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The ElectronicThe ElectronicStructure of AtomsStructure of Atoms
Chapter VII
Do Do you seeyou see………… the the Ideas around you Ideas around you ??????
From clasicalphysics toquantum
theoryChapter VIIVII-I
Is Light a Wave or a Particle?
• 1690 Christian Huygens claimed that lightwas a wave.
• 1704 Isaac Newton claimed light was aparticle whose motion was governed byhis Laws of Motion.
Chapter VIIVII-I
Electromagnetic Waves
• Recall that moving chargescreate magnetic fields andmagnetic fields induce electriccurrents.
• An E-M waves are selfsustaining electric andmagnetic fields.
• Speed of light (c) invacuum C = 3 x 108 m/s
Maxwell (1873), proposed that visible light consists ofelectromagnetic waves.
Electromagnetic radiation is the emission and transmission ofenergy in the form of electromagnetic waves.
All electromagnetic radiationλ x ν = c Chapter VIIVII-I
ELECTROMAGNETICELECTROMAGNETICRADIATIONRADIATION
Electromagnetic wave• A wave of energy having a frequency
within the electromagnetic spectrumand propagated as a periodicdisturbance of the electromagnetic fieldwhen an electric charge oscillates oraccelerates.
Chapter VIIVII-I
Electromagnetic Radiation
E l e c t r o m a g n e t i cwave:
•wavelength
•frequency
•amplitude
Chapter VIIVII-I
VII-I Chapter VII
wavelength Visible light
wavelength
Ultaviolet radiation
Amplitude
Node
Wavelength (λ) is the distance between identical points on successive waves.
Amplitude is the vertical distance from the midline of a wave to the peak ortrough.
Properties of Waves
Frequency (ν) is the number of waves that pass through a particular point in 1second (Hz = 1 cycle/s).
The speed (u) of the wave = λ x ν Chapter VIIVII-I
Electromagnetic Radiation
νλ= c
where ν => frequency
λ => wavelength
c => speed of light
•• Waves have a frequencyWaves have a frequency•• Use the Greek letter Use the Greek letter ““nunu””, , νν, for frequency, and units are, for frequency, and units are
““cycles per seccycles per sec””•• All radiation: All radiation: λλ •• νν = c = c
where c = velocity of light = 3.00 x 10where c = velocity of light = 3.00 x 1088 m/sec m/sec
Chapter VIIVII-I
Electromagnetic Radiation
E = hc/λ
where E => energy
h => Planck's constant
c => speed of light λ => wavelength
Chapter VIIVII-I
Photons
The quantum of electromagneticenergy, generally regarded as adiscrete particle having zeromass, no electric charge, and anindefinitely long lifetime.
Chapter VIIVII-I
λ x ν = cλ = c/νλ = 3.00 x 108 m/s / 6.0 x 104 Hz λ = 5.0 x 103 m
Radio wave
A photon has a frequency of 6.0 x 104 Hz. Convertthis frequency into wavelength (nm). Does this frequencyfall in the visible region?
λ = 5.0 x 1012 nm
λ
ν
Chapter VIIVII-I
Max Planck (1858-1947)
• Resolved the problem in1900.
• Energy is not continuous.
• Energy is quantized isdiscrete packets.
• Each packet has aspecific amount ofenergy.
• E = hf h = 6.63x10-34 J-s
• Quantum physics wasborn.
Chapter VIIVII-I
Mystery #1, “Black Body Problem”Solved by Planck in 1900
Energy (light) is emitted orabsorbed in discrete units(quantum).
E = h x νPlanck’s constant (h)h = 6.63 x 10-34 J•s
Chapter VIIVII-I
Chapter VII
Photoelectric Effect
VII-II
Light has both:1. wave nature2. particle nature
hν = KE + W
Mystery #2, “Photoelectric Effect”Solved by Einstein in 1905
Photon is a “particle” of light
KE = hν -W
hν
KE e-
Chapter VII
E = hν
VII-II
The Photoelectric Effect• In the late 1800’s it was
observed that electronswere emitted by certainmetals when certainmetals were exposed tolight.
• If light were a wave itwould take time for thewave to transmit itsenergy to the electrons.
• However, it was observedthat the electron wasinstantly emitted.
• Shorter wavelength lightejected higher energyelectrons. Chapter VIIVII-II
The Photoelectric Effect
• In 1905 Albert Einsteinused Planck’s quantizedenergy to explain thephotoelectric effect.
• Light was quantized inpackets of energy hecalled photons.
• Therefore, only photonswith high enough energycould knock electrons outof an atom.
• E = hf
Chapter VIIVII-II
Photoelectric Effect
• the emission of electrons by substances,especially metals, when light falls on theirsurfaces.
Chapter VIIVII-II
E = h x ν
E = 6.63 x 10-34 (J•s) x 3.00 x 10 8 (m/s) / 0.154 x 10-9 (m)
E = 1.29 x 10 -15 J
E = h x c / λ
When copper is bombarded with high-energy electrons,X rays are emitted. Calculate the energy (in joules)associated with the photons if the wavelength of the Xrays is 0.154 nm.
Chapter VIIVII-II
Bohr’s theory of the hydrogen Atom
VII-III Chapter VII
Atomic Line EmissionAtomic Line EmissionSpectra and Spectra and Niels Niels BohrBohr
BohrBohr’’s greatest contribution tos greatest contribution toscience was in building ascience was in building asimple model of the atom. Itsimple model of the atom. Itwas based on anwas based on anunderstanding of theunderstanding of the LINELINEEMISSION SPECTRAEMISSION SPECTRA ofofexcited atoms.excited atoms.
•• Problem is that the modelProblem is that the modelonly works for Honly works for H
Niels Niels BohrBohr
(1885-1962)(1885-1962)
VII-III Chapter VII
1. e- can only have specific(quantized) energyvalues
2. light is emitted as e-
moves from one energylevel to a lower energylevel
Bohr’s Model ofthe Atom (1913)
En = -RH( )1n2
n (principal quantum number) = 1,2,3,…
RH (Rydberg constant) = 2.18 x 10-18JVII-III Chapter VII
Neil Bohr’s Model of Hydrogen(1913)
• Solves problem of whyelectrons to do fall intonucleus.
• Used quantized orbitswith specific energies.
• Electron can only movebetween orbits by gettingor losing the exactamount of energyrequired.
• It could not take fractionalsteps.
Neil Bohr’s Model of Hydrogen
• Bohr’s model alsoexplained Kirchhoff’sLaws of Spectroscopy.
• Absorption spectraproduced when electronabsorbed energy neededto go to a higher orbit.
• Emission spectraproduced when electronreleases energy anddrops to a lower orbit.
Explains:Quantized energyHydrogen spectra (only)
E = hν
E = hν
7.3VII-III
Ephoton = ΔE = Ef - Ei
Ef = -RH ( )1n2
f
Ei = -RH ( )1n2
i
i f
ΔE = RH( )1n2
1n2
nf = 1
ni = 2
nf = 1
ni = 3
nf = 2
ni = 3
When a photon is emitted:ni > nf
When a photon is absorbedni<nf
VII-III
Ephoton = 2.18 x 10-18 J x (1/25 - 1/9)
Ephoton = ΔE = -1.55 x 10-19 J
λ = 6.63 x 10-34 (J•s) x 3.00 x 108 (m/s)/1.55 x 10-19J
λ = 1280 nm
Calculate the wavelength (in nm) of a photonemitted by a hydrogen atom when its electrondrops from the n = 5 state to the n = 3 state.
Ephoton = h x c / λ
λ = h x c / Ephoton
i f
ΔE = RH ( )1n2
1n2Ephoton =
VII-III
Photons
The quantum of electromagnetic energy,generally regarded as a discrete particlehaving zero mass, no electric charge, andan indefinitely long lifetime.
VII-III
Line Spectrum
A spectrum produced by a luminous gas orvapor and appearing as distinct linescharacteristic of the various elementsconstituting the gas.
VII-III
Emission Spectrum
The spectrum of bright lines, bands, orcontinuous radiation characteristic of anddetermined by a specific emittingsubstance subjected to a specific kind ofexcitation.
VII-III
Ground State
The state ofleast possibleenergy in aphysicalsystem, as ofelementaryparticles. Alsocalled groundlevel.
Excited State
Being at anenergy levelhigher than theground state.
VII-III
Photons
Line Spectrum
Emission Spectrum
Ground State
Excited State
VII-III
Absorption & Emission Spectra
• Bohr’s model alsoexplained Kirchhoff’sLaws of Spectroscopy.
• Emission spectraproduced when electronreleases energy anddrops to a lower orbit.
• Absorption spectraproduced when electronabsorbed energy neededto go to a higher orbit.
Bohr’s Hydrogen Atom
Hydrogen Energy Level Diagram
• Energy levels constructedbased on spectral linesobserved for Hydrogen.
• The Spectrum ofHydrogen is like a verymagnified view of theelectron energy levelsaround the atom.
• WAY COOL!!!!!!!!!!
Emission Line Spectra
Each element has itown unique electronenergy levels withdifferent energyspacing betweeneach level.
Emission Line Spectra
Each element has itown unique electronenergy levels withdifferent energyspacing betweeneach level.
Line Emission Spectrum of Hydrogen Atoms
VII-III
The dual natureof electron
VII-IV
Planck’s Constant
• ΔE = change in energy, in J
• h = Planck’s constant, 6.626 × 10−34 J s
• ν = frequency, in s−1
• λ = wavelength, in m
Transfer of energy is quantized, andTransfer of energy is quantized, andcan only occur in discrete units, calledcan only occur in discrete units, calledquanta.quanta.
VII-IV
Energy and Mass
• Einstein- When a system loses energy, itloses mass
• m = E/c2
• E = energy
• m = mass
• c = speed of light
VII-IV
Energy and Mass
Einstein’s calculations show that photons doexhibit momentum, and are affected by gravity.However, it is important to recognize that thephoton is in no sense a typical particle. Aphoton has mass only in a relativistic sense- ithas no rest mass.
(Hence the (Hence the dualdual nature of light.) nature of light.)
VII-IV
Wavelength and Mass- Do allparticles exhibit wave properties?
• λ = wavelength, in m
• h = Planck’s constant, 6.626 × 10−34
J s = kg m2 s−1
• m = mass, in kg
• ν = frequency, in s−1
de de BroglieBroglie’’s s Equation- relates theEquation- relates thewavelength of a particle to itswavelength of a particle to itsmomentum.momentum.
VII-IV
Electromagnetic Radiation
VII-IV
Dual Nature of Light• Energy is quantized. It can be
transferred only in discrete units calledquanta.
• Electromagnetic radiation, which waspreviously though to exhibit only waveproperties, seems to show certaincharacteristics of particulate matter aswell.
VII-IV
Ephoton = 2.18 x 10-18 J x (1/25 - 1/9)
Ephoton = ΔE = -1.55 x 10-19 J
λ = 6.63 x 10-34 (J•s) x 3.00 x 108 (m/s)/1.55 x 10-19J
λ = 1280 nm
Calculate the wavelength (in nm) of a photonemitted by a hydrogen atom when its electrondrops from the n = 5 state to the n = 3 state.
Ephoton = h x c / λ
λ = h x c / Ephoton
i f
ΔE = RH( )1n2
1n2Ephoton =
VII-IV
De Broglie (1924) reasonedthat e- is both particle andwave.
2πr = nλ n=1,2,3,4,…λ = h/mu
u = velocity of e-
m = mass of e-
Why is e- energy quantized?
VII-IV
The Standing Waves Causedby the Vibration of a GuitarString Fastened at Both Ends
The HydrogenElectron Visualized asa Standing WaveAround the Nucleus
λ = h/mu
λ = 6.63 x 10-34 / (2.5 x 10-3 x 15.6)
λ = 1.7 x 10-32 m = 1.7 x 10-23 nm
What is the de Broglie wavelength (in nm)associated with a 2.5 g Ping-Pong balltraveling at 15.6 m/s?
m in kgh in J•s u in (m/s)
VII-IV
Wave models for electron orbitals
QuantumMechanics
VII-V