the classical hall effect
DESCRIPTION
The Classical Hall effect. Reminder: The Lorentz Force. F = q [ E + ( v B )]. Lorentz Force: Review. Velocity Filter : Undeflected trajectories in crossed E & B fields: v = (E/B). Cyclotron motion : F B = ma r qvB = (mv 2 /r). - PowerPoint PPT PresentationTRANSCRIPT
![Page 1: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/1.jpg)
The Classical Hall effect
![Page 2: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/2.jpg)
Reminder: The Lorentz Force
F = q[E + (v B)]
![Page 3: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/3.jpg)
Crossed E & B Fields•In the configurationshown here, can haveseveral practical uses!
The Lorentz Force: Review
F = q[E + (v B)]
1.Velocity Filters: Undeflected trajectories
of charged particles. Choose E & B so thatthe particles have a desired v = (E/B)2.Cyclotron Motion:
FB = mar qvB = (mv2/r)
![Page 4: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/4.jpg)
• Cyclotron Motion:FB = mar qvB = (mv2/r)
Orbit Radius: r = [(mv)/(|q|B)] = [p/(q|B|])
A Momentum (p) Filter!!Orbit Frequency: ω = 2πf = (|q|B)/m A Mass Measurement Method! Orbit Energy: K = (½)mv2 = (q2B2r2)/2m
Crossed E & B Fields
![Page 5: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/5.jpg)
Standard Hall Effect Experiment
e- v e+ v
E field
![Page 6: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/6.jpg)
Standard Hall Effect Experiment
e- v e+ v
E field
Current from the applied E-field
![Page 7: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/7.jpg)
Standard Hall Effect Experiment
e- v e+ v
E field
Current from the applied E-field
Lorentz force frommagnetic field on a moving particle
![Page 8: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/8.jpg)
Standard Hall Effect Experiment
e- v e+ v
E field
Current from the applied E-field
Top view: electronsdrift from back to front
Lorentz force frommagnetic field on a moving particle
![Page 9: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/9.jpg)
The Hall Effect
Lorentz force: Balance equation:
HeE evB
neRJBRE HHH
1 ,
RH is independent of and m An excellent method for determining n
y
x z
yBve ˆ
![Page 10: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/10.jpg)
),0,0( ),0,,( ),0,,( , ),( BBEEEvvvvneJBvEm
ev
dt
vdyxyx
y
x
y
x
y
x
y
x
E
E
J
J
J
J
E
E ~or ~
1
1
)(1~ ,
1
11~2
0
0
c
c
cc
c
σ
magneto-resistivity tensor
magneto-conductivity tensor
Jy = 0ne
RBJRJEE
JJEE
HxHxc
Hy
xxLx
1 ,
1
0
00
The Hall Effect: A more formal derivation
![Page 11: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/11.jpg)
Charge Density in the Drude Model
For Li, m = 0.542 × 103, A = 6.941 × 10-3, Z = 1
m [kg/m3]: mass densityA [kg]: atomic mass (mass of one mole)
m/A moles atoms per m3
NAm/A atoms per m3, NA = 6.02 × 1023
n = NAmZ/A electrons per m3, Z: # of valence electrons
n = 4.70 × 1028 m-3
![Page 12: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/12.jpg)
Comparison with Experiment
For Li, m = 0.542 × 103, A = 6.941 × 10-3, Z = 1 n = 4.70 × 1028 m-3
RH = 1.33 × 10-10 m3/Cgood
RH(exp) = 1.7 × 10-10 m3/C
For Zn, m = 7.13 × 103, A = 65.38 × 10-3, Z = 2 n = 1.31 × 1029 m-3
RH = × 10-11 m3/Cbad RH(exp) = 3 × 10-11 m3/C
Positive Hall coefficient!
![Page 13: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/13.jpg)
Cyclotron Frequency and the Hall Angle
Newtonian equation of motion in E and B:
dp p pe E B
dt m
steadystate
0
0
z c y z
y c z y
E J J
E J J
, tanc c
eB
m
![Page 14: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/14.jpg)
Deviation from the Deviation from the Classical Hall EffectClassical Hall Effect
![Page 15: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/15.jpg)
How Difficult is How Difficult is cc > 1 ? > 1 ?
* *1c e
eB eB B
m m
e = 10000 cm2/Vs B > 1 Tesla
e = 1000 cm2/Vs B > 10 Tesla
e = 100 cm2/Vs B > 100 Tesla
![Page 16: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/16.jpg)
Electrons flowing without a magnetic fieldElectrons flowing without a magnetic field
t
d
semiconductor slice
+ _
I I
![Page 17: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/17.jpg)
When the magnetic field is turned on ..When the magnetic field is turned on ..
B-field
I qBv
![Page 18: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/18.jpg)
As time goes by...As time goes by...
I
qBv = qElowpotential
highpotential
qE
![Page 19: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/19.jpg)
Finally...Finally...
B-field
I
VH
![Page 20: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/20.jpg)
Page 20Phys 320 - Baski Solid-State Physics
• Why is the Hall Effect useful? It can determine the carrier type (electron vs. hole) & the carrier density n for a semiconductor.
• How? Place the semiconductor into external B field, push current along one axis, & measure the induced Hall voltage VH along the perpendicular axis. The following can be derived:
Derived from the Lorentz force FE = qE = FB = (qvB).n = [(IB)/(qwVH)]
Semiconductors: Charge Carrier Density via Hall Effect
Hole Electron
+ charge – charge
BF qv B
![Page 21: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/21.jpg)
The surface current density sx = vxσ q, (σ = surface charge density)
Again, RH = 1/σ e. But, now: Rxy = Vy / ix = RH Bz since
sx = ix /ly . & Ey = Vy /ly. That is, Rxy does NOT depend on the sample shape of the sample. This is a very importantaspect of the Quantum Hall Effect (QHE)
The 2Dimensional Hall effect
![Page 22: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/22.jpg)
The Integer Quantum Hall Effect
The Hall Conductance is quantized in units of e2/h, or The Hall Resistance Rxy = h/(ie2) where i is an integer. The quantum of conductance h/e2 is now known as the
“Klitzing” !! Has been measured to 1 part in 108
Very important:
For a 2D electron
system only
First observed in 1980 by Klaus von Klitzing
Awarded the 1985 Nobel Prize.
![Page 23: The Classical Hall effect](https://reader034.vdocuments.net/reader034/viewer/2022050802/56813d1f550346895da6df02/html5/thumbnails/23.jpg)
The Royal Swedish Academy of Sciences awarded The 1998 Nobel Prize in Physics
jointly to Robert B. Laughlin (Stanford),
Horst L. Störmer (Columbia & Bell Labs) & Daniel C. Tsui, (Princeton)
The Fractional Quantum Hall effect
The 3 researchers were awarded the Nobel Prize for discovering that electrons acting together in strong magnetic fields can form new types of "particles", with charges that are fractions of an electron charge.
Citation: “For their discovery of a new form of quantum fluid with fractionally charged excitations.”
Störmer & Tsui made the discovery in 1982 in an experiment using extremely high magnetic fields very low temperatures. Within a year Laughlin had succeededin explaining their result. His theory showed that electrons in high magnetic fields & low temperatures can condense to form a quantum fluid similar to the quantum fluids that occur in superconductivity & liquid helium. Such fluids are important because events in a drop of quantum fluid can give deep insight into the inner structure & dynamics of matter. Their contributions were another breakthrough in the understanding of quantum physics & to development of new theoretical concepts of significance in many branches of modern physics.