Energy Levels & Photon Emission

Test yourself

Energy Levels in Atoms

Electrons in atoms must occupy a discrete energy level.

Energy levels

Electrons do not float around randomly in atoms.
They can only be found at set energy levels.
Each energy level is given a 'quantum number'.
The ground state is the lowest energy level. The ground state has n = 1.
The higher the energy level, the larger its quantum number, n.

Transitions between energy levels

An electron can transition between energy levels by absorbing or emitting a photon of a specific frequency.
If an electron emits a photon, it will drop in energy level.
If an electron absorbs a photon, it will rise to a higher level.
- In both cases, the photon must have energy exactly equal to the energy difference between the levels.

Equation

The movement of electrons between energy levels can be represented in the equation:
- $\Delta E = E_1 - E_2 = hf = \frac{hc}{\lambda}$
This shows that the energy difference between levels one and two is equal to the energy of the emitted (or absorbed) photon.

Excitation and ionisation

If an electron absorbs a photon and jumps up an energy level, we say it has been excited.
If an electron absorbs a photon that is so energetic it is knocked out of the atom altogether, the electron has been ionised.

Absorption Spectra

Electrons in atoms can only move between discrete energy levels. So an atom can only absorb or emit photons with particular frequencies (or wavelengths).

White light - continuous spectrum

White light contains all the colours in the visible part of the spectrum.
When white light is passed through a prism or a diffraction grating, the colours are split up to produce a continuous spectrum.
Continuous means there aren't any gaps or black lines.

Cool gas - absorption spectra

A cool gas means a gas containing atoms in their ground state.
When white light is passed through a cool gas, electrons in the ground state of the atom absorb certain frequencies of light and become excited.
Most frequencies of the white light are not absorbed because they do not correspond to the difference between two energy levels in the atom.

Absorption spectra 2

If the light coming out of the cool gas is split by a prism (or diffraction grating), we see a continuous spectrum with black lines.
- These lines are called absorption lines.
- They are unique to each type of atom.

Emission Spectra

Electrons in atoms can only move between discrete energy levels. So an atom can only absorb or emit photons with particular frequencies (or wavelengths).

Excited gas

An excited gas contains atoms in excited energy states.
These excited atoms contain electrons in high energy levels.
As these electrons de-excite and fall back to lower energy levels, photons are emitted.

Photon emission

These photons carry away energy from the atoms.
The amount of energy (and so what frequency) the photons have depends on the difference in energy levels in the atom.
- For every possible electron transition, there will be a unique frequency photon emitted.
We see a series of bright lines when we pass the emitted light through a prism or diffraction grating.

Emission vs absorption

Compare the emission and absorption spectra produced by this gas.
We can see that the emission lines exactly match the frequencies of the absorption lines.
This is because the lines correspond to the same energy differences in the atoms. The same energy photons are either emitted or absorbed.

1Physical Quantities & Units

1.1Physical Quantities & Units

1.1.1Use of SI Units

1.1.2SI Prefixes, Standard Form & Converting Units

1.1.3End of Topic Test - Units & Prefixes

1.1.4Avogadro's Constant

1.1.5Scalars & Vectors

2Measurement Techniques

2.1Measurement, Errors & Uncertainty

2.1.1Measuring Length, Time & Volume

2.1.2Measuring Temperature

2.1.3Circuit Measurements

2.1.4Limitation of Physical Measurements

2.1.5Uncertainty

2.1.6Estimation

2.1.7Displaying Data

2.1.8End of Topic Test - Measurements & Errors

3Kinematics

3.1Equations of Motion

3.1.1Motion in a Straight Line

3.1.2Graphs of Motion

3.1.3Bouncing Ball Example

3.1.4End of Topic Test - Motion in a Straight Line

3.1.5Acceleration Due to Gravity

4Dynamics

4.1Momentum & Newton's Laws of Motion

4.1.1Mass & Inertia

4.1.2Newton's Laws

4.1.3Momentum

4.1.4End of Topic Test - Newton's Laws & Momentum

4.1.5A-A* (AO3/4) - Newton's Third Law

4.2Non-Uniform Motion

4.2.1Projectile Motion

4.3Linear Momentum & Conservation

4.3.1Conservation of Momentum

4.4Force, Density & Pressure

4.4.1Fields

4.4.2Force in Uniform Fields

4.4.3Friction

4.4.4Buoyancy

4.4.5Terminal Speed

4.4.6End of Topic Test - Acceleration Due to Gravity

4.4.7Centre of Mass

4.4.8Forces & Equilibrium

4.4.9End of Topic Test - Scalars & Vectors

4.4.10Moments

4.4.11End of Topic Test - Moments & Centre of Mass

4.4.12Density

4.4.13Pressure

4.5Work, Energy & Power

4.5.1Work & Energy

4.5.2Power & Efficiency

4.5.3Conservation of Energy

4.5.4End of Topic Test - Work, Energy & Power

4.6Circular Motion

4.6.1Circular Motion

4.6.2Circular Motion 2

4.6.3End of Topic Test - Circular Motion

5Gravitational Fields

5.1Gravitational Fields (A2 only)

5.1.1Newton's Law

5.1.2Gravitational Field Strength

5.1.3Gravitational Potential

6Deformation of Solids

6.1Materials

6.1.1Bulk Properties of Solids

6.1.2Energy in Materials

6.1.3Young Modulus

6.1.4End of Topic Test - Materials

7Thermal Physics

7.1Thermal Physics

7.1.1Temperature

7.1.2Measuring Temperature

7.1.3Ideal Gas Law

7.1.4Ideal Gases

7.1.5Boyle's Law & Charles' Law

7.1.6Molecular Kinetic Theory Model

7.1.7Molecular Kinetic Theory Model 2

7.1.8Thermal Energy Transfer

7.1.9Thermal Energy Transfer Experiments

7.1.10End of Topic Test - Thermal Energy & Ideal Gases

7.1.11First Law of Thermodynamics

8Oscillations

8.1Simple Harmonic Motion

8.1.1Simple Harmonic Motion

8.1.2Simple Harmonic Systems

8.1.3Energy in Simple Harmonic Motion

8.1.4Resonance

8.1.5End of Topic Test - Simple Harmonic Motion

8.1.6A-A* (AO3/4) - Simple Harmonic Motion

8.1.7End of Topic Test - Gravitational Fields

8.2Waves

8.2.1Progressive Waves

8.2.2Intensity of Waves

8.2.3Wave Speed & Phase Difference

8.2.4Longitudinal & Transverse Waves

8.2.5End of Topic Test - Progressive Waves

8.2.6Electromagnetic Waves

8.2.7Doppler Effect

8.2.8Sound Waves

8.2.9Measuring Sound Waves

8.2.10End of Topic Test - Waves

8.2.11Ultrasound Imaging

8.2.12Ultrasound Imaging 2

8.3Superposition

8.3.1Stationary Waves

8.3.2Stationary Waves 2

8.3.3End of Topic Test - Stationary Waves

8.3.4A-A* (AO3/4) - Stationary Waves

8.3.5Interference

8.3.6Interference 2

8.3.7End of Topic Test - Interference

8.3.8Diffraction

8.3.9Diffraction Gratings

8.3.10End of Topic Test - Diffraction

9Communication

9.1Communication Channels

9.1.1Communication Channels

9.1.2Modulation

9.1.3Attenuation

9.2Digital Communication

9.2.1Digital & Analogue Signals

9.2.2Representing Sound

10Electric Fields

10.1Electric Fields

10.1.1Coulomb's Law

10.1.2Electric Field Strength

10.1.3Electric Field Strength 2

10.1.4Electric Potential

10.1.5End of Topic Test - Electric Fields

10.1.6A-A* (AO3/4) - Electric and Gravitational Field

10.2Capacitance

10.2.1Capacitance

10.2.2Parallel Plate Capacitor

10.2.3Energy Stored by a Capacitor

10.2.4Capacitor Discharge

10.2.5Capacitor Charge

11Current Electricity

11.1Current Electricity

11.1.1Basics of Electricity

11.1.2Mean Drift Velocity

11.1.3Current-Voltage Characteristics

11.1.4End of Topic Test - Basics of Electricity

11.1.5Resistivity

11.1.6End of Topic Test - Resistivity & Superconductors

11.1.7Power and Conservation

11.1.8Microphones

11.1.9Components

11.1.10Relays

11.1.11Strain Gauges

11.2DC Circuits

11.2.1Circuits

11.2.2Potential Divider

11.2.3Emf & Internal Resistance

11.2.4End of Topic Test - Power & Potential

12Magnetic Fields

12.1Magnetic Fields

12.1.1Magnetic Flux Density

12.1.2End of Topic Test - Capacitance & Flux Density

12.1.3Moving Charges in a Magnetic Field

12.1.4Magnetic Flux & Flux Linkage

12.1.5Electromagnetic Induction

12.1.6Electromagnetic Induction 2

12.1.7Magnetic Flux Density

12.1.8Magnetic Resonance Scanning

12.2Alternating Currents

12.2.1Alternating Currents

12.2.2Operation of a Transformer

12.2.3End of Topic Test - Electromagnetic Induction & AC

12.2.4Rectification

13Modern Physics

13.1Quantum Physics

13.1.1The Photoelectric Effect

13.1.2The Photoelectric Effect Explanation

13.1.3End of Topic Test - The Photoelectric Effect

13.1.4Collisions of Electrons with Atoms

13.1.5Energy Levels & Photon Emission

13.1.6Wave-Particle Duality

13.1.7End of Topic Test - Absorption & Emission

13.1.8Band Theory

13.1.9Diagnostic X-Rays

13.1.10X-Ray Image Processing

13.1.11Absorption of X-Rays

13.1.12CT Scanners

13.2Nuclear Physics

13.2.1Rutherford Scattering

13.2.2Atomic Model

13.2.3Isotopes

13.2.4Stable & Unstable Nuclei

13.2.5A-A* (AO3/4) - Stable & Unstable Nuclei

13.2.6Alpha & Beta Radiation

13.2.7Gamma Radiation

13.2.8Particles, Antiparticles & Photons

13.2.9Quarks & Antiquarks

13.2.10Particle Interactions

13.2.11Radioactive Decay

13.2.12Half Life

13.2.13End of Topic Test - Radioactivity

13.2.14Nuclear Instability

13.2.15Mass & Energy

13.2.16Binding Energy

13.2.17A-A* (AO3/4) - Nuclear Fusion

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