4. Wavefunctions and orbitals Flashcards

1
Q

Explain the de Broglie equation

A
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2
Q

Explain the Heisenber Uncertainty Principle

A

Probability of finding an e at certain location

Principle states that the more precisely the position of some particle is determined, the less precisely its momentum (quantity of motion of a moving body, measured as a product of its mass and velocity) can be predicted from initial conditions, and vice versa

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3
Q

What is a wavefunction

A

Wavefunction (Ψ) - a mathematical description of a wave

  • Schrodinger defined the wavefunction to describe an e
  • Bohr interpreted Ψ2 as the probability of finding an e anywhere in a certain space
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4
Q

Explain Schrodingers equation

A

Used to find the allowed energy levels of quantum mechanical systems (such as atoms)

  • time independent (this particular)
  • H - Hamiltonian operator (representing the energy of the electrons and nuclei in a molecule)
  • E - possible energies
  • Ψ (psi) - wavefunction
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5
Q

How are the Schrodinger and Bohr equations related?

A

The solution of H atom (two body system = e and proton) e to the Schrodinger matches the Bohr equation

  • n - principal quantum number
  • R - Rydberg constant

=> in H the E only depends on the quantum number

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6
Q

Which quantum numbers are used to characterise atomic orbitals?

A

For H:

  • n: energy - can be any energy
  • l: shape - can be any from 0 to n-1

l = 0 -> s

l = 1 -> p

l = 2 -> d

l = 3 -> f

  • ml: orientation - can be any whole number from -l to +l (L not 1)
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7
Q

What are the two possible coordinate systems for describing atomic orbitals?

A
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8
Q

How is distance from the nucleus and the shape of the orbital noted?

A
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9
Q

Explain R on R(r) graphs

A

Info on d_istribution of charge density inside an orbital_

Density as the distance from nucleus increases / amplitude of the wavefunction (???)

  • 2s a point where equals 0 - a node (where R(r)=0) - the phase changes (from + to -)
  • 3s - two nodes → 3 phases
  • the more nodes → the higher the E
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10
Q

Explain radial distribution functions

A

Show the probability of finding an e at a cretain distance from the nucleus

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11
Q

Explain the phase changes in 1s, 2s and 3s orbitals

A
  • All s orbitals are spherical
  • 1s no phase changes
  • 2s on phase change (positive darker inside region, negative - lighter region)
  • 3s → 2 phase changes (3 phases in total)
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12
Q

Explain the phases of p orbitals

A
  • each lobe is a new phase - differently coloured (doesn’t matter which)
  • 3 perpenticular orbitals (x, z, y)
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13
Q

Explain nodal planes in p orbitals

A
  • nodal planes - where the wavefunction is equal to 0
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14
Q

What are the shapes of d orbitals?

A
  • x, y, z
  • phases go: light, dark, light, dark (positive - negative phases)
  • in dz2 3 orbitals - 2 merged
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15
Q

What are the nodal planes in d orbitals?

A
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16
Q

What is a phase of an orbital?

A

Positive

Negative