Test 6 & 7 Flashcards

1
Q

what is hund’s rule?

A

e⁻ fill up all orbitals before they start pairing in them

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2
Q

eqn for lightspeed, c

A

λ * ν = c

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3
Q

symbol for wavelength

A

λ, lambda

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4
Q

symbol for frequency

A

ν, nu

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5
Q

units of frequency

A

cycles/second → 1/s → s⁻¹ → Hertz (Hz)

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6
Q

eqn for E w/ Planck’s constant h and what it means

A

E = hν or Energy = Planck’s Constant * frequency to find E in J of 1 photon

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7
Q

what did einstein discover about light, x 2

A

confirmed Planck’s theory and discovered dual wave/particle nature of light

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8
Q

what is de Broccoli’s eqn for matter wave lengths?

A

λ = h/(momentum * velocity), where units are in meters

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9
Q

elec config for Cu

A

[Ar]4s¹ 3d¹⁰

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10
Q

elec config for Cr

A

[Ar]4s¹ 3d⁵

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11
Q

10⁻⁶

A

micro

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12
Q

10⁻⁹

A

nano

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13
Q

10⁻¹²

A

pico

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14
Q

acronym to remember order of electromagnetic spectrum

A

Red Meat Is Very Unhealthy, Xspecially Grilled

Radio, Microwave, Infrared, Visible, UV, Xray, Gamma

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15
Q

when d-block elements form ions, which orbital loses e⁻ first?

A

the s orbital

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16
Q

what is the aufbau principle

A

The statement that an electron occupies the lowest available energy orbital

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17
Q

what is the Pauli Exclusion Principle

A

No 2 electrons in the same atom can have the same 4 quantum numbers

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18
Q

decrease in ionization energy is due to an increase in what?

A

electron shielding

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19
Q

e⁻ affinity trend

A

Increases towards top and right of PT, except for at (½) filled orbitals

20
Q

ionization E trend

A

Increases towards top and right of PT, except for at (½) filled orbitals

21
Q

atom radius size trend

A

Increases towards bottom and left of PT

22
Q

define diamagnetism

A

all e⁻ are paired, only very slightly repelled

23
Q

define paramagnatism

A

some unpaired e⁻ leads to a strong attraction to magnetic field

24
Q

the number of valence electrons is equal to what

A

the atom’s main group number

25
Q

how to solve for Zₑբբ charge of an electron when determining e⁻ shielding

A

Zₑբբ = nuclear charge - # e⁻ below

For P on level 3: +15 - (2 + 2 + 6) = +5 for e⁻ on level 3

26
Q

define excited state

A

e⁻ hops to higher orbit

27
Q

define ground state

A

e⁻ goes to lowest E level possible

28
Q

define degenerate orbitals

A

orbitals w/ same E

29
Q

how does λ change from L→R on EMS

A

long → short

30
Q

how does ν change from L→R on EMS

A

low → high

31
Q

how does E change from L→R on EMS

A

low → high

32
Q

who found the H spectrum to compare against a prism rainbow’s continuous spectrum

A

Balmer

33
Q

what did Bohr do, and how did he support the Balmer series

A

made e⁻ E levels; n = 1, UV; n = 2, visible (which Balmer’s spectrum is on); n = 3, infrared

34
Q

what did de Broccoli come up with?

A

matter has a dual particle/wave nature

35
Q

define Heisenberg’s uncertainty principal

A

can’t know both e⁻ location and momentum, only probability of both

36
Q

Schrodinger’s wave equation

A

ψ(x, y, z)² = probability density of e⁻ = orbitals; x, y, and z = e⁻ coordinates and a function of quantum #s: n, l, mₗ, mₛ

37
Q

occurrence and shape of s orbital

A

1 @ each E level

spherical

38
Q

occurrence and shape of p orbital

A

3 @ each E level when n ≥ 2

dumbbell shaped

39
Q

occurrence and shape of d orbital

A

5 @ each E level when n ≥ 3

multi-lobed (like petals)

40
Q

occurrence and shape of f orbital

A

7 @ each E level when n ≥ 4

weird shapes bro

41
Q

3 things about quantum # n

A

principal quantum number
E level of e⁻
goes from 1, 2, 3, 4 … on to infinity

42
Q

3 things about quantum # l

A

angular momentum quantum number
orbital type s, p, d, or f
goes from 0, 1, 2, 3 … on to n - 1

43
Q

3 things about quantum # mₗ

A

magnetic quantum number
3D coordinates of orbital; or the shape
from -l…0…l (so, if l = 2, then mₗ could be -2, -1, 0, 1, 2

44
Q

3 things about quantum # mₛ

A

spin quantum number
spin direction of the e⁻ in the orbital
±½

45
Q

how to write mₛ and mₗ on test

A

write like “m sub s/l”, DO NOT write it as a subscript T-T