High School Physics Overview Notes
Electrostatics
- Electric Charge: Matter possesses positive or negative electric charge q=±ne, where e≈1.6×10−19C is the elementary charge.
- Law of Conservation of Charge: The total electric charge of an isolated system remains constant across all processes.
- Coulomb's Law: The electrostatic force between two point charges is given by F=kr2∣q1q2∣, where k \approx 9 \times 10^9\,\text{N}\cdot\text{m}^2/\text{C}^2$.\n* **Electric Field & Potential:**\n * Field lines originate on positive charges and terminate on negative charges.\n * Electric potential Vdefinespotentialenergyperunitcharge(E_e = q V).VoltageispotentialdifferenceU = V_A - V_B$.
- Work done by the electric field moving a charge: W = q U$.\n* **Conductors & Insulators in Fields:**\n * In electrostatic equilibrium, the internal electric field and voltage difference inside a conductor are zero (E = 0,U = 0); excess charges reside entirely on the outer surface, concentrating at sharp edges.\n * A *Faraday cage* shields its interior from external electric fields.\n * Insulators contain bound charges that form electric dipoles under external fields (polarization).\n* **Capacitors:**\n * Systems of two conductors separated by an insulator, characterized by capacitance C = \frac{q}{U}(measuredinfarads,\text{F}).\n * Stored electrical energy: E_e = \frac{1}{2} C U^2 = \frac{1}{2} q U$.
Electric Current
- Current Intensity: Defined as I=tq, measured in amperes (A). Conventional current flows from higher to lower potential.
- Ohm's Law: Current intensity is proportional to applied voltage: I=RU, where R is resistance in ohms (Ω).
- Resistance of conductors increases with temperature; resistance of semiconductors decreases with temperature.
- Electric Work & Power:
- Energy transformed in an electric receiver: E = U I t$.\n * Electric power: P = U I,measuredinwatts(\text{W})orkilowatt−hours(1\,\text{kWh} = 3.6 \times 10^6\,\text{J}).\n* **Kirchhoff's First Law:** The sum of currents entering a circuit junction equals the sum of currents leaving it: \sum I_{\text{in}} = \sum I_{\text{out}}.\n* **Parallel Connections:** Voltage across parallel branches is identical (U);totalcurrentI = I_1 + I_2 + \dots;totalpowerP = P_1 + P_2 + \dots\n* **Circuit Safety:** Residual-current devices (*bezpieczniki różnicowoprądowe*) disconnect power when leak currents exceed 30\,\text{mA}; circuit breakers (*bezpieczniki przeciążeniowe*) protect against short circuits and overloads.\n\n# Electromagnetism\n\n* **Magnetic Field & Induction:**\n * Magnetic field strength is characterized by magnetic induction \mathbf{B}inteslas(\text{T}). Field lines form closed loops.\n * *Ferromagnets* strongly magnetize in external fields and retain residual magnetization.\n* **Magnetic Forces:**\n * **Electrodynamic Force:** Acts on a current-carrying conductor in a magnetic field: F = B I l (for perpendicular orientation, direction given by the left-hand rule).\n * **Lorentz Force:** Acts on a moving charge q:F_L = q v B(forperpendicularvelocity).Altersparticledirectionwithoutchangingkineticenergy,resultingincircularmotionwithradiusr = \frac{m v}{q B}.\n* **Electromagnetic Induction & Waves:**\n * A changing magnetic field induces a swirling electric field and current in closed circuits (Faraday's Law of Induction).\n * Electromagnetic waves consist of coupled oscillating electric and magnetic fields propagating at light speed c \approx 3 \times 10^8\,\text{m/s}(\lambda f = c).\n* **Alternating Current (AC) & Transformers:**\n * Effective values: U_{\text{sk}} = \frac{U_{\text{max}}}{\sqrt{2}},I_{\text{sk}} = \frac{I_{\text{max}}}{\sqrt{2}}.AverageACpower:P = U_{\text{sk}} I_{\text{sk}}.\n * Transformer voltage ratio: \frac{U_2}{U_1} = \frac{n_2}{n_1}.\n\n# Atomic Physics\n\n* **Electromagnetic Spectrum:** Encompasses radio waves, microwaves, infrared, visible light (400\,\text{nm} - 700\,\text{nm}), ultraviolet, X-rays, and gamma rays.\n* **Photons:**\n * Quantized light particles carrying energy E = h f = \frac{h c}{\lambda},whereh \approx 6.63 \times 10^{-34}\,\text{J}\cdot\text{s} is Planck's constant.\n * Energy unit conversion: 1\,\text{eV} = 1.6 \times 10^{-19}\,\text{J}.\n* **Atomic Structure & Energy Levels:**\n * Electrons occupy discrete energy levels (E_n).\n * Photon emission or absorption condition: h f = E_n - E_k$.
- Thermal sources produce continuous spectra; non-thermal gas sources produce discrete line spectra.
- Band Theory & Semiconductor Devices:
- Energy levels form energy bands (pasma energetyczne) separated by band gaps (przerwa energetyczna).
- p-n Junction / Diode: Conducts current in one direction only. LEDs emit photons during electron transitions across the junction.
- MOSFET Transistor: Uses gate voltage UGS to control current flow through a semiconductor channel.
- Photoelectric Effect:
- Emission or excitation of electrons by light above a cutoff frequency fgr=hW, where W is the work function.
Nuclear Physics
- Nuclear Structure:
- Nucleus ZAX contains Z protons and N=A−Z neutrons (nucleons).
- Held together by strong, short-range nuclear forces.
- Isotopes: Atoms of the same element with equal Z but different A$.\n* **Radioactivity & Decay Law:**\n * Decay types: \alpha(emissionof2^4\text{He}),\beta^-(neutronconvertstoproton,electron_{-1}^0 e,andantineutrino),\gamma (high-energy photon emission).\n * Radioactive Decay Law: N = N_0 \left(\frac{1}{2}\right)^n = N_0 \left(\frac{1}{2}\right)^{\frac{t}{T{1/2}}},whereT_{1/2} is the half-life.\n* **Dosimetry:**\n * Absorbed dose: D = \frac{E}{m}inGrays(\text{Gy}).\n * Equivalent dose in Sieverts (\text{Sv})incorporatesbiologicaleffect(1\,\text{Sv} = 1\,\text{Gy}for\beta, \gamma;1\,\text{Sv} = 0.05\,\text{Gy}for\alpha).Averagenaturalbackground:\sim 2.5\,\text{mSv/year}.\n* **Binding Energy & Mass Deficit:**\n * Mass-energy equivalence: E_0 = m c^2$.
- Mass deficit: Δm=∑mnucleons−mnucleus.
- Nuclear binding energy: Ew=Δmc2. Peak binding energy per nucleon occurs near iron (56Fe).
- Fission & Fusion:
- Nuclear Fission: Heavy nuclei (e.g., 235U) split upon neutron absorption, releasing ∼200MeV and additional neutrons, sustaining a chain reaction above critical mass. Controlled in reactors using moderators and control rods.
- Nuclear Fusion: Light nuclei combine (e.g., proton-proton chain 41H→4He+2e++2νe+γ), releasing substantial energy; powers stars and thermonuclear reactors.
- Stellar Evolution & Compact Objects:
- Stars fuse hydrogen to helium during main sequence.
- Solar-mass stars expand into red giants, shed outer layers as planetary nebulae, leaving white dwarfs.
- Massive stars (>9M⊙) undergo core collapse, exploding as supernovae (synthesizing elements heavier than iron) and leaving neutron stars or black holes (Rg=c22GM).