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This is the last part of my guest 
lectures on electron spin, in which I'll 

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focus on normally non-magnetic systems 
which are pushed out of spin degeneracy 

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equilibrium. 
By spin injection from an external 

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thermomagnetic source. 
I'm going to first tell you why we 

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want to study these systems, and why this 
is such a hard problem or at least why 

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the most straight forward approach to 
solving it is bound to fail. 

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Then I'll show you one particular way 
that I have personally used, to obtain 

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spin injection in silicon and germanium 
semiconductor devices. 

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And a little bit about what can be 
learned as a result. 

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To motivate the kinds of information 
about non-equilibrium spin transport 

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we're after, I want to appeal to the 
history of non-equilibrium charge 

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transport. 
Namely minority carriers and 

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semi-conductors. 
The seminal measurements were done by 

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Haynes and Shockley in the mid-20th 
century at Bell Labs. 

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In these timed domain experiments, a 
narrow pulse of minority electrons, were 

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injected into p-type semi-conductors 
filled with equilibrium holes. 

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An electric field carried these electrons 
to a charge detector, where the pulse 

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could be analyzed. 
By measuring the time of flight, they 

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could determine the minority carrier 
mobility or the proportionality constant 

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between applied electric field and 
electron velocity. 

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By measuring the spreading of the pulse 
in time, they determined the strength of 

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random thermal fluctuations from 
scattering, the minority carrier 

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diffusion coefficient. 
And by integrating over the pulse and 

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determining how many electrons made it 
without annihilating with a positively 

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charged hull, the minority carrier 
lifetime could be determined. 

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Without these values, none of the solid 
state devices we use today could be 

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designed and successfully made. 
So, if we speculate any use for 

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spin-polarized electrons out of 
equilibrium in semi-conductor devices. 

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Then we at least need to be able to 
measure the spin analogs of these 

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parameters. 
So, let's first look at why it's not so 

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easy to transfer the substantial spin and 
balance, spin polarization. 

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From a ferromagnet, into a non-magnetic 
electronic material, especially when 

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using a semiconductor in an effort to 
make, for example, new kinds of spin 

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transistors. 
The most straight forward way one might 

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naively try, is to make an ohmic or 
linearly resistive contact between the 

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ferromagnet and a semiconductor. 
Let's see how this works for plain old 

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charge injection. 
Ohm's law says that the charge current 

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density flowing, is proportional to the 
conductivity, and driven by a spacial 

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gradient of an electro-chemical 
potential. 

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This combines the effects of electric 
field, gradient of electro-static 

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potential, with flow from high 
concentration to low via random thermal 

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fluctuations comprising the random watts 
of diffusion. 

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If we incorporate the device geometry, we 
can use this expression to recover the 

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more familiar V equals IR form of Ohms 
Law. 

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In metal-semiconductor ohmic contacts, 
current is conserved across the interface 

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but the connectivity in the metal is 
large. 

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So, the potential energy provided by 
voltage q times v drops mostly across the 

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lower connectivity semiconductor. 
Now, if we want spin injection to 

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accompany this charge injection, then, 
the currents for spin up and down must be 

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different. 
Since the conductivities for up and down 

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are the same in a semi-conductor, the re, 
the respective electrochemical gradients 

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must be different. 
This, is what we need to happen on the 

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semi-conductor side. 
Spin up and down electrochemical 

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potentials have different gradients to 
drive asymmetric current densities 

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comprising a spin current. 
The unavoidable consequence of this 

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asymmetry, is an electrochemical 
splitting at the ohmic interface. 

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Using Ohm's law, we can obtain a 
relationship between current polarization 

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and this electrochemical potential 
splitting. 

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The first tern, in parenthesis, is due to 
the average potential drop over the 

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transport length scale, L. 
Note that, although, J up and J down are 

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not equal, their sum does equal the total 
charge current, as expected. 

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Now, we have to derive equivalent 
expressions, on the ferromagnet side, or 

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we will see the deleterious effect of the 
splitting on spin eject. 

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On the ferromagnet side, the 
electrochemical potential splitting 

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relaxes to zero in equilibrium, due to 
spin flips away from the interface. 

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The spin relaxation length scale is a so 
called spin diffusion length, lambda. 

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By once again applying Ohm's Law, we get 
the following expressions for the current 

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densities of spin up and, and down on the 
ferromagnet side. 

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Note that there are two important 
differences between these expressions for 

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the ferromagnet and the ones above 
describing transport in a semi-conductor. 

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First, the spin dependent connectivities 
are not equal to the ferromagnet, due to 

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their dependence on the asymmetric 
carrier densitites. 

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Second, and as a result, the deviation of 
the interface electrochemical potentials 

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from equilibrium are not symmetric. 
In other words, c-up is not equal to 

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c-down in this figure. 
However, because the ideal interface 

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preserves spin, the electrochemical 
potentials are continuous. 

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So, we do have the sum rule, giving us a 
total splitting, which we need to 

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determine the spin polarization, flowing 
across the interface in the 

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semiconductor. 
Using the definitions of both the 

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injected current polarization and the 
bulk ferromagnetic polarization, we can 

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derive a simple expression for the 
splitting on the ferromagnet side. 

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In intimate ohmic contact, the 
electrochemical potentials are 

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continuous, so this is the same as the 
splitting of the semiconductor side. 

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We can therefore substitute it into our 
previously-derived expression to obtain 

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this result. 
Note that this is very different from our 

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naive expectation, since it depends 
strongly on the magnitude of the 

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dimensionalist parameter, epsilon. 
The ratio of conductivities and transport 

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lengths across the interface. 
If epsilon is much less than 1, then, 

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only when the bulk magnetic polarization, 
beta, is approximately 1 a half-metallic 

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ferromagnet. 
Do we recover the desired case, where the 

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injected current polarization P, is 
approximately equal to the bulk 

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ferromagnetic polarization beta. 
Unfortunately, the bulk polarization of 

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typical ferromagnets is around 50%, so as 
this plot shows ohmic injection is doomed 

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unless epsilon is at least 0.01. 
However, the relevant materials 

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properties are not forgiving in this 
respect. 

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The ratio of conductivities between a 
semi-conductor and a ferromagnetic metal 

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is significantly below unity. 
Even for highly-doped semi-conductors, 

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and highly disordered, amorphous 
ferromagnetic metals. 

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Likewise, the ratio of length scales is 
small, due to the fast spin relaxation in 

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the ferromagnet, leading to a spin 
diffusion length Lambda of approximately 

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ten nanometers. 
Whereas in semiconductors with low spin 

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orbit interaction, such as silicon, 
transport lengths can be ten microns or 

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longer even at elevated ambient 
temperatures. 

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Therefore, even in the best scenario, 
epsilon is approximately ten to the minus 

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four. 
Leading to the negligible polarization 

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shown in the figure. 
Over the range of expected values for 

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epsilon, one needs bulk polarization of 
at least 95% for injected polarization of 

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greater than 10%, or so. 
So, elemental ferromagnets, Iron, Cobalt 

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and Nickel, are you useless for spin 
injection in the ohmic regime. 

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In fact, the problem is evident even 
graphically. 

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The splitting delta mu, which is 
necessary for a non-zero injected current 

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polarization, also tends to reverse the 
spin up electrochemical potential 

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gradient at the interface on the 
ferromagnet side. 

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Inhibiting injection of the very spin 
specise we want to inject into the 

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semi-conductor. 
Therefore, in order to maintain the 

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constraint of current conservation across 
the interface. 

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The steady state inter-facial splitting 
is small, and the injected current 

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polarization, p, is negligible. 
Modern techniques to overcome this 

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problem include quantum mechanical 
tunneling. 

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And, in my lab Ballistic hot electron 
injection, which circumvents the issues 

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relevant for ohmic injection, here. 
I'm not going to describe the details of 

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spin injection and detection, that's a 
whole other course in device physics and 

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magnetism. 
But rather, what we can learn from 

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measurements of spin transport and 
manipulation, by any means. 

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The key to extracting the most 
information from these measurements, is 

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exploiting a topic I mentioned several 
segments ago, spin procession. 

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Again, this is magnetic analog of a 
spinning top or gyroscope, with an off 

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axis gravitational force causing a 
mechanical torque. 

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In spin transport devices, we apply a 
magnetic field perpendicular to the 

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injective spin direction. 
But parallel to the transport direction 

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caused by electric fields and the spin 
with process in a plane. 

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The final spin procession angle, is 
determined by the product of spin 

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procession frequency determined by 
magnetic field strength. 

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About 28 gigahertz per Tesla in a 
material with weak spin orbit coupling 

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like silicon, and the transit time 
inversely proportional to electric field 

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strength. 
If we apply a perpendicular magnetic 

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field with the appropriate strength. 
Then you cause the spins to process an 

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average of 180 degrees, fully flipping 
with respect to their injected 

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polarization. 
Your experimental measurement of sigma z, 

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the spin along the initialization axis, 
will then vary. 

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Doubling the magnetic field doubles the 
procession frequency and therefore 

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results in an average procession angle of 
360 degrees. 

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A coherent full rotation restoring the 
expectation value of sigma z. 

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As you can see from this actual 
experimental data, it doesn't matter 

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whether the field polarity is positive or 
negative. 

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In other words, it doesn't matter if the 
spin processes clockwise or counter 

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clockwise. 
Now if all electrons had the same transit 

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time from injector to detector, We would 
expect this cosine-like oscillation to 

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continue indefinitely for higher and 
higher orders of procession rotations. 

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But that's not what happens. 
In reality, not all electrons have the 

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same transit time due to random 
scattering processes. 

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Therefore, an uncertainty in transit time 
gives rise to an uncertainty in 

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procession angle. 
When the precession frequency grows in 

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higher an higher magnetic field, the 
affects of partial cancellation can be 

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seen an the oscillations diminish. 
We can model this measurement with a 

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transport simulation. 
Summing up the cosine like contributions 

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from electrons, or the distribution of 
arrival times, in order to fit the non 

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equilibrium spin mobility. 
And diffusion coefficients we're after. 

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However, there's a model independent 
method with far greater utility. 

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The key is to recognize that this 
integral summation, is really just a 

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fourier transform. 
Therefore, the oscillations we measure, 

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can be inverted to yield the empirical 
transport distribution without any model 

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dependence whatsoever. 
In this example we can see the effects of 

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increasing the electric field. 
Oscillation period increases, and the 

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number of oscillation themselves grows. 
But the transformed, clearly shows that 

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this is the result of smaller from mean 
and transit time and standard deviation. 

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This method of obtaining time of flight 
is called the Larmor clock. 

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We don't make a explicit measurement of 
transit time, we measure the angle of 

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rotation at a known angular velocity, the 
same way we measure time from an analog 

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clock. 
We know the rotation speed of the hand 

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for the clock, 360 degrees per hour for 
the minute hand, and infer time from the 

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instantatous oreintation. 
We're likewise measuring the spin 

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orientation and determining how long it 
processed in a known magnetic field. 

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For measurements of spin transport, we 
can correlate the transit time with final 

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spin polarization and extract the spin 
lifetime. 

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In silicon, we can see that, although the 
non-equilibrium lifetimes of hundreds of 

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nanoseconds are fairly long. 
In comparison to the momentum relaxation 

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time of picoseconds or less, they're 
strongly dependent on temperature, 

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increasing dramatically as the sample is 
cooled. 

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This demonstrates the importance of 
relaxation, via a nominally 

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spin-independent process, electrons 
scattering off of thermal phonons, 

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distortions in the crystal lattice. 
This electron-phonon spin relaxation 

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process, results from the fact that due 
to the weak but non-zero spin-orbit 

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coupling. 
The electron wave functions are not pure 

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00:12:28,045 --> 00:12:32,670
spin eigenstates up and down. 
Rather, spin up has a small amount of 

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spin down and vice versa, but remain 
fully orthogonal. 

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00:12:37,170 --> 00:12:40,602
We can calculate the transition rate 
between these states constituting a spin 

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00:12:40,602 --> 00:12:44,034
flip, due to momentum scattering of these 
free electrons from wave vector k to k 

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00:12:44,034 --> 00:12:48,200
prime. 
By using the so-called Fermi Golden rule. 

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00:12:49,490 --> 00:12:52,370
This first order expression is 
proportional to the square of the matrix 

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00:12:52,370 --> 00:12:55,202
element of a scattering potential, 
coupling the two initial and final 

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states. 
And the density of final states row. 

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00:12:58,475 --> 00:13:02,763
Now, even if the scattering potential 
only couples states of different momenta 

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00:13:02,763 --> 00:13:05,873
k. 
Due to the spin-orbit mixing of the wave 

195
00:13:05,873 --> 00:13:10,117
function, we see that there is a non-zero 
matrix element. 

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And this exactly equal to the quantity 
determining the spin preserving momentum 

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relaxation rate. 
The spin relaxation is therefore 

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proportional to the momentum relaxation, 
and also proportional to the square of 

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the typically small spin mixing 
amplitude. 

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This being the end of my contribution to 
this course, I'm obliged to acknowledge 

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support, not only from my experimental 
research on spin transport. 

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But also support for scientific outreach 
efforts for students and the public 

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outside my institution, the University of 
Maryland. 

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In particular, the National Science 
Foundation Career Award has made this 

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00:13:43,275 --> 00:13:47,510
work possible. 
It's been my great pleasure to share this 

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00:13:47,510 --> 00:13:51,531
quick story of electron spin with you. 
And I invite you to learn more about spin 

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through own study and perhaps even 
original research in Physics and 

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Engineering labs around the world. 

