Introduction to X-Ray Diffraction Physics Wave Properties
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Glossary Physics (I-Introduction)
1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay. -
25 Geometric Optics
CHAPTER 25 | GEOMETRIC OPTICS 887 25 GEOMETRIC OPTICS Figure 25.1 Image seen as a result of reflection of light on a plane smooth surface. (credit: NASA Goddard Photo and Video, via Flickr) Learning Objectives 25.1. The Ray Aspect of Light • List the ways by which light travels from a source to another location. 25.2. The Law of Reflection • Explain reflection of light from polished and rough surfaces. 25.3. The Law of Refraction • Determine the index of refraction, given the speed of light in a medium. 25.4. Total Internal Reflection • Explain the phenomenon of total internal reflection. • Describe the workings and uses of fiber optics. • Analyze the reason for the sparkle of diamonds. 25.5. Dispersion: The Rainbow and Prisms • Explain the phenomenon of dispersion and discuss its advantages and disadvantages. 25.6. Image Formation by Lenses • List the rules for ray tracking for thin lenses. • Illustrate the formation of images using the technique of ray tracking. • Determine power of a lens given the focal length. 25.7. Image Formation by Mirrors • Illustrate image formation in a flat mirror. • Explain with ray diagrams the formation of an image using spherical mirrors. • Determine focal length and magnification given radius of curvature, distance of object and image. Introduction to Geometric Optics Geometric Optics Light from this page or screen is formed into an image by the lens of your eye, much as the lens of the camera that made this photograph. Mirrors, like lenses, can also form images that in turn are captured by your eye. 888 CHAPTER 25 | GEOMETRIC OPTICS Our lives are filled with light. -
Multidisciplinary Design Project Engineering Dictionary Version 0.0.2
Multidisciplinary Design Project Engineering Dictionary Version 0.0.2 February 15, 2006 . DRAFT Cambridge-MIT Institute Multidisciplinary Design Project This Dictionary/Glossary of Engineering terms has been compiled to compliment the work developed as part of the Multi-disciplinary Design Project (MDP), which is a programme to develop teaching material and kits to aid the running of mechtronics projects in Universities and Schools. The project is being carried out with support from the Cambridge-MIT Institute undergraduate teaching programe. For more information about the project please visit the MDP website at http://www-mdp.eng.cam.ac.uk or contact Dr. Peter Long Prof. Alex Slocum Cambridge University Engineering Department Massachusetts Institute of Technology Trumpington Street, 77 Massachusetts Ave. Cambridge. Cambridge MA 02139-4307 CB2 1PZ. USA e-mail: [email protected] e-mail: [email protected] tel: +44 (0) 1223 332779 tel: +1 617 253 0012 For information about the CMI initiative please see Cambridge-MIT Institute website :- http://www.cambridge-mit.org CMI CMI, University of Cambridge Massachusetts Institute of Technology 10 Miller’s Yard, 77 Massachusetts Ave. Mill Lane, Cambridge MA 02139-4307 Cambridge. CB2 1RQ. USA tel: +44 (0) 1223 327207 tel. +1 617 253 7732 fax: +44 (0) 1223 765891 fax. +1 617 258 8539 . DRAFT 2 CMI-MDP Programme 1 Introduction This dictionary/glossary has not been developed as a definative work but as a useful reference book for engi- neering students to search when looking for the meaning of a word/phrase. It has been compiled from a number of existing glossaries together with a number of local additions. -
9.2 Refraction and Total Internal Reflection
9.2 refraction and total internal reflection When a light wave strikes a transparent material such as glass or water, some of the light is reflected from the surface (as described in Section 9.1). The rest of the light passes through (transmits) the material. Figure 1 shows a ray that has entered a glass block that has two parallel sides. The part of the original ray that travels into the glass is called the refracted ray, and the part of the original ray that is reflected is called the reflected ray. normal incident ray reflected ray i r r ϭ i air glass 2 refracted ray Figure 1 A light ray that strikes a glass surface is both reflected and refracted. Refracted and reflected rays of light account for many things that we encounter in our everyday lives. For example, the water in a pool can look shallower than it really is. A stick can look as if it bends at the point where it enters the water. On a hot day, the road ahead can appear to have a puddle of water, which turns out to be a mirage. These effects are all caused by the refraction and reflection of light. refraction The direction of the refracted ray is different from the direction of the incident refraction the bending of light as it ray, an effect called refraction. As with reflection, you can measure the direction of travels at an angle from one medium the refracted ray using the angle that it makes with the normal. In Figure 1, this to another angle is labelled θ2. -
Linear Elastodynamics and Waves
Linear Elastodynamics and Waves M. Destradea, G. Saccomandib aSchool of Electrical, Electronic, and Mechanical Engineering, University College Dublin, Belfield, Dublin 4, Ireland; bDipartimento di Ingegneria Industriale, Universit`adegli Studi di Perugia, 06125 Perugia, Italy. Contents 1 Introduction 3 2 Bulk waves 6 2.1 Homogeneous waves in isotropic solids . 8 2.2 Homogeneous waves in anisotropic solids . 10 2.3 Slowness surface and wavefronts . 12 2.4 Inhomogeneous waves in isotropic solids . 13 3 Surface waves 15 3.1 Shear horizontal homogeneous surface waves . 15 3.2 Rayleigh waves . 17 3.3 Love waves . 22 3.4 Other surface waves . 25 3.5 Surface waves in anisotropic media . 25 4 Interface waves 27 4.1 Stoneley waves . 27 4.2 Slip waves . 29 4.3 Scholte waves . 32 4.4 Interface waves in anisotropic solids . 32 5 Concluding remarks 33 1 Abstract We provide a simple introduction to wave propagation in the frame- work of linear elastodynamics. We discuss bulk waves in isotropic and anisotropic linear elastic materials and we survey several families of surface and interface waves. We conclude by suggesting a list of books for a more detailed study of the topic. Keywords: linear elastodynamics, anisotropy, plane homogeneous waves, bulk waves, interface waves, surface waves. 1 Introduction In elastostatics we study the equilibria of elastic solids; when its equilib- rium is disturbed, a solid is set into motion, which constitutes the subject of elastodynamics. Early efforts in the study of elastodynamics were mainly aimed at modeling seismic wave propagation. With the advent of electron- ics, many applications have been found in the industrial world. -
1 Fundamental Solutions to the Wave Equation 2 the Pulsating Sphere
1 Fundamental Solutions to the Wave Equation Physical insight in the sound generation mechanism can be gained by considering simple analytical solutions to the wave equation. One example is to consider acoustic radiation with spherical symmetry about a point ~y = fyig, which without loss of generality can be taken as the origin of coordinates. If t stands for time and ~x = fxig represent the observation point, such solutions of the wave equation, @2 ( − c2r2)φ = 0; (1) @t2 o will depend only on the r = j~x − ~yj. It is readily shown that in this case (1) can be cast in the form of a one-dimensional wave equation @2 @2 ( − c2 )(rφ) = 0: (2) @t2 o @r2 The general solution to (2) can be written as f(t − r ) g(t + r ) φ = co + co : (3) r r The functions f and g are arbitrary functions of the single variables τ = t± r , respectively. ± co They determine the pattern or the phase variation of the wave, while the factor 1=r affects only the wave magnitude and represents the spreading of the wave energy over larger surface as it propagates away from the source. The function f(t − r ) represents an outwardly co going wave propagating with the speed c . The function g(t + r ) represents an inwardly o co propagating wave propagating with the speed co. 2 The Pulsating Sphere Consider a sphere centered at the origin and having a small pulsating motion so that the equation of its surface is r = a(t) = a0 + a1(t); (4) where ja1(t)j << a0. -
Light Bending and X-Ray Echoes from Behind a Supermassive Black Hole D.R
Light bending and X-ray echoes from behind a supermassive black hole D.R. Wilkins1*, L.C. Gallo2, E. Costantini3,4, W.N. Brandt5,6,7 and R.D. Blandford1 1Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA 2Department of Astronomy & Physics, Saint Mary’s University, Halifax, NS. B3H 3C3, Canada 3SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands 4Anton Pannekoeck Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands 5Department of Astronomy and Astrophysics, 525 Davey Lab, The Pennsylvania State University, University Park, PA 16802, USA 6Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA 7Department of Physics, 104 Davey Lab, The Pennsylvania State University, University Park, PA 16802, USA *Corresponding author. E-mail: [email protected] Preprint version. Submitted to Nature 14 August 2020, accepted 24 May 2021 The innermost regions of accretion disks around black holes are strongly irradiated by X-rays that are emitted from a highly variable, compact corona, in the immediate vicinity of the black hole [1, 2, 3]. The X-rays that are seen reflected from the disk [4] and the time delays, as variations in the X-ray emission echo or ‘reverberate’ off the disk [5, 6] provide a view of the environment just outside the event horizon. I Zwicky 1 (I Zw 1), is a nearby narrow line Seyfert 1 galaxy [7, 8]. Previous studies of the reverberation of X-rays from its accretion disk revealed that the corona is composed of two components; an extended, slowly varying component over the surface of the inner accretion disk, and a collimated core, with luminosity fluctuations propagating upwards from its base, which dominates the more rapid variability [9, 10]. -
Physics-272 Lecture 21
Physics-272Physics-272 Lecture Lecture 21 21 Description of Wave Motion Electromagnetic Waves Maxwell’s Equations Again ! Maxwell’s Equations James Clerk Maxwell (1831-1879) • Generalized Ampere’s Law • And made equations symmetric: – a changing magnetic field produces an electric field – a changing electric field produces a magnetic field • Showed that Maxwell’s equations predicted electromagnetic waves and c =1/ √ε0µ0 • Unified electricity and magnetism and light . Maxwell’s Equations (integral form) Name Equation Description Gauss’ Law for r r Q Charge and electric Electricity ∫ E ⋅ dA = fields ε0 Gauss’ Law for r r Magnetic fields Magnetism ∫ B ⋅ dA = 0 r r Electrical effects dΦB from changing B Faraday’s Law ∫ E ⋅ ld = − dt field Ampere’s Law r Magnetic effects dΦE from current and (modified by ∫ B ⋅ dl = µ0ic + ε0 Maxwell) dt Changing E field All of electricity and magnetism is summarized by Maxwell’s Equations. On to Waves!! • Note the symmetry now of Maxwell’s Equations in free space, meaning when no charges or currents are present r r r r ∫ E ⋅ dA = 0 ∫ B ⋅ dA = 0 r r dΦ r dΦ ∫ E ⋅ ld = − B B ⋅ dl = µ ε E dt ∫ 0 0 dt • Combining these equations leads to wave equations for E and B, e.g., ∂2E ∂ 2 E x= µ ε x ∂z20 0 ∂ t 2 • Do you remember the wave equation??? 2 2 ∂h1 ∂ h h is the variable that is changing 2= 2 2 in space (x) and time ( t). v is the ∂x v ∂ t velocity of the wave. Review of Waves from Physics 170 2 2 • The one-dimensional wave equation: ∂h1 ∂ h 2= 2 2 has a general solution of the form: ∂x v ∂ t h(x,t) = h1(x − vt ) + h2 (x + vt ) where h1 represents a wave traveling in the +x direction and h2 represents a wave traveling in the -x direction. -
EE1.El3 (EEE1023): Electronics III Acoustics Lecture 12 Principles Of
EE1.el3 (EEE1023): Electronics III Acoustics lecture 12 Principles of sound Dr Philip Jackson www.ee.surrey.ac.uk/Teaching/Courses/ee1.el3 Overview for this semester 1. Introduction to sound 2. Human sound perception 3. Noise measurement 4. Sound wave behaviour 5. Reflections and standing waves 6. Room acoustics 7. Resonators and waveguides 8. Musical acoustics 9. Sound localisation L.1 Introduction to sound • Definition of sound • Vibration of matter { transverse waves { longitudinal waves • Sound wave propagation { plane waves { pure tones { speed of sound L.2 Preparation for Acoustics • What is a sound wave? { look up a definition of sound and its properties • Example of a device for manipulating sound { write down or draw your example { explain how it modifies the sound L.3 Definitions of sound \Sensation caused in the ear by the vibration of the surrounding air or other medium", Oxford En- glish Dictionary \Disturbances in the air caused by vibrations, in- formation on which is transmitted to the brain by the sense of hearing", Chambers Pocket Dictionary \Sound is vibration transmitted through a solid, liquid, or gas; particularly, sound means those vi- brations composed of frequencies capable of being detected by ears", Wikipedia L.4 Vibration of a string Let us consider forces on an element of the vibrating string with tension T and ρL mass per unit length, to derive its equation of motion T y + dy dx dx y ds θ dy x y dx T x x + dx Net vertical force from tension between points x and x + dx: dFY = (T sin θ)x+dx − (T sin θ)x (1) Taylor -
Music 170 Assignment 7 1. a Sinusoidal Plane Wave at 20 Hz
Music 170 assignment 7 1. A sinusoidal plane wave at 20 Hz. has an SPL of 80 decibels. What is the RMS displacement (in millimeters.) of air (in other words, how far does the air move)? 2. A rectangular vibrating surface one foot long is vibrating at 2000 Hz. Assuming the speed of sound is 1000 feet per second, at what angle off axis should the beam's amplitude drop to zero? 3. How many dB less does a cardioid microphone pick up from an incoming sound 90 degrees (π=2 radians) off-axis, compared to a signal coming in frontally (at the angle of highest gain)? 4. Suppose a sound's SPL is 0 dB (i.e., it's about the threshold of hearing at 1 kHz.) What is the total power that you ear receives? (Assume, a bit generously, that the opening is 1 square centimeter). 5. If light moves at 3 · 108 meters per second, and if a certain color has a wavelength of 500 nanometers (billionths of a meter - it would look green to human eyes), what is the frequency? Would it be audible if it were a sound? [NOTE: I gave the speed of light incorrectly (mixed up the units, ouch!) - we'll accept answers based on either the right speed or the wrong one I first gave.] 6. A speaker one meter from you is paying a tone at 440 Hz. If you move to a position 2 meters away (and then stop moving), at what pitch to you now hear the tone? (Hint: don't think too hard about this one). -
Reflections and Refractions in Ray Tracing
Reflections and Refractions in Ray Tracing Bram de Greve ([email protected]) November 13, 2006 Abstract materials could be air (η ≈ 1), water (20◦C: η ≈ 1.33), glass (crown glass: η ≈ 1.5), ... It does not matter which refractive index is the greatest. All that counts is that η is the refractive When writing a ray tracer, sooner or later you’ll stumble 1 index of the material you come from, and η of the material on the problem of reflection and transmission. To visualize 2 you go to. This (very important) concept is sometimes misun- mirror-like objects, you need to reflect your viewing rays. To derstood. simulate a lens, you need refraction. While most people have heard of the law of reflection and Snell’s law, they often have The direction vector of the incident ray (= incoming ray) is i, difficulties with actually calculating the direction vectors of and we assume this vector is normalized. The direction vec- the reflected and refracted rays. In the following pages, ex- tors of the reflected and transmitted rays are r and t and will actly this problem will be addressed. As a bonus, some Fres- be calculated. These vectors are (or will be) normalized as nel equations will be added to the mix, so you can actually well. We also have the normal vector n, orthogonal to the in- calculate how much light is reflected or transmitted (yes, it’s terface and pointing towards the first material η1. Again, n is possible). At the end, you’ll have some usable formulas to use normalized. -
4.4 Total Internal Reflection
n 1:33 sin θ = water sin θ = sin 35◦ ; air n water 1:00 air i.e. ◦ θair = 49:7 : Thus, the height above the horizon is ◦ ◦ θ = 90 θair = 40:3 : (4.7) − Because the sun is far away from the fisherman and the diver, the fisherman will see the sun at the same angle above the horizon. 4.4 Total Internal Reflection Suppose that a light ray moves from a medium of refractive index n1 to one in which n1 > n2, e.g. glass-to-air, where n1 = 1:50 and n2 = 1:0003. ◦ If the angle of incidence θ1 = 10 , then by Snell's law, • n 1:50 θ = sin−1 1 sin θ = sin−1 sin 10◦ 2 n 1 1:0003 2 = sin−1 (0:2604) = 15:1◦ : ◦ If the angle of incidence is θ1 = 50 , then by Snell's law, • n 1:50 θ = sin−1 1 sin θ = sin−1 sin 50◦ 2 n 1 1:0003 2 = sin−1 (1:1487) =??? : ◦ So when θ1 = 50 , we have a problem: Mathematically: the angle θ2 cannot be computed since sin θ2 > 1. • 142 Physically: the ray is unable to refract through the boundary. Instead, • 100% of the light reflects from the boundary back into the prism. This process is known as total internal reflection (TIR). Figure 8672 shows several rays leaving a point source in a medium with re- fractive index n1. Figure 86: The refraction and reflection of light rays with increasing angle of incidence. The medium on the other side of the boundary has n2 < n1.