To Teach a Monkey (beta)

Photons

Photon

A particle representing a quantum of light.

Quantum

Smallest discrete amount of something.

Discrete

An individually separate and distinct thing. Not made of anything else.

Wave-Particle Duality

Photons exhibit wave properties under refraction and interference.

Photons exhibit particle properties under emission or absorption.

Photon Energy

E=hf=hcλE = hf = \frac{hc}{\lambda}

Where h is Planck's constant, c is the speed of light, and λ is its wavelength.

The Photoelectric Effect

Threshold Frequency

The minimum frequency for the emission of electrons due to incident radiation.

Work Function

The minimum quantity of energy required to remove an electron from a solid.

Stopping Potential

The minimum negative voltage applied to the anode to stop the photocurrent, representing the maximum kinetic energy of the electron.

Φ=hf0\Phi = hf_0, where f0f_0 is the threshold frequency.

Total energy: hf=Φ+Ekhf = \Phi + E_k

Threshold wavelength: λc=hcΦ\lambda_c = \frac{hc}{\Phi}

Matter Waves

De Broglie proposed that all matter has wave-like properties.

Momentum-wavelength relation: p=hλp = \frac{h}{\lambda}

Bohr Model

Electrons orbit the nucleus in discrete paths with quantized angular momentum.

Nuclear radius: R=R0A13R = R_0 A^{\frac{1}{3}}

Energy levels: En=RH(1n2)E_n = -R_H \left(\frac{1}{n^2}\right)

Angular momentum: mvr=nh2πmvr = \frac{nh}{2\pi}

Energy of an electron in orbit: E=(13.6n2)eVE = -\left(\frac{13.6}{n^2}\right) eV

Rutherford Scattering

Rutherford's students shot alpha particles at gold foil.

The Plum Pudding Model predicted uniform density, meaning no deflection, but scattering was observed, proving the nuclear model of the atom.

Nuclear Energy Levels

The nucleus moves between discrete energy levels, often emitting gamma rays corresponding to distinct energy transitions.

Absorption and Emission Spectra

Electrons moving down in energy levels emit photons, forming an emission spectrum.

Absorption spectra show wavelengths absorbed as electrons move up energy levels.

Compton Scattering

Arthur Compton observed an increase in photon wavelength after colliding with an electron, leading to a wavelength shift formula:

Δλ=hmec(1cosθ)\Delta \lambda = \frac{h}{m_e c} (1 - \cos \theta)

The energy used to accelerate electrons equals their kinetic energy.

λ=h2mqV\lambda = \frac{h}{\sqrt{2mqV}}