Chapter 7 Flashcards

(39 cards)

1
Q

wavelength(λ)

A
  • the distance from crest to crest or trough to trough on a wave
  • c=λv
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2
Q

frequency(v)

A
  • the number of crests of a wave that pass a stationary point of reference per second
    • cycles per second
  • c=λv
    • c=spped of light=3x108
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3
Q

electromagnetic properties of radiant energy

A
  • when electromagnetic properties of radiant energy pass through air, it interacts with fewer atoms than thru solids or liquids
    • more interactions btwn the oscillating waves and the electrons within the atoms and molecules in solids and liquids slow the waves and bend their paths
      • shorter wavelengths bend more than long ones which is why violet is at the bottom of rainbows
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4
Q

quantum theory

A
  • quantum theory: a model based on the idea that energy is absorbed + emitted in discrete quantities of energy(quanta)
    • the smallest discrete quantity of a particular form of energy
  • Planck proposed that light and all other forms of electromagnetic radiation have not only wavelike properties, but also particle-like properties on the atomic level.
  • Light from an object made of large, but discrete #s of atoms or molecules must be quantized
    • having values restricted to whole# multiples of a specific base value
    • steps are quantized while a ramp is continuous
  • A quantum of light(EM radiation) is called a photon
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5
Q

photoelectric effect

A
  • the phenomenon of light striking a metal surface and producing an electric current(a flow of e-)
    • electrons are emitted from metals when they are illuminated by and absorb electromagnetic radiation
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6
Q

threshold frequency(v0)

A
  • the minimum frequency of light required to produce the photoelectric effect.
  • radiation at frequencies less than the threshold value produces NO photoelectrons aka if incoming light has v<v>0
    </v><ul>
    <li>even a dim source of radiant energy produces at least a few phtoelectrons when the frequencies it emits are equal to or greater than v0
    </li></ul>

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* Einstein proposed the threshold frequency of the minimum quantum of absorbed energy needed to remove a single electron from the surface of

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7
Q

work function (𝛟)

A
  • the amount of energy needed to remove an electron from the surface of a metal
    • 𝛟 = hv0
  • If a photoelectric material is illuminated with radiation frequencies above threshold frequency(v>v0), any energy in excess of 𝛟 is imparted to each ejected e- as KE
    • extra energy = KE of emitted electrons
    • KEelectron=hv-hv0=hv-𝛟
    • Ephoton=𝛟+KEelectron
    • the higher the frequency is above the threshold, the higher the KE and hence the velocity of ejected e-
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8
Q

wave-particle duality

A
  • thebehavior of an objectthat exhibits the properties of both a wave and a particle
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9
Q

the hydrogen emission spectrum

A
  • Balmer determined lines corresponding to the visible emission spectrum of hydrogen fit the simple equation:
    • λ = 364.5 nm(m2/m2-n2)
    • n is 2 and m is whole# >2
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10
Q

Rydberg’s equation

A
  • revised Balmer’s eqn(made a more general form)
    • 1/λ = 1.097x10-2nm-1
      • n1 is a postive fixed whole number
      • n2 is a whole number equal to n1+1, n2+2….
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11
Q

the Bohr model of hydrogen

A
  • a theoretical model for the hydrogen atom that assumed its one electron travels around the nucleus in a concentric orbit. Electrons can only exist in these discrete orbits. Each orbit represents an allowed energy level and is designated by the value of n as shown in
    • E = 2.178 x 10-18J(1/n2)
    • in the bohr an electron in the orbit closest to the nucles(n=1) has the lowest energy
    • lines in the absorption and emission spectra represent electrons moving btwn energy levels(orbits)
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12
Q

ground+excited state

A
  • ground state: when the e- in a hydrogen atom is in the lowest (n=1) energy level
    • most stable
  • excited state: if the electron in a hydrogen atom is above n=1 energy level
  • hydrogen atom’s e- can move from ground to excited state(up energy level) it absorbs a quantity of energy(deltaE) that exactly matches the energy difference btwn the two excited states
  • electron transition: any change in e- energy that occurs by absorption or emission of energy
    • movement of an e- btwn energy levels
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13
Q

De Broglie Wavelengths

A
  • Light is a wave that has particle properties and an electron is a particle which must have wave properties
    • this would mean electrons moving in atoms should have a wavelength
    • De Brolgie wavelength: λ = h/mv
      • m is momentum, a particle property
      • λ is wavelength, a wave property
    • λ = h/mu
      • m is mass in kg
      • u is velocity in m/s
  • not restricted to electrons
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14
Q

classical and quantum mechanics

A
  • classical mechanics(Newton)
    • good for large objects
    • not good for atoms, electrons, etc
  • the issue: chemistry occurs at the atomic level
    • solution: Quantum mechanics: combines both wave and particle aspects of matter into a unified theory
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15
Q

nodes

A
  • a location in a standing wave that experiences no displacement
    • In the context of orbitals, nodes are locations at which electron density goes to zero
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16
Q

standing wave

A
  • a wave confined to a given space, with a wavelength (λ) related to the length L of the space by L 5 n(λ/2), where n is a whole number.
17
Q

matter wave

A
  • the wave associated with any particle
18
Q

Heating a blackbody

A
  • Blackbody radiation(heated objects emit EM radiation): classical theory does not match observations
    • explanation: electromagnetic radiation has particle-like properties in addition to wavelike properties
19
Q

The Heisenberg Uncertainty Principle

A
  • the principle that we cannot determine both the position and the momentum of an e- in an atom at the same time
    • since we can’t know both position and momemntum of an e- in a hydrogen atom, the e- cannot be moving in circular orbits as implied by Bohr’s og model.
    • Heisenberg uncertainty principle limits us to knowing only the probability of finding an electron at a particular location in an atom
  • (∆x)(∆mv) ≥ h/4π
    • ∆x = uncertainty in position
    • ∆mv = uncertainty in momentum
20
Q

wave mechanics aka quantum mechanics

A

a mathematical description of the wavelike behavior of particles on the atomic level

21
Q

Schrodinger wave equation

A
  • a description of how the e- matter wave varies with location and time around the nucles of a hydrogen atom
    • wave function(𝛙): a solution the the Schrodinger wave eqn
      • Mathematical expressions that descrive how the matter wave of an e- in an atom varies both with time and with the location of the e- in the aotm
      • wave functions define energy levels in H atoms
      • 𝛙 2 defines an orbital
        • ​aka probability of finding an e-
22
Q

orbital

A
  • a region around the nucleus of an atom where the probability of finding an e- is high; each orbital is defined by 𝛙 2 and identified by a unique combination of 3 quantum #s
23
Q

quantum number/principle quantum number(n)

A
  • a number that specifies the energy, the probable location or orientation of an orbital, or the spin of an electron within an orbital(ALL quantum numbers are integers)
    • principle quantum number(n): a positive integer describing the relative size and energy of an atomic orbital or group of orbitals in an atom
      • same as Bohr’s n
      • orbitals with same n are in same shell
      • as n increases, orbital size increases and e- are further from nucleus and, in the H atom, represent higher energy levels
        • generally, this is also true in multielectron atoms
24
Q

angular momentum quantum number(l)

A
  • an integer having any value from 0 to n-1 that defines the shape of an orbital
    • orbitals with same n and l are in same subshell and have equal energy levels
      • l=0 → s
      • l=1 → p
      • l=2 → d
      • l=3 → f
25
magnetic quantum number(ml)
* an integer with a value from -l to +l. It defines the **3d orientation** of an orbital in the space around the nucleus of an atom
26
spin magnetic quantum number(ms)
* either +1/2 or -1/2, indicating that the spin orientation of an e- ie either up or down
27
Pauli exclusion principle
* the principle that no two e- in an atom can have the same set of four quantum numbers * therefore, each orbital can hold two e- with opposite spins
28
aufbau principle
* states the most stable atomic structures are those in which the e- are in the lowest-energy orbitals available * Three rules: * 1) e- always go into lowest-energy orbital available * 2)each orbital can hold up to 2 e- with opposite spins(Pauli) * 3) for degenerate orbitals, e- fill each orbital singly before pairing up (Hund)
29
effective nuclear charge (Zeff)
* the attraction toward the nucleus experienced by an e- in an atom, equal to the positive charge on the nucleus redfuced by the extent to which other e- in the atom shield the e- from the nucleus
30
core electrons
* e- in the filled, inner shells of an atom or ion that are not incolved in chemical rxns
31
valence electrons
* e- in the outermost occupied shell of an atom * these are the e- that are transferred or shared in chemical rxns
32
valence shell
the outermost occupied shell of an atom
33
degenerate(orbitals)
describes orbitals of the same energy
34
Hund's rule
* the lowest-energy electron configuration of an atom has the maximum number of unpaired electrons, all of which have the same spin, in degenerate orbitals * this is the third rule we apply when doing e- configuration
35
isoelectronic
* atoms or ions that have identical e- configurations and identical # of e- * **increasing nuclear charge(Zeff)** corresponds to **smaller ions**
36
37
Periodic trends
* As atomic # increases, atomic radii increases(aka as we move right and down) * As we move towards the right, each successive element has one additional e-, so we expect an inc. in size of atom * this isn't true because: * 1) **increasing Zeff**: as atomic # inc, so does positive charge of the nucleus * as Zeff inc, the size of atoms dec. * 2) **increasing repulsion btwn valence e-:** as atomic # inc, so does # valence e- * more e- = more electron-electron repulsions(b/c two negs repel), which inc size of atoms
38
Ionization energy(IE)
* the quantity of energy needed to remove 1 mole of electrons from 1 mole of ground-state atoms or ions in the gas phase * doing so always requires energy entering system b/c a negatively charged e- is attracted to a positively charged nucleus, and overcoming that attravtice force requires energy * the amount of energy needed to remove 1 mole of e- from 1 mole of atoms to make 1 mole of cations with a 1+ charge is called the **first ionization energy(IE1)** * **​**generally inc as we go towards the right and up * ​easiest element to ionize is group 1 * this pattern makes sense b/c as the charge of a nucleus inc. across a row, so does Zeff and the attractions btwn nucleus and valence e- * the amount of energy needed to remove 1 mole of e- from 1 mole of 1+ cations to make 1 mole of cations with a 2+ charge is called the **second ionization energy(IE2)** * **​total IE = IE1+IE2**
39
electron affinity (EA)
* the energy change that occurs when 1 mole of e- combines with 1 mole of atoms or monatomic cations in the gas phase * the EA of many elements are negative b/c the formation of anions with a 1- should release energy * can be endothermis or exothermic * very large negative EA means it is favorable to form the anion * **Trends:** * EA increases going down * generally, EA becomes more negative(decreases) when going right(as atomic# inc) * the halogens of group 17 have the most negative(lowest) EA values