Physics 1-T Final Exam Comprehensive Notes

Vector and Scalar Quantities

  • Vector ≡ quantity with both magnitude and direction

    • Canonical examples: displacement d\vec d, velocity v\vec v, acceleration a\vec a, force F\vec F, momentum p\vec p, impulse J\vec J, electric field E\vec E, magnetic field B\vec B.
    • Significance: vectors must obey head-to-tail (graphical) or component (analytical) addition. Direction determines physical effect (e.g.
    • Opposite forces cancel.
    • Parallel vectors may be added/subtracted algebraically.)
  • Scalar ≡ quantity with magnitude only

    • Common examples: distance dd, speed vspeedv_{\text{speed}}, mass mm, energy EE, work WW, power PP, temperature TT, electric potential VV, charge magnitude q|q|, time tt.
  • Practical tip: when vectors are parallel / antiparallel (share line of action) you may simply add or subtract their magnitudes with sign. At any other relative angle, draw a diagram and use components or the Law of Cosines.

Measurement, Significant Figures, & Units

  • Magnitude → the size/amount of a physical quantity (always positive).
  • Significant–figure (sig-fig) count examples:
    • 97  m97\;\text{m} → 2 sig figs.
    • 97.0  m97.0\;\text{m} → 3.
    • 0.97  m0.97\;\text{m} → 2.
    • 0.0097  m0.0097\;\text{m} → 2 (leading zeros are placeholders).
    • 970  m970\;\text{m} → 2 (trailing zero not significant without a decimal point).
  • If unsure of units, dimensional analysis (treat units like algebra) will restore correct dimensions.
  • Slope of a graph = ΔyΔx\dfrac{\Delta y}{\Delta x} ⇒ always interpret by reading the axis labels and units.

Vector & Free-Body Diagrams (FBD)

  • Vector diagram: sketch of all vectors (displacements, velocities, etc.) tip-to-tail; resultant drawn from start to finish.
  • Free-body diagram: isolate one object; draw and label every real force acting now (gravitational W\vec W, normal N\vec N, friction f\vec f, tension T\vec T, applied Fapp\vec F_{\text{app}}, electric qEq\vec E, magnetic qv×Bq\vec v\times\vec B, etc.). Usually begin with weight W\vec W because it is almost always present and points toward Earth.
    • Velocities and accelerations are placed off to the side—they are not forces.
  • Normal = “perpendicular” to a surface. Friction acts parallel to the surface, opposite the direction of (impending) motion.

Fundamental Conservation Laws

  • A quantity is “conserved” when its total remains constant in an isolated system.
    • Throughout Physics 1-T we used conservation of momentum p=const\sum\vec p = \text{const} and energy E=const\sum E = \text{const}.

Kinematics & Dynamics Essentials

  • Average speed v<em>avg=d</em>totalttotalv<em>{\text{avg}} = \dfrac{d</em>{\text{total}}}{t_{\text{total}}}.
  • “Rates” hierarchy (all take a time derivative):
    1. Speed: v=dddtv = \dfrac{\mathrm d d}{\mathrm d t}.
    2. Acceleration: a=dvdta = \dfrac{\mathrm d v}{\mathrm d t} (rate of velocity change).
    3. Power: P=dEdtP = \dfrac{\mathrm d E}{\mathrm d t}.
    4. Current: I=dQdtI = \dfrac{\mathrm d Q}{\mathrm d t}.
    5. Net force: Fnet=dpdt\vec F_{\text{net}} = \dfrac{\mathrm d \vec p}{\mathrm d t} (Newton’s Second Law in its most general, momentum form).
  • Weight = gravitational force: W=mg\vec W = m\vec g.
  • Newton’s 3rd Law: forces between two interacting bodies are equal in magnitude, opposite in direction.

Mass & Force Comparisons

  • Same force on masses MM and 4M4M ⇒ accelerations are inversely proportional to mass; a<em>M=4a</em>4Ma<em>{M} = 4 a</em>{4M}.
  • Same force on equal-mass charges +QQ and –4Q4Q: acceleration magnitudes are equal (direction may differ if fields differ).

Friction & Applied-Force Scenarios (55 kg block)

  1. No friction: push with 245N245\,\text N → block accelerates a=Fm=24555.04.45m/s2a = \dfrac{F}{m} = \dfrac{245}{55.0} \approx 4.45\,\text{m/s}^2.
  2. Encounter rough patch: friction 225N225\,\text N opposite motion.
    • Continue to push 245 N ⇒ net F=245225=20NF = 245-225 = 20\,\text N ⇒ smaller acceleration.
    • Push 225 N ⇒ net F=0F = 0 ⇒ constant velocity.
    • Push 175 N ⇒ net F=(225175)=50NF = -(225-175) = -50\,\text N ⇒ deceleration.
    • Let go ⇒ only friction acts; object slows over time, not instantaneously.

Spring–Piston Two-Mass System (M & 1.5 M)

  • Work done compressing spring: W=25JW=25\,\text J ⇒ potential energy stored Us=25JU_s=25\,\text J.
  • When lock is released on frictionless surface:
    • Internal spring force equal & opposite on each mass (Newton III).
    • Smaller mass MM gains larger acceleration.
    • Final speeds differ (inverse mass ratio); directions opposite.
  • Conserved: total mechanical energy (25 J) & total momentum of the system.
  • Post-interaction energy form: pure kinetic Ek=25JE_k = 25\,\text J—converted from spring potential.

Momentum, Impulse & Work Example (3.2 kg block)

  • Δv=2.41.9=0.5m/s West\Delta v = 2.4-1.9 = 0.5\,\text{m/s West}, so
    • \Delta \vec p = m\Delta \vec v = 3.2\times 0.5 = 1.6\,\text{kg·m/s West}.
    • \Delta KE = \tfrac12 m (vf^2-vi^2) = \tfrac12\times 3.2(2.4^2-1.9^2) \approx 0.4\,\text J}.
    • Impulse J=Δp\vec J = \Delta\vec p; Net work Wnet=ΔKEW_{\text{net}} = \Delta KE.

Energy & Momentum Scaling Relations

  • Reduce speed to 15v0\tfrac15 v_0:
    • pvp \propto vp<em>new=15p</em>0p<em>{\text{new}} = \tfrac15 p</em>0.
    • KEv2KE \propto v^2KE<em>new=(15)2KE</em>0=125KE0KE<em>{\text{new}} = (\tfrac15)^2 KE</em>0 = \tfrac1{25} KE_0.
  • Halve mass and triple speed: KEmv2KE \propto m v^2KE<em>new=(12)(32)KE</em>0=4.5KE0KE<em>{\text{new}} = (\tfrac12)(3^2) KE</em>0 = 4.5 KE_0.
  • Uniform circular motion: a<em>c=v2ra<em>c = \dfrac{v^2}{r}. If v14v</em>0v\to\tfrac14 v</em>0 and r2r<em>0r\to 2r<em>0a</em>c(14v<em>0)22r</em>0=132ac0a</em>c\to\dfrac{(\tfrac14 v<em>0)^2}{2r</em>0}=\tfrac1{32} a_{c0}.

Gravitation & Electrostatics Scaling

  • Newton: F<em>g=Gm</em>1m<em>2r2F<em>g = G\dfrac{m</em>1 m<em>2}{r^2}. Coulomb: F</em>e=kq<em>1q</em>2r2F</em>e = k\dfrac{|q<em>1 q</em>2|}{r^2}.
  • Separation r32rr\to\tfrac32 rF(23)2F<em>0=49F</em>0F\to (\tfrac23)^2 F<em>0 = \tfrac49 F</em>0.
  • Separation r6rr\to 6r, mass m<em>112m</em>1m<em>1\to\tfrac12 m</em>1F(12)(136)F<em>0=172F</em>0F\to (\tfrac12)(\tfrac1{36}) F<em>0 = \tfrac1{72} F</em>0.
  • Tripling both charges and halving separation: F(33)(12)2F<em>0=36F</em>0F\to (3\cdot3)(\tfrac12)^{-2}F<em>0 = 36F</em>0.
  • Electric field between parallel plates is uniform, magnitude E=VdE = \dfrac{V}{d}, direction from + to –.
    • Replacing a test charge does not change the field. Force scales with charge: F=qE\vec F = q \vec E. Acceleration a=Fm=qEma = \dfrac{F}{m} = \dfrac{qE}{m} ⇒ halving mass & dividing charge by 3 doubles acceleration.

Circuit Principles

  • Series resistors: Req=RR_{\text{eq}} = \sum R, same current. Adding two identical resistors in series triples total resistance ⇒ current drops to 13\tfrac13.
  • Parallel resistors: equal voltage across each branch. Each path must drop the full source voltage before charges return to the battery.
  • Power: P=IV=V2R=I2RP = IV = \dfrac{V^2}{R} = I^2 R. Quadrupling VV increases power by factor 42=164^2 = 16 (since PV2P\propto V^2).
  • Junction rule (Kirchhoff’s): current entering = current leaving (charge conservation).

Waves & Optics

  • Wave speed (no dispersion): v=fλv = f\lambda determined solely by medium properties (e.g.
    string tension & mass per unit length: v=Tμv = \sqrt{\tfrac{T}{\mu}}).
  • Frequency is fixed by the source (oscillating object).
  • If f54f<em>0f\to \tfrac54 f<em>0 with same medium, λ45λ</em>0\lambda\to \tfrac{4}{5}\lambda</em>0 (inverse proportionality).
  • Defining wave behaviors: reflection, refraction, diffraction, interference.
  • All incident, reflected, and refracted angles are measured with respect to the normal.
  • Reality checks: speeds > cc or negative discriminants under radicals signal algebraic mistakes—re-check.

Lenses & Refraction Quick Reference

  • Converging lens: thick in center, positive focal length, can form real inverted images (object outside ff) or virtual upright images (object inside ff), used in magnifiers, cameras.
  • Diverging lens: thin center, negative focal length, always forms smaller virtual upright images, used in peepholes, laser beam expanders.
  • Sense-making questions:
    • Is the second index of refraction higher or lower? Light slows in higher index (bends toward normal) and speeds up in lower index.
    • Do computed angles obey Snell’s Law n<em>1sinθ</em>1=n<em>2sinθ</em>2n<em>1\sin\theta</em>1 = n<em>2\sin\theta</em>2 and lie between 00^\circ and 9090^\circ?

Magnetic Phenomena

  • Magnetic forces act on moving charges, current-carrying wires, and magnetic dipoles.
  • All magnetic fields originate from moving charges (currents) or intrinsic spin of electrons (microscopic currents).

Strategy & Heuristics

  1. Always start physics problems with a clear diagram (vectors, FBD, circuit, rays, waves). It prevents sign errors.
  2. Check limiting cases (e.g. friction = 0, mass → ∞) to test formulas.
  3. Keep units throughout—catches algebra errors early.
  4. Conservation laws often replace kinematics/dynamics when forces are unknown.
  5. Never leave a calculation with more significant figures than the given data justify.

Common Formula Sheet (Physics 1-T)

  • vavg=ΔrΔt\vec v_{\text{avg}} = \dfrac{\Delta \vec r}{\Delta t}, a=ΔvΔt\vec a = \dfrac{\Delta \vec v}{\Delta t}.
  • Fnet=ma\vec F_{\text{net}} = m\vec a.
  • Work: W=Fd=FdcosθW = \vec F \cdot \vec d = Fd\cos\theta.
  • Kinetic energy: KE=12mv2KE = \tfrac12 m v^2.
  • Potential (spring): Us=12kx2U_s = \tfrac12 k x^2.
  • Potential (gravity near Earth): U<em>g=mghU<em>g = mgh; universal gravity: U</em>g=Gm<em>1m</em>2rU</em>g = -G\dfrac{m<em>1 m</em>2}{r}.
  • Power: P=Wt=IV=I2R=V2RP = \dfrac{W}{t} = IV = I^2R = \dfrac{V^2}{R}.
  • Impulse–momentum: J=Fdt=Δp\vec J = \int \vec F\,dt = \Delta \vec p.
  • Centripetal acceleration: ac=v2ra_c = \dfrac{v^2}{r}.
  • Coulomb’s Law: F=kq<em>1q</em>2r2F = k\dfrac{|q<em>1 q</em>2|}{r^2}.
  • Ohm’s Law: V=IRV = IR.
  • Snell’s Law: n<em>1sinθ</em>1=n<em>2sinθ</em>2n<em>1\sin\theta</em>1 = n<em>2\sin\theta</em>2.
  • Lens/Mirror equation: 1f=1d<em>o+1d</em>i\dfrac1f = \dfrac1d<em>o + \dfrac1d</em>i.

Final Reminders

  • Weight is just another name for gravitational force (appears three times on the review!).
  • Three ways to accelerate: speed up, slow down, change direction.
  • Uniform electric field exists only between parallel plates with opposite charges.
  • Direction of electrostatic force: like charges repel, unlike attract.
  • Series circuits share current; parallel circuits share voltage.
  • Any speed claim > cc or negative under a square root is unphysical → re-evaluate.