Exam 3 Flashcards

(72 cards)

1
Q

Specific heat capacity

A

amount of (thermal) energy required to change temperature of 1 degree Celsius of 1.0 g material

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2
Q

Exothermic

A

Delta T < 0

-q

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3
Q

Endothermic

A

Delta T > 0

+q

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4
Q

calorimetry

A

the study of heat flow accompanies a chemical process

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5
Q

When does Delta H=q

A
As long as q is measured with masses equivalent to make ratios in balanced rxn
ie Ch4(16g/mol)+2O2 etc eqn
question: 16gCh4 in excess O2
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6
Q

-qrxn =

A

+qsoln

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7
Q

+qsoln=

A

(mcDeltaT)soln

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8
Q

light admitted at specific energy values in the spectrum, light source produced light of

A

only specific (or certain) wavelengths

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9
Q

Bohr’s model of the H atom

A

Neils Bohr
-The presence of 4 distinct bands of light in the visible region of the atomic emission spectrum for hydrogen is based on the way energy reacts with certain electorons

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10
Q

how long do electrons stay in an excited state

A

short time

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11
Q

+E to system

A

e- jumps up

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12
Q

from system

A

e- jumps down

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13
Q

Neils bohr’s model to explain the lines spectrum of hydrogen

A

based on classical physics explaining macro scale phenomenon: 4 points

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14
Q

four points of Neil boars model

A
  1. only specific orbits allowed e- resides on orbits
  2. e- in orbit has specific E
    -e- won’t radiate E
    -e- won’t spiral into nucleus
  3. e- jump low –> high must absorb E
    e- jumps high –>low must emit E
  4. use precipitate number (n) to identify orbits
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15
Q

e- wants to be

A

in lowest E

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16
Q

Quantized E

A

specific amount needed for a specific transition Exact! no more no less

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17
Q

e- from high states to low

A

can make stops

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18
Q

e- from low states to high

A

can’t make stops

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19
Q

Delta energy and wavelength

A

as E goes up wave length goes down

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20
Q

frequency and wavelength

A

as wavelength goes up frequency goes down

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21
Q

frequency and delta energy

A

as E goes up frequency goes up

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22
Q

Spectrum

A

400 0

V I B G Y O R

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23
Q

boars model of H atom was good because

A

explained absorption and emissions

-H atom only has 1 e-

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24
Q

boars model of H bad because

A
  • only explains few (one electron) systems
  • violates classical physics
  • violates uncertainty principle:
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25
what was the uncertainty principle
can't know both E and position at the same time
26
treating electrons as waives in an atom
- particle/wave duality of light | - particle/wave duality of e-
27
how does light behave
like a particle
28
how fast does the wave travel through space at
speed of light | frequency)(wave length
29
photon
light particle, smallest packet of energy | E=h(frequency)
30
how does matter emit and absorb energy
in units of hu's
31
plancles constant
h
32
wave calc
c=(length)(frequency)
33
particle calc
e=h(frequency)
34
what is light
the one type of electromagnetic radiation (emr). Oscilating orthogonal wave traveling through space at c (constant speed)
35
waves interacting with atoms
Dif waves react Dif w atoms
36
Quantum mechanics
treats e- behavior as a wave | -Describe e- wave functions equation
37
Regions in space with high probability of electron density
orbitals
38
how many electrons does each orbital hold
2
39
S orbital
probability density is spherical | -only one allowed
40
P orbital
prob. density is peanut shaped | - only 3 allowed
41
D orbital
Prob density is doubled up or doughnut | -only 5 allowed
42
F orbital
prob density is fancy | -only 7 allowed
43
Energy related to orbitals
``` 1 S 2 S P 3 S P D 4 S P D F 5 S P D F 6 S P D F 7 S P D F ```
44
n
principle quantum number | -Energy level
45
l
angular momentum shape
46
Ml
magnetic orientation
47
Letter related to l number
``` S 0 P 1 D 2 F 3 Have a value of n, l is allowed from 0 up to n-1 ```
48
L number related to Ml number
0 0 1 -1,0,1 2 -2,-1,0,1,2 3 -3.-2,-1,0,1,2,3
49
Pauli exclusion principle
no two e- can have the same set of quantum numbers
50
how to name a quantum
(n,l,Ml,Ms)
51
Ms
electron
52
Hunds rule
maximize parallels spins before spin pair
53
Degenerate
same enegy
54
AUFBAV principle
fill orbitals from low E-->high E
55
Noble gasses
Stable because of electron conferrence are composed of full and closed shells
56
Valence electron
Do all the work: gained, lost, involved in reactions, and bonding
57
Transition metals
Don’t follow an 8 valence electron rule; follow an 18 valence electronic rule
58
What are the exceptions to transition metals following the 18 valence e rule
Cr Mg Cu Ag
59
Spin pairing energy
When energy change costs energy | -delta E between orbits
60
Energy to promote v energy to pair
Less energy to promote than to pair
61
Atom to cation
Size decreases because it | Loses electrons and more protons pull electrons harder
62
Atom to anion
Size increases bc gains electrons and less protons so weaker pull
63
Period left to right in terms of atom size
Size decreases because pull towards nucleus increases
64
Size of atoms group top to bottom
Size increases because N is related to size
65
Effective nuclear charger (Zeff) period left to right
Increases (#P-#core electrons)
66
Effective nuclear charge (Zeff) group too to bottom
Stays the same
67
Number of core electrons
Atomic number of noble gas before element
68
Zeff
Never negative | Always less than Z
69
Trends on periodic table
``` Effective nuclear charge (Zeff) Size of atoms/ions Ionization energy (Ez) ```
70
Valence electron attraction
Only attracted to a portion of the total net nuclear charge
71
Isoelectronic Set
Cations, anions, neutral all with same electron configuration
72
What is shield build from between inside protons and outside valence electron
Build from core electrons block full nuclear charge from pulling on valence electrons