Chapter 7 Flashcards
(39 cards)
wavelength(λ)
- the distance from crest to crest or trough to trough on a wave
- c=λv
frequency(v)
- 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
electromagnetic properties of radiant energy
- 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
- 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
quantum theory
- 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
photoelectric effect
- 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
threshold frequency(v0)
- 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
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<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
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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
work function (𝛟)
- 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-
wave-particle duality
- thebehavior of an objectthat exhibits the properties of both a wave and a particle
the hydrogen emission spectrum
- 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
Rydberg’s equation
- 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….
- 1/λ = 1.097x10-2nm-1
the Bohr model of hydrogen
- 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)
ground+excited state
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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
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electron transition: any change in e- energy that occurs by absorption or emission of energy
- movement of an e- btwn energy levels
De Broglie Wavelengths
- 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
classical and quantum mechanics
- 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
nodes
- 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
standing wave
- 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.
matter wave
- the wave associated with any particle
Heating a blackbody
- 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
The Heisenberg Uncertainty Principle
- 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
wave mechanics aka quantum mechanics
a mathematical description of the wavelike behavior of particles on the atomic level
Schrodinger wave equation
- 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-
- wave function(𝛙): a solution the the Schrodinger wave eqn
orbital
- 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
quantum number/principle quantum number(n)
- 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)
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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
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principle quantum number(n): a positive integer describing the relative size and energy of an atomic orbital or group of orbitals in an atom
angular momentum quantum number(l)
- 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
- orbitals with same n and l are in same subshell and have equal energy levels