2.3.11Modern Physics

Quantum tunneling — concept, transmission coefficient

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WHAT is tunneling?

WHY it happens: A particle is described by a wavefunction ψ(x)\psi(x). Schrödinger's equation forces ψ\psi and its slope ψ\psi' to be continuous everywhere. Inside a barrier where E<V0E<V_0, ψ\psi cannot oscillate — but it also cannot vanish abruptly. The only continuous, normalizable behaviour left is an exponential decay. Decay ≠ zero, so some amplitude reaches the other side.


HOW to derive the transmission coefficient

Setup: a particle of energy EE hits a rectangular barrier of height V0V_0 and width LL (0<x<L0<x<L), with E<V0E<V_0.

Step 1 — Write Schrödinger's equation in each region

Time-independent Schrödinger equation: 22md2ψdx2+V(x)ψ=Eψ-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2} + V(x)\psi = E\psi

Why? This is the energy eigenvalue equation; solving it gives the spatial shape of the matter wave.

Region I (x<0x<0, V=0V=0): ψ=2mE2ψk2ψ,k=2mE\psi'' = -\frac{2mE}{\hbar^2}\psi \equiv -k^2\psi,\qquad k=\frac{\sqrt{2mE}}{\hbar} Solution: ψI=Aeikx+Beikx\psi_I = A e^{ikx} + B e^{-ikx} (incoming + reflected waves).

Region II (0<x<L0<x<L, V=V0V=V_0): ψ=+2m(V0E)2ψ+κ2ψ,κ=2m(V0E)\psi'' = +\frac{2m(V_0-E)}{\hbar^2}\psi \equiv +\kappa^2\psi,\qquad \kappa=\frac{\sqrt{2m(V_0-E)}}{\hbar} Why a +sign? Because V0>EV_0>E, the bracket is positive, so the equation gives real exponentials, not oscillations: ψII=Ceκx+De+κx\psi_{II} = C e^{-\kappa x} + D e^{+\kappa x}

Region III (x>Lx>L, V=0V=0): ψIII=Feikx\psi_{III} = F e^{ikx} Why only e+ikxe^{+ikx}? Nothing comes back from ++\infty; only a transmitted wave moves rightward.

Step 2 — Define transmission

Transmission coefficient = (transmitted probability flux)/(incident flux). Since kk is the same on both sides: T=F2A2T = \frac{|F|^2}{|A|^2}

Step 3 — Apply boundary conditions

Continuity of ψ\psi and ψ\psi' at x=0x=0 and x=Lx=L gives four equations. Solving (algebra) yields the exact result:

Step 4 — The useful thick/high-barrier limit

When κL1\kappa L \gg 1, sinh(κL)12eκL\sinh(\kappa L)\approx \tfrac12 e^{\kappa L}, so sinh214e2κL\sinh^2 \approx \tfrac14 e^{2\kappa L}, dominating the "1": T16E(V0E)V02e2κLT \approx \frac{16E(V_0-E)}{V_0^2}\, e^{-2\kappa L}


Figure — Quantum tunneling — concept, transmission coefficient

Worked Examples


Common Mistakes (Steel-manned)


Recall Feynman: explain to a 12-year-old

Imagine throwing a tennis ball at a wall. Normally it bounces back. But picture the ball as a fuzzy cloud instead of a hard dot. When the cloud hits the wall, most of it bounces, but a tiny faint bit of the fog seeps through the wall and reappears faintly on the other side. If the wall is thin, a little fog gets across — and once in a while the ball is found there! Thin walls and light balls = more leaking. That seepage is tunneling.


Recall Active-recall checklist
  • Why is ψ\psi exponential (not oscillatory) inside the barrier?
  • What is κ\kappa and what controls it?
  • Where does the factor of 2 in e2κLe^{-2\kappa L} come from?
  • Does the emerging particle have more energy? Less? Same?

Flashcards

What is quantum tunneling?
A particle passing through a barrier with V0>EV_0>E, impossible classically, allowed because ψ\psi is continuous and nonzero (exponentially decaying) inside the forbidden region.
Why is ψ\psi exponential inside the barrier?
Because V0>EV_0>E makes Schrödinger's equation read ψ=+κ2ψ\psi''=+\kappa^2\psi, whose real solutions are e±κxe^{\pm\kappa x}, not oscillations.
Define the decay constant κ\kappa.
κ=2m(V0E)/\kappa=\sqrt{2m(V_0-E)}/\hbar, the rate at which ψ\psi decays inside the barrier.
Approximate transmission coefficient?
TGe2κLT\approx G\,e^{-2\kappa L} with G=16E(V0E)/V02G=16E(V_0-E)/V_0^2.
Exact transmission coefficient?
T=[1+V02sinh2(κL)4E(V0E)]1T=\left[1+\frac{V_0^2\sinh^2(\kappa L)}{4E(V_0-E)}\right]^{-1}.
Why the factor of 2 in e2κLe^{-2\kappa L}?
Amplitude decays as eκLe^{-\kappa L}; probability ψ2\propto|\psi|^2 squares it to e2κLe^{-2\kappa L}.
Does a tunneling particle gain energy?
No — it emerges with the same energy E<V0E<V_0; energy is conserved.
How does TT depend on mass?
Through κm\kappa\propto\sqrt{m}; heavier particles tunnel exponentially less, so macroscopic objects effectively never tunnel.
Real application of tunneling?
Scanning Tunneling Microscope (STM), alpha decay, tunnel diodes, flash memory.

Connections

  • Schrödinger Equation — source of the decaying solution
  • Wavefunction and Boundary Conditions — continuity gives the BCs used
  • Alpha Decay — Gamow's tunneling of α\alpha particles out of nuclei
  • Scanning Tunneling Microscope — exponential T(L)T(L) → atomic resolution
  • Potential Barrier and ReflectionR=1TR=1-T
  • de Broglie Wavelengthk=2mE/k=\sqrt{2mE}/\hbar links wave number to energy

Concept Map

resolved by

must be

forces

amplitude survives

solved per region

Region II real exponential

match at boundaries

four equations solved

defined as

thick barrier limit kappa L large

quantifies

decay rate

appears in

Classically forbidden barrier E less than V0

Wavefunction psi

Continuous psi and slope

Exponential decay inside barrier

Quantum tunneling

Schrodinger equation

Regions I II III

Boundary conditions psi and slope

Exact T formula

T equals F squared over A squared

T approx 16 E times V0-E over V0 squared times exp -2 kappa L

kappa equals sqrt 2m V0-E over hbar

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, classical physics kehti hai ki agar particle ke paas barrier se kam energy hai (E<V0E<V_0), to wo kabhi paar nahi kar sakta — wapas bounce ho jayega. Lekin quantum world mein particle ek wavefunction ψ\psi hai, aur Schrödinger equation force karti hai ki ψ\psi aur uska slope har jagah continuous ho. Barrier ke andar, kyunki V0>EV_0>E, ψ\psi oscillate nahi karta — wo exponentially decay karta hai (eκxe^{-\kappa x}). Decay ka matlab zero nahi hota! Thoda sa amplitude doosri side tak pohanch jata hai. Yahi tunneling hai.

Transmission coefficient TT batata hai ki kitni probability se particle paar hota hai. Mota/important result hai TGe2κLT \approx G\,e^{-2\kappa L}, jahan κ=2m(V0E)/\kappa=\sqrt{2m(V_0-E)}/\hbar. Yaad rakho: TT exponential hai — yani barrier ki width LL thodi si badhao to TT bahut tezi se girta hai. Example mein dekha, LL double karne par TT ~170 guna kam ho gaya. Yeh sensitivity STM (Scanning Tunneling Microscope) ki super-resolution ka raaz hai.

Mass ka effect bhi samajh lo: κm\kappa\propto\sqrt{m}, to bhaari particle (jaise proton ya cricket ball) ka TT practically zero ho jata hai — isliye macroscopic cheezein kabhi tunnel nahi karti. Halki cheez jaise electron asaani se tunnel karti hai. Aur ek important baat: tunneling mein energy conserve hoti hai — particle jis energy se aata hai, usi energy se nikalta hai, koi energy "udhaar" nahi leta. Bas wavefunction ka magic hai.

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Connections