Maxwells Equations Four equations integral form Gausss law

  • Slides: 19
Download presentation
Maxwell’s Equations Four equations (integral form) : Gauss’s law for magnetism Faraday’s law Ampere-Maxwell

Maxwell’s Equations Four equations (integral form) : Gauss’s law for magnetism Faraday’s law Ampere-Maxwell law + Lorentz force

Sinusoidal Electromagnetic Radiation Acceleration: Sinusoidal E/M field

Sinusoidal Electromagnetic Radiation Acceleration: Sinusoidal E/M field

Energy and Momentum of E/M Radiation According to particle theory of light: photons have

Energy and Momentum of E/M Radiation According to particle theory of light: photons have energy and momentum Classical E/M model of light: E/M radiation must carry energy and momentum

Energy of E/M Radiation A particle will experience electric force during a short time

Energy of E/M Radiation A particle will experience electric force during a short time d/c: What will happen to the ball? It will oscillate Energy was transferred from E/M field to the ball Amount of energy in the pulse is ~ E 2

Energy of E/M Radiation Ball gained energy: Pulse energy must decrease E/M radiation: E=c.

Energy of E/M Radiation Ball gained energy: Pulse energy must decrease E/M radiation: E=c. B

Energy Flux There is E/M energy stored in the pulse: Pulse moves in space:

Energy Flux There is E/M energy stored in the pulse: Pulse moves in space: there is energy flux Units: J/(m 2 s) = W/m 2 During t: used: E=c. B, 0 0=1/c 2

Energy Flux: The Poynting Vector The direction of the E/M radiation was given by

Energy Flux: The Poynting Vector The direction of the E/M radiation was given by Energy flux, the “Poynting vector”: John Henry Poynting (1852 -1914) • S is the rate of energy flux in E/M radiation • It points in the direction of the E/M radiation

Exercise In the vicinity of the Earth, the energy density of radiation emitted by

Exercise In the vicinity of the Earth, the energy density of radiation emitted by the sun is ~1400 W/m 2. What is the approximate magnitude of the electric field in the sunlight? Solution: Note: this is an average (rms) value

Exercise A laser pointer emits ~5 m. W of light power. What is the

Exercise A laser pointer emits ~5 m. W of light power. What is the approximate magnitude of the electric field? Solution: 1. Spot size: ~2 mm 2. flux = (5. 10 -3 W)/(3. 14. 0. 0012 m 2)=1592 W/m 2 3. Electric field: (rms value) What if we focus it into 2 a micron spot? Flux will increase 106 times, E will increase 103 times:

Momentum of E/M Radiation • E field starts motion • Moving charge in magnetic

Momentum of E/M Radiation • E field starts motion • Moving charge in magnetic field: Fmag What if there is negative charge? ‘Radiation pressure’: What is its magnitude? Average speed: v/2 Fmag

Momentum Flux Net momentum: in transverse direction: 0 in longitudinal direction: >0 Relativistic energy:

Momentum Flux Net momentum: in transverse direction: 0 in longitudinal direction: >0 Relativistic energy: Quantum view: light consists of photons with zero mass: Classical (Maxwell): it is also valid, i. e. momentum = energy/speed Momentum flux: Units of Pressure

Exercise: Solar Sail Solution: If reflective surface? Total force on the sail: Atmospheric pressure

Exercise: Solar Sail Solution: If reflective surface? Total force on the sail: Atmospheric pressure is ~ 105 N/m 2

Re-radiation: Scattering Positive charge Electric fields are not blocked by matter: how can E

Re-radiation: Scattering Positive charge Electric fields are not blocked by matter: how can E decrease?

Cardboard Why there is no light going through a cardboard? Electric fields are not

Cardboard Why there is no light going through a cardboard? Electric fields are not blocked by matter Electrons and nucleus in cardboard reradiate light Behind the cardboard reradiated E/M field cancels original field

In which of these situations will the bulb light? A) B) C) D) E)

In which of these situations will the bulb light? A) B) C) D) E) A B C None B and C

Refraction: Bending of Light In transparent media, the superposition can result in change of

Refraction: Bending of Light In transparent media, the superposition can result in change of wavelength and speed of wavefront Rays perpendicular to wavefront bend at surface

Refraction: Snell’s Law A ray bends as it goes from one transparent media to

Refraction: Snell’s Law A ray bends as it goes from one transparent media to another

Total Internal Reflection and transmission

Total Internal Reflection and transmission