Atomic Physics - PowerPoint PPT Presentation

1 / 42
About This Presentation
Title:

Atomic Physics

Description:

Atomic Physics Quantization of Energy Atomic Models Quantum Mechanics Matter Waves Frequency of matter waves can be found with Planck s equation Evidence for Matter ... – PowerPoint PPT presentation

Number of Views:2935
Avg rating:5.0/5.0
Slides: 43
Provided by: Prefer397
Category:
Tags: atomic | physics

less

Transcript and Presenter's Notes

Title: Atomic Physics


1
Atomic Physics
  • Quantization of Energy
  • Atomic Models
  • Quantum Mechanics

2
Electric and Magnetic FieldsSummary
  • A changing magnetic field can induce a current in
    a circuit (Faradays Law of Induction)
  • A magnetic field is created around a
    current-carrying wire (Amperes Law)
  • Electric field lines start on positive charges
    and end at negative charges (Coulombs Law /
    Gausss Law)
  • Magnetic field lines always form closed loops
    with no beginning and no end (Gausss Law for
    magnetism)
  • These unrelated observations, experiments and
    equations were all known by the mid-1800s, but
    nothing linked them together.

3
Maxwells Equations
  • James Clerk Maxwell (1831-1879)
  • Scottish theoretical physicist mathematician
  • Maxwells Equations
  • Set of differential equations that describe the
    relationship between electric and magnetic field
  • Summarized all previous work of Coulomb, Ampere,
    Gauss, Faraday others

4
Maxwells Equations
Relax!!! You dont need to use these.
5
Maxwells Equations
  • Predicted
  • a changing magnetic field would create a changing
    electric field, which would, in turn, create a
    changing magnetic field, and so on
  • existence of electromagnetic waves that move
    through space at the speed of light
  • light is an electromagnetic wave
  • Confirmed
  • Heinrich Hertz in 1887
  • generated and detected the first E/M waves

6
Electromagnetic Waves
  • Oscillating electric and magnetic fields
  • E-field and B-field are at right angles to each
    other
  • Propagates at a right angle to both fields
    (transverse wave)

7
Electromagnetic Waves
  • EM waves can be produced most easily by an
    oscillating charged particle
  • Frequency of oscillation determines frequency of
    the EM wave
  • Wavelength related to frequency by

8
Electromagnetic Radiation
  • Energy is the ability to do work
  • E-fields B-fields store energy because they
    exert a force (do work) on charged particles
  • Electromagnetic Radiation
  • transfer of energy associated with electric and
    magnetic fields
  • can be transferred to objects in the EM waves
    path
  • can be converted to other forms, such as heat
  • Continuous distribution of wavelengths on the
    electromagnetic spectrum.

9
Electromagnetic Spectrum
10
Blackbody Radiation
  • All objects emit electromagnetic radiation
  • Continuous distribution of wavelengths from the
    infrared, visible, and UV portions of the EM
    spectrum
  • Intensity distribution of different wavelengths
    varies with temperature
  • At low temps mostly infrared (invisible)
  • Temp increases distribution shifts to visible
    UV
  • Metals glow red gt yellow gt white gt blue

11
Blackbody Radiation
  • Most objects absorb some incoming radiation and
    reflect the rest
  • Blackbody
  • Ideal system that absorbs all incoming radiation
  • Hollow object with a small opening
  • Perfect absorber and perfect radiator
  • Emits radiation based only on its temperature
  • In 1900, Max Planck (1858-1947), proposed that
    the walls of a blackbody contained billions of
    submicroscopic electric oscillators, which he
    called resonators. These resonators, produced the
    blackbody radiation.

12
Blackbody Radiation
13
Quantization of Energy
  • Planck found that the total energy of a resonator
    is an integer multiple of the frequency
  • Because the energy of each resonator comes in
    discrete units, it is said to be quantized.
  • Allowed energy states are called quantum states
    or energy levels.
  • Einstein applied the concept of quantized energy
    to light.
  • Photon quantized unit of light energy
  • Photons are absorbed or given off by electrons
    jumping from one quantum state to another.

14
Quantization of Energy
15
The Photoelectric Effect
When light strikes a metal surface, the surface
may emit electrons, called photoelectrons.
  • Classical physics predicts
  • Light waves of any frequency should have enough
    energy to eject electrons if the intensity is
    high enough
  • At low intensities, electrons should be ejected
    if light shines on the metal for a long enough
    period of time
  • Increasing the intensity of the light waves
    should increase the kinetic energy of the
    photoelectrons.
  • Maximum kinetic energy of a photoelectron should
    be determined by the lights intensity

16
The Photoelectric Effect
  • Experimental evidence shows that
  • No photoelectrons emitted if the light frequency
    falls below a certain threshold frequency, even
    if the intensity is very high
  • Threshold frequency, ft, depends on material
  • If light frequency exceeds ft
  • of photoelectrons emitted is proportional to
    light intensity
  • Maximum kinetic energy of photoelectrons is
    proportional to the frequency and is independent
    of the intensity
  • Electrons are emitted instantaneously, even at
    low intensities
  • Classical physics could not explain the
    photoelectric effect but Einstein could!

17
Einsteins Explanation
  • EM waves are quantized
  • Think of light as a stream of particles, called
    photons
  • Photon energy given by Plancks equation
  • When photons collide with electrons in metal,
    they transfer energy to electrons

18
Einsteins Explanation
  • If photon energy is greater than work function of
    the metal, photoelectrons are ejected
  • If photon has more energy than the work function,
    the difference is the kinetic energy of the
    photoelectrons ejected from the surface

19
Maximum KE of Photoelectrons
20
Compton Shift
  • American physicist Arthur Compton (1892-1962)
    proposed that momentum energy should be
    conserved in a collision between photons
    electrons
  • After a collision, scattered photon should have a
    lower energy, therefore a lower frequency (longer
    wavelength)
  • In 1923, conducted experiments with X rays to
    demonstrate this change in wavelength, known as
    Compton shift.

21
Models of the Atom
  • Thomson Model / Plum Pudding Model
  • Discovery of electron in 1897
  • Negative electrons in sphere of positive charge

22
Models of the Atom
  • Rutherford Model / Planetary Model
  • 1911 experiment by Geiger Marsden demonstrated
    that practically all of atoms mass and all
    positive charge must be centrally located in atom
    (nucleus)
  • Electrons orbit nucleus like planets around Sun

23
Problems with theRutherford Model
  • Electrons orbiting the nucleus would undergo
    centripetal acceleration
  • Accelerating electrons would radiate EM waves
  • Electrons radiating EM waves would lose energy
  • Loss of energy would cause electrons orbital
    radius to drop
  • Frequency of emitted radiation would increase
  • Electrons would rapidly collapse into nucleus
  • Need a better model!

24
Atomic Spectra
  • Fill a glass tube with pure atomic gas
  • Apply a high voltage between electrodes
  • Current flows through gas tube glows
  • Color depends on type of gas
  • Light emitted is composed of only certain
    wavelengths

25
Atomic Spectra
  • Emission Spectrum diagram or graph that
    indicates the wavelengths of radiant energy that
    a substance emits (bright lines)
  • Absorption Spectrum same thing, just for light
    absorbed by a substance (dark lines)
  • What does this have to do with atomic models?

26
The Bohr Model
  • Similar to Rutherfords model, but only allows
    certain, discrete orbits
  • Electrons are never found between orbits, but can
    jump from one orbit to another
  • Electrons only emit radiation when they jump from
    an outer orbit to an inner one
  • Energy of emitted photon is equal to energy
    decrease of electron. This determines frequency
    of emitted radiation.
  • Energy of emitted photon is quantized only
    certain quantities are allowed. Hence, electrons
    undergo quantum leaps. (Obligatory pop culture
    reference)

27
Energy Levels Emission Spectra
  • Lowest energy state ground state
  • Radius of this state Bohr radius
  • Electrons usually here at ordinary temps
  • How do electrons jump between states?
  • Absorb photon with energy (hf) exactly equal to
    energy difference between ground state excited
    state
  • Absorbed photons account for dark lines in
    absorption spectrum

28
Energy Levels Emission Spectra
  • Spontaneous emission
  • Electron in excited state jumps back to a lower
    energy level by emitting a photon
  • Does NOT need to jump all the way back to the
    ground state
  • Emitted photon has energy equal to energy
    difference between levels
  • Accounts for bright lines on emission spectrum
  • Jumps between different energy levels correspond
    to various spectral lines

29
The Bohr Model
  • Successes
  • Failures
  • Account for wavelengths of all spectral lines of
    hydrogen
  • Provides explanation for auroras
  • Gave expression for radius of hydrogen atom
  • Predicted energy levels of hydrogen
  • Also successful when applied to hydrogen-like
    atoms (only one electron)
  • Unsuccessful when applied to multi-electron atoms
  • Did not explain why electrons do not radiate
    energy when in a stable orbit
  • Did not explain why other orbits do not occur
  • Combined classical and non-classical physics

30
The Dual Nature of Light
  • Is light a particle or a wave?
  • Particle blackbody radiation, photoelectric
    effect
  • Wave interference, diffraction
  • Which model is correct?
  • Both are correct, but depends on the situation
  • Each phenomenon exhibits only one or the other
    natures of light
  • True nature of light is not describable in terms
    of a single classical idea

31
The Dual Nature of Light
  • Low Frequency Light
  • (Wave Nature)
  • High Frequency Light
  • (Photon Nature)
  • Very low energy
  • Difficult to detect a single photon
  • Photon nature of light not evident
  • Long wavelength
  • Wave effects, like diffraction and interference
    are easy to observe
  • Very high energy
  • Easy to detect single photons
  • Photon nature of light is evident
  • Short wavelength
  • Wave effects, like diffraction and interference
    are more difficult to observe

32
Matter Waves
  • Since light can be described as either a particle
    or a wave, can we do the same for all objects,
    like atoms and people and cars?
  • Louis de Broglie thought so!
  • In 1924, proposed that all matter may have wave
    properties and particle properties
  • Matter has a dual nature, just like light!
  • Proposed idea of matter waves

33
Matter Waves
  • The larger the momentum of an object, the smaller
    its wavelength

34
Matter Waves
  • Frequency of matter waves can be found with
    Plancks equation

35
Evidence for Matter Waves
  • 1927 Davisson Germer, showed that electrons
    can be diffracted by a single crystal of nickel
  • Electron diffraction is possible because the de
    Broglie wavelength of an electron is approx.
    equal to distance between atoms (the size of the
    diffraction grating)
  • Large-scale objects dont demonstrate this well
    because large momentum generates wavelengths much
    smaller than any possible aperture through which
    the object could pass (wont be diffracted)

36
Bohr Model Explained
  • De Broglie hypothesized that only certain
    electron orbits are stable
  • Circumference of orbit must contain an integral
    multiple of electron wavelengths
  • Similar to standing waves on a string

37
The Uncertainty Principle
  • Wave nature of particles restricts the precision
    of our measurements
  • Werner Heisenberg (1927)
  • It is fundamentally impossible to make
    simultaneous measurements of a particles
    position and momentum with infinite accuracy
  • The more we learn about a particles momentum,
    the less we know of its position, and vice versa.

38
The Uncertainty PrincipleA Thought Experiment
  • Imagine trying to measure an electrons position
    and momentum with a powerful microscope
  • In order to see the electron, thereby determining
    its location, at least one photon of light must
    bounce off the electron and pass through the
    microscope to your eye
  • When the photon strikes the electron, it
    transfers some energy momentum to the electron.
    So we are less sure of the electrons momentum.

39
The Uncertainty PrincipleA Thought Experiment
40
Schrodingers Wave Equation
  • Erwin Schrodinger (1926) proposed a wave equation
    for de Broglies matter waves
  • Each particle can be represented by a wave
    function , ?, dependent on the position of the
    particle and time

41
The Electron Cloud
  • Max Born (1926) interpreted Schrodingers wave
    function to show probability of finding an
    electron at certain locations
  • ?2 is proportional to probability of finding
    the electron at a certain position
  • Peak probability for an electron in the ground
    state corresponds to Bohr radius

42
Quantum Mechanical Model
  • Electrons are not confined to particular orbital
    distances as assumed in Bohr model
  • Electron cloud a probability cloud
  • Density at each location related to probability
    of finding electron at that location
  • Wave function predicts geometry for energy levels
    (some spherical, others more complex)
  • Most probable location still corresponds to Bohr
    radii, but impossible to determine actual
    location
  • Mathematical picture of the atom that explains
    certain aspects of atomic structure that Bohr
    model cannot explain
Write a Comment
User Comments (0)
About PowerShow.com