Idaho - FOR - 426

During this lesson we are going to review the fundamental concepts of fire as a physical process.1Specifically we are going to discuss the chemical reactions involved in producing and consuming combustible material and than discuss the process

Idaho - FORP - 495

ProductandProcessDevelopment andCommercializationLectureSlidesBUS/FORP495ThesecourseslidesareoriginalworkspreparedbyStevenR.Shook. Theuseoftheseslideswithoutexpresswrittenpermissionofthe authorisstrictlyprohibited.[shook@uidaho.edu]Chapter3 Ulr

Syracuse - PHY - 212

Syracuse - PHY - 307

Lecture 5 Recap - driven nonlinear pendulum - chaos Period doubling, strange attractors, fractals Sierpinski triangle, chaotic dynamics Fractal dimension1 Last week examined a "real" pendulum nonlinear restoring force, damping plus driven

Syracuse - PHY - 212

PHY212 Lecture 7 1)2006 exams/solutions is at http:/physics.syr.edu/courses/PHY212.07Fall/Quizzes Exams.htm 2)You may bring a formula sheet(written on one page only) to the exam (Exam1 Thursday Sept 20). 1. Review mechanics Net Force (F) on point obj

Syracuse - PHY - 211

Physics 211 Problem Set 2 Due Friday, 02/02/07 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 1. Ea

Syracuse - PHY - 211

Syracuse - PHY - 211

Physics 211 Problem Set 3 Due Friday, 02/08/08 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 1. A

Syracuse - PHY - 211

Syracuse - PHY - 211

Physics 211 Problem Set 4 Due Friday, 02/14/08 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 1. So

Syracuse - PHY - 211

Physics 211 Problem Set 5 Due Friday, 02/22/08 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 1. A

Syracuse - PHY - 211

Syracuse - PHY - 211

IUPUI - DN - 893

Basis Shifting Tax Shelter Notice 2001-45 The Internal Revenue Service and the Treasury Department have become aware of a type of transaction, described below, that is being used by taxpayers for the purpose of generating losses or reducing income or

IUPUI - DN - 893

SECTION F-070 - PROTEST FORM NUMBER ONE PROTEST A. Name, Social Security Number Of Taxpayer, And Other Personal Information Concerning The Taxpayer. Taxpayer's Name: Estate of Jane Doe Taxpayer's Social Security Number: Taxpayer's Address: Taxpayer's

Syracuse - PHY - 312

PHY312- Homework 1Take the speed of light to be 3 108 m/s. 1. At 9:00 pm Pacific daylight time on August 14 1989, the planetary probe Voyager II passed by the planet Neptune. Images of the planet were coded and sent back to Earth my microwave relay

Syracuse - PHY - 312

PHY312 - Homework 41. Consider a photon moving along the positive x-direction with energy 1 1019 Joules (the Joule is the S.I unit of energy). Call this photon A. Imagine a second photon B of energy 2 1019 Joules moving also along the x-direction.

Syracuse - PHY - 312

PHY312 - Homework 51. A lift in empty space is accelerated using a rocket motor (relative to some inertial frame) such that its velocity increases by 2m/s every 2 seconds. An observer is inside the lift. (a) Would the observer be weightless ? (b) Su

Syracuse - PHY - 312

%A 4) X U AU 9 AU 9 i) 8 2 1 8 G 2 2 2 9U G A X) V 8 A 9 1&yBQT8EDbQQvE@bWpW@UyTXpW@Ux0d5)x@8545)e9@8E56W0D)F&w7)xE5CE154ETC2 8 G A U A 8 4 v 9 X 9 A U 9 8 A A b X S A 2 b 8 2 1 U V b 9 i b 36 e 0IQ5C@6E6wT)ET8EDbeWvE@bE5C(D8EW@)r5)@6T8E7VV

Syracuse - PHY - 312

PHY312 - Homework 71. Consider a solar mass black hole (M = 2 1030 kg). An observer standing on a shell with r coordinate r = 5km shines his flashlight radially outward. The light produced by the flashlight has wavelength 4 10-7 m (violet light).

Syracuse - PHY - 312

PHY312 - Homework 81. Decide on a project/term for the class. You can look at the suggestions listed under projects on the course webpage. But you can also choose a dierent topic as long as you can justify to me how it ts with the subject material i

Syracuse - PHY - 312

PHY312 - Homework 91. A black hole has an event horizon size of 10km. A stone starting from rest at innity falls radially into the black hole. (a) At what speed does a shell observer at r = 35km measure the stone to be going as it passes him ? (b) W

Syracuse - PHY - 212

L3-1; L3-2Gauss' LawChapter 22 Gauss' LawGoals:- learn to calculate the electric flux through surfaces - understand and apply Gauss' Law - calculate E fields for certain configurationsMeta-comments: Gauss' Law describes how electric fields ar

Syracuse - AST - 101

Our Corner of the Universe AST 101, Fall 2007ASTRONOMY GO-ROUNDWeek of August 28 Astronomy, pp. 7-10There are many questions about the sky, the stars, what we see and why we see it. In todays lab we will produce a skit in which you will play plan

Syracuse - AST - 101

Our Corner of the Universe AST 101, Fall 2007Lunar Phases II LabWeek of September 4 Astronomy, pp. 12-14Material: Flashlight, white ball. Procedure: Each group will simulate the motion of the Moon around the Earth, in order to understand the rela

Syracuse - PHY - 211

Physics 211, Spring 2009Practice before Exam 21. [20pts total] A person is pushing a crate. Coefficient of static friction between the crate and the floor is s=0.1. Coefficient of kinetic friction is k =0.05. The crate has a mass of 6 kg (Assume

Syracuse - PHY - 312

PHY312 - lecture 3Simon CatterallPHY312 - lecture 3 p. 1ReviewIn Special Relativity there is no absolute (observer independent) notion of space and time separately only a funny fusion of the two the thing we have been calling spacetime.Hend

Syracuse - PHY - 312

PHY312 - lecture 5Simon CatterallPHY312 - lecture 5 p.ReviewDerived Lorentz transformations relating coordinates of events as seen by different inertial observers. Saw how to add velocities in special relativity. Examples Today: talk about vec

Syracuse - PHY - 312

PHY312 - lecture 6Simon CatterallPHY312 - lecture 6 p. 1ReviewVectors in spacetime: sets of 4 numbers (at , ax , ay , az ) which transform like spacetime coordinates under LT. Length squared a2 a2 a2 a2 same for all inertial z y x t observe

Syracuse - PHY - 312

PHY312 - lecture 7Simon CatterallPHY312 - lecture 7 p. 1Reviewenergy-momentum vector P = (E/c, px , py , pz ) Contains relavistic energy, momentum. Invariant length is rest mass. Conserved.PHY312 - lecture 7 p. 2ExampleA photon moving wi

Syracuse - PHY - 312

PHY312 - lecture 9Simon CatterallPHY312 - lecture 9 p.RecapSaw that free fall frames serve as good approximations to inertial frames. Indeed, effects of gravity can be almost eliminated by jumping to such a FFF. Relies on equality of gravitati

Syracuse - PHY - 312

PHY312 - lecture 10Simon CatterallPHY312 - lecture 10 p.RecapFFF serve as good approxs to inertial frames in presence of gravity Principle of equivalence POE. Using POE learn that light is bent, clocks slow and light is redshifted in gravita

Syracuse - PHY - 312

PHY312 - lecture 12Simon CatterallPHY312 - lecture 12 p. 1RecapIngredients of GR principle of equivalence, principle of general relativity. Importance of tidal gravity. Consequences of POE slowing of clocks in gravitational eld, deforming of

Syracuse - PHY - 312

PHY312 - lecture 13Simon CatterallPHY312 - lecture 13 p. 1Summary so far .(Tidal) gravity caused by geodesic motion on curved spacetime. Curved space(time) described by metric - matrix which varies from point to point. If spacetime at possible

Syracuse - PHY - 312

PHY312 - lecture 14Simon CatterallPHY312 - lecture 14 p. 1Summary so far .POGR and POE guided Einstein to propose a radical new way of thinking about (tidal) gravity as curved spacetime. Curvature related to distribution of energy-momentum sp

Syracuse - PHY - 312

PHY312 - lecture 15Simon CatterallPHY312 - lecture 15 p. 1Summary of lecture14Exterior spacetime to spherically symmetric, time independent, non-spinning gravitational source is given by Schwarzschild metric1 s = A(r)c t r2 r2 2 A(r)2 2 2

Syracuse - PHY - 312

PHY312 - lecture 16Simon CatterallPHY312 - lecture 16 p.Summary of lecture15Exterior spacetime to spherically symmetric, time independent, non-spinning gravitational source is given by Schwarzschild metric1 s = A(r)c t - r2 - r2 2 A(r)2 2 2

Syracuse - PHY - 312

Realtivity and Cosmologylecture 17Realtivity and Cosmology p.Recap lecture 16Energy:EGR = mc22GM 1- 2 c rt Radial speed:r = -c t 2GM c2 r1 22GM 1- 2 c rShell observer sees justrshell = -c tshell 2GM c2 r1/2Realtivity and Cosm

Syracuse - PHY - 312

Relativity and Cosmologylecture 18Relativity and Cosmology p. 1Recap lecture 17Discussed radial motion of massive and massless bodies in Schwarschild spacetime Used several frames; global far away frame, local shell observer and freely falling

Syracuse - PHY - 581

11Analysis of Complex FunctionsLets jump right in and begin with some denitions: Denition 1.1 The complex plane C is (a representation in R2 of ) the set {z : |z| <corresponding to the origin under the transformation z z 1 .}, and the exte

Syracuse - PHY - 212

Syracuse - PHY - 212

Syracuse - PHY - 212

Solutions for Friday Homework 3, Feb 15, 200823.58a) From equation (23.9), treating the small spheres as point charges kq1 q2 (9 109 )(2.00 106 C)(3.50 106 C) = = 0.252J r .250mU=b) The idea is we want the second spheres velocity to be zero

Syracuse - PHY - 212

Solutions for Friday Homework 4, Feb 22, 200824.50) a) C= b) c) E= d) U= Q2 (5.7 10-10 )2 = = 3.4 10-9 J 2C 2(4.8 10-11 ) V 12V = = 2553V /m d 0.0047m0Ad=(8.85 10-12 C 2 /N m2 )(0.16m)2 = 4.8 10-11 F = 48pF 0.0047mQ = CV = (4.8 10-1

Syracuse - PHY - 212

Solutions for Friday Homework 7, Feb 29, 2008 25.57.a) The area of the wire isa = r2 d r= 2 a= = d 22d2 4 (0.0025m)2 = 4 = 5.0 106 m2Then for the resistivityR=L A AR = L (5.0 106 m2 )(.104) = (14.0m) = 3.64 108 mb) E = J so J = E/.

Syracuse - PHY - 212

Solutions for Friday Homework 8, Mar 07, 200826.59) Any collections of wires that are connected with no circuit elements in between may be treated as single pieces of metal, and recall that a single conductor is an equipotential. Therefore such reg

Syracuse - PHY - 212

Solutions for Friday Homework 10, Mar 28, 200827.53) Starting with F1 = qv1 B we have that the force is in the z direction, so: Fz k = q v1 cos(45) + v1 sin(45) Bx + By + Bz k i j i j v1 q = 2 v1 q = 2 v1 q = 2 + Bx + By + Bz k i j i j

Syracuse - PHY - 212

Solutions for Friday Homework 11, Apr 04, 200828.54) First we need to know the magnetic field at the indicated point. First note that this point is 2.50 cm from each wire. Then by superposition the field here will be the sum of the fields from each

Syracuse - PHY - 212

Solutions for Friday Homework 13, Apr 25, 200830.43.a) This is similar to example (30.1)M=0 AN1 N2 l 0 AN1 N2 = l (4 107 )(0.0060m)2 )(15)(6750) = (0.003m)= 4.7 106 henryb) From eqn (30.4): E = M di = (4.7 106 H)(37.5A/s) = 0.18mV dt30

Syracuse - PHY - 307

Homework 1Due Thursday September 4 1. Download the code euler.py o the homework web page. Save it to My Documents (les on this drive are not local but exist on a backed up central drive) . Fire up IDLE and load the code into the Python editor. Run i

Syracuse - PHY - 307

Homework 4Due Thursday October 2 1. Download the code lorenz.py available from the HWS page. This code simulates the lorenz model which is a extremely simplied model for uid ow in a heated liquid. There are three variables labeled x,y,z which corres

Syracuse - PHY - 211

Physics 211 Problem Set 4 Due Friday, 02/13/09 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 1. So

Syracuse - PHY - 211

Physics 211 Problem Set 5 Due Friday, 02/20/09 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 1. A

Syracuse - PHY - 211

Physics 211 Problem Set 8 Due Fri, 03/20/09 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 2. A 3 k

Syracuse - PHY - 211

Physics 211 Problem Set 9 Due Fri, 03/27/09 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 1. A rai

Syracuse - PHY - 211

Physics 211 Problem Set 10 Due Fri, 04/03/09 Last Name:_ First Name _ Workshop time or section:_TA name or Room # _ Please submit your homework on this sheet. If you need more space than is available, please attach additional sheets of paper. 1. Find

IUPUI - STAT - 113

3/27/2009WIAS Chapter 6: Designing a Questionnaire & MeasurementMeasuringChapter 8Many of the considerations for designing a questionnaire are related to the concepts of measurement Most of the considerations apply to all statistical studies,

Idaho - CS - 448

Fault-tolerant AgreementHaving discussed the issues of addressing malicious act in the context of dependability, we will now look at a classic solution to agreeing in the presents of faults: Byzantine AgreementThis paper was not written with o

Idaho - CS - 449

Fault Tolerant SystemsHOMEWORK 3Due 11/09/2005 (EO 11/23/2005)1. (20) Lets take another shot at the candy machine. Assume we are dealing with a general candy machine. Now, the price can vary, depending on which candy one selects. Again, the di

Idaho - CS - 448

ProjectPrepara+onRecoveryinWirelessCommunica+onEarlyStart Wirelesscommunica+ons Wirelessprotocols E.g.IEEE208.11(a,b,g,) Wirelesspersonalareanetworks(WPAN) Bluetooth upto720Kbps,10m,100withpowerboost, Bluetooth2.0+EDR(enhanceddatarate,dier

Virginia Tech - CS - 6504

CS6504 Mobile ComputingDr. Ayman Abdel-HamidComputer Science Department Virginia TechOutlineRouting Protocols for Ad hoc Networks Example of a reactive routing protocol AODV: Ad hoc On-demand Distance Vector RoutingRouting Protocols in MANETs