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Syracuse - PHY - 209

Syracuse - PHY - 209

Syracuse - PHY - 211

PHY211 Fall 2005 Final ExamName (please print): _ Last First SUID_ _It is very important that you print your name at the top of every exam page. Please do it before you read any questions! Document your work. There are portions of the problems on b

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Welcome back to Physics 211Todays agenda: Rotational dynamics Angular momentum Problems with moving axis of rotationPhysics 211 Fall 2006Lecture 12-11Current homework assignments WHW10: In blue Tutorials in Physics homework book HW-65

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Welcome to Physics 211!(General Physics I)Physics 211 Fall 2005Lecture 01-11SU PHY211Course staff: General Physics IFall 2005Lecturers: Prof. Simon Catterall (first 1/2 semester) smc@physics.syr.edu Prof. Britton Plourde (second 1/2

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Welcome back to Physics 211Today's agenda: summary of relativity so far events, frames, and spacetime intervalexamples relativistic mechanicsPhysics 211 Fall 2002Lecture 15-21Final Friday 13 Dec 10:15am -12:15pm here Comprehensive. (

Syracuse - PHY - 307

Orbital Precession of MercuryA little background Mercurys orbit rotates 5600 arc seconds per century, but 43 arc seconds per century was unaccounted for Newtonian physics couldnt explain the extra precession Einsteins General Relativity to the r

Syracuse - PHY - 307

Lec6 Chaos - logistic map Period doubling, strange attractors, fractals Sierpinski triangle, chaotic dynamics Fractal dimension1Logistic Map lab 5 Simplest example of chaotic dynamical system Exhibits period doubling approach to chaos

Syracuse - PHY - 307

Lec3 Graphing, multiple displays Many particles - Newtonian gravity Higher order integrators1Graphing So far we have used Python to animate a simulation of simple motion. For more quantitative work need to be able to plot aspects of the m

Syracuse - PHY - 307

Lec5 Nonlinear systems chaos Phase space, Poincare maps, strange attractors Period doubling Lorenz model, balls in boxes .1Real pendulumVariables (t), (t) equation of motion: d g d = - sin () - k + F sin (D t) dt l dt d = dt Integrate/s

Syracuse - PHY - 307

Lab 12 - The Ising ModelThursday 16 November, 2006 - Due: t.b.a. In this lab, you will study a simple model of ferromagnetism, called the Ising model. As always, please include in your writeup any sections of Python code you write. there was no Lab

Syracuse - PHY - 307

Lab 9 - Complex Dynamics: Julia SetsThursday 25 October, 2006 - Due: Thursday 3 November In this lab, you will take a closer look at a particular Complex Dynamical System, called a Julia Set. Since we will need complex numbers, you'll learn about wo

Syracuse - PHY - 307

Lab 10 - Sand[piles] and Earth[quakes]Thursday 2 November, 2006 - Due: Thursday 9 November In this lab, you will study aspects of self-organized critical phenomena, which have been used to study general universal properties of some interesting compl

Syracuse - PHY - 307

Lec1 - intro, basic tools Mechanics, syllabus General comments What is computational science ? Derivatives, integrals and root finding Intro to Python1General comments Not programming course. Not traditional physics course. Topics dra

Syracuse - PHY - 307

Lec12 Phase transitions, critical phenomena Magnetic systems - Ising model1Commerical break Next semester there will be a successor course PHY300 a.k.a PHY308 Tuesdays/Thursdays 12:30-1:50 pm (lab times to be decided) Similar to PHY307 wit

Syracuse - PHY - 307

Lab 7 - PercolationThursday 12 October, 2006 - Due: Thursday 19 October The aim of this lab is (1) to get you familiar with the computational implementation of a lattice and (2) to become familiar with some of the concepts in percolation. As for the

Syracuse - PHY - 307

Lab 5 - Chaotic DynamicsThursday 28 September, 2006 - Due: Thursday 05 October The aim of this lab is to explore some aspects of chaotic dynamics. First, we have another look at the Pendulum example presented in lecture. Then, we will study the Logi

Syracuse - PHY - 307

Lab 7 - PercolationThursday 12 October, 2006 - Due: Thursday 19 October The aim of this lab is (1) to get you familiar with the computational implementation of a lattice and (2) to become familiar with some of the concepts in percolation. As for the

Syracuse - PHY - 307

Lab 6 - Fractal DimensionThursday 05 October, 2006 - Due: Thursday 12 October We will take a closer look (pun intended) at the self-similar Sierpinski Triangle. Then, youll modify the parameters of the dynamical model to obtain a dierent fractal. Fi

Syracuse - PHY - 307

Homework 6Due: Thursday 12 October In this homework you will investigate another discrete time nonlinear dynamics the Henon map. It is similar to the Sierpinski map as it involves two dynamical variables x and y. The update equation is xn+1 = yn +

Syracuse - PHY - 307

Lab 3 - Modeling the Solar System (part I)Thursday 14 September, 2006 - Due: Thursday 21 September The aim of this lab is to get you started with the construction of a solar system, using some of the ideas that you have already been introduced to. I

Syracuse - PHY - 307

Homework 3Due: Thursday 21 September 1. In Lab3 you constructed a table showing the error in the energy of a harmonic oscillator as a function of the time step dt for the Euler algorithm. In lecture 3 we discussed an improved algorithm the leapfrog

Syracuse - PHY - 307

Homework 21. Cut/paste the code for the projectile problem discussed in class (note: that listing is not quite complete: you will need to look at earlier codes to see how to access the 3D environment and how to set the scaling and range). 2. Modify

Syracuse - PHY - 307

Lec2 - mechanics and simple simulation Newtons laws, Euler method 1D and 2D examples: projectiles, harmonic motion, damping Simulation code and graphics More on functions1Newtons lawsOne particle, one dimension: dx = v dt dv = a = F/m dt

Syracuse - PHY - 307

Homework 11. Tabulate the values of the symmetric dierence approximation to the derivative for the functions f = sin x at x = 0.1 and f = x2 for x = 2 using step sizes h = 0.1, 0.01, 0.001, 0.0001. You may simply edit the Python program given in cla

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Homework 10Due: Thursday 9 November Choose a topic for your class project. Hand in the title of your topic together with a brief (one paragraph) description of what you intend to do. Please see me if you would like help choosing a topic.1

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Homework 4Due: Thursday 28 September For this homework you will use your codes solar.py and integrator.py from lab4 to investigate the motion of a object near a black hole (or any object with a strong gravitational field). In this case the leading c

Syracuse - PHY - 307

Lec10 Self-organized critical phenomena Earthquakes, sand piles1Self-similarity and criticalityWe have so far seen several examples of systems which exhibit power law behavior eg. Fractal dimensions. Number of cells needed to cover points o

Syracuse - PHY - 307

Lec11 Earthquakes a more realistic model1Recap Last week we discussed a very simplified model for understanding the statistics of Earthquakes how many Earthquakes occur of a certain magnitude. Saw that the dynamics led to self-organized cri

Syracuse - PHY - 307

Mercury's Orbital PrecessionBy Gavin HartnettEllipses Planetary Orbits are ellipses Earlier lab simplified these orbits to circles planet moves faster near the sun Perihelion-closest point to sun Aphelion-farthest Two foci-Sun is located at

Syracuse - PHY - 307

Newton's Cradle in Actionor The Mechanics of a ToyThe Physics A Newton's Cradle generally consists of: two or more massive (spherical) bodies whose motions are physically restricted to circular paths; and an equal number of pendula fixed at one e

Syracuse - PHY - 307

The Transition to the Jamming ClusterWhat is a jamming cluster? The point at which a percolating network of forces "solidifies". The jamming cluster is most likely to occur in a system made of many smaller pieces of matter (like sand). When a sy

Syracuse - PHY - 307

List of project topics: 1. Precession of Mercurys perihelion due to General Relativity. An extension of an earlier homework problem. To the usual inverse square gravitational force add a term r4 . Compute the rate of rotation of the resulting ellipt

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Lec4 Many particles - Newtonian gravity Solar system simulations1Inverse law Newtons Law of Universal Gravitation: Between two bodies with (gravitational) masses Ma and Mb distance r apart there is a force of attraction acting along their r

Syracuse - PHY - 307

Lab 4 - Modeling the Solar System (part II)Thursday 21 September, 2006 - Due: Thursday 28 September The aim of this lab is to continue development of the solar system model we started in lab3. In this lab we continue with our discussion in lecture b

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Lecture 5.1Copyright 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.Review of Last LectureElectric FluxCopyright 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.Conductors in Electrostatic Equilibrium

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Syracuse - PHY - 212

Phy212 - Spring 2007 Mid Term Exam 3 (100pts + 20pts extra credits) April 5, 2007 Name_Don Bunk: Steluta Dinca: Renata Jora: 10:35am, 2:15pm, 8:25am, 11:40am, 12:45pm, 9:30am, 5:15pm 3:45pm 10:35amPlease write your name on the line above and circl

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PRS RF Student Clicker/RemoteTwo line display for indicating response and status of receiptPRS rfScroll KeysSend/EnterBackspace Setup KeyAlpha, Numeric and T/F Keys Diagnostics include Battery level %AAA batteries used to keep future cost

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AnnouncementA new lab session for phy222 is open nowM011 Wednesday 6:00-8:00 PM Class # 34159Copyright 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.Review of Last Lecture: Charge Model1. Objects can be charged by rubbing

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Phy212 - Spring 2007 Mid Term Exam 1 (100pts) Name_Don Bunk: 10:35am, 11:40am, 5:15pm Steluta Dinca: 10:35am, 12:45pm, 3:45pm Renata Jora: 8:25am, 9:30am, 2:15pmPlease write your name on the line above and circle your workshop section (both TA an

Syracuse - PHY - 212

Syracuse - PHY - 212

!"#$%#! &'()*+! "#$%&!'(%!)&*+',-!+)(%.%+!*+!)#,/'!-(*.0%+1!,-./0*-1)+2 !! ! 3'*4)+! 506!2(%!-(*.0%!3!"4515!/6!%7%.'+!*!8#.-%! "3!#/!9 #/!9!"4515!/6!'#!'(%!.,0(':!*/$!'(%!-(*.0%!9!%7%.'+! ! *!8#.-%! "9!#/!3 !#/!3!'#!'(%!&%8'1!;+,/0!6#<&#=>?+!&*@:!

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Syracuse - PHY - 212

Consider the arrangement of two positive charges shown in the figure. Give your answers below in terms of Q, a, and universal constants. Choose a coordinate system and indicate the direction of any vector with respect to this coordinate system.A a

Syracuse - PHY - 212

Syracuse - PHY - 212

Syracuse - PHY - 212

Syracuse - PHY - 212

Syracuse - PHY - 212

Syracuse - PHY - 212

Syracuse - PHY - 212

Syracuse - PHY - 212

Syracuse - PHY - 212

Phy212 - Spring 2007 Mid Term Exam 2 (100pts) Name_Don Bunk: Steluta Dinca: Renata Jora: 10:35am, 2:15pm, 8:25am, 11:40am, 12:45pm, 9:30am, 5:15pm 3:45pm 10:35amPlease write your name on the line above and circle your workshop section (both TA and

Syracuse - PHY - 211

Welcome back to Physics 211Todays agenda: Midterm #1 Thursday 9/25 Finish Chapter 2!Physics 211 Fall 2008Lecture 03-2Construct a Velocity Graph from a Motion Diagram Demo Stand still, walk away slowly at constant speed for 2 s, stand still

Syracuse - PHY - 211

Welcome back to Physics 211Today's agenda: Work and kinetic energy Scalar product of vectors Finish circular motion .Physics 211 Fall 2005Lecture 07-11Reminder etc Tutorial HW5 due wed. (N's 2nd and 3rd laws) MPHW4 available noon Fr