Week 2 - Intro Quantum II Flashcards

1
Q

The higher the energy level…

A

the further from the nucleus the orbit is.

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2
Q

What must an atom do to change to another stationary state (electron moves to another orbit)?

A

Absorb or emit a photon

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3
Q

In the equation E = ΔE = E(f) - E(i), what does each part mean?

A

E = energy of photon
ΔE = change in energy
E(f), E(i)= final and initial orbit energy

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4
Q

What does the value ‘n’ tell us about the electron in an atom?

A
  • Distance from the nucleus
  • Energy
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5
Q

Ground state vs excited state

A

GS: when an electron is in the first orbit (n=1) closest to the nucleus
ES: electron is in any other orbit

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6
Q

Electron absorption

A

if an electron absorbs a photon whose energy equals the difference between lower and higher energy levels, the electron moves to the outer (higher energy) level

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7
Q

Electron emission

A

If an electron goes from a higher to a lower energy level, the atom emits a photon whose energy equals the difference between the two levels (typically or always going to ground state, n=1)

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8
Q

In the equation E = -2.18x10^-18 ((Z^2)/(n^2)), what does each part mean?

A

E = energy of an electron in orbit ‘n’
number = Bohr’s Constant
Z = atomic number (H=1,He=2…)
n = orbit number

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9
Q

Which atoms does Bohr’s model explain the spectra for?

A

Hydrogen and other 1-electron species (cannot be used for multi-electron species)

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10
Q

Which energy difference between orbitals is the largest?

A

n = 1 to n = 2

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11
Q

Which range do emissions to the first three orbits fall into?

A

Emissions to n=1 are UV
Emissions to n=2 are visible
Emissions to n=3 are infrared

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12
Q

What do matter and light have in common?

A

Both have wavelengths

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13
Q

In the equation (λ = h/mu), what does each part mean and what is this equation used for?

A

λ = wavelength
h = Planck’s constant
m = mass
u = velocity
Used for calculating wavelength of matter (De Broglie’s principle)

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14
Q

In the equation ΔxΔp≥h/4𝝅, what does each part mean and what is this principle?

A

Δx = uncertainty in position
Δp = uncertainty in momentum
h = Planck’s constant
This is Heisenberg’s Uncertainty Principle

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15
Q

Precision of position and momentum have an ______ relation

A

Inverse

i.e. if the position of a particle can be determined more precisely, then the momentum of the particle is predicted less precisely. You cannot determine both precisely.

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16
Q

Schrodinger described electron distribution as a…

A

standing wave

17
Q

Each wavefunction is defined by what three quantum numbers?

A

n, l, and m

18
Q

What do we get if we square the wave function (Ψ)?

A

The probability of finding an electron at a given point

19
Q

Orbitals are…

A

mathematically derived regions of space with different probabilities of containing an electron

20
Q

Describe the principal quantum number, n

A
  • positive integer (1,2,3…)
  • indicates size of orbital
  • specifies energy level
21
Q

Describe the angular quantum number, l

A
  • positive integer (0 to n-1)
  • shape of orbital
  • value of n limits l
    when l=0, s orbital
    when l=1, p orbital
    when l=2, d orbital
    when l=3, f orbital
22
Q

Describe the magnetic quantum number, m(l)

A
  • integer (-l to +l)
  • orientation of the orbital around the nucleus
  • value of l limits m(l); if l=1, m(l) can be -1,0,1
23
Q

Shape of s-2s orbital? Value of l?

A

Spherical, l=0

24
Q

Shape of p-2p orbital? l value?

A

Dumbbell shaped (two circles), l=1

25
Q

Electron probability density is highest at…

A

r = 0; closer to the nucleus

26
Q

What are nodes?

A

Regions where there is no probability of finding an electron

27
Q

What is a radial node? How do you determine how many an orbital has?

A

In s orbitals, radial nodes depend on quantum numbers n and l; located at n-1-l

28
Q

What is an angular node? How do you determine how many an orbital has?

A

In p orbitals, angular nodes depend on quantum number l; they are equal to l

29
Q

Describe the n/l table for determining orbital.

A

l across the top, going from 0 to 2
n along the left, from 1 to 4
n values determine number (same)
l values determine letter:0=s,1=p,2=d

30
Q

How do you determine radial/angular nodes?

A

Radial = n-1-l
Angular = l

31
Q

What is N subscript A?

A

the number of photons in one mol of photons; Avogadro’s number

32
Q

What does n^2 give you?

A

The number of orbitals with that n as their principal quantum number

33
Q

Formulas to calculate momentum of a proton

A

p = h/λ, p = mu, p = E/c