Physics SL
Physics SL
5
Chapters
329
Notes
Theme A - Space, Time & Motion
Theme A - Space, Time & Motion
Theme B - The Particulate Nature Of Matter
Theme B - The Particulate Nature Of Matter
Theme C - Wave Behaviour
Theme C - Wave Behaviour
Theme D - Fields
Theme D - Fields
Theme E - Nuclear & Quantum Physics
Theme E - Nuclear & Quantum Physics
IB Resources
Theme E - Nuclear & Quantum Physics
Physics SL
Physics SL

Theme E - Nuclear & Quantum Physics

Unlocking the Secrets: Bohr Model & Spectra Insights

Word Count Emoji
697 words
Reading Time Emoji
4 mins read
Updated at Emoji
Last edited on 5th Nov 2024

Table of content

The Bohr Model & Emission Spectra

  • The Lyman series involves transitions where an atom moves to its ground state.

  • Balmer and Paschen series: Transitions to n=2 and n=3 states.

  • Brackett series: Transitions to n=4 from higher states.

Real-world example: Imagine an elevator. Each floor is a different energy level (n). The elevator moving between floors is like electrons transitioning between energy levels. The elevator stopping at ground floor? That's the Lyman series!

Linking Bohr with Empirical Work

  • Bohr model links with Rydberg & Balmer formulas.

  • Derived equation for energy of an electron in nth energy level
  • E = \(\frac{ -13.6}{n^2}\) eV

Fun Fact: Think of the Bohr model as a puzzle. Each piece (or equation) connects with another, building a bigger picture of the atomic world!

Angular Momentum in Bohr Model

  • Angular momentum = moment of inertia × angular speed 

  • For a particle in orbit: L = mvr [where v = rω]

For Teens: It's like spinning a ball on a string. The speed of the spin and the length of the string determine its angular momentum.

The De Broglie Wavelength

  • Every particle has wave-like properties.

  • De Broglie wavelength (λ) relates to momentum (p) of a particle: λ = \(\frac hp\)

Fun Analogy: Picture a skateboarder (particle) cruising along. The trails left behind are like the de Broglie wavelength!

Bohr's Assumption

  • Electron orbits must match an integer number of de Broglie wavelengths.

  • For n = 2, wavelength = \(\frac {circum ference}{2}; for n = 3, \frac {circum ference}{3},\) etc.

    Think:
    If you're looping a song, it should complete perfectly as you finish a lap around a track!

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IB Resources
Theme E - Nuclear & Quantum Physics
Physics SL
Physics SL

Theme E - Nuclear & Quantum Physics

Unlocking the Secrets: Bohr Model & Spectra Insights

Word Count Emoji
697 words
Reading Time Emoji
4 mins read
Updated at Emoji
Last edited on 5th Nov 2024

Table of content

The Bohr Model & Emission Spectra

  • The Lyman series involves transitions where an atom moves to its ground state.

  • Balmer and Paschen series: Transitions to n=2 and n=3 states.

  • Brackett series: Transitions to n=4 from higher states.

Real-world example: Imagine an elevator. Each floor is a different energy level (n). The elevator moving between floors is like electrons transitioning between energy levels. The elevator stopping at ground floor? That's the Lyman series!

Linking Bohr with Empirical Work

  • Bohr model links with Rydberg & Balmer formulas.

  • Derived equation for energy of an electron in nth energy level
  • E = \(\frac{ -13.6}{n^2}\) eV

Fun Fact: Think of the Bohr model as a puzzle. Each piece (or equation) connects with another, building a bigger picture of the atomic world!

Angular Momentum in Bohr Model

  • Angular momentum = moment of inertia × angular speed 

  • For a particle in orbit: L = mvr [where v = rω]

For Teens: It's like spinning a ball on a string. The speed of the spin and the length of the string determine its angular momentum.

The De Broglie Wavelength

  • Every particle has wave-like properties.

  • De Broglie wavelength (λ) relates to momentum (p) of a particle: λ = \(\frac hp\)

Fun Analogy: Picture a skateboarder (particle) cruising along. The trails left behind are like the de Broglie wavelength!

Bohr's Assumption

  • Electron orbits must match an integer number of de Broglie wavelengths.

  • For n = 2, wavelength = \(\frac {circum ference}{2}; for n = 3, \frac {circum ference}{3},\) etc.

    Think:
    If you're looping a song, it should complete perfectly as you finish a lap around a track!

Unlock the Full Content! File Is Locked Emoji

Dive deeper and gain exclusive access to premium files of Physics SL. Subscribe now and get closer to that 45 🌟

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