{Q}{V}
    Measures a capacitor's ability to store charge per unit voltage.

Thermal Physics

Thermal physics explores energy transfer and particle behavior.

  • Ideal gas law: pV=nRTpV = nRT
    Relates pressure, volume, and temperature for an ideal gas.
  • Mean kinetic energy: Ek=32kTE_k = \frac{3}{2}kT
    Average energy of gas particles due to their motion.

Fields

Fields describe the influence of forces over a distance.

  • Gravitational force (FF): F=Gm1m2r2F = \frac{Gm_1m_2}{r^2}
    Force between two masses due to gravity.
  • Electric force (FF): F=kq1q2r2F = \frac{kq_1q_2}{r^2}
    Coulomb’s law for forces between charges.
  • Magnetic force: F=BqvsinθF = Bqv \sin\theta
    Force on a moving charge in a magnetic field.

Atomic and Nuclear Physics

This area studies atoms, nuclei, and their interactions.

  • Energy of a photon: E=hf=hcλE = hf = \frac{hc}{\lambda}
    Relates a photon's energy to its frequency or wavelength.
  • Nuclear decay: N=N0eλtN = N_0 e^{-\lambda t}
    Describes the number of undecayed nuclei over time.
  • Half-life: T1/2=ln2λT_{1/2} = \frac{\ln 2}{\lambda}
    Time for half the nuclei in a sample to decay.
  • Mass-energy equivalence: E=mc2E = mc^2
    Fundamental relationship between mass and energy.

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