OPTI 511R: OPTICAL PHYSICS & LASERS
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1 OPTI 511R: OPTICAL PHYSICS & LASERS Instructor: R. Jason Jones Office Hours: TBD Teaching Assistant: Robert Rockmore Office Hours: Wed. (TBD) h"p://wp.op)cs.arizona.edu/op)511r/
2 h"p://wp.op)cs.arizona.edu/op)511r/
3 OPTI 511R: OPTICAL PHYSICS & LASERS
4 h"p://wp.op)cs.arizona.edu/op)551r/
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7 Descriptions of Optics Geometrical Optics Physical Optics Quantum Optics à à à
8 Descriptions of Optics Geometrical Optics Physical Optics Quantum Optics à light as a ray à light as a wave à light as wave/particle
9 Models of Light-Matter Interaction Classical picture: classical light, classical matter Semi-classical picture: classical light, quantum matter Quantum picture: quantum light, quantum matter
10 Light, matter, and their interaction: overview of optical physics Quantum description of matter The semi-classical model Introduction to Quantum Optics Lasers
11 Overview Classical electron-oscillator model (~1900) Lorentz ad hoc hypothesis: atom responds as if it were attached to nucleus with a spring. NOT meant a model for the atom itself
12 Overview Classical electron-oscillator model (~1900) Lorentz ad hoc hypothesis: atom responds as if it were attached to nucleus with a spring.
13 Overview Classical electron-oscillator model (~1900) Lorentz ad hoc hypothesis: atom responds as if it were attached to nucleus with a spring.
14 Overview Classical electron-oscillator model (~1900) Lorentz ad hoc hypothesis: atom responds as if it were attached to nucleus with a spring.
15 Overview Classical electron-oscillator model (~1900) Lorentz ad hoc hypothesis: atom responds as if it were attached to nucleus with a spring.
16 Overview Classical electron-oscillator model (~1900) Lorentz ad hoc hypothesis: atom responds as if it were attached to nucleus with a spring. Why?
17 Overview Classical electron-oscillator model (~1900) Lorentz ad hoc hypothesis: atom responds as if it were attached to nucleus with a spring. Damped & driven simple harmonic oscillator:
18 Overview Classical electron-oscillator model (~1900) Lorentz ad hoc hypothesis: atom responds as if it were attached to nucleus with a spring. Damped & driven simple harmonic oscillator:
19 Overview Predictions of the CEO model: From E&M:
20 Overview Predictions of the CEO model: From E&M: index of refractionà absorption, dispersion Rayleigh Scattering
21 Overview Predictions of the CEO model: From E&M: index of refractionà absorption, dispersion Rayleigh Scattering However, fails to predict: saturation, optical gain, spontaneous emission à We need a better model for the atom!
22 Quantum matter Elements of quantum theory Wave equations for light and matter Quantum description of the atom
23 Quantum matter Elements of quantum theory Wave equations for light and matter Quantum description of the atom
24 Quantum matter Historical events in the development of quantum theory
25 Quantum matter Historical events in the development of quantum theory
26 Quantum matter Historical events in the development of quantum theory
27 Quantum matter Historical events in the development of quantum theory
28 Quantum matter Historical events in the development of quantum theory 1924: de Broglie and wave-particle duality of matter
29 Quantum matter Historical events in the development of quantum theory 1924: de Broglie and wave-particle duality of matter
30 Quantum matter Analogy with classical light waves
31 2-slit diffraction of light Quantum matter
32 2-slit diffraction of light Quantum matter
33 Quantum matter 1927: Davisson & Germer experiment à electron diffraction
34 Quantum matter Historical events in the development of quantum theory 1901: Planck and Blackbody Radiation 1905: Einstein and the photoelectric effect 1913: Bohr model of the atom 1924: de Broglie and wave-particle duality of matter 1927: Davisson & Germer experiment Wave-particle duality of light Atomic energy levels Electron diffraction
35 Quantum matter How to describe the matter waves?
36 Quantum matter Some postulates of quantum mechanics: The wavefunction for a particle tells us everything we can know about that particle.
37 Quantum matter Some postulates of quantum mechanics: The wavefunction for a particle tells us everything we can know about that particle.
38 Quantum matter Analogy with classical light waves
39 Quantum matter Analogy with classical light waves Wave equation for light
40 Quantum matter Analogy with classical light waves Plane waves Wave equation for light Spherical waves
41 Quantum matter Analogy with classical light waves Plane waves Wave equation for light Spherical waves
42 Quantum matter Some postulates of quantum mechanics: The Schrodinger equation describes the time evolution of the wavefunction. à The wave equation for matter!
43 Quantum matter For time-independent problems, it can be shown
44 Quantum matter For example, if it is a free particle (V=0)
45 Quantum matter For example, if it is a free particle (V=0)
46 Quantum matter For example, if it is a free particle (V=0)
47 Free particle continued Quantum matter
48 Free particle continued Quantum matter
49 Free particle continued Quantum matter
50 Free particle continued Quantum matter
51 Free particle continued Quantum matter
52 Quantum matter Now consider these two wavefunctions:
53 Quantum matter Now consider these two wavefunctions:
54 Quantum matter Now consider these two wavefunctions:
55 Quantum matter Now consider these two wavefunctions:
56 Quantum matter Now consider these two wavefunctions:
57 Quantum matter Now consider these two wavefunctions:
58 Quantum matter Quantum model of the hydrogen atom
59 Quantum matter Quantum model of the hydrogen atom
60 Quantum matter Quantum model of the hydrogen atom
61 Quantum matter Quantum model of the hydrogen atom Rydberg formula:
62 Quantum matter Quantum model of the hydrogen atom Rydberg formula: Spectroscopy can directly test quantum theory
63 Semi-classical model of light-matter interaction Quantum model of the hydrogen atom But it s not quite so simple
64 Semi-classical model of light-matter interaction Quantum model of the hydrogen atom But it s not quite so simple electron spin and orbital angular momentum (relativistic effects)
65 Semi-classical model of light-matter interaction Quantum model of the hydrogen atom But it s not quite so simple electron spin and orbital angular momentum (relativistic effects)
66 Semi-classical model of light-matter interaction Quantum model of the hydrogen atom But it s not quite so simple empty space is not so empty àvacuum fluctuations
67 Semi-classical model of light-matter interaction Quantum model of the hydrogen atom But it s not quite so simple proton spin interacts with the total electron angular momentum
68 Semi-classical model of light-matter interaction Quantum model of the hydrogen atom But it s not quite so simple proton spin interacts with the total electron angular momentum Precision spectroscopy required for testingà ultrastable lasers, cooling, trapping
69 Quantum matter Current example: the proton radius puzzle hydrogen vs. muonic hydrogen vs
70 Semi-classical model of light-matter interaction
71 Semi-classical model of light-matter interaction Classical light field - quantum atom: solve the full Schrodinger equation
72 Semi-classical model of light-matter interaction Classical light field - quantum atom: solve the full Schrodinger equation
73 Semi-classical model of light-matter interaction Semi-classical picture predicts: -real atom with discrete energy levels (infinite lifetime) n=1 n=2
74 Semi-classical model of light-matter interaction Semi-classical picture predicts: -real atom with discrete energy levels (infinite lifetime) -optical absorption -optical gain n=1 n=2 à dipole selection rules
75 Semi-classical model of light-matter interaction Semi-classical picture predicts: -real atom with discrete energy levels (infinite lifetime) -optical absorption -optical gain n=1 n=2 à dipole selection rules -saturation of absorption or gain
76 Semi-classical model of light-matter interaction Semi-classical picture predicts: -real atom with discrete energy levels (infinite lifetime) -optical absorption -optical gain n=1 n=2 à dipole selection rules -saturation of absorption or gain spontaneous emission?
77 Semi-classical model of light-matter interaction Semi-classical picture predicts: -real atom with discrete energy levels (infinite lifetime) -optical absorption -optical gain n=1 n=2 à dipole selection rules -saturation of absorption or gain spontaneous emission?
78 Lasers Light Amplification by Stimulated Emission of Radiation Basic elements:
79 Lasers Light Amplification by Stimulated Emission of Radiation Basic elements:
80 Lasers Light Amplification by Stimulated Emission of Radiation Basic elements:
81 Lasers Light Amplification by Stimulated Emission of Radiation Basic elements:
82 Optical cavities & Gaussian beams Lasers
83 Lasers Optical cavities & Gaussian beams Resonant modes of the optical cavity: -find solutions of the wave equation given certain approximations and boundary conditions
84 Lasers Optical cavities & Gaussian beams Resonant modes of the optical cavity: -find solutions of the wave equation given certain approximations and boundary conditions
85 Lasers Optical cavities & Gaussian beams Resonant modes of the optical cavity: -find solutions of the wave equation given certain approximations and boundary conditions paraxial approximation Paraxial wave equation
86 Lasers Solutions to the paraxial wave equation: Paraxial wave equation
87 Lasers Solutions to the paraxial wave equation: Paraxial wave equation Example: Hermite-Gaussian polynomials
88 Lasers Optical gain: need at least 3 energy levels to have more gain than absorption
89 Lasers Optical gain: need at least 3 energy levels to have more gain than absorption
90 Lasers Optical gain: need at least 3 energy levels to have more gain than absorption Rate equations determine population densities i.e. pumping rate, decay rate, emission rate
91 Lasers Steady-state lasing: gain requires population inversion initial field provided by spontaneous emission power in field grows until it significantly reduces population in level 2 à gain saturation steady-state lasing threshold is reach when round-trip gain = round-trip losses
OPTI 511R: OPTICAL PHYSICS & LASERS
OPTI 511R: OPTICAL PHYSICS & LASERS Instructor: R. Jason Jones Office Hours: Monday 1-2pm Teaching Assistant: Sam Nerenburg Office Hours: Wed. (TBD) h"p://wp.op)cs.arizona.edu/op)551r/ h"p://wp.op)cs.arizona.edu/op)551r/
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