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Faraday Rotation

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Faraday Rotation Theory, Application, and Issues With a neat Tangent Zachary Marshall Faraday Rotation First noticed in 1845 by Michael Faraday Linearly polarized ... – PowerPoint PPT presentation

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Title: Faraday Rotation


1
Faraday Rotation
  • Theory, Application, and Issues
  • With a neat Tangent
  • Zachary Marshall

2
Faraday Rotation
  • First noticed in 1845 by Michael Faraday
  • Linearly polarized light near resonance travels
    through a material (esp. alkali metal gas) in a
    B-Field
  • The B-Field must have a component in the
    direction of propagation.
  • Polarization rotates
  • He wrote in his notebook, "I have at last
    succeeded in illuminating a magnetic curve or
    line of force and in magnetising a ray of light"

3
Some Hand Waving
  • Applied magnetic field creates Zeeman splitting
    of energy levels
  • LHC and RHC polarized light see different
    scattering cross-sections, so different
    refractive indices, and so have different phase
    velocities
  • Their different propagation means the linear
    polarization of light rotates

4
Again, with Math
  • Zeeman shift changes resonance by gFm0Bz
  • Dq V B L
  • Dq p (n- - n) L / l
  • Dq CRb L alkali B / Dl2
  • n S pi c2 ni

5
Faraday Rotator / Isolator
  • Optical element rotating the polarization of
    light
  • Polarizer - Faraday Rotator Polarizer
  • Prevents contamination and backsplash of
    electromagnetic waves
  • Common materials for use in 700-1100 nm range
    terbium doped borosillicate glass and terbium
    gallium garnet crystal (TGG).
  • They can be magnetized before hand.

6
For Measuring Number Density
  • Cell filled with a gas, at least some of which is
    an alkali metal (usually below its boiling point)
  • Tunable laser (e.g. TiSaph) through the center
    of a cell

7
What could possibly go wrong?
  • Optical pumping during measurement
  • Laser heats the cell interior
  • Thermal fluctuations in a cell
  • Remember What ever can go wrong, will go wrong.
    But there are ways around each problem.

8
How else could we find Rb?
  • Here comes the thermo

9
Killian Equations
  • First developed in the 1920s, credit is usually
    given to Killian (1926).
  • d(ln P)/dT DH/(R T2) (Clausius-Clapeyron)
  • In a small range, DH is temp. invar.
  • Resulting equation is of the form
  • log P A B/T
  • Additional terms like C log T, D / T2 are common

10
So What are A and B for Rb?
11
And what did they get?
12
Faraday to the Rescue?
  • Claimed to be the only safe method.
  • But why do we care so much?

13
Pumping Nobel Gasses
  • Rubidium is polarized with circularly polarized
    laser
  • Collisions transfer spin to Xe / He
  • Nitrogen prevents immediate spin loss
  • Depolarization comes from collisions
  • Rb depolarization term depends on Rb number
    density

14
He-3 Lung Image
15
And Some Secret Projects
16
And in Space
  • Faraday rotation occurs in the interstellar
    medium due to free electrons
  • Dq l2 C integral of Bne ds
  • If we know ne, we can determine B along the path
    to us.
  • Radio waves going through the ionosphere rotate
    as well.
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