1. Modern Physics: PHYS 344 Professor Michael Manfra Office: Physics 84 Phone: 494-3016 Email: mmanfra@purdue.edummanfra@purdue.edu Lecture schedule: MWF 2:30am to 3:20am in Physics 203 Office hours: Fridays, Physics 84 from 9:00am to 10:00am or appointments via email

2. Course description for PHYS344 Modern Physics will introduce you to some of the most amazing developments in our understanding of Nature that took place in the beginning of the 20 th century Principal among these: Relativity theory: fundamentally changed our understanding of the notions of space and time from those of Newtonian mechanics Quantum theory: a completely new way to understand the behavior of matter at small (atomic) length scales

3. Prerequisites PHYS 272H, or 241 Everyone should have completed a course in classical mechanics Everyone should have completed a course in electricity and magnetism It helps to know some thermodynamics too

4. Examinations and Grading A problem set will be given each week. Total points available for all problem sets (combined) 100 points There will be two exams given in class: tentative schedule: the 1 st on Friday Oct. 3 rd and the 2 nd on Friday Nov. 14 th. These exams will be graded on a 100 point scale. The final exam will occur during finals week at the normally scheduled time and will be graded on a 200 point scale. The final grade will be determined as follows: Average of problem sets: 100 points max Two in-class exams: 200 points max (total) Final exam: 200 points max Total: 500 points max

5. TA and graders TA: Nirajan Mandal Email: nmandal@purdue.edu Office: Physics 104 Graders: Yonggang Luo Email: ygluo@purdue.edu Office: Physics 133 Shih-Chieh Liu Email: liu998@purdue.edu Office: Physics 175

6. Bedtime reading Course required text: Modern Physics, Kenneth Krane, 3 rd Edition, Wiley & Sons You should start by reading by reading Chapter 1: Review of Classical Mechanics I will also be drawing on heavily on the lectures on Modern Physics by Prof. Rick Trebino from Georgia Institute of Technology

7. Problem Sets Problem sets will be assigned on Wednesday and due in class the following Wednesday. Problem sets must be turned in on time to receive full credit. We will try to return graded problem sets within one week. Students are encouraged to work together and discuss problems – this is a good way to learn. Nevertheless, blind copying of another student’s work is not acceptable – Don’t do this – we will spot it. Problem sets shouldn’t be torture, so if you’re having trouble, talk to us.

8. To report an emergency, call 911. To obtain updates regarding an ongoing emergency, sign up for Purdue Alert text messages, view www.purdue.edu/ea. www.purdue.edu/ea. There are nearly 300 Emergency Telephones outdoors across campus and in parking garages that connect directly to the PUPD. If you feel threatened or need help, push the button and you will be connected immediately. If we hear a fire alarm during class we will immediately suspend class, evacuate the building, and proceed outdoors. Do not use the elevator. If we are notified during class of a Shelter in Place requirement for a tornado warning, we will suspend class and shelter in [the basement]. If we are notified during class of a Shelter in Place requirement for a hazardous materials release, or a civil disturbance, including a shooting or other use of weapons, we will suspend class and shelter in the classroom, shutting the door and turning off the lights. Please review the Emergency Preparedness website for additional information. http://www.purdue.edu/ehps/emergency_preparedness/index.html http://www.purdue.edu/ehps/emergency_preparedness/index.html EMERGENCY PREPAREDNESS – A MESSAGE FROM PURDUE

9. Modern Physics has very some unintuitive ideas. In fact, this course will hit you with more than any other course you’ll ever take. The goal is simply to expose you to them, and later courses will cover them on more detail.

10. Understanding the ideas of each lecture requires the knowledge of the previous lectures. If you keep up, you won’t end up looking like this the night before the exams!

11. Modern Physics is 20 th century physics (maybe not so modern….) We’ll start with Einstein’s Special Theory of Relativity Then move to Quantum Theory

12. Before Special Relativity One frame moving at velocity v with respect to another Basically, this seems so obvious as to not to be necessary to say it. Unfortunately, it’s wrong. x z y x’x’ z’z’ y’y’

13. James Clerk Maxwell (1831-1879) In the mid-19 th century, Maxwell unified electricity and magnetism with his now famous equations and showed that light is an electromagnetic wave. where is the electric field, is the magnetic field, and c is the velocity of light. Why is this a problem?

14. Light is an electromagnetic wave. The electric ( E ) and magnetic ( B ) fields are in phase. The electric field, the magnetic field, and the propagation direction are all perpendicular.

15. Michelson & Morley Waves typically occur in a medium. So in 1887 Michelson and Morley attempted to measure the earth's velocity with respect to what was then called the aether and found it always to be zero, effectively disproving the existence of the aether. Edward Morley (1838-1923) Albert Michelson (1852-1931)

16. In 1905, Einstein had a very good year. Albert Einstein (1879-1955) In 1905, Einstein explained Brownian motion and the photoelectric effect (for which he later won the Nobel prize). Einstein also explained Michelson’s and Morley’s experiment: he realized that light didn’t need a medium and was a property of free space. And it traveled at the same velocity no matter what speed you were going. This idea forms the basis of the Theory of Special Relativity.

17. With Special Relativity The Lorentz transformations are the correct way to transform from one frame to the other. They yield a constant speed of light and are NOT at all obvious! Lorentz himself didn’t believe them. x z y x’x’ z’z’ y’y’

18. Quantum Theory

19. Blackbody Radiation When matter is heated, it not only absorbs light, but it also spontaneously emits it. A blackbody is a medium that’s black when it’s cool and so can spontaneously emit and absorb all colors. Blackbodies are interesting because their optical properties are independent of the material and only depend on the temperature.

20. The Ultraviolet Catastrophe Lord Rayleigh used the classical theories of electromagnetism and thermodynamics to show that the blackbody spectrum should be: This worked at longer wavelengths but deviates badly at short ones. This problem became known as the ultraviolet catastrophe and was one of the many effects classical physics couldn’t explain. Rayleigh-Jeans Formula

21. Max Planck showed that if light is considered as a particle, bye bye Ultraviolet Catastrophe. Indeed, photographs taken in dimmer light look grainier. Very very dimVery dimDim BrightVery brightVery very bright When we detect very weak light, we find that it’s made up of particles. We call them photons.

22. 19 th -century scientists could not explain spectra. 1/Wavelength 

23. The Planetary model for the atom was also a problem. From classical E&M theory, an accelerated electric charge radiates energy (electromagnetic radiation), which means total energy must decrease. Why doesn’t the electron crash into the nucleus? And the radius r must decrease!

24. In his thesis in 1923, Prince Louis V. de Broglie suggested that mass particles should have wave properties similar to light. The wavelength of a matter wave is called the de Broglie wavelength: If a light-wave also acted like a particle, why shouldn’t matter-particles also act like waves? And the mass particles would be subject to their own Uncertainty Principle! where h = Planck’s constant and p is the particle’s momentum

25. Quantum theory explains the Periodic Table.