
Slides from Lecture 9-11
... Often we’re interested in quantum numbers, not the wave pattern: vector approach avoids calculating wave functions when not needed. Wave function picture incomplete: If you know ψ(r) you know everything about: position, momentum, KE, orbital angular momentum …but nothing about spin (+ other mo ...
... Often we’re interested in quantum numbers, not the wave pattern: vector approach avoids calculating wave functions when not needed. Wave function picture incomplete: If you know ψ(r) you know everything about: position, momentum, KE, orbital angular momentum …but nothing about spin (+ other mo ...
Fall 2005
... a) What is the force attracting this particle to the origin? b) According to the Bohr theory, what are the allowed values of the radius rn and the total energy En ? (Restrict yourself to circular orbits.) c) What is the analog of the Rydberg formula? Show that the correspondence principle is satisfi ...
... a) What is the force attracting this particle to the origin? b) According to the Bohr theory, what are the allowed values of the radius rn and the total energy En ? (Restrict yourself to circular orbits.) c) What is the analog of the Rydberg formula? Show that the correspondence principle is satisfi ...
The non-interacting Bose gas
... and particles with the reservoir. The constants in this ensemble are the chemical potential µ and the temperature T . Applying the concept of the grand canonical ensemble to trapped gases is valid under the assumption of the local density approximation: as long as the correlation length of the gas i ...
... and particles with the reservoir. The constants in this ensemble are the chemical potential µ and the temperature T . Applying the concept of the grand canonical ensemble to trapped gases is valid under the assumption of the local density approximation: as long as the correlation length of the gas i ...
Document
... a particle which is not its own antiparticle, eg , K , ˆ ˆ | a C C | a C C 1 (7.20) Cˆ | a Ca | a ; Cˆ | a Ca | a CC a a a a C =C -parity is a useful quantum number for particles which are their own antiparticles and are eigenstates of Cˆ , eg 0 , , . Can also b ...
... a particle which is not its own antiparticle, eg , K , ˆ ˆ | a C C | a C C 1 (7.20) Cˆ | a Ca | a ; Cˆ | a Ca | a CC a a a a C =C -parity is a useful quantum number for particles which are their own antiparticles and are eigenstates of Cˆ , eg 0 , , . Can also b ...
Zero energy non-zero momentum particles
... In the article with title “Matter-light duality and speed greater than light” [1], we formulated energy and momentum equations for particles with speed greater than light. In this article we see a special case of it where the energy becomes zero and momentum is non-zero for a particle (we named them ...
... In the article with title “Matter-light duality and speed greater than light” [1], we formulated energy and momentum equations for particles with speed greater than light. In this article we see a special case of it where the energy becomes zero and momentum is non-zero for a particle (we named them ...
Question 1 Consider the mechanical system with three degrees of
... your answer to 3 decimal places. Take the magnitude of the acceleration due to gravity to be 9.81 ms-2.Hint : Apply Newton’s 2nd Law to each of the two particles A and B. ...
... your answer to 3 decimal places. Take the magnitude of the acceleration due to gravity to be 9.81 ms-2.Hint : Apply Newton’s 2nd Law to each of the two particles A and B. ...
WP1
... phenomenon. Quantum physicists think that undisturbed particles (wavicles) just don’t have exact positions and momenta! A consequence of the HUP is that particles do NOT have trajectories! So what happens to the notion of an external reality with QM????!! ...
... phenomenon. Quantum physicists think that undisturbed particles (wavicles) just don’t have exact positions and momenta! A consequence of the HUP is that particles do NOT have trajectories! So what happens to the notion of an external reality with QM????!! ...