Physics NOV

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26 Terms

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The 7 base SI units and their corresponding base quantities

  • Mass: kilogram (kg\text{kg})
  • Length: metre (m\text{m})
  • Time: second (s\text{s})
  • Electric current: ampere (A\text{A})
  • Temperature: kelvin (K\text{K})
  • Amount of substance: mole (mol\text{mol})
  • Luminous intensity: candela (cd\text{cd})
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Derived units and dimensional consistency in physics

  • Derived unit: A unit created by multiplying or dividing base units (e.g., 1 N=1 kg m s−21\,\text{N} = 1\,\text{kg}\,\text{m}\,\text{s}^{-2}).
  • Dimensional consistency: An equation is dimensionally consistent if both sides reduce to the exact same combination of base SI units.
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Metric unit prefixes from pico to tera

  • pico (p\text{p}): 10−1210^{-12}
  • nano (n\text{n}): 10−910^{-9}
  • micro (μ\mu): 10−610^{-6}
  • milli (m\text{m}): 10−310^{-3}
  • kilo (k\text{k}): 10310^3
  • mega (M\text{M}): 10610^6
  • giga (G\text{G}): 10910^9
  • tera (T\text{T}): 101210^{12}
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Differences between scalar and vector quantities

  • Scalar: Has magnitude only. Examples include mass, distance, speed, and energy.
  • Vector: Has both magnitude and direction. Examples include displacement, velocity, acceleration, force, and momentum.
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Techniques for adding, subtracting, and resolving vectors

  • Addition and subtraction: Combine using tip-to-tail vector diagrams or using trigonometry and the Pythagorean theorem.
  • Vector resolution: For a vector VV at an angle θ\theta to the horizontal:
    • Horizontal component: Vx=Vcos⁡(θ)V_x = V \cos(\theta)
    • Vertical component: Vy=Vsin⁡(θ)V_y = V \sin(\theta)
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Key kinematic definitions: displacement, speed, velocity, and acceleration

  • Displacement (ss): Straight-line distance in a specified direction (m\text{m}).
  • Speed: Rate of change of distance (m s−1\text{m}\,\text{s}^{-1}).
  • Velocity (vv): Rate of change of displacement (m s−1\text{m}\,\text{s}^{-1}).
  • Acceleration (aa): Rate of change of velocity (m s−2\text{m}\,\text{s}^{-2}).
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Interpretation of gradients and areas on motion graphs

  • Displacement-time graph: Gradient = velocity.
  • Velocity-time graph: Gradient = acceleration; area under graph = displacement (ss).
  • Acceleration-time graph: Area under graph = change in velocity (Δv\Delta v).
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The 4 SUVAT equations for uniform acceleration

  • v=u+atv = u + at
  • s=12(u+v)ts = \frac{1}{2}(u + v)t
  • s=ut+12at2s = ut + \frac{1}{2}at^2
  • v2=u2+2asv^2 = u^2 + 2as
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Principles and modeling of projectile motion under gravity

  • Perpendicular motions are completely independent.
  • Horizontal motion: Constant velocity with zero acceleration (ax=0a_x = 0), governed by sx=vxts_x = v_x t.
  • Vertical motion: Uniform acceleration downwards due to gravity (ay=−g=−9.81 m s−2a_y = -g = -9.81\,\text{m}\,\text{s}^{-2}).
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Laboratory measurement of velocity and acceleration using light gates

  • Velocity: A card of known length dd interrupts a light gate for time tt, giving instantaneous velocity v=dtv = \frac{d}{t}.
  • Acceleration: A double interrupt card or two spaced light gates record initial velocity uu, final velocity vv, and time interval tt to calculate acceleration using a=v−uta = \frac{v - u}{t} or v2=u2+2asv^2 = u^2 + 2as.
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Newton's Three Laws of Motion

  • First Law: An object remains at rest or at constant velocity unless acted upon by a net external force.
  • Second Law: The net force is proportional to the rate of change of momentum: F=ΔpΔt=maF = \frac{\Delta p}{\Delta t} = ma.
  • Third Law: If body A exerts a force on body B, body B exerts an equal and opposite force of the same type on body A.
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Distinctions between mass, weight, and center of gravity

  • Mass (mm): The amount of matter in an object (kg\text{kg}, scalar, invariant).
  • Weight (WW): Gravitational pull on a body (W=mgW = mg, N\text{N}, vector, varies with gg).
  • Center of Gravity: The single point through which the entire weight of an object is considered to act.
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Free-body diagrams and the properties of friction

  • Free-body diagram: A vector diagram showing all external forces acting exclusively on a single isolated object.
  • Friction: A contact force that always acts parallel to the interface and opposes the relative motion or intended motion between surfaces.
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Definitions and relationships of linear momentum and impulse

  • Linear Momentum (pp): The product of mass and velocity: p=mvp = mv (kg m s−1\text{kg}\,\text{m}\,\text{s}^{-1} or N s\text{N}\,\text{s}).
  • Impulse: Change in momentum given by Δp=FΔt=mv−mu\Delta p = F \Delta t = mv - mu, which equals the area under a force-time graph.
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Principle of Conservation of Linear Momentum in 1D and 2D

  • For a closed system with no external resultant forces, total linear momentum is conserved before and after an interaction.
  • In two dimensions, momentum is conserved independently in perpendicular directions:
    • ∑px,initial=∑px,final\sum p_{x,\text{initial}} = \sum p_{x,\text{final}}
    • ∑py,initial=∑py,final\sum p_{y,\text{initial}} = \sum p_{y,\text{final}}
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Differences between elastic and inelastic collisions

  • Elastic collision: Both total momentum and total kinetic energy are conserved.
  • Inelastic collision: Momentum is conserved, but kinetic energy is not conserved (energy is transformed into thermal energy, sound, or deformation).
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Methods for calculating work done by constant and variable forces

  • Constant force at an angle θ\theta to motion: W=Fxcos⁡(θ)W = F x \cos(\theta)
  • Variable force: Work done equals the area under a force-displacement (FF-xx) graph.
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The Principle of Conservation of Energy

  • Energy cannot be created or destroyed, only transferred from one store to another.
  • The total energy of an isolated system remains constant over time.
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Kinetic and potential energy formulas and the derivation of kinetic energy

  • Formulas: Ek=12mv2E_k = \frac{1}{2}mv^2 and ΔEp=mgh\Delta E_p = mgh
  • Derivation:
    • Work done is W=FsW = Fs.
    • By Newton's second law, F=maF = ma, giving W=masW = mas.
    • From kinematics with u=0u = 0, v2=2as  ⟹  as=12v2v^2 = 2as \implies as = \frac{1}{2}v^2.
    • Substituting yields W=m(12v2)=12mv2W = m\left(\frac{1}{2}v^2\right) = \frac{1}{2}mv^2.
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Definition and fundamental formulas for power

  • Definition: Power is the rate of energy transfer or work done (1 W=1 J s−11\,\text{W} = 1\,\text{J}\,\text{s}^{-1}).
  • General: P=Wt=ΔEtP = \frac{W}{t} = \frac{\Delta E}{t}
  • Electrical: P=IVP = IV
  • Mechanical: P=FvP = Fv (for a force acting at constant speed vv)
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Definition and formula for efficiency

  • Efficiency η=Useful Energy (or Power) OutputTotal Energy (or Power) Input×100%\text{Efficiency } \eta = \frac{\text{Useful Energy (or Power) Output}}{\text{Total Energy (or Power) Input}} \times 100\%
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Tensile vs. compressive forces, Hooke's Law, and force-extension graphs

  • Tensile forces stretch an object, whereas compressive forces squish or shorten it.
  • Hooke's Law: Extension xx is directly proportional to applied force FF up to the limit of proportionality: F=kxF = kx.
  • Force-extension graph: Displays a straight line through the origin up to the limit of proportionality, where gradient equals stiffness kk.
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Key mechanical limits and transition points on a stress-strain curve

  • Elastic limit: The maximum stress beyond which a material deforms plastically and will not return to its original length.
  • Yield point: The point at which a small stress increase causes a large, permanent plastic strain.
  • Ultimate Tensile Strength (UTS): The maximum stress a material can withstand before necking begins.
  • Breaking point: The stress at which the material fractures.
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Stress, strain, and Young modulus definitions and experimental measurement

  • Tensile stress: σ=FA\sigma = \frac{F}{A} (Pa\text{Pa} or N m−2\text{N}\,\text{m}^{-2})
  • Tensile strain: ε=Δll0\varepsilon = \frac{\Delta l}{l_0} (dimensionless)
  • Young modulus: E=σε=Fl0AΔlE = \frac{\sigma}{\varepsilon} = \frac{F l_0}{A \Delta l} (gradient of linear region of stress-strain graph)
  • Measurement: Hang loads F=mgF = mg on a long wire of original length l0l_0 measured with a tape measure; record diameter dd with a micrometer (A=πd24A = \frac{\pi d^2}{4}); determine extension Δl\Delta l using a vernier scale; plot σ\sigma against ε\varepsilon.
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Elastic strain energy calculation from a force-extension graph

  • Elastic strain energy equals the area under the force-extension curve:
  • Strain Energy=12Fx=12kx2\text{Strain Energy} = \frac{1}{2} F x = \frac{1}{2} k x^2
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Distinction between elastic and plastic deformation

  • Elastic deformation: The material returns to its original dimensions when the deforming load is removed; stored strain energy is fully recoverable.
  • Plastic deformation: The material experiences permanent set and does not return to its original shape; work done is dissipated primarily as thermal energy.