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Quantum Mechanics and Atomic Orbitals ohr and Einstein particle nature of light DeBroglie wave nature of particles Schrödinger theoretical descriptions of at Heisenberg Dirac quantum or wave mechanics wave function = every allowed e - state has unique to calculate energy use Ĥ Ĥ = E

Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

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Page 1: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

Quantum Mechanics and Atomic Orbitals

Bohr and Einstein particle nature of light

DeBroglie wave nature of particles

Schrödinger theoretical descriptions of atomsHeisenberg Dirac

quantum or wave mechanics

wave function =

every allowed e- state has unique

to calculate energy use Ĥ

Ĥ = E

Page 2: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

solved for hydrogen wave functions

energies 2 = probability distribution

Ĥ = E

E

probability of finding an e- in Hat a particular distance from the nucleus

orbital

Page 3: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

orbital requires 3 quantum numbersn l ml

principal 1, 2, 3, …size and energy

angular momentum

0, 1, 2, …, (n - 1)shape

magnetic-l, …, lorientation

“address”

Page 4: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

orbital requires 3 quantum numbersn l ml

principal quantum number sizeenergy

as n increases orbitals become larger

e- is further from the nucleusn = 1n = 2n = 3n = 4n = 5n = 6n = 7

Page 5: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

orbital requires 3 quantum numbersn l ml

angular momentum shape n - 1n = 1 l = 0n = 2 l = 0, 1n = 3 l = 0, 1, 2n = 4 l = 0, 1, 2, 3

designated by letters

l = 0 s orbitall = 1 p orbital

l = 2 d orbitall = 3 f orbital

0

Page 6: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

n = 1 l = 0n = 2 l = 0, 1n = 3 l = 0, 1, 2n = 4 l = 0, 1, 2, 3

designated by letters

l = 0 s orbitall = 1 p orbital

l = 2 d orbitall = 3 f orbital

n = 1n = 2n = 3n = 4n = 5n = 6n = 7

sp

d

f

Page 7: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

orbital requires 3 quantum numbersn l ml

magnetic quantum number -l,…, l

n = 1 l = 0 m = 0

n = 2 l = 0 m = 0

l = 1 m = -1m = 0m = 1

n = 3 l = 0 m = 0

l = 2

l = 1 m = -1m = 0m = 1

m = -2m = -1m = 0m = 1m = 2

row s

s

p

sp

d

1

1

3

3

1

51 s orbital3 p orbitals

5 d orbitals

Page 8: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

1 s orbital3 p orbitals

5 d orbitals

n = 1n = 2n = 3n = 4n = 5n = 6n = 7

p

d

f

s

each orbital holds 2e- 4th quantum number ms

f orbitals7

spin

Page 9: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

1s orbital

spherical

2

2s and 3s 2

Page 10: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

1p orbital

2p orbitals 3dumbbell shape

3p, 4p, 5p etc. similar shapes larger

Page 11: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

d orbitals3 5cloverleaf

larger n same shapes larger

Page 12: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

Pauli exclusion principle

Polyelectronic Atoms

no 2 electrons same 4 quantum numbers

lowest energy orbitals fill first

1s orbital is lowest energy

H 1e- 1s1

He 2e- 1s2

which orbital fills next?

2s2p3s3p4s where is 3d?

Page 13: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

1s 2s 2px 2py 2pz 3s 3px 3py 3pz 4s 3d 3d 3d 3d 3d

HHeLiBeBC

no! Hund’s rule parallel spins

NOF

Ne

Na [Ne]

Page 14: Quantum Mechanics and Atomic Orbitals Bohr and Einsteinparticle nature of light DeBrogliewave nature of particles Schrödinger theoretical descriptions

K [Ar]4s 3dxz 3dxy3dyz 3dx2-z2 3dz2 4px

Ca [Ar]Sc [Ar]

Ti [Ar]

V [Ar]

Cr [Ar] no

half full shell stable

Mn [Ar]

Cu [Ar] no

full shell stable