Lectures 9&10 (Magnons, Landau Theory & Anisotropy Intro) Flashcards

1
Q

How can the dispersion relation for magnons be measured?

A

Inelastic neutron scattering

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2
Q

How does inelastic neutron scattering work?

A

Neutron fired at sample, hits iron and spin waves excited

Neutron transmitted or reflected with lower energy (given up energy to create spin waves)

Higher k vector - higher energy spin waves excited

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3
Q

What is each magnon equivalent to?

A

The reversal of a single-1/2 spin (but spread over the whole lattice)

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4
Q

In terms of magnetisation, what can number of magnons be equated to?

A

∆M

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5
Q

What is the Bloch law?

A

Far below Tc, that ∆M ~ T^3/2

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6
Q

Briefly, describe how to derive the Bloch law

A

Need to find the number of magnons, which is the integral over the DOS * the occupation number

Use B-E stats since magnons are bosons

Use the dispersion relation to find simplify the density of states

Find ∆M/M0 = no. magnons / total no. of spins to get the Block law

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7
Q

What are the experimental issues with the Bloch law?

A

In the lab, fairly easy to reach low temperatures in the magnon regime and measure M using magnetometer

But may not be possible to reach Tc and trace the full curve

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8
Q

How can Bloch law be used to predict the Curie temperature?

A

Easy to reach low temps (magnon regime) and measure M using magnetometer

But may not be possible to reach Tc and trace the full curve

Fit Bloch law to see where M goes to 0

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9
Q

Issues with using Bloch law to find Tc?

A

Only valid in low temperature regime (~0.5Tc)

But don’t know what Tc is, so don’t know where halfway is

More rapid dropoff than Bloch’s predicts

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10
Q

What can we use to predict M(T) closer to Tc, instead of Bloch’s law?

A

Landau theory of phase transitions

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11
Q

Is the Heisenberg Hamiltonian isotropic?

A

Yes

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12
Q

How to derive the Langevin function?

A

For a FM particle in H, find the energy, find the expectation value of the component of µ parallel to H

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13
Q

What does deriving the Langevin function from a FM particle in H show?

A

That our current definition of FM means that all particles are actually paramagnetic

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14
Q

Is exchange alone enough to give FM?

A

No

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15
Q

Without anisotropy, what does exchange do?

A

Couples all moments together into a giant spin that acts like a classical PM

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16
Q

What can reduce thermal fluctuations?

A

Anisotropy term - holds moment in place at H=0

17
Q

What can easy and hard directions be thought of as?

A

Easy directions - energy wells

Hard directions - energy barriers

18
Q

When will a magnetic moment sit in an energy well?

A

As long as kT &laquo_space;barrier height