Solved radial equation: Last time For two simple cases: infinite and finite spherical wells Spherical analogs of 1D wells We introduced auxiliary func
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1 Quantum Mechanics and Atomic Physics Lecture 16: The Coulomb Potential h / d/361 Prof. Sean Oh
2 Solved radial equation: Last time For two simple cases: infinite and finite spherical wells Spherical analogs of 1D wells We introduced auxiliary function And radial equation became: Today: we will find radial solutions for Coulomb Potential!
3 The Hydrogen Atom Model for hydrogen Electron: charge Q 1 = -e, mass = m e Nucleus (proton): charge Q 2 = Ze =+ +e, mass = m p Coulomb Potential: Reduced Mass: Two particles orbiting around each other is mathematically identical to one particle of the reduced mass orbiting around the other infinitely massive particle located at the center of mass. For hydrogen atom, practically
4 Revisit the Radial Equation
5 Asymptotic Behavior r 0
6 Asymptotic Behavior r
7 Look at term in exponential This has units of 1/r Let s call it 1/a 0 And let s note that we expect E 1/n 2, according to Bohr s result. So, See your book kf for full lld derivation i for L n,l () (r) using a power series method
8 Simplest case: Ground state Let s try a solution to S.E. for the ground state n=1 and zero angular momentum l = 0 Therefore, we can assume the ground state is spherically symmetric so: Ψ(r, (r,θ,φ)) = Ψ( ( r) So, let s try this solution:
9 This is the Bohr radius found in the Bohr model!
10 Let s put this expression for a 0 back into equation above: This is the same expression as the Bohr model energy in the ground state!
11 Normalization of the ground state Note that Ψ = Ψ 100 and also that After two integrations by parts, or just look in the appendix of your book: Ground state eigenfunction for Hydrogen. Same energy as Bohr model, but r is not fixed at a 0! Not a circular orbit - something like an electron cloud around nucleus.
12 Hydrogen Radial Wavefunctions Complete radial function solutions are: n is called the principal quantum number and must be an integer with n>l These are called Associated Laguerre Polynomials Reed Chapter 7
13 Hydrogen Radial Wavefunctions
14 Summary of Hydrogen Atom Solutions Ψ is a product of Φ which is just Θ which is a polynomial in cosθ R which is a product of a decaying exponential and a polynomial in r Ψ depends on 3 quantum numbers Principal quantum number n=1, 2, 3, Orbital angular momentum quantum number l = 0, 1, 2, (n-1) Magnetic quantum number m l = 0, ±1,. ± l or m l =-l, l,-l+1,, l-1, l
15 Hydrogen Atom Wavefunctions This is the one we derived. Ground state wavefunction Reed Chapter 7
16 Energy Degeneracy Energy only depends on n For each n, there are n values of l (from zero to n-1) For each l,, there are (2l+1) values of m l (from l to l ) So, for each n, the degeneracy is:
17 Quantum numbers and Degeneracy Question: So if energy is the same, what s different about the various degenerate states? Answer: The probability distribution of the electron around the nucleus, i.e. the shape of the electron cloud.
18 For historical reasons, all states with same quantum number n are said to form a shell. And states having the same value of both n and l are said to form a subshell (s, p, d, f, ) The probability distributions for these different states t have important features, which we will cover next time. Spectroscopic Notation In Schrodinger theory, different l states with same n have same energy Called l-degeneracy Energy level diagram omits different m l states - independent of m l due to spherical symmetry of the atom. This is for no external magnetic field!
19 Probability Distribution What is the probability of finding the electron in a volume of space dv?
20 Example What is the probability of finding the electron at a distance r < r 0 for the ground state (ψ 1,0 10 )?
21 Use this to determine the probability of finding the electron inside the first Bohr radius (r<a 0 )? Or r<2a 0 or r<3a 0?
22 Summary/Announcements Next time: More on the probability bili distributions ib i of the Hydrogen atom Next homework due on Monday Nov 14. QUIZ next class, covering topics since Midterm!
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