WEBVTT

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Why should energy ever
come in separate amounts?

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I do not want to begin
by declaring that it does.

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Let us begin with a familiar
object instead: a stretched string,

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fixed at both ends, and the waves
that can actually live on it.

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The string runs from zero to L.

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Each end is clamped,

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so neither endpoint can move, however
strongly the rest of the string vibrates.

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That physical fact
becomes a boundary condition.

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The displacement y must be zero
at the left wall and zero again

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at the right wall.

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Try an arbitrary sinusoidal candidate.

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It begins correctly at zero,
but look at its right end.

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The curve reaches the wall above the fixed
point, so this shape cannot be a standing

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wave of this string.

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The simplest accepted shape places
one half-wave between the walls.

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Both endpoints are nodes, and the entire
string rises and falls as one arch.

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The next shape fits two half-waves.

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It still vanishes at both walls, and it
gains another node exactly in the middle.

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A third shape fits three half-waves.

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Two interior nodes divide the string
into three vibrating sections,

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with neighboring sections
moving in opposite directions.

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We can continue forever,
but not continuously.

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The length L must contain a whole
number n of half-wavelengths.

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Solving for wavelength gives
lambda n equals two L over n.

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The allowed wavelengths form a list:
two L, L, two L over three, and so on.

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The same statement
can be written using wave number k.

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Only n pi over L is allowed, with n
equal to one, two, three, and onward.

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The important word is allowed.

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The material string
could have many amplitudes,

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but its spatial patterns
are selected by the two boundaries.

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Continuous guesses went in;
a discrete family came out.

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Now replace the string

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by a particle trapped between
two perfectly impenetrable walls.

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Quantum mechanics describes
its state with a wavefunction, psi.

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What survives from the string argument?

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Here is the region
available to the particle.

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Outside the two walls the particle cannot
exist, so the wavefunction is zero there.

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At an ideal infinite wall,

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the wavefunction must meet
that outside value continuously.

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Therefore psi is zero at x
equals zero and again at x equals L.

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The first allowed
state is one smooth arch.

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This is not a little
particle following the curve.

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The curve is the wavefunction
that will determine probabilities.

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The second state has two
lobes and one interior zero.

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The third has three lobes
and two interior zeros.

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They are the same spatial fitting
patterns we met on the string.

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Write a sinusoidal candidate A sine k x.

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The left boundary is already
satisfied because sine zero is zero.

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At the right wall, x becomes L.

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The amplitude there is A sine k L, and the
wall requires that expression to vanish.

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Sine vanishes at whole multiples of pi.

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So k L must equal n pi,
not an arbitrary number.

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Dividing by L gives
the allowed wave numbers.

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Once again the boundaries
have turned a continuous range

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of guesses into a numbered list.

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A fitting rule selects wave numbers.

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To find energies,

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we now use the stationary
Schrödinger equation inside the box.

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Its left side measures
the curvature of the wavefunction.

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The coefficient h squared over eight pi
squared m is the familiar h bar squared

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over two m, written
using Planck's constant h.

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The right side is energy
times the same wavefunction.

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Differentiate sine twice and the
original wave returns with a factor

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of minus k squared.

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Substitute that curvature
into the equation.

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The common wavefunction cancels,

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leaving E equal to h squared k
squared over eight pi squared m.

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Finally substitute the allowed k values.

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The energy of state n is n squared
h squared over eight m L squared.

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That is where quantised energy enters.

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The equation relates energy to wavelength,

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while the walls permit
only certain wavelengths.

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The discrete energies are the
consequence of both facts together.

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The energy formula contains
a powerful prediction.

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Keep the particle and its mass unchanged,
but make the confining region wider.

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Beside the box
are its first three energies.

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They are separate horizontal lines,
and even the lowest state sits above zero.

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That nonzero ground-state
energy is unavoidable.

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A wave trapped in a finite
region cannot be perfectly flat,

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so it cannot have zero
curvature and zero kinetic energy.

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The difference between
neighboring levels is delta E n.

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Start with E n plus one minus E n.

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Insert the box energies.

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The numerator contains n plus
one squared minus n squared,

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while every level carries
the same factor one over L squared.

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The difference
of the squares is two n plus one.

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So the gap is also proportional
to one over L squared.

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Now widen the box.

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Watch both walls move apart

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while the three energy levels
descend and crowd together.

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Nothing has changed
about the integer labels.

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The allowed states are still
numbered one, two, three, and onward.

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What changed is the energy
scale attached to that list.

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A very wide box therefore has many
levels inside any modest energy interval.

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The spectrum is discrete in principle,

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but the gaps may become too small
for an experiment to distinguish.

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This is one route back
toward classical physics.

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First, increasing L lowers the entire
spectrum and shrinks every gap as one

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over L squared.

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There is a second effect
at high quantum number.

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Divide a gap by the energy
itself, and most constants cancel.

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The relative gap is two n plus one over n
squared, which approaches two over n.

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At large n, neighboring states differ
by a tiny fraction of their total energy.

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Finally, every real
measurement has limited resolution.

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If thousands of allowed energies fall
inside one unresolved band, changing

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energy appears continuous even though
the microscopic list remains discrete.

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The classical world does not require
the quantum rules to switch off.

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Large dimensions, high quantum numbers,

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and limited resolution make
the steps too fine to notice.

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A wavefunction is not
itself a probability.

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It can be positive,
negative, or even complex.

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What predicts where the particle
may be detected is its absolute square.

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Here is the second state.

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Its left lobe is positive

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and its right lobe is negative, but
a probability density cannot be negative.

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Square the amplitude at every position.

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Both lobes rise above the axis, producing
two regions where detection is likely.

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The total shaded area
is one after normalization.

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That does not say
the particle has a known position.

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It says some detection somewhere
in the box has total probability one.

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At the middle,
the wavefunction is exactly zero.

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Squaring zero still gives zero, so the
particle is never detected at this node.

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Now compare the first
three stationary states.

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The first density has one
broad peak and no internal node.

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The probability still
vanishes at both walls.

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Those zeros come from the confinement
condition shared by every state.

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The second density has two peaks. Between
them is one internal node at L over two,

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a position with exactly zero probability.

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The third density has three
peaks and two internal nodes,

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at L over three and two L over three.

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A node is stronger than
a low-probability region.

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At a node the wavefunction
vanishes exactly, so an ideal position

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measurement never returns that point
while the particle remains in that state.

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The pattern is systematic.

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State n has n lobes in its density
and n minus one internal nodes.

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Higher states oscillate more rapidly

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because their allowed
wavelengths are shorter.

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More oscillations produce more exact
cancellations and therefore more nodes.

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These densities also warn

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us against imagining a classical
bead bouncing between the walls.

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A classical bead can pass
through every interior position.

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A stationary quantum state can forbid
particular positions completely.

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The allowed energy tells us
which stationary pattern we have.

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The square of that pattern tells
us where detections can occur,

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and its nodes mark where they cannot.

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A toy model earns its keep only
if it explains something real.

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Consider a conjugated dye molecule,

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built from a chain of neighboring
atoms with overlapping p orbitals.

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The green skeleton marks the chain,

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while the blue region represents
the shared pi-electron system.

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These electrons are not
assigned to one particular bond;

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they are delocalised
along much of the chain.

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That finite delocalised length acts,
approximately, like a one-dimensional box.

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The detailed molecular
potential is not perfectly square,

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but the familiar expression
makes the dependence clear:

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every energy contains one over L squared.

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So the molecular orbitals form
a numbered set of wave-like states.

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Their exact shapes are more
complicated than sines,

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but confinement still
produces separated energies.

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Electrons now fill the allowed
levels from the bottom upward.

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Each spatial level can hold two
electrons with opposite spin.

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If the conjugated system has N
pi electrons and N is even,

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the highest filled level
has index n equal to N over two.

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The next level is empty.

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Absorbing light can lift an electron
across this frontier gap from level n

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to level n plus one.

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Begin with the difference
E n plus one minus E n.

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Insert the particle-in-a-box energies.

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The two levels differ only
in their squared quantum numbers.

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Simplifying gives a gap proportional
to two n plus one divided by L squared.

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A photon is absorbed
when its energy matches that gap.

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Delta E equals h f,
or h c over wavelength.

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Solving for wavelength
makes the trend explicit.

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A smaller energy gap corresponds
to a longer absorbed wavelength.

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Compare two related conjugated systems.

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The shorter chain confines
its pi electrons more tightly,

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so the frontier levels
stand farther apart.

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The longer chain spreads the
wavefunctions across a greater distance.

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Its relevant levels are closer together,

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so the transition needs
a lower-energy photon.

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Lower photon energy
means longer wavelength.

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As conjugation is extended
through a family of dyes,

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the absorption band commonly shifts
toward longer visible wavelengths.

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A dye looks coloured

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because it absorbs some visible
wavelengths more strongly than others.

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The colour we observe
comes from the light left

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over or transmitted, so it is not
simply the colour of the absorbed photon.

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Now the complete chain
of reasoning fits together.

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First, finite boundaries
select standing-wave states.

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Second, electrons fill those states,

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leaving a particular gap between the
highest filled and lowest empty levels.

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Third, light is absorbed
when a photon matches that gap.

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Extending the conjugated region generally
reduces the gap and moves the absorption

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toward longer wavelength.

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Finally, this remains a model.

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Real molecules have non-square
potentials, electron interactions,

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vibrations, and environmental effects.

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Detailed spectra require more
complete quantum chemistry.

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But the model has earned its keep.

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Fixed ends selected wavelengths;

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confined wavefunctions selected energies;

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molecular length
controlled an optical gap.

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Energy is quantised because a bounded
wave cannot fit in arbitrary ways.