Understanding Pendulums and Light Scattering

Sep 19, 2024

Lecture Notes

Introduction

  • Lecture duration: 40 minutes, followed by a 15-20 minute Q&A session.
  • Book signing event after the lecture.

Physics of a Pendulum

  • Pendulum Description: Mass (m), Length (L).
  • Period of a Pendulum: Derived as ( T = 2\pi \sqrt{\frac{L}{g}} ).
    • ( g ) = gravitational acceleration (approximately 9.80 m/s² in Boston).
    • Period is independent of amplitude and mass of the bob.
  • Demonstration: Period calculated for L = 1m gives T = 2 seconds.
  • Measurement and Accuracy:
    • Pendulum mass: 15.5 kg.
    • Length: 5.21 meters (with 1% uncertainty).
    • Predicted period: 4.58 ± 0.02 seconds.
    • Challenges in measurement due to human reaction time.

Conservation of Energy

  • Potential Energy: ( mgh ) where ( h ) is height.
  • Kinetic Energy: ( \frac{1}{2}mv^2 ).
  • Energy Transfer: Total energy is conserved, converted between potential and kinetic.
  • Pendulum Conservation: Height at release equals height on return (no higher).

Demonstrations

  • Building Demolition: Use of potential energy converted to kinetic energy.
  • Personal Experiment: Demonstrated conservation of energy by standing in the path of a pendulum.

Rayleigh Scattering

  • White Light Composition: Contains all rainbow colors.
  • Rayleigh Scattering: Blue light scattered more than red.
    • Scattering proportional to ( \frac{1}{\lambda^4} ).
    • Blue light wavelength ~1.5x lower than red.
  • Demonstrations: Cigarette smoke and lung experiment.
    • Blue light scatters from smoke; white light scatters from larger particles.

Blue Sky and Red Sunset

  • Rayleigh Scattering Explanation: Sky appears blue due to scattering of blue light by small particles in the atmosphere.
  • Sunset and Sunrise: Red due to longer path through the atmosphere, scattering out shorter wavelengths.
  • Demonstration: Use of sodium thiosulfate and sulfuric acid to simulate blue sky and red sunset in the lecture hall.

End of Lecture and Q&A

  • Questions and Interactions: Engaged audience with questions on pi, personal experiences, and career inspirations.
  • Advice to Students: Passion in physics is essential; bad experiences often due to poor teaching.

Book Signing

  • Instructions for signing: Use a paper with the name for personalization.

Key Takeaways

  • Physics principles demonstrated with practical examples.
  • Importance of understanding energy conservation and scattering phenomena.
  • Engaging teaching style with interactive elements and demonstrations.