Course Descriptions. Appendix F
|
|
|
- Aron Rogers
- 5 years ago
- Views:
Transcription
1 Appendix F Course Descriptions Seven new courses are required to implement the Space Physics program, and their course descriptions are contained in this appendix. 51
2 F.1 Course Description: Physics II Lab Course No: PS2xx Title: Physics II Lab (1 credit hour) One three hour laboratory session per week with experiments chosen primarily from wave motion, transverse and longitudinal waves, superposition of waves, traveling waves and standing waves. Corequisites: PS160 or PS208 This lab will develop the students understanding of wave motion, the principle means by which we make measurements (e.g., sight and sound). The student will measure the properties of transverse and longitudinal waves, including the superposition and propagation of waves. Free oscillations of simple systems: Measure the frequency of simple harmonic systems and describe their equations of motion. Forced Oscillations: Measure the resonance properties of oscillating systems. Traveling waves: Study of the forced oscillations of an open system. Phase velocity and impedance. Topic 6: Topic 8: Topic 9: Optional Standing waves: Study of the forced oscillations of a closed system. Inertia and return force. Reflection: Study of the superposition of standing and traveling waves. Derive reflection coefficients. Polarization: Study of the polarization of electromagnetic waves. Relationship between partial polarization and coherence. Phase and group velocity: Study the phase velocity of sound and group velocity of water waves. Interference and diffraction: Measure the superposition of waves that have traveled different paths from the source to the detector. Physical meaning of coherence. Report writing: written presentation of experiments, including error analysis. Modulations, pulses, and wave packets: Superposition involving different frequencies to form pulses and wave packets. 52
3 F.2 Course Description: Senior Physics Lab I Course No: PS 4XX Title: Senior Physics Lab I (3 credit hours) Mirror optics, lens optics, emission and absorption line spectroscopy, diffraction grating spectroscopy. Prerequisites: PS 305 To familiarize the student with laboratory optics experiments. (Note: There will be several lab experiments for each topic). Plane Waves: Refraction and reflection of plane waves. Mirrors: Concave mirrors, convex mirrors, telescope design. Lenses: Concave lenses, convex lenses, chromatic abberation, microscope design. Emission and Absorption line spectroscopy: Hydrogen spectrum, Mercury spectrum, sodium spectrum, Zeeman effect. Diffraction gratings: physical optics, Fresnel diffraction, Fraunhoffer diffraction, Youngs slits, circular apertures, spectrometer design. Topic 6: Lasers: Coherence length, interferometers, polarization of light. Report Writing: written presentation of experiments, including error analysis. 53
4 F.3 Course Description: Atomic/Nuclear Physics Course No: PS4xx Title: Atomic/Nuclear Physics (3 credit hours) Multi-electron atoms, X-rays and gamma rays, radiative transitions in the atom and the nucleus. Basic properties of nuclei, systematics of nuclear stability, dynamics of nuclear reactions, nuclear models and nuclear forces. Introduction to particle physics and its applications to cosmic rays, stellar energy, and the formation of the elements. Prerequisites: EP455 Topic 6: Topic 8: Topic 9: This course is designed to give the student an understanding of atomic, nuclear, and particle interactions. The student will learn to calculate cross-sections and transition rates associated with atomic, nuclear, and particle interactions. Atomic Spectroscopy: L S and j-j coupling, energy-level diagrams for complex atoms, the Zeeman effect, excitation of atoms and the breadth of spectral lines. X-rays: Production of X-rays, interaction of X-rays with matter, X-ray diffraction, refraction and reflection of X-rays. Basic properties of nuclei: Angular momentum, magnetic moments, nuclear magnetic resonance, electric quadrapole moments, radioactivity, excited states of nuclei. Particle scattering: Rutherford scattering, transformation from CM to laboratory coordinates, multiple coulomb scattering and energy loss by ionization, range, straggling, and general properties of particle scattering. Radioactivity: the four radioactive series, age of minerals and of the earth, natural radionuclides, artificial radiactivity, alpha particle decay, beta-decay, neutrinos, theory of beta-decay and the study of the weak force. Nuclear Models: the alpha-particle model, liquid-drop model, fission and fusion, the Fermi-gas model, the shell model. Nuclear forces: two-nucleon system, scattering experiments, Fermi motion, and the study of the strong force. Introduction to elementary particles: The Standard Model, the four fundamental forces in nature, the Dirac Theory of the electron. Modern Physics in Nature: Cosmic rays, stellar energy, the formation of the elements. 54
5 F.4 Course Description: Astrophysics II Course No: PS 4XX Title: Astrophysics II (3 credit hours) Radiative transfer in astrophysical environments; stellar atmospheres, stellar interiors, and gaseous nebulae. Emission and absorption processes. Interaction of radiation with matter. Prerequisites: MA 345, PS 401. This course is designed to give the student a theoretical, computational and physical understanding of the various means by which radiation is transported within the cosmos. Basic Definitions: Specific intensity, flux, mean intensity, solid angle, energy density, Planck function, Boltzmann formula, Maxwell-Boltzmann distribution. Interaction of radiation with matter: Einstein coefficients, statistical equilibrium, the two level atom, emission and absorption coefficients, free-free emission, radiative transfer equation. Stellar Atmospheres: Gray atmosphere, Eddington approximate solution, emergent intensity, limb darkening, Saha equation. Realistic Stellar atmospheres: Absorption coefficients for atomic hydrogen, bound - free absorption, free-free absorption, formation of absorption lines, equivalent widths, spectral line broadning. Gaseous nebulae: HII regions, collisional excitation, collisional and radiative deexcitation, Stromgren sphere, emission line intensities, forbidden lines. 55
6 F.5 Course Description: Senior Physics Lab IIa Course No: PS 4XX Title: Senior Physics Lab IIa (3 credit hours) Binary stars, spectroscopic binaries, proper motion, galaxy rotation curves, image processing. Prerequisites: PS 4XX (Senior Physics Lab I) Topic 6: To familiarize the student with the various techniques that astronomers use to determine useful physical quantities from astronomical observations. (Note: There will be several lab experiments for each topic). Binary stars: Calculating orbital elements for visual binaries. Spectroscopic binaries: Calculating mass ratios for spectroscopic binaries. Proper Motion: Calculating distances to nearby stars, asteroids and planets. Galaxy rotation curves: Calculating the distribution of mass and the amount of dark matter in galaxies. Introduction to IRAF: Basic image processing and image analysis. Report Writing: written presentation of experiments, including error analysis. 56
7 F.6 Course Description: Particle Physics & Cosmology Course No: PS4xx Title: Particle Physics & Cosmology (3 credit hours) Study of the evolution of the universe including large scale structure, Big-Bang cosmology, general relativity and the search for dark matter. Prerequisites: MA441, PS4xx (Atomic/Nuclear Physics) This course is designed to give the student a working knowledge of the structure and evolution of the universe. The student will learn how nuclear and particle physics played a significant role in the dynamics of the early universe, and explore some of the current models. Large-scale structure of the universe: homogeneity, high-redshift objects, pregalactic history. The Standard Model: the unified theory of elementary particles and forces. Big-Bang cosmology: hot-big-bang hypothesis, evolution of big-bang including quantum gravity, inflation, baryosynthesis, nucleosynthesis, and matter dominating universe leading to star and galaxy formation. Microwave background. The cosmic asymmetry between matter and antimatter: introduction to particle symmetries in Charge-conjugation/Parity violation. Some fundamental questions: gravity, inflationary models, etc. Topic 6: Introduction to general relativity: Equivalence principle, bending of light, gravitational shift of spectral lines, concept of curved space-time, the Schwarzschild metric. Topic 8: Experimental tests of Einstein s theory of gravitation: Precession of the perihelion of mercury, deflection of light rays, radar echoes from planets. The search for dark matter: physics of black holes, neutrinos, WIMPS and MACHOS. Galactic rotation rates. Topic 9: Cosmic Kinematics: the Robertson-Walker metric, Hubble s law, Red shifts, angular size, apparent luminosity, and galaxy counts. Topic 10: Cosmic Dynamics: Solution of Friedmann s equations, open vs. closed universe, and the cosmological constant. 57
8 F.7 Course Description: Senior Physics Lab IIb Course No: PS4xx Title: Senior Physics Lab IIb (3 credit hours) Measurements of nuclear and particle systems using high-precision detectors and high-speed data acquisition. Prerequisites: PS303, PS305, PS2xx (Physics III) Topic 6: This course is designed to enhance the students laboratory skills for making high-precision measurements of nuclear and particle systems. The student will successfully complete 3 of the following labs with formal writeups. More labs may be added in the future. Measure the lifetime of a muon: muons created from cosmic ray interactions in the earth s atmosphere are observed to decay into electrons in the laboratory. Students will measure the half-life of muons and learn about the weak interaction (one of the four forces of nature) responsible for radioactive decay. Nuclear magnetic resonance: the properties of NMR will be studied, including the spin-flip of protons, spin-relaxation times, and NMR imaging. Measure ionizing cosmic rays: measure the flux and angular dependence of cosmic rays (and their daughters) in the laboratory. Students will also learn the health risks associated with ionizing radiation. Rutherford scattering: measure the angular distribution of charged particles scattered by the nucleus. Students will learn the concepts of double-differential cross sections used in nuclear/particle physics. Compton scattering: measure the recoil electron energy due to Compton Scattering of X-rays on electrons. Students will learn the concepts used in X-ray telescopes. Trapping antimatter in a Penning trap: confine and study the positrons (antielectrons) emitted from a radioactive source. Students will learn how to confine and trap antimatter for several hours and days. Report Writing: written presentation of experiments, including error analysis. 58
Charles Keeton. Principles of Astrophysics. Using Gravity and Stellar Physics. to Explore the Cosmos. ^ Springer
Charles Keeton Principles of Astrophysics Using Gravity and Stellar Physics to Explore the Cosmos ^ Springer Contents 1 Introduction: Tools of the Trade 1 1.1 What Is Gravity? 1 1.2 Dimensions and Units
Switching to OCR from AQA
Switching to OCR from AQA The content within the OCR Physics A specification covers the Big Ideas of physics and will be very familiar. We ve laid it out in a logical progression to support co-teaching
Relativity, Gravitation, and Cosmology
Relativity, Gravitation, and Cosmology A basic introduction TA-PEI CHENG University of Missouri St. Louis OXFORD UNIVERSITY PRESS Contents Parti RELATIVITY Metric Description of Spacetime 1 Introduction
Nuclear and Particle Physics
Nuclear and Particle Physics W. S. С Williams Department of Physics, University of Oxford and St Edmund Hall, Oxford CLARENDON PRESS OXFORD 1991 Contents 1 Introduction 1.1 Historical perspective 1 1.2
PHYSICS (PHYS) Physics (PHYS) 1. PHYS 5880 Astrophysics Laboratory
Physics (PHYS) 1 PHYSICS (PHYS) PHYS 5210 Theoretical Mechanics Kinematics and dynamics of particles and rigid bodies. Lagrangian and Hamiltonian equations of motion. PHYS 5230 Classical Electricity And
Foundations of Astrophysics
Foundations of Astrophysics Barbara Ryden The Ohio State University Bradley M. Peterson The Ohio State University Preface xi 1 Early Astronomy 1 1.1 The Celestial Sphere 1 1.2 Coordinate Systems on a Sphere
Switching to OCR from Pearson (Edexcel)
Switching to OCR from Pearson (Edexcel) The content within the OCR Physics A specification covers the Big Ideas of physics and will be very familiar. We ve laid it out in a logical progression to support
Massachusetts Tests for Educator Licensure (MTEL )
Massachusetts Tests for Educator Licensure (MTEL ) FIELD 11: PHYSICS TEST OBJECTIVES Subarea Multiple-Choice Range of Objectives Approximate Test Weighting I. Nature of Science 01 05 12% II. Force and
International Olympiad on Astronomy and Astrophysics (IOAA)
Syllabus of International Olympiad on Astronomy and Astrophysics (IOAA) General Notes 1. Extensive contents in basic astronomical concepts are required in theoretical and practical problems. 2. Basic concepts
Contents. Preface to the First Edition Preface to the Second Edition
Contents Preface to the First Edition Preface to the Second Edition Notes xiii xv xvii 1 Basic Concepts 1 1.1 History 1 1.1.1 The Origins of Nuclear Physics 1 1.1.2 The Emergence of Particle Physics: the
Physics Courses. Courses. Physics Courses 1
Physics Courses 1 Physics Courses Courses PHYS 1403. General Physics I (C). General Physics I (3-2) A non-calculus treatment of mechanics and heat. Laboratory experience is an essential component of this
College Physics 10th edition
College Physics 10th edition Raymond A. Serway and Chris Vuille Publisher: Cengage Learning Table of Contents PHY101 covers chapters 1-8 PHY102 covers chapters 9-25 Chapter 1: Introduction 1.1: Standards
MIDTERM 3 REVIEW SESSION. Dr. Flera Rizatdinova
MIDTERM 3 REVIEW SESSION Dr. Flera Rizatdinova Summary of Chapter 23 Index of refraction: Angle of reflection equals angle of incidence Plane mirror: image is virtual, upright, and the same size as the
ASTRONOMY (ASTRON) ASTRON 113 HANDS ON THE UNIVERSE 1 credit.
Astronomy (ASTRON) 1 ASTRONOMY (ASTRON) ASTRON 100 SURVEY OF ASTRONOMY 4 credits. Modern exploration of the solar system; our galaxy of stars, gas and dust; how stars are born, age and die; unusual objects
Unified School District of De Pere Physics Benchmarks
Content Standards: A. Students will understand that among the science disciplines, there are unifying themes: systems, order, organization, and interactions; evidence, models, and explanations; constancy,
MODERN PHYSICS Frank J. Blatt Professor of Physics, University of Vermont
MODERN PHYSICS Frank J. Blatt Professor of Physics, University of Vermont McGRAW-HILL, INC. New York St. Louis San Francisco Auckland Bogota Caracas Lisbon London Madrid Mexico Milan Montreal New Delhi
FYS 3510 Subatomic physics with applications in astrophysics. Nuclear and Particle Physics: An Introduction
FYS 3510 Subatomic physics with applications in astrophysics Nuclear and Particle Physics: An Introduction Nuclear and Particle Physics: An Introduction, 2nd Edition Professor Brian Martin ISBN: 978-0-470-74275-4
Topics Covered in Chapter. Light and Other Electromagnetic Radiation. A Subatomic Interlude II. A Subatomic Interlude. A Subatomic Interlude III
Light and Other Electromagnetic Radiation Topics Covered in Chapter 1.Structure of Atoms 2.Origins of Electromagnetic Radiation 3.Objects with Different Temperature and their Electromagnetic Radiation
Light and Other Electromagnetic Radiation
Light and Other Electromagnetic Radiation 1 Topics Covered in Chapter 1.Structure of Atoms 2.Origins of Electromagnetic Radiation 3.Objects with Different Temperature and their Electromagnetic Radiation
Galaxies and Cosmology
F. Combes P. Boisse A. Mazure A. Blanchard Galaxies and Cosmology Translated by M. Seymour With 192 Figures Springer Contents General Introduction 1 1 The Classification and Morphology of Galaxies 5 1.1
hij Teacher Resource Bank GCE Physics A Changes to Content
hij Teacher Resource Bank GCE Physics A Changes to Content Copyright 2008 AQA and its licensors. All rights reserved. The Assessment and Qualifications Alliance (AQA) is a company limited by guarantee
PHYS 4 CONCEPT PACKET Complete
PHYS 4 CONCEPT PACKET Complete Written by Jeremy Robinson, Head Instructor Find Out More +Private Instruction +Review Sessions WWW.GRADEPEAK.COM Need Help? Online Private Instruction Anytime, Anywhere
Unit title: Atomic and Nuclear Physics for Spectroscopic Applications
Unit title: Atomic and Nuclear Physics for Spectroscopic Applications Unit code: Y/601/0417 QCF level: 4 Credit value: 15 Aim This unit provides an understanding of the underlying atomic and nuclear physics
Astronomy Today. Eighth edition. Eric Chaisson Steve McMillan
Global edition Astronomy Today Eighth edition Eric Chaisson Steve McMillan The Distance Scale ~1 Gpc Velocity L Distance Hubble s law Supernovae ~200 Mpc Time Tully-Fisher ~25 Mpc ~10,000 pc Time Variable
Subject Area Competencies and Skills (22nd Edition)
Science Education (Physics) Program Requirements Physics 6-12 "C" below indicates where content is covered through coursework 1. Knowledge of the nature of scientific investigation and instruction in physics
Prioritized Curriculum PHYSICAL SCIENCE GRADE 9 Updated: July CSO s Essential Important Need to Know
Prioritized Curriculum PHYSICAL SCIENCE GRADE 9 Updated: July 2011 CSO s Essential Important Need to Know SC.O.PS. 1.1 X 1.2 X 1.3 X 1.4 X 1.5 X 1.6 X 1.7 X SC.O.PS.2.1 2.1 X 2.2 X 2.3 X 2.4 X 2.5 X 2.6
TEACHER CERTIFICATION STUDY GUIDE
Table of Contents Pg. Domain I. Mechanics Vectors (properties; addition and subtraction)... 129H1 Vector multiplication (dot and cross product)... 130H3 Motion along a straight line (displacement, velocity,
Rb, which had been compressed to a density of 1013
Modern Physics Study Questions for the Spring 2018 Departmental Exam December 3, 2017 1. An electron is initially at rest in a uniform electric field E in the negative y direction and a uniform magnetic
INTRODUCTION TO THE STRUCTURE OF MATTER
INTRODUCTION TO THE STRUCTURE OF MATTER A Course in Modern Physics John J. Brehm and William J. Mullin University of Massachusetts Amherst, Massachusetts Fachberelch 5?@8hnlsdie Hochschule Darmstadt! HochschulstraSa
Radiochemistry and Nuclear Methods of Analysis
Radiochemistry and Nuclear Methods of Analysis WILLIAM D. EHMANN Professor, Department of Chemistry University of Kentucky Lexington, Kentucky DIANE E. VANCE Staff Development Scientist Analytical Services
The Mystery of Dark Matter
The Mystery of Dark Matter Maxim Perelstein, LEPP/Cornell U. CIPT Fall Workshop, Ithaca NY, September 28 2013 Introduction Last Fall workshop focused on physics of the very small - elementary particles
COX & GIULI'S PRINCIPLES OF STELLAR STRUCTURE
COX & GIULI'S PRINCIPLES OF STELLAR STRUCTURE Extended Second Edition A. Weiss, W. Hillebrandt, H.-C. Thomas and H. Ritter Max-Planck-lnstitut fur Astrophysik, Garching, Germany C S P CONTENTS PREFACE
PHYSICS. Course Syllabus. Section 1: Mathematical Physics. Subject Code: PH. Course Structure. Electromagnetic Theory
PHYSICS Subject Code: PH Course Structure Sections/Units Topics Section 1 Section 2 Section 3 Section 4 Section 5 Section 6 Section 7 Section 8 Mathematical Physics Classical Mechanics Electromagnetic
Dynamics inertia, mass, force. Including centripetal acceleration
For the Singapore Junior Physics Olympiad, no question set will require the use of calculus. However, solutions of questions involving calculus are acceptable. 1. Mechanics Kinematics position, displacement,
U n 3 n Ba Kr (D) Br (C) Kr (B) Rb (E) 94 37
1984 36. The critical angle for a transparent material in air is 30. The index of refraction of the material is most nearly (A) 0.33 (B) 0.50 (C) 1.0 (D) 1.5 (E) 2.0 37. An object is placed as shown in
Introduction to Particle Physics
Introduction to Particle Physics The Particle Zoo Symmetries The Standard Model Thomas Gajdosik Vilnius Universitetas Teorinės Fizikos Katedra Introduction to Particle Physics http://web.vu.lt/ff/t.gajdosik/wop/
PHYSICS Course Structure Units Topics Marks Electrostatics Current Electricity III Magnetic Effect of Current & Magnetism
PHYSICS Course Structure Units Topics Marks I Chapter 1 Chapter 2 II Chapter 3 III Chapter 4 Chapter 5 IV Chapter 6 Chapter 7 V Chapter 8 VI Chapter 9 Electrostatics Electric Charges and Fields Electrostatic
History of Physics: History of Physics: - Identify the contributions of key figures in the history of physics.
Texas University Interscholastic League Contest Event: Science (Physics) The contest challenges students to read widely in physics, to understand the significance of experiments rather than to recall obscure
AP Physics B - Syllabus G. Bonney
AP Physics B - Syllabus G. Bonney George_A_Bonney@mcpsmd.org Texts: Physics, Cutnell & Johnson; 6 th Ed. New York: John Wiley College Physics, Serway & Faughn; 5th Ed. Harcourt College Publishers Supplementary:
The Final Exam (Exam 4) will be on FRIDAY MAY 11 From 3 5 PM in LR1 VAN
1 --------------------------------------------------------------------------------------------------------------------- 29:006 SPRING 2012 PRACTICE EXAM 4 ---------------------------------------------------------------------------------------------------------------------
NERS 311 Current Old notes notes Chapter Chapter 1: Introduction to the course 1 - Chapter 1.1: About the course 2 - Chapter 1.
NERS311/Fall 2014 Revision: August 27, 2014 Index to the Lecture notes Alex Bielajew, 2927 Cooley, bielajew@umich.edu NERS 311 Current Old notes notes Chapter 1 1 1 Chapter 1: Introduction to the course
Introduction. Introduction. Forces An. Forces An. Forces in Action. Forces in Action. Pressure and Pressure. Pressure and Pressure.
Forces An Introduction A force is a vector quantity. What does this mean? Forces An Introduction A vector quantity, such as force, has a direction as well as a magnitude. 1 1 Forces in Action The moment
Particle Detectors and Quantum Physics (2) Stefan Westerhoff Columbia University NYSPT Summer Institute 2002
Particle Detectors and Quantum Physics (2) Stefan Westerhoff Columbia University NYSPT Summer Institute 2002 More Quantum Physics We know now how to detect light (or photons) One possibility to detect
Advanced Stellar Astrophysics
v Advanced Stellar Astrophysics William K. Rose University of Maryland College Park CAMBRIDGE UNIVERSITY PRESS Contents Preface xiii Star formation and stellar evolution: an overview 1 1 A short history
Nuclear Astrophysics - I
Nuclear Astrophysics - I Carl Brune Ohio University, Athens Ohio Exotic Beam Summer School 2016 July 20, 2016 Astrophysics and Cosmology Observations Underlying Physics Electromagnetic Spectrum: radio,
An Introduction to Radio Astronomy
An Introduction to Radio Astronomy Bernard F. Burke Massachusetts Institute of Technology and Francis Graham-Smith Jodrell Bank, University of Manchester CAMBRIDGE UNIVERSITY PRESS Contents Preface Acknowledgements
Modified Physics Course Descriptions Old
Modified Physics Course Descriptions Old New PHYS 122, General Physics II, 4 cr, 3 cl hrs, 2 recitation hrs Prerequisite: PHYS 121 Corequisites: MATH 132; PHYS 122L Continuation of PHYS 121 including electricity
Name: Class: Date: Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.
Name: Class: Date: AP REVIEW 3 Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.. For a mass hanging from a spring, the maximum displacement the
Chapter 1. Introduction
Chapter 1 Introduction The book Introduction to Modern Physics: Theoretical Foundations starts with the following two paragraphs [Walecka (2008)]: At the end of the 19th century, one could take pride in
PHYSICS CURRICULUM. Unit 1: Measurement and Mathematics
Chariho Regional School District - Science Curriculum September, 2016 PHYSICS CURRICULUM Unit 1: Measurement and Mathematics OVERVIEW Summary Mathematics is an essential tool of physics. This unit will
PELLISSIPPI STATE COMMUNITY COLLEGE MASTER SYLLABUS CALCULUS BASED PHYSICS II PHYS 2120
PELLISSIPPI STATE COMMUNITY COLLEGE MASTER SYLLABUS CALCULUS BASED PHYSICS II PHYS 2120 Class Hours: 3.0 Credit Hours: 4.0 Laboratory Hours: 3.0 Revised: Spring 2011 Catalog Course Description: For students
IoP. An Introduction to the Science of Cosmology. Derek Raine. Ted Thomas. Series in Astronomy and Astrophysics
Series in Astronomy and Astrophysics An Introduction to the Science of Cosmology Derek Raine Department of Physics and Astronomy University of Leicester, UK Ted Thomas Department of Physics and Astronomy
Physics Overview. Assessments Assessments Adopted from course materials Teacher-created assessments Standard Physical Science
Physics Curriculum Physics Overview Course Description Physics is the study of the physical world and is a mathematical application of science. The study includes an investigation of translational and
Moment of beginning of space-time about 13.7 billion years ago. The time at which all the material and energy in the expanding Universe was coincident
Big Bang Moment of beginning of space-time about 13.7 billion years ago The time at which all the material and energy in the expanding Universe was coincident Only moment in the history of the Universe
Conceptos generales de astrofísica
Tema 14 Conceptos generales de astrofísica Asignatura de Física Nuclear Curso académico 2009/2010 Universidad de Santiago de Compostela 1 1. Nuclear Astrophysic s domain Nuclear Astrophysics is a relatively
Fundamentals of Spectroscopy for Optical Remote Sensing. Course Outline 2009
Fundamentals of Spectroscopy for Optical Remote Sensing Course Outline 2009 Part I. Fundamentals of Quantum Mechanics Chapter 1. Concepts of Quantum and Experimental Facts 1.1. Blackbody Radiation and
Atomic Structure & Radiative Transitions
Atomic Structure & Radiative Transitions electron kinetic energy nucleus-electron interaction electron-electron interaction Remember the meaning of spherical harmonics Y l, m (θ, ϕ) n specifies the
ASTROPHYSICS. K D Abhyankar. Universities Press S T A R S A ND G A L A X I E S
ASTROPHYSICS S T A R S A ND G A L A X I E S K D Abhyankar Universities Press Contents Foreword vii Preface ix 1 Introduction 1 1.1 ' Astronomy and astrophysics 1 1.2 Importance of astronomy 2 1.3 Methods
Physics Curriculum Pacing Guide MONTGOMERY COUNTY PUBLIC SCHOOLS
MONTGOMERY COUNTY PUBLIC SCHOOLS Physics Curriculum Pacing Guide 1 st 9 Weeks SOL Objectives Vocabulary 2 Days INTRODUCTION: PH.1 The student will plan and conduct investigations using experimental design
2. Determine the excess charge on the outer surface of the outer sphere (a distance c from the center of the system).
Use the following to answer question 1. Two point charges, A and B, lie along a line separated by a distance L. The point x is the midpoint of their separation. 1. Which combination of charges will yield
Major Option C1 Astrophysics. C1 Astrophysics
C1 Astrophysics Course co-ordinator: Julien Devriendt jeg@astro.ox.ac.uk C1 offers a total of ~40 lectures on five themes covering a broad range of topics in contemporary astrophysics. Each theme takes
Brock University. Test 1, February, 2017 Number of pages: 9 Course: ASTR 1P02 Number of Students: 480 Date of Examination: February 6, 2017
Brock University Test 1, February, 2017 Number of pages: 9 Course: ASTR 1P02 Number of Students: 480 Date of Examination: February 6, 2017 Number of hours: 50 min Time of Examination: 18:00 18:50 Instructor:
Cumulative Review 1 Use the following information to answer the next two questions.
Cumulative Review 1 Use the following information to answer the next two questions. 1. At what distance from the mirror is the image located? a. 0.10 m b. 0.20 m c. 0.30 m d. 0.40 m 2. At what distance
Highenergy Nuclear Optics of Polarized Particles
Highenergy Nuclear Optics of Polarized Particles Vladimir G. Baryshevsky Research Institute for Nuclear Problems Belarusian State University 1> World Scientific NEW JERSEY LONDON SINGAPORE BEIJING SHANGHAI
With Modern Physics For Scientists and Engineers
With Modern Physics For Scientists and Engineers Third Edition Richard Wolfson Middlebury College Jay M. Pasachoff Williams College ^ADDISON-WESLEY An imprint of Addison Wesley Longman, Inc. Reading, Massachusetts
Astronomy Chapter 12 Review
Astronomy Chapter 12 Review Approximately how massive is the Sun as compared to the Earth? A. 100 times B. 300 times C. 3000 times D. 300,000 times E. One million times Approximately how massive is the
Unit assessments are composed of multiple choice and free response questions from AP exams.
AP Physics B Text: Serway, Raymond A., and Jerry S. Faugh, College Physics, 7 th ed. Belmont, CA: Thomson Brooks/Cole, 2006. Course evaluation: - Grade determination Final Exam 15% Unit Exams 42.5% Daily
Review: Properties of a wave
Radiation travels as waves. Waves carry information and energy. Review: Properties of a wave wavelength (λ) crest amplitude (A) trough velocity (v) λ is a distance, so its units are m, cm, or mm, etc.
Physics 126 Practice Exam #4 Professor Siegel
Physics 126 Practice Exam #4 Professor Siegel Name: Lab Day: 1. Light is usually thought of as wave-like in nature and electrons as particle-like. In which one of the following instances does light behave
Physics For Scientists and Engineers A Strategic Approach 3 rd Edition, AP Edition, 2013 Knight
For Scientists and Engineers A Strategic Approach 3 rd Edition, AP Edition, 2013 Knight To the Advanced Placement Topics for C *Advanced Placement, Advanced Placement Program, AP, and Pre-AP are registered
Prentice Hall EARTH SCIENCE
Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 24 Studying the Sun 24.1 The Study of Light Electromagnetic Radiation Electromagnetic radiation includes gamma rays, X-rays, ultraviolet light, visible
PELLISSIPPI STATE TECHNICAL COMMUNITY COLLEGE MASTER SYLLABUS CALCULUS BASED PHYSICS II PHYS 2120
PELLISSIPPI STATE TECHNICAL COMMUNITY COLLEGE MASTER SYLLABUS CALCULUS BASED PHYSICS II PHYS 2120 Class Hours: 3.0 Credit Hours: 4.0 Laboratory Hours: 3.0 Revised: Spring 05 Catalog Course Description:
Brock University. Test 1, January, 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 500 Date of Examination: January 29, 2015
Brock University Test 1, January, 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 500 Date of Examination: January 29, 2015 Number of hours: 50 min Time of Examination: 18:00 15:50 Instructor:
LESSON PLAN. B.Sc. THIRD YEAR ( REGULATION) FIXTH SEMESTER
DEPARTMENT OF PHYSICS AND NANOTECHNOLOGY LESSON PLAN B.Sc. THIRD YEAR (2015-2016 REGULATION) FIXTH SEMESTER SRM UNIVERSITY FACULTY OF SCIENCE AND HUMANITIES SRM NAGAR, KATTANKULATHUR 603 203 1 Subject
Unity in the Whole Structure
Cosmology II Unity in the Whole Structure How is it possible by any methods of observation yet known to the astronomer to learn anything about the universe as a whole? It is possible only because the universe,
Physics HW Set 3 Spring 2015
1) If the Sun were replaced by a one solar mass black hole 1) A) life here would be unchanged. B) we would still orbit it in a period of one year. C) all terrestrial planets would fall in immediately.
PHYS1118 Astronomy II
PHYS1118 Astronomy II Course Description: This course is designed for non-science students. A study of astronomy as related to humans and society. Topics include elements of Newtonian physics, Relativity,
Physics 1C. End of Chapter 30 Exam Preparationds
Physics 1C End of Chapter 30 Exam Preparationds Radioactive Decay Example The isotope 137 Cs is a standard laboratory source of gamma rays. The half-life of 137 Cs is 30 years. (a) How many 137 Cs atoms
Chapter 27 The Early Universe Pearson Education, Inc.
Chapter 27 The Early Universe Units of Chapter 27 27.1 Back to the Big Bang 27.2 The Evolution of the Universe More on Fundamental Forces 27.3 The Formation of Nuclei and Atoms 27.4 The Inflationary Universe
Name Final Exam December 7, 2015
Name Final Exam December 7, 015 This test consists of five parts. Please note that in parts II through V, you can skip one question of those offered. Part I: Multiple Choice (mixed new and review questions)
Number of Stars: 100 billion (10 11 ) Mass : 5 x Solar masses. Size of Disk: 100,000 Light Years (30 kpc)
THE MILKY WAY GALAXY Type: Spiral galaxy composed of a highly flattened disk and a central elliptical bulge. The disk is about 100,000 light years (30kpc) in diameter. The term spiral arises from the external
Chapter 28. Atomic Physics
Chapter 28 Atomic Physics Quantum Numbers and Atomic Structure The characteristic wavelengths emitted by a hot gas can be understood using quantum numbers. No two electrons can have the same set of quantum
Astronomy. Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes
Astronomy Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes are hot, compact stars whose mass is comparable to the Sun's and size to the Earth's. A. White dwarfs B. Neutron stars
School of Physics & Astronomy
School of Physics & Astronomy Important Degree Information: B.Sc./M.A. Honours The general requirements are 480 credits over a period of normally 4 years(and not more than 5 years) or part-time equivalent;
Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical
Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical Trigonometry p. 9 The Earth p. 12 The Celestial Sphere p. 14 The
29:50 Stars, Galaxies, and the Universe Final Exam December 13, 2010 Form A
29:50 Stars, Galaxies, and the Universe Final Exam December 13, 2010 Form A There are 40 questions. Read each question and all of the choices before choosing. Budget your time. No whining. Walk with Ursus!
Bachelor s Degree in Chemistry. 1 st YEAR Mechanics and Thermodynamics ECTS credits: 6 Semester: 1. Teaching objectives
1 st YEAR 5263 Mechanics and Thermodynamics ECTS credits: 6 Semester: 1 The student should be able to: 1. Understand the concepts and describe the fundamental aspects of Mechanics and Thermodynamics. 2.
VU lecture Introduction to Particle Physics. Thomas Gajdosik, FI & VU. Big Bang (model)
Big Bang (model) What can be seen / measured? basically only light _ (and a few particles: e ±, p, p, ν x ) in different wave lengths: microwave to γ-rays in different intensities (measured in magnitudes)
13. Basic Nuclear Properties
13. Basic Nuclear Properties Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 13. Basic Nuclear Properties 1 In this section... Motivation for study The strong nuclear force Stable nuclei Binding
Introduction to Modern Physics
SECOND EDITION Introduction to Modern Physics John D. McGervey Case Western Reserve University Academic Press A Subsidiary of Harcourt Brace Jovanovich Orlando San Diego San Francisco New York London Toronto
There are three units of study within the Physics Specialisation. ATPPHY001 - Unit 1:
The Physics Specialisation applies to those who require foundation Physics knowledge and skills for entrance to tertiary study in a relevant discipline or field. There are three units of study within the
MIDSUMMER EXAMINATIONS 2001 PHYSICS, PHYSICS WITH ASTROPHYSICS PHYSICS WITH SPACE SCIENCE & TECHNOLOGY PHYSICS WITH MEDICAL PHYSICS
No. of Pages: 6 No. of Questions: 10 MIDSUMMER EXAMINATIONS 2001 Subject PHYSICS, PHYSICS WITH ASTROPHYSICS PHYSICS WITH SPACE SCIENCE & TECHNOLOGY PHYSICS WITH MEDICAL PHYSICS Title of Paper MODULE PA266
SPRING GROVE AREA SCHOOL DISTRICT. Course Description. Instructional Strategies, Learning Practices, Activities, and Experiences.
SPRING GROVE AREA SCHOOL DISTRICT PLANNED COURSE OVERVIEW Course Title: Advanced Placement Physics 1 Grade Level(s): 10-12 Units of Credit: 1.5 credits Classification: Elective Length of Course: 30 cycles
AP Goal 1. Physics knowledge
Physics 2 AP-B This course s curriculum is aligned with College Board s Advanced Placement Program (AP) Physics B Course Description, which supports and encourages the following broad instructional goals:
32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES
32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES 32.1 Biological Effects of Ionizing Radiation γ-rays (high-energy photons) can penetrate almost anything, but do comparatively little damage.
PHYS 340 ( From Atoms to the Universe ): SECTION A
PHYS 340 ( From Atoms to the Universe ): (Tuesday, April 26th, 2011) 12.00-2.30 pm, Room Hennings 301 FINAL EXAM This exam will last 2 hrs and 30 mins. The only material allowed into the exam will be pens,
Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999
Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999 Reminder: When I write these questions, I believe that there is one one correct answer. The questions consist of all parts a e. Read the entire
A) n L < 1.0 B) n L > 1.1 C) n L > 1.3 D) n L < 1.1 E) n L < 1.3
1. A beam of light passes from air into water. Which is necessarily true? A) The frequency is unchanged and the wavelength increases. B) The frequency is unchanged and the wavelength decreases. C) The
Marcelo Alonso. Edward J. Finn. Georgetown University. Prentice Hall
PHYSICS Marcelo Alonso Florida Institute of Technology Edward J. Finn Georgetown University PEARSON Prentice Hall Harlow, England " London " New York " Boston " San Francisco -Toronto Sydney " Tokyo "
Atomic & Nuclear Physics
Atomic & Nuclear Physics Life and Atoms Every time you breathe you are taking in atoms. Oxygen atoms to be exact. These atoms react with the blood and are carried to every cell in your body for various