Modern Physics - Modern Physics -I – An introduction
Overview of Modern Physics
Historical background
Key features of Modern Physics
Importance in the field of Science
Topics to be covered
Historical Background
Development of Modern Physics in the late 19th century
Significant discoveries and breakthroughs
Contributions of renowned physicists such as Albert Einstein, Max Planck, and Niels Bohr
Transition from classical physics to modern physics
Impact on our understanding of the universe
Key Features of Modern Physics
Quantum Mechanics
Theory of Relativity
Particle Physics
Wave-Particle Duality
Uncertainty Principle
Quantum Mechanics
Introduction to quantum theory
Wavefunctions and probability
Dual nature of particles
Quantum superposition
Measurement problem
Theory of Relativity
Basics of Special Theory of Relativity
Einstein’s postulates
Time dilation and length contraction
Mass-energy equivalence (E=mc^2)
General Theory of Relativity and its implications
Particle Physics
Fundamental particles and forces
Standard Model of Particle Physics
Subatomic particles and their interactions
Quarks, leptons, and gauge bosons
Higgs Boson and the Higgs field
Wave-Particle Duality
Particle behavior vs. wave behavior
De Broglie wavelength
Interference and diffraction phenomena
Young’s double-slit experiment
Davisson-Germer experiment
Uncertainty Principle
Werner Heisenberg’s principle
Limitations on simultaneous measurement of complementary properties
Importance in quantum mechanics
Implications for our understanding of the physical world
Examples illustrating the uncertainty principle
Importance of Modern Physics
Advancements in technology and industry
Applications in healthcare and medicine
Understanding the behavior of matter and energy
Contribution to space exploration and astronomy
Influence on other branches of science
Topics to be Covered
Quantum Mechanics
Theory of Relativity
Atomic and Nuclear Physics
Particle Physics
Applications of Modern Physics
Quantum Mechanics
Schrödinger’s wave equation
Energy quantization in atomic systems
Quantum numbers and electron orbitals
Pauli exclusion principle
Electron configuration and periodic table
Theory of Relativity
Principle of equivalence
Curvature of spacetime
Black holes and gravitational waves
Time dilation and space contraction in general relativity
Cosmological implications and the expanding universe
Atomic and Nuclear Physics
Structure of the atom
Bohr’s model of the hydrogen atom
Atomic spectra and emission lines
Radioactivity and nuclear decay
Nuclear reactions, fission, and fusion
Particle Physics
Elementary particles and their classification
Quark model and hadrons
Leptons and the weak interaction
Gauge theories and the strong force
Unification theories and the search for the theory of everything
Applications of Modern Physics
MRI and medical imaging
Laser technology and its applications
Nuclear power generation
Nanotechnology and materials science
Quantum computing and cryptography
Examples: Wave-Particle Duality
Young’s double-slit experiment with electrons
Davisson-Germer experiment with electrons and diffraction
Photons and the photoelectric effect
Compton scattering and the dual nature of light
Matter waves and electron diffraction in crystals
Examples: Uncertainty Principle
Position-momentum uncertainty
Energy-time uncertainty
Measurement limitations in quantum systems
Thought experiments illustrating the uncertainty principle
Implications for our understanding of reality
Equations: Quantum Mechanics
Schrödinger’s wave equation: Hψ = Eψ
Uncertainty principle: ΔxΔp ≥ ħ/2
Time-independent Schrödinger equation
Stationary states and probability density function
Hydrogen atom energy levels: E = -13.6 eV / n^2
Equations: Theory of Relativity
Lorentz transformation equations
Time dilation: Δt’ = Δt / √(1 - v^2/c^2)
Length contraction: L’ = L√(1 - v^2/c^2)
Energy-momentum relation: E^2 = (mc^2)^2 + (pc)^2
Einstein field equations: Rμν - (1/2)Rgμν = (8πG/c^4)Tμν
Equations: Atomic and Nuclear Physics
Bohr radius: a₀ = 0.529 × 10^(-10) m
Rydberg formula: 1/λ = R(1/n₁^2 - 1/n₂^2)
Binding energy: E = mc^2
Decay constant: λ = ln(2) / t₁/₂
Einstein’s mass-energy equivalence: E = mc^2
Let’s continue with the remaining slides:
Examples: Atomic and Nuclear Physics
Alpha decay of uranium-238
Beta decay of carbon-14
Gamma ray emission in nuclear reactions
Nuclear fusion in stars and the sun
Nuclear power generation and the fission process
Examples: Particle Physics
Properties and interactions of quarks in hadrons
Electron-positron annihilation into photons
Weak interactions in radioactive decay
High-energy particle collisions at the Large Hadron Collider
Discovery of the Higgs boson and its significance
Examples: Applications of Modern Physics
Magnetic resonance imaging (MRI) in medical diagnostics
Laser technology in telecommunications and research
Nuclear power plants for electricity generation
Carbon nanotubes in electronics and materials science
Quantum cryptography and secure communication
Equations: Wave-Particle Duality
de Broglie wavelength: λ = h / p
Interference equation: sin(θ) = mλ / d
Double-slit intensity pattern: I = I₁ + I₂ + 2√(I₁I₂)cos(δ)
Photoelectric effect equation: hf = φ + KE
Compton scattering equation: λ’ - λ = (h / mc)(1 - cos(θ))
Equations: Uncertainty Principle
Position uncertainty: Δx ≥ ħ / (2Δp)
Energy uncertainty: ΔEΔt ≥ ħ / 2
Heisenberg’s uncertainty principle: ΔxΔp ≥ ħ / 2
Momentum uncertainty: Δp ≥ ħ / (2Δx)
Time-energy uncertainty: ΔEΔt ≥ ħ / 2
Examples: Equations in Quantum Mechanics
Schrödinger’s time-independent equation: Hψ = Eψ
Time-dependent Schrödinger equation: iħ∂ψ/∂t = Hψ
Probability density function: P = |ψ|^2
Wavefunction normalization: ∫ |ψ|^2 dV = 1
Hydrogen atom energy levels: Eₙ = -13.6 eV / n²
Examples: Equations in Theory of Relativity
Time dilation equation: Δt’ = Δt / √(1 - (v/c)²)
Length contraction equation: L’ = L√(1 - (v/c)²)
Energy-momentum relation: E² = (mc²)² + (pc)²
Einstein field equations: Rµν - (1/2)Rgµν = (8πG/c⁴)Tµν
Equivalence principle equation: F = m₁a₁ = m₂a₂
Examples: Equations in Atomic and Nuclear Physics
Bohr radius equation: a₀ = 0.529 × 10⁻¹⁰ m
Rydberg formula equation: 1/λ = R(1/n₁² - 1/n₂²)
Binding energy equation: E = mc²
Decay constant equation: λ = ln(2) / t₁/₂
Einstein’s mass-energy equivalence equation: E = mc²
Examples: Equations in Particle Physics
Standard Model equation: Q = (I³ + YW² + HY²)/2 + B(L + 2S)
Conservation of electric charge equation: ∑Q = 0
Kinematic equations for particle collisions: E₁ + E₂ = E₁’ + E₂’ and p₁ = p₁’ + p₂'
Gauge boson mass equation: m = gv / 2
Relativistic Doppler effect equation: Δλ/λ₀ = sqrt((c+v)/(c-v)) - 1
Conclusion
Recap of the main topics covered in the lecture
Importance of Modern Physics in understanding the physical world
Contributions of prominent physicists to the field
Applications of Modern Physics in various disciplines
Encouragement for further exploration and study of Modern Physics