PHYS 408 Applied Optics (Lecture 15)

Slides:



Advertisements
Similar presentations
Class question: Why do we use Gaussian beams? One clue: there was no Gaussian beam before Answer 1: It is the simplest fundamental solution that.
Advertisements

Chapter 2 Propagation of Laser Beams
Nonlinear Optics Lab. Hanyang Univ. Chapter 2. The Propagation of Rays and Beams 2.0 Introduction Propagation of Ray through optical element : Ray (transfer)
 Light can take the form of beams that comes as close
Course outline Maxwell Eqs., EM waves, wave-packets
Fundamental of Optical Engineering Lecture 4.  Recall for the four Maxwell’s equation:
C F V Light In Side S > 0 Real Object Light Out Side S ’ > 0 Real Image C This Side, R > 0 S < 0 Virtual Object S ’ < 0 Virtual Image C This Side, R
PHYS 408 Applied Optics (Lecture 3) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
PHYS 408 Applied Optics (Lecture 4) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
Space-time analogy True for all pulse/beam shapes
GEOMETRICAL OPTICS. Laws of Reflection Laws of Refraction.
PHYS 408 Applied Optics (Lecture 11) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
Stability Diagram and Stability Criterions As described in textbooks for instance LASERS of A. E. Siegman, the stability diagram initially has been de-
Principal planes method For the purposes of finding images, we can reduce any* optical system to a thin lens. Principal plane distances p 1 and p 2 are.
PHYS 408 Applied Optics (Lecture 12) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
PHYS 408 Applied Optics (Lecture 16) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
PHYS 408 Applied Optics (Lecture 19) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
Announcements Exam 3 starts Thur noon, and continues through Mon close, in the Testing Center. It will include both conceptual questions and homework style.
PHYS 408 Applied Optics (Lecture 6) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
PHYS 408 Applied Optics (Lecture 20) JAN-APRIL 2016 EDITION JEFF YOUNG AMPEL RM 113.
Geometrical Optics.
PHYS 408 Applied Optics (Lecture 8)
PHYS 408 Applied Optics (Lecture 7)
PHYS 408 Applied Optics (Lecture 12)
PHYS 408 Applied Optics (Lecture 3)
Reflection & Mirrors.
PHYS 408 Applied Optics (Lecture 15)
Chapter 32Light: Reflection and Refraction
PHYS 408 Applied Optics (Lecture 16)
PHYS 408 Applied Optics (Lecture 21)
Physics 7E Prof. D. Casper.
Interaction of radiation with atoms and ions (I)
Thin lenses Lec. three.
SPHERICAL MIRROR EQUATIONS
Mirrors and Lenses Images can be formed by reflection from mirrors.
Geometric Optics Ray Model assume light travels in straight line
PHYS 408 Applied Optics (Lecture 17)
PHYS 408 Applied Optics (Lecture 8)
PHYS 408 Applied Optics (Lecture 14)
Reflection and Refraction
PHYS 408 Applied Optics (Lecture 13)
PHYS 408 Applied Optics (Lecture 2)
Mirrors, Plane and Spherical Spherical Refracting Surfaces
PHYS 408 Applied Optics (Lecture 7)
PHYS 408 Applied Optics (Lecture 13)
PHYS 408 Applied Optics (Lecture 14)
PHYS 408 Applied Optics (Lecture 18)
PHYS 408 Applied Optics (Lecture 17)
PHYS 408 Applied Optics (Lecture 9)
Scalar theory of diffraction
PHYS 408 Applied Optics (Lecture 10)
Chapter II The Propagation of Rays and Beams
PHYS 408 Applied Optics (Lecture 5)
Lasers, resonators, Gaussian beams
. y y’ A B a a’ = C D OPTICAL SYSTEM GEOMETRICAL OPTICS
Space-time analogy True for all pulse/beam shapes
Scalar theory of diffraction
PHYS 408 Applied Optics (Lecture 4)
PHYS 408 Applied Optics (Lecture 18)
PHYS 408 Applied Optics (Lecture 2)
Light and Lenses While Mirrors involve the reflection of light and the images we see, Lenses involve another property of light, refraction, or the effects.
PHYS 408 Applied Optics (Lecture 6)
PHYS 408 Applied Optics (Lecture 11)
The Thin-Lens Equation
Sándor Egri Physics 2 - Physics Sándor Egri
PHYS 408 Applied Optics (Lecture 20)
PHYS 408 Applied Optics (Lecture 21)
SPACE TIME Fourier transform in time Fourier transform in space.
PHYS 408 Applied Optics (Lecture 19)
SPHERICAL MIRROR EQUATIONS
Presentation transcript:

PHYS 408 Applied Optics (Lecture 15) Jan-April 2016 Edition Jeff Young AMPEL Rm 113

Quick review of key points from last lecture Using ABCD matrix elements to propagate Gaussian beams through optical systems is formally straight forward, but you have to be very aware of coordinate systems and conventions to get the right results. One can transform either q(z) or 1/q(z) using the ABCD matrix elements in slightly different ways. Both can provide useful insight and/or efficient ways of understanding the effect of the optical element on a Gaussian beam. A double-convex thin lens at the focus of one Gaussian input beam generates a second output Gaussian beam with a beam waist located not quite at the focal length away from the lens, and the beam waist is approximately equal to l f#, where the f# is the focal length f divided by the diameter of the lens.

Resonators/Cavities What is a resonator? Examples? From earlier in the course? Fabry-Perot (plane mirrors) Preface this change of topics with the fact we now have a bunch of tools that can be used to analyze resonators/cavities in more generality.

Generalize General considerations? Stability? Since paraxial, lateral size of mirrors limited, so for plane mirrors, any angular mismatch would be fatal, for example General considerations? Stability? Stability necessary, but is it sufficient? What else? Resonance Wavefunction/Eigenmode shape?

Stability Criterion How can we formulate a stability analysis using tools we have acquired? Like a differential equation, but called a difference equation.

Stability con’t

Stability con’t

Can do same with Gaussian beam First prove that the following geometry is self-consistent. See hand written notes…keep track of direction of z1 and z2! How?

Actually stable? R(z1) is the Gaussian convention and negative since assume Gaussian positive z direction is to the right. R1 uses ray optics convention and is negative also for a concave mirror, so they are both negative. R(z2) is positive, but R2 is still negative, hence the negative sign in 7.64

Stable? Have we completely determined the Gaussian parameters? Stability criterion?

Stability? Just because you know the field can be expanded as plane waves doesn’t mean they satisfy the boundary conditions. Does satisfying this stability criterion mean that any Gaussian with the “right parameters” would actually be a solution of the Maxwell Equations, for any l? Think of limit of plane mirrors?