applying hyperbolic functions to quantum tunneling and ... · how they help with radiation problems...

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UCF EXCEL I. Warmup questions concerning calculus II. Hyperbolic functions cosh(x) and sinh(x) III. Excellent properties of the derivative is cosh(x) and sinh(x) IV. How they help with radiation problems Applying hyperbolic functions to quantum tunneling and electromagnetic wave problems in physics and engineering (Lecture 1) Dr. Thomas J. Brueckner, Department of Physics 1

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UCF EXCEL

I. Warmup questions concerning calculusII. Hyperbolic functions cosh(x) and

sinh(x)III. Excellent properties of the derivative is

cosh(x) and sinh(x)IV. How they help with radiation problems

Applying hyperbolic functions to quantum tunneling and electromagnetic wave problems in physics and

engineering (Lecture 1)

Dr. Thomas J. Brueckner, Department of Physics

1

UCF EXCEL

1. If 10a = b, then log10(b) =

A. log10(b) = 0.1a

B. log10(2b) = 2a

C. log10(b) = a

D. log10(b/100) =100+a

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UCF EXCEL

1. If 10a = b, then log10(b) =

A. log10(b) = 0.1a

B. log10(2b) = 2a

C. log10(b) = a

D. log10(b/100) =100+a

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UCF EXCEL

Let’s take it apart!

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Let’s take it apart!

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Let’s take it apart!

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Let’s take it apart!

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Let’s take it apart!

So, you need a w value of 1.0955!

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Let’s pull this apart!

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Let’s pull this apart!

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Let’s pull this apart!

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Let’s pull this apart!

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Let’s pull this apart!

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What it means geometrically

Left of origin, in the

negatives…

…it is up side down!

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Differentiation of a sum = sum of derivatives

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Differentiation of a sum = sum of derivatives

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UCF EXCEL

Differentiation of a sum = sum of derivatives

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Differentiation of a sum = sum of derivatives

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Differentiation of a sum = sum of derivatives

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Differentiation of a sum = sum of derivatives

YAY!

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Why does this catch the eye of a mathematician or a scientist?

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Why does this catch the eye of a mathematician or a scientist?

A. Differentiate once, you get the other guy.

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Why does this catch the eye of a mathematician or a scientist?

A. Differentiate once, you get the other guy.

B. Differentiate again, you get back home!

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Why does this catch the eye of a mathematician or a scientist?

A. Differentiate once, you get the other guy.

B. Differentiate again, you get back home!

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Why does this catch the eye of a mathematician or a scientist?

A. Differentiate once, you get the other guy.

B. Differentiate again, you get back home!

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Why does this catch the eye of a mathematician or a scientist?

C. Very useful!!!D. Because

derivatives have various physical interpretations, like vectors!

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What our goal is this afternoon

Penetrate material with electromagnetic waves that reshape into hyperbolic functions.

2L

y

x z

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What our goal is this afternoon

Penetrate material with electromagnetic waves that reshape into hyperbolic functions.

2L

y

x zCh. 2 in

Applicationsof

Calculus II

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What are we talking about?

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What are we talking about?

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What are we talking about?

cosh

sinh

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What are we talking about?

weird…but handy in physics!

cosh

sinh

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Recall: Euler’s formula…

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Recall: Euler’s formula…

We need this today!

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Recall: Euler’s formula…

We need this today!

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Recall: Euler’s formula…

We need this today!

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How are they proportional?

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How are they proportional?

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What we are talking about

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What we are talking about

cos(kx), sin(kx)

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What we are talking about

cos(kx), sin(kx)

exp(kx), exp(-kx)

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What we are talking about

cos(kx), sin(kx)

cosh(kx), sinh(kx)

exp(kx), exp(-kx)

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What we are talking about

k = 2.7 for each

cos(kx), sin(kx)

cosh(kx), sinh(kx)

exp(kx), exp(-kx)

15

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What we are talking about

Each graphed over [-1, 2]

k = 2.7 for each

cos(kx), sin(kx)

cosh(kx), sinh(kx)

exp(kx), exp(-kx)

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Here we go. Let’s look at derivatives.

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Here we go. Let’s look at derivatives.

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Here we go. Let’s look at derivatives.

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Here we go. Let’s look at derivatives.

Let’s check sines, too!

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Here we go. Let’s look at derivatives.

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UCF EXCEL

Here we go. Let’s look at derivatives.

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UCF EXCEL

Here we go. Let’s look at derivatives.

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UCF EXCEL

Here we go. Let’s look at derivatives.

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Here we go. Let’s look at derivatives.

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Here we go. Let’s look at derivatives.

In general: after two diff’s you get back to same function… but with an extra factor of -ω2.

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General derivatives relationships here:

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General derivatives relationships here:

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General derivatives relationships here:

What do these two add up to?

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General derivatives relationships here:

0

What do these two add up to?

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We like that because…

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We like that because…

A. That kind of derivative relationship is needed in spring systems, e.g.,

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We like that because…

A. That kind of derivative relationship is needed in spring systems, e.g., Oscillators

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We like that because…

A. That kind of derivative relationship is needed in spring systems, e.g., Oscillators Vibrating systems

Simple seismometer

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We like that because…

A. That kind of derivative relationship is needed in spring systems, e.g., Oscillators Vibrating systems

B. F = -kx in springs

Simple seismometer

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We like that because…

A. That kind of derivative relationship is needed in spring systems, e.g., Oscillators Vibrating systems

B. F = -kx in springsC. F = ma…as always

Simple seismometer

20

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We like that because…

A. That kind of derivative relationship is needed in spring systems, e.g., Oscillators Vibrating systems

B. F = -kx in springsC. F = ma…as alwaysD. a = second deriv. of x!

Simple seismometer

20

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We like that because…

A. That kind of derivative relationship is needed in spring systems, e.g., Oscillators Vibrating systems

B. F = -kx in springsC. F = ma…as alwaysD. a = second deriv. of x!

Simple seismometer

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Brainiac iClicker question coming…

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Brainiac iClicker question coming…

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For this derivatives relationship, what will the ω2 factor be?

A. It comes out to be k/m.

And the temporal scale in ω depends upon the mass (m) of the object on the spring and on the strength (k) of the spring.

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Onward to radiation

in vacuum E” = 1

c2

d2

dt2 E

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Onward to radiation

A. The relationship for radiation involves the electric field (E) and magnetic field (B)in vacuum

E” = 1

c2

d2

dt2 E

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Onward to radiation

A. The relationship for radiation involves the electric field (E) and magnetic field (B)

B. They are coupledin vacuum

E” = 1

c2

d2

dt2 E

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Onward to radiation

A. The relationship for radiation involves the electric field (E) and magnetic field (B)

B. They are coupledC. In space-time

in vacuum E” = 1

c2

d2

dt2 E

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Onward to radiation

A. The relationship for radiation involves the electric field (E) and magnetic field (B)

B. They are coupledC. In space-timeD. With second

derivative in space and in time.

in vacuum E” = 1

c2

d2

dt2 E

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Onward to radiation

A. The relationship for radiation involves the electric field (E) and magnetic field (B)

B. They are coupledC. In space-timeD. With second

derivative in space and in time.

E. Wiggles that move

in vacuum E” = 1

c2

d2

dt2 E

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Spacetime implications

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Spacetime implications

6. Sines and cosines of time and space

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Spacetime implications

6. Sines and cosines of time and space

7. Sin(kx ± ωt)

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Spacetime implications

6. Sines and cosines of time and space

7. Sin(kx ± ωt)8. Cos(kx ± ωt)

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Spacetime implications

6. Sines and cosines of time and space

7. Sin(kx ± ωt)8. Cos(kx ± ωt)9. Kosher ω and k,

if…

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Spacetime implications

6. Sines and cosines of time and space

7. Sin(kx ± ωt)8. Cos(kx ± ωt)9. Kosher ω and k,

if…

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Spacetime implications

6. Sines and cosines of time and space

7. Sin(kx ± ωt)8. Cos(kx ± ωt)9. Kosher ω and k,

if…

d2

dt2 E = −ω2E

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Another brainiac question coming…

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Space-time dependence of radiation and its speed of propagation

Speed of light couples the temporal and spatial dependences…

a.k.a. frequency and wavelength!

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What is this physical relationship to c?

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What is this physical relationship to c?

A. Dispersion relation (fancy terminology)

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What is this physical relationship to c?

A. Dispersion relation (fancy terminology)

B. Refraction of light (transmission)

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What is this physical relationship to c?

A. Dispersion relation (fancy terminology)

B. Refraction of light (transmission) E.g., prisms disperse

the colors of sunlight

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What is this physical relationship to c?

A. Dispersion relation (fancy terminology)

B. Refraction of light (transmission) E.g., prisms disperse

the colors of sunlightC. Absorption of light

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What is this physical relationship to c?

A. Dispersion relation (fancy terminology)

B. Refraction of light (transmission) E.g., prisms disperse

the colors of sunlightC. Absorption of light

E.g., Superman, lead absorbs xrays.

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Penetrating a material with radiation

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Penetrating a material with radiation

A. Inside material, the physics changes.

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Penetrating a material with radiation

A. Inside material, the physics changes.B. Light moves more slowly.

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Penetrating a material with radiation

A. Inside material, the physics changes.B. Light moves more slowly.C. Energy is absorbed from E and B.

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Penetrating a material with radiation

A. Inside material, the physics changes.B. Light moves more slowly.C. Energy is absorbed from E and B.D. Heat flows, outer surfaces cool off

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Penetrating a material with radiation

A. Inside material, the physics changes.B. Light moves more slowly.C. Energy is absorbed from E and B.D. Heat flows, outer surfaces cool offE. New spatial and temporal derivatives

for E and B fields.

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UCF EXCEL

Penetrating a material with radiation

A. Inside material, the physics changes.B. Light moves more slowly.C. Energy is absorbed from E and B.D. Heat flows, outer surfaces cool offE. New spatial and temporal derivatives

for E and B fields.» sine, cosine = NO GO!

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Now a new derivatives relation must hold.

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Now a new derivatives relation must hold.

F. The old derivatives relationship changes, i.e.., for Ez...

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Now a new derivatives relation must hold.

F. The old derivatives relationship changes, i.e.., for Ez...

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Now a new derivatives relation must hold.

F. The old derivatives relationship changes, i.e.., for Ez...

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Now a new derivatives relation must hold.

F. The old derivatives relationship changes, i.e.., for Ez...

G. New deriv. rel. means new functions do the work.

H. Hyperbolic functions, cosh(u) and sinh(u).

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Next Monday:

A. Radiation penetrating “cheese”

B. Quantum tunnelingC. Space-time structure

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