Atomic Structure and Atomic Spectra

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Atomic Structure and Atomic Spectra. Chapter 13. Table 10.1 Hydrogenic radial wavefunctions. R = (N n,l ) (polynomial in r) (decaying exponential in r). L n,l (p) is an associated Laguerre polynomial. Fig 10.4. Potential energy between an electron and proton in a hydrogen atom. +. - PowerPoint PPT Presentation

Transcript of Atomic Structure and Atomic Spectra

Chapter 13

Atomic Structure and Atomic Atomic Structure and Atomic SpectraSpectra

Table 10.1 Hydrogenic radial wavefunctionsTable 10.1 Hydrogenic radial wavefunctions

n2e)(Ln

N)r(R l,n

l

l,nl,n

oaZr2

LLn,ln,l(p) is an (p) is an associatedassociated

Laguerre polynomialLaguerre polynomial

R = (NR = (Nn,ln,l) (polynomial in r) (decaying exponential in r)) (polynomial in r) (decaying exponential in r)

Fig 10.4

Potential energy between an electron and proton

in a hydrogen atom

ao

++ + -- -

One-electron wavefunction = an atomic orbital

Fig 10.5 Energy levels of a hydrogen atom

2H

n

hcR

• Principle quantum number

n = 1, 2, 3,...,∞

• Angular momentum QN

l = 0, 1, 2,..., (n-1)

• Magnetic QN

ml = -l, ..., +l• Spin QN

ms = ±1/2

in cm-1

Bound

states

Unbound

states

Fig 10.7 Energy of orbitals in a hydrogenic atom

Energy only depends on principal quantum number n

En = -RH ( )1n2

n=1

n=2

n=3

Why the degeneracy?!

Fig 10.9 Balance of kinetic and potential energies that

accounts for the ground state of hydrogenic atoms

Fig 10.10 Electron densities of 1s and 2s orbitals

in a hydrogen atom

Fig 10.11 Boundary surface of an s-orbital within which

there is a 90% probability of finding Mz. Electron

r90

Orbitals don’t have edges!

Fig 10.13 Probability density for an s-orbital

s-orbital is

spherically symmetrical

Fig 10.14 Radial distribution function for an s-orbital

oaZr2

eraZ

4)r(P 2

3

o

Fig 10.15 Boundary surfaces for p-orbitals

ml = -1 ml = 0 ml = 1

Fig 10.16 Boundary surfaces for d-orbitals

ml = -2 ml = -1 ml = 0 ml = 1 ml = 2

Fig 10.17 Grotrian diagram for the spectrum of H

Selection rules for allowed

transitions:

Δl = ±1 and Δml = 0, ±1

• A photon can carry only one unitof angular momentum

• Some transitions are allowed,other are forbidden