The projects that have been chosen so far include 36 people,13 teams. So far, So Good, expect 2/3 get >=B+

Size: px
Start display at page:

Download "The projects that have been chosen so far include 36 people,13 teams. So far, So Good, expect 2/3 get >=B+"

Transcription

1 PHYS 342 Modern Physics Project Discussion III Today's Projects for Discussion: a) Study a particle accelerators Large Hadron Collider (LHC) b) Search for Dark Matter The projects that have been chosen so far include 36 people,13 teams. 1. Stevie Bastin, Stjepan Kraljic, Zack Rowe, Gravitational wave/gravitons 2. Lifu Wang, Weiyuan Deng, and Yufeng Zhang, Modern Experiment to Test Special Relativity 3.Uladzimir Kasacheuski, Jonathan Brown, and Vishal Patel, interview researchers at IUPUI 4. Zongying Xu, Zheng Huang, and Jiani Xie, Blackbody Radiation 5. Chuanyi Chen, Zihao Fu, and Lingbin Meng, Introduction to General Relativity 6. Hongkun Zhu, Guiming Chen, and Jiawen Wang, First gravitational wave observation 7. Aaron, Joseph, and Will, atomic physics explanation of the helium laser 8. Daulton Eaton, Robert McKay, and Guy Wiss, Monte Carlo Simulation Method for the Schrodinger equation 9. Tianyang Wu, Haizhen Xie, and Bingcheng Zhou, Neutrino physics 10. Josiah Alstott, Thomas Freestone, and Ross Wallgren, Atomic clock 11. Chase Howard and Alex Canner, Gravitational lensing 12. Kailiang Chen, Zhong Jin, Peiming Zhu, Quantum Information 13. Ryan, Particle Acclerator LHC So far, So Good, expect 2/3 get >=B+ You must /give me your electronic version of.ppt or report (.doc,.pdf) before Apr.15 to secure a presentation time slot. Bottom Line: We already have 413 points, only ~300 points left. You need at least 420 points in the end to safely pass. 1

2 Large Hadron Collider (LHC) Large Hadron Collider (LHC) Projects: You need to write a short review about the history of LHC and the problems that LHC will address. You also need to introduce the basic structure and instrumentation of LHC. You can also introduce the recent discoveries found by LHC and the future plan of LHC

3 3

4 4

5 Big Bang The beginning of the universe 5

6 Problems that LHC will address Higgs Boson Projects for Discussion The God Particle: The Higgs Boson Use water to understand the Higgs Boson upyw Today's Projects for Discussion: a) Study a Particle accelerators Large Hadron Collider (LHC) b) Search for Dark Matter c) Project selected by you! 6

7 Unknown Matter in the Universe In Ursa Major constellation. Distance is 30 million light years. For comparison, distance from Earth to the galactic center is a factor of ~1000 times less. 30 millions light years Horsehead Nebula. Pink background is hydrogen emission from IC434 emission. Search for Dark Matter Question: Is the mass in the universe all observable through emission or absorption of electromagnetic radiation? Dark Matter...is matter that does not shine or absorb light, and has therefore escaped direct detection by electromagnetic transducers like telescopes, radio antennas, x-ray satellites... There is strong experimental evidence that there is more dark matter than luminous matter in the universe! Search for Dark Matter Projects: You need to write a short review about the search for dark matter. You need to introduce the evident of existing dark matter in the universe, the possible candidates for dark matter, and how physicist detect dark matter in ongoing projects. 7

8 Examples of Rotation Curves DM Evidence I Rotation Curves for Our Galaxy The Correct Way to Think about Our Galaxy Gravitational Microlensing 8

9 DM Evidence II Gravitational Lensing in Clusters of Galaxies Microlensing Targets Large Magellanic Cloud Small Magellanic Cloud Possible Dark-Matter Candidates DIRECT DETECTION Dark matter elastically scatters off nuclei DM Nuclear recoils detected by phonons, scintillation, ionization,, e, 9

10 Neutrinos as Nonbaryonic Dark Matter Other Types of Nonbaryonic Dark Matter XENON Dark Matter Detector About 100 neutrinos per cubic cm, throughout space. Superkamiokande, an Example of a Neutrino Observatory Mass is about 0.05 ev = 1 / 10,000,000 mass of electron, although some uncertainty. Neutrinos in the Universe have nearly as much mass as all of the stars! Large Hadron Collider at CERN X-ray Evidence for Dark Matter in Clusters of Galaxies Need enough gravity to keep the X-ray gas from boiling off into intergalactic space. The LHC will search for supersymmetric and other new subatomic particles. 10

11 Dark Matter Dark Matter The most powerful machine: for people love experiments 11

t b e - d -1/3 4/18/2016 Particle Classification 3 Generations of Leptons and Quarks Standard Model

t b e - d -1/3 4/18/2016 Particle Classification 3 Generations of Leptons and Quarks Standard Model PHYS 342 Moern Physics Elementary Particles an Stanar Moel II Toay's Contents: a) Particle Collier b) Stanar Moel of Elementary Particles c) Fiel Bosons: qantization of for basic forces ) Higgs Boson:

More information

Project Paper May 13, A Selection of Dark Matter Candidates

Project Paper May 13, A Selection of Dark Matter Candidates A688R Holly Sheets Project Paper May 13, 2008 A Selection of Dark Matter Candidates Dark matter was first introduced as a solution to the unexpected shape of our galactic rotation curve; instead of showing

More information

On the track of the dark forces. A.J. Krasznahorkay Inst. for Nucl. Res., Hung. Acad. of Sci. (ATOMKI)

On the track of the dark forces. A.J. Krasznahorkay Inst. for Nucl. Res., Hung. Acad. of Sci. (ATOMKI) On the track of the dark forces A.J. Krasznahorkay Inst. for Nucl. Res., Hung. Acad. of Sci. (ATOMKI) Outline Introduction: the light dark matter Previous results and new plans The internal pair creation

More information

Dark Matter ASTR 2120 Sarazin. Bullet Cluster of Galaxies - Dark Matter Lab

Dark Matter ASTR 2120 Sarazin. Bullet Cluster of Galaxies - Dark Matter Lab Dark Matter ASTR 2120 Sarazin Bullet Cluster of Galaxies - Dark Matter Lab Mergers: Test of Dark Matter vs. Modified Gravity Gas behind DM Galaxies DM = location of gravity Gas = location of most baryons

More information

The Mystery of Dark Matter

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

More information

ASTR 1P02 Test 2, March 2017 Page 1 BROCK UNIVERSITY. Test 2: March 2017 Number of pages: 9 Course: ASTR 1P02, Section 2 Number of students: 1193

ASTR 1P02 Test 2, March 2017 Page 1 BROCK UNIVERSITY. Test 2: March 2017 Number of pages: 9 Course: ASTR 1P02, Section 2 Number of students: 1193 ASTR 1P02 Test 2, March 2017 Page 1 BROCK UNIVERSITY Test 2: March 2017 Number of pages: 9 Course: ASTR 1P02, Section 2 Number of students: 1193 Examination date: 4 March 2017 Time limit: 50 min Time of

More information

A100H Exploring the Universe: Quasars, Dark Matter, Dark Energy. Martin D. Weinberg UMass Astronomy

A100H Exploring the Universe: Quasars, Dark Matter, Dark Energy. Martin D. Weinberg UMass Astronomy A100H Exploring the :, Dark Matter, Dark Energy Martin D. Weinberg UMass Astronomy astron100h-mdw@courses.umass.edu April 19, 2016 Read: Chaps 20, 21 04/19/16 slide 1 BH in Final Exam: Friday 29 Apr at

More information

Today. The nature of the Universe - Beyond the Standard Model

Today. The nature of the Universe - Beyond the Standard Model Today The nature of the Universe - Beyond the Standard Model Dark Matter and Dark Energy String Theory and the quest to unify gravity and quantum theory Begin watching PBS NOVA special The Elegant Universe

More information

Today. The goals of science. The nature of the Universe - Beyond the Standard Model

Today. The goals of science. The nature of the Universe - Beyond the Standard Model Today The nature of the Universe - Beyond the Standard Model Dark Matter and Dark Energy String Theory and the quest to unify gravity and quantum theory Begin watching PBS NOVA special The Elegant Universe

More information

Other Galaxy Types. Active Galaxies. A diagram of an active galaxy, showing the primary components. Active Galaxies

Other Galaxy Types. Active Galaxies. A diagram of an active galaxy, showing the primary components. Active Galaxies Other Galaxy Types Active Galaxies Active Galaxies Seyfert galaxies Radio galaxies Quasars Origin??? Different in appearance Produce huge amount of energy Similar mechanism a Galactic mass black hole at

More information

Particle accelerators

Particle accelerators Particle accelerators Charged particles can be accelerated by an electric field. Colliders produce head-on collisions which are much more energetic than hitting a fixed target. The center of mass energy

More information

Dark Matter: Finding the Invisible

Dark Matter: Finding the Invisible Dark Matter: Finding the Invisible Laura Storch Boston University WR150 LA Image courtesy of Hubble Deep Field Overview: Dark Matter: -Why do we think it exists? -Observational evidence -What are its properties?

More information

UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC. Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009

UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC. Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009 UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009 OUTLINE! Some things we ve learned about the physical

More information

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

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

More information

3/6/12! Astro 358/Spring 2012! Galaxies and the Universe! Dark Matter in Spiral Galaxies. Dark Matter in Galaxies!

3/6/12! Astro 358/Spring 2012! Galaxies and the Universe! Dark Matter in Spiral Galaxies. Dark Matter in Galaxies! 3/6/12 Astro 358/Spring 2012 Galaxies and the Universe Dark Matter in Galaxies Figures + Tables for Lectures (Feb 16-Mar 6) Dark Matter in Spiral Galaxies Flat rotation curve of Milky Way at large radii

More information

Card Appendix Quantum Concepts

Card Appendix Quantum Concepts 1 Physics 310 Card Appendix Quantum Concepts Table of Contents 0. Blackbody Radiation 2 3. Normalize 2 4. Angular Momentum 3 4. Hydrogen 4 5. Wavefunction 4 6. Photoelectric Effect 5 7. Lowering Operator

More information

Number of Stars: 100 billion (10 11 ) Mass : 5 x Solar masses. Size of Disk: 100,000 Light Years (30 kpc)

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

More information

Week 3 - Part 2 Recombination and Dark Matter. Joel Primack

Week 3 - Part 2 Recombination and Dark Matter. Joel Primack Astro/Phys 224 Spring 2012 Origin and Evolution of the Universe Week 3 - Part 2 Recombination and Dark Matter Joel Primack University of California, Santa Cruz http://pdg.lbl.gov/ In addition to the textbooks

More information

Dark Side of the Universe

Dark Side of the Universe Dark Side of the Universe Bhaskar Dutta Department of Physics & Astronomy Texas A&M University Dark Side of the Universe 1 Content of the Universe 4% The 23% is still unobserved in the laboratory.. (This

More information

Windows on the Cosmos

Windows on the Cosmos Windows on the Cosmos Three types of information carriers about what s out there arrive on Earth: Electromagnetic Radiation Visible light, UV, IR => telescopes (Earth/Space) Radio waves => Antennae ( Dishes

More information

REALIZING EINSTEIN S DREAM. Exploring Our Mysterious Universe

REALIZING EINSTEIN S DREAM. Exploring Our Mysterious Universe REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe Mysteries of the Universe Quarks Leptons Higgs Bosons Supersymmetric Particles SuperString Theory Dark Matter Dark Energy and the cosmological

More information

An Introduction to Particle Physics

An Introduction to Particle Physics An Introduction to Particle Physics The Universe started with a Big Bang The Universe started with a Big Bang What is our Universe made of? Particle physics aims to understand Elementary (fundamental)

More information

Dark Matter Searches. Marijke Haffke University of Zürich

Dark Matter Searches. Marijke Haffke University of Zürich University of Zürich Structure Ι. Introduction - Dark Matter - WIMPs Ι Ι. ΙΙΙ. ΙV. V. Detection - Philosophy & Methods - Direct Detection Detectors - Scintillators - Bolometer - Liquid Noble Gas Detectors

More information

32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES

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.

More information

The first 400,000 years

The first 400,000 years The first 400,000 years All about the Big Bang Temperature Chronology of the Big Bang The Cosmic Microwave Background (CMB) The VERY early universe Our Evolving Universe 1 Temperature and the Big Bang

More information

Cosmologists dedicate a great deal of effort to determine the density of matter in the universe. Type Ia supernovae observations are consistent with

Cosmologists dedicate a great deal of effort to determine the density of matter in the universe. Type Ia supernovae observations are consistent with Notes for Cosmology course, fall 2005 Dark Matter Prelude Cosmologists dedicate a great deal of effort to determine the density of matter in the universe Type Ia supernovae observations are consistent

More information

LHC searches for dark matter.! Uli Haisch

LHC searches for dark matter.! Uli Haisch LHC searches for dark matter! Uli Haisch Evidence for dark matter Velocity Observed / 1 p r Disk 10 5 ly Radius Galaxy rotation curves Evidence for dark matter Bullet cluster Mass density contours 10 7

More information

The Big Bang Theory. Rachel Fludd and Matthijs Hoekstra

The Big Bang Theory. Rachel Fludd and Matthijs Hoekstra The Big Bang Theory Rachel Fludd and Matthijs Hoekstra Theories from Before the Big Bang came from a black hole from another universe? our universe is part of a multiverse? just random particles? The Big

More information

Detectors for astroparticle physics

Detectors for astroparticle physics Detectors for astroparticle physics Teresa Marrodán Undagoitia marrodan@physik.uzh.ch Universität Zürich Kern und Teilchenphysik II, Zürich 07.05.2010 Teresa Marrodán Undagoitia (UZH) Detectors for astroparticle

More information

PART 3 Galaxies. Gas, Stars and stellar motion in the Milky Way

PART 3 Galaxies. Gas, Stars and stellar motion in the Milky Way PART 3 Galaxies Gas, Stars and stellar motion in the Milky Way The Interstellar Medium The Sombrero Galaxy Space is far from empty! Clouds of cold gas Clouds of dust In a galaxy, gravity pulls the dust

More information

Notes for Wednesday, July 16; Sample questions start on page 2 7/16/2008

Notes for Wednesday, July 16; Sample questions start on page 2 7/16/2008 Notes for Wednesday, July 16; Sample questions start on page 2 7/16/2008 Wed, July 16 MW galaxy, then review. Start with ECP3Ch14 2 through 8 Then Ch23 # 8 & Ch 19 # 27 & 28 Allowed Harlow Shapely to locate

More information

Neutrino Astronomy. Ph 135 Scott Wilbur

Neutrino Astronomy. Ph 135 Scott Wilbur Neutrino Astronomy Ph 135 Scott Wilbur Why do Astronomy with Neutrinos? Stars, active galactic nuclei, etc. are opaque to photons High energy photons are absorbed by the CMB beyond ~100 Mpc 10 20 ev protons,

More information

The Nature of Light and Matter: 3

The Nature of Light and Matter: 3 The Nature of Light and Matter: 3 Doppler Effect, Mater and Energy ASTR 101 10/31//2017 1 Light from Moving objects: Doppler effect When there is a relative motion between the source and the observer,

More information

Stars and Galaxies 1

Stars and Galaxies 1 Stars and Galaxies 1 Characteristics of Stars 2 Star - body of gases that gives off great amounts of radiant energy as light and heat 3 Most stars look white but are actually different colors Antares -

More information

The Search for Dark Matter, and Xenon1TP

The Search for Dark Matter, and Xenon1TP The Search for Dark Matter, and Xenon1TP by Jamin Rager Hillsdale College Assistant Prof. Rafael Lang Purdue University Dept. of Physics Galaxy NGC 3198 2 Galaxy NGC 3198 Rotation Curves http://bustard.phys.nd.edu/phys171/lectures/dm.html

More information

AST1100 Lecture Notes

AST1100 Lecture Notes AST1100 Lecture Notes 4 Stellar orbits and dark matter 1 Using Kepler s laws for stars orbiting the center of a galaxy We will now use Kepler s laws of gravitation on much larger scales. We will study

More information

Science advances by a combination of normal science and discovery of anomalies.

Science advances by a combination of normal science and discovery of anomalies. Science advances by a combination of normal science and discovery of anomalies. Many revolutions come from long periods of normal science reinforced by exceptional science. example: accelerating universe

More information

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016 Elementary Particle Physics Glossary Course organiser: Dr Marcella Bona February 9, 2016 1 Contents 1 Terms A-C 5 1.1 Accelerator.............................. 5 1.2 Annihilation..............................

More information

Galaxies and the Universe. Our Galaxy - The Milky Way The Interstellar Medium

Galaxies and the Universe. Our Galaxy - The Milky Way The Interstellar Medium Galaxies and the Universe Our Galaxy - The Milky Way The Interstellar Medium Our view of the Milky Way The Radio Sky COBE Image of our Galaxy The Milky Way Galaxy - The Galaxy By Visual Observation

More information

Today. Gravitational Lenses 11/19/2013. Astronomy Picture of the Day

Today. Gravitational Lenses 11/19/2013. Astronomy Picture of the Day ASTR 1020: Stars & Galaxies November 15, 2013 Reading for Monday: Chapter 23, section 23.1-23.3. MasteringAstronomy homework on Galaxy Evolution is due tonight at midnight. Exam 3 is on Wednesday, Nov.

More information

Particle + Physics at ATLAS and the Large Hadron Coillder

Particle + Physics at ATLAS and the Large Hadron Coillder Particle + Physics at ATLAS and the Large Hadron Coillder Discovering the elementary particles of the Universe Kate Shaw The International Centre for Theoretical Physics + Overview Introduction to Particle

More information

Astronomy 104: Second Exam

Astronomy 104: Second Exam Astronomy 104: Second Exam Stephen Lepp October 29, 2014 Each question is worth 2 points. Write your name on this exam and on the scantron. Short Answer A The Sun is powered by converting hydrogen to what?

More information

Large Scale Structure

Large Scale Structure Large Scale Structure Measuring Distance in Universe-- a ladder of steps, building from nearby Redshift distance Redshift = z = (λ observed - λ rest )/ λ rest Every part of a distant spectrum has same

More information

Potentially useful formulas: F = G m 1m 2 r 2 F = k q 1q 2 F = ma Distance = Speed Time

Potentially useful formulas: F = G m 1m 2 r 2 F = k q 1q 2 F = ma Distance = Speed Time PHY100 May 4, 2010 Final Exam Name: Aran Garcia-Bellido Please read the problems carefully and answer them in the space provided. Write on the back of the page, if necessary. Show your work where requested

More information

Standard LHC

Standard LHC Standard Model@LHC Prof. E. Barberio Prof. G. Taylor, Dr. P. Urquijo Successful theory of fundamental interactions Survived numerous experimental tests Only missing the Higgs boson LHC built to look for

More information

Galaxies Guiding Questions

Galaxies Guiding Questions Galaxies Guiding Questions How did astronomers first discover other galaxies? How did astronomers first determine the distances to galaxies? Do all galaxies have spiral arms, like the Milky Way? How do

More information

What does Dark Matter have to do with the Big Bang Theory?

What does Dark Matter have to do with the Big Bang Theory? Lunar Society What does Dark Matter have to do with the Big Bang Theory? Prof. David Toback Texas A&M University Mitchell Institute for Fundamental Physics and Astronomy Prologue We live in a time of remarkable

More information

Exam 3 Astronomy 100, Section 3. Some Equations You Might Need

Exam 3 Astronomy 100, Section 3. Some Equations You Might Need Exam 3 Astronomy 100, Section 3 Some Equations You Might Need modified Kepler s law: M = [a(au)]3 [p(yr)] (a is radius of the orbit, p is the rotation period. You 2 should also remember that the period

More information

The atom cont. +Investigating EM radiation

The atom cont. +Investigating EM radiation The atom cont. +Investigating EM radiation Announcements: First midterm is 7:30pm on Sept 26, 2013 Will post a past midterm exam from 2011 today. We are covering Chapter 3 today. (Started on Wednesday)

More information

Chapter 22 Lecture. The Cosmic Perspective. Seventh Edition. The Birth of the Universe Pearson Education, Inc.

Chapter 22 Lecture. The Cosmic Perspective. Seventh Edition. The Birth of the Universe Pearson Education, Inc. Chapter 22 Lecture The Cosmic Perspective Seventh Edition The Birth of the Universe The Birth of the Universe 22.1 The Big Bang Theory Our goals for learning: What were conditions like in the early universe?

More information

v = H o d Hubble s Law: Distant galaxies move away fastest Velocity (v) is proportional to Distance (d):

v = H o d Hubble s Law: Distant galaxies move away fastest Velocity (v) is proportional to Distance (d): Hubble s Law: Distant galaxies move away fastest Velocity (v) is proportional to Distance (d): v = H o d The Hubble Constant was measured after decades of observation: H 0 = 70 km/s/mpc Velocity (km/s)

More information

Chapter 22: Cosmology - Back to the Beginning of Time

Chapter 22: Cosmology - Back to the Beginning of Time Chapter 22: Cosmology - Back to the Beginning of Time Expansion of Universe implies dense, hot start: Big Bang Future of universe depends on the total amount of dark and normal matter Amount of matter

More information

Exam Results. Force between charges. Electric field lines. Other particles and fields

Exam Results. Force between charges. Electric field lines. Other particles and fields Exam: Exam scores posted on Learn@UW No homework due next week Exam Results F D C BC B AB A Phy107 Fall 2006 1 Particles and fields We have talked about several particles Electron,, proton, neutron, quark

More information

What does Dark Matter have to do with the Big Bang Theory?

What does Dark Matter have to do with the Big Bang Theory? MSC Bethancourt Lecture What does Dark Matter have to do with the Big Bang Theory? Prof. David Toback Texas A&M University Mitchell Institute for Fundamental Physics and Astronomy Prologue We live in a

More information

Exam #3. Final Exam. Exam 3 review. How do we measure properties of a star? A detailed outline of study topics is here:

Exam #3. Final Exam. Exam 3 review. How do we measure properties of a star? A detailed outline of study topics is here: Exam #3 Exam #3 is Thursday 4/9 in this room You can bring page of notes (front and back) Bring your calculator and a # pencil Exam 3 covers material from 4/1 onward (only 8 lectures) Consequently, no

More information

Preface to Presentation

Preface to Presentation Preface to Presentation I gave a presentation last October about time travel, warp drive, travel to a Goldilocks Planet etc. to provide some possible place to escape a possible dying world I mentioned

More information

Chapter 19 Galaxies. Hubble Ultra Deep Field: Each dot is a galaxy of stars. More distant, further into the past. halo

Chapter 19 Galaxies. Hubble Ultra Deep Field: Each dot is a galaxy of stars. More distant, further into the past. halo Chapter 19 Galaxies Hubble Ultra Deep Field: Each dot is a galaxy of stars. More distant, further into the past halo disk bulge Barred Spiral Galaxy: Has a bar of stars across the bulge Spiral Galaxy 1

More information

The Formation of the Solar System

The Formation of the Solar System Earth and the Solar System The Formation of the Solar System Write a number beside each picture to rank each from the oldest (1) to the youngest (4). The universe includes everything that exists: all matter,

More information

Phys333 - sample questions for final

Phys333 - sample questions for final Phys333 - sample questions for final USEFUL INFO: c=300,000 km/s ; AU = 1.5 x 10 11 m ; 1000 nm hc/ev ; ev/k 10 4 K; H-ionization energy is 13.6 ev Name MULTIPLE CHOICE. Choose the one alternative that

More information

John Ellis King s College London (& CERN) Welcome! Introduction to CERN. CERN: Accelerating Science and Innovation

John Ellis King s College London (& CERN) Welcome! Introduction to CERN. CERN: Accelerating Science and Innovation Welcome! John Ellis King s College London (& CERN) Introduction to CERN CERN: Accelerating Science and Innovation The Mission of CERN Push back the frontiers of knowledge E.g. the secrets of the Big Bang

More information

Dark Matter in Particle Physics

Dark Matter in Particle Physics High Energy Theory Group, Northwestern University July, 2006 Outline Framework - General Relativity and Particle Physics Observed Universe and Inference Dark Energy, (DM) DM DM Direct Detection DM at Colliders

More information

> News < AMS-02 will be launched onboard the Shuttle Endeavour On May 2nd 2:33 P.M. from NASA Kennedy space center!

> News < AMS-02 will be launched onboard the Shuttle Endeavour On May 2nd 2:33 P.M. from NASA Kennedy space center! > News < Anti-matter, dark matter measurement By measuring the cosmic rays (Mainly electron, positron, proton, anti-proton and light nuclei) AMS-02 will be launched onboard the Shuttle Endeavour On May

More information

Information in Radio Waves

Information in Radio Waves Summative Assessment: Natural Sources of Radio Performance expectation: Develop and use a model of two objects interacting through electric or magnetic fields to illustrate the forces between objects and

More information

2) On a Hertzsprung-Russell diagram, where would you find red giant stars? A) upper right B) lower right C) upper left D) lower left

2) On a Hertzsprung-Russell diagram, where would you find red giant stars? A) upper right B) lower right C) upper left D) lower left Multiple choice test questions 2, Winter Semester 2015. Based on parts covered after mid term. Essentially on Ch. 12-2.3,13.1-3,14,16.1-2,17,18.1-2,4,19.5. You may use a calculator and the useful formulae

More information

Frontier Particle Accelerators

Frontier Particle Accelerators AAAS February 2005 Frontier Particle Accelerators For Elementary Particle Physics Together with Cosmology and Astrophysics, Elementary Particle Physics seeks understanding of the basic physical character

More information

Active Galaxies and Galactic Structure Lecture 22 April 18th

Active Galaxies and Galactic Structure Lecture 22 April 18th Active Galaxies and Galactic Structure Lecture 22 April 18th FINAL Wednesday 5/9/2018 6-8 pm 100 questions, with ~20-30% based on material covered since test 3. Do not miss the final! Extra Credit: Thursday

More information

5) What spectral type of star that is still around formed longest ago? 5) A) F B) A C) M D) K E) O

5) What spectral type of star that is still around formed longest ago? 5) A) F B) A C) M D) K E) O HW2 Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) The polarization of light passing though the dust grains shows that: 1) A) the dust grains

More information

Lecture 6: The Physics of Light, Part 1. Astronomy 111 Wednesday September 13, 2017

Lecture 6: The Physics of Light, Part 1. Astronomy 111 Wednesday September 13, 2017 Lecture 6: The Physics of Light, Part 1 Astronomy 111 Wednesday September 13, 2017 Reminders Star party tonight! Homework #3 due Monday Exam #1 Monday, September 25 The nature of light Look, but don t

More information

CHAPTER 28 STARS AND GALAXIES

CHAPTER 28 STARS AND GALAXIES CHAPTER 28 STARS AND GALAXIES 28.1 A CLOSER LOOK AT LIGHT Light is a form of electromagnetic radiation, which is energy that travels in waves. Waves of energy travel at 300,000 km/sec (speed of light Ex:

More information

A fantastic experiment

A fantastic experiment The Large Hadron Collider A fantastic experiment Duncan Carlsmith, Professor of Physics, University of Wisconsin-Madison What is the LHC? The Large Hadron Collider (LHC) is a new proton-proton colliding

More information

Earth Science, 13e Tarbuck & Lutgens

Earth Science, 13e Tarbuck & Lutgens Earth Science, 13e Tarbuck & Lutgens Beyond Our Solar System Earth Science, 13e Chapter 24 Stanley C. Hatfield Southwestern Illinois College Properties of stars Distance Distances to the stars are very

More information

Relative Sizes of Stars. Today Exam#3 Review. Hertzsprung-Russell Diagram. Blackbody Radiation

Relative Sizes of Stars. Today Exam#3 Review. Hertzsprung-Russell Diagram. Blackbody Radiation Today Exam#3 Review Exam #3 is Thursday April 4th in this room, BPS 40; Extra credit is due 8:00 am Tuesday April 9 Final Exam is 3:00pm Monday April 8 in BPS 40 The exam is 40 multiple choice questions.

More information

BROCK UNIVERSITY. Test 2, March 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 420 Date of Examination: March 5, 2015

BROCK UNIVERSITY. Test 2, March 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 420 Date of Examination: March 5, 2015 BROCK UNIVERSITY Page 1 of 9 Test 2, March 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 420 Date of Examination: March 5, 2015 Number of hours: 50 min Time of Examination: 18:00 18:50

More information

The unknown part of the universe, dark matter. Krasznahorkay Attila MTA Atomki, Debrecen

The unknown part of the universe, dark matter. Krasznahorkay Attila MTA Atomki, Debrecen The unknown part of the universe, dark matter Krasznahorkay Attila MTA Atomki, Debrecen ATOMKI, Debrecen The Institute for Nuclear Research in the downtown of Debrecen! 4 main divisions: Nuclear Physics

More information

Stars and Galaxies. The Big History of our Planet The 2nd threshold

Stars and Galaxies. The Big History of our Planet The 2nd threshold Stars and Galaxies The Big History of our Planet The 2nd threshold Big Bang Our universe starts from a Big Bang The early universe was simple, with little structure A thin mist of H & He atoms + photons

More information

Dennis Silverman UC Irvine Physics and Astronomy Talk to UC Irvine OLLI May 9, 2011

Dennis Silverman UC Irvine Physics and Astronomy Talk to UC Irvine OLLI May 9, 2011 Dennis Silverman UC Irvine Physics and Astronomy Talk to UC Irvine OLLI May 9, 2011 First Discovery of Dark Matter As you get farther away from the main central mass of a galaxy, the acceleration from

More information

1. Why photons? 2. Photons in a vacuum

1. Why photons? 2. Photons in a vacuum Photons and Other Messengers 1. Why photons? Ask class: most of our information about the universe comes from photons. What are the reasons for this? Let s compare them with other possible messengers,

More information

Recent developments in the understanding of Dark Matter

Recent developments in the understanding of Dark Matter Liverpool Physics Teachers Conference 20th June 2013 Recent developments in the understanding of Dark Matter Phil James Liverpool John Moores University Astrophysics Research Institute OUTLINE OF TALK

More information

Chapter 33 The History of a Star. Introduction. Radio telescopes allow us to look into the center of the galaxy. The milky way

Chapter 33 The History of a Star. Introduction. Radio telescopes allow us to look into the center of the galaxy. The milky way Chapter 33 The History of a Star Introduction Did you read chapter 33 before coming to class? A. Yes B. No You can see about 10,000 stars with the naked eye. The milky way Radio telescopes allow us to

More information

A100H Exploring the Universe: Big Bang Theory. Martin D. Weinberg UMass Astronomy

A100H Exploring the Universe: Big Bang Theory. Martin D. Weinberg UMass Astronomy A100H Exploring the : Martin D. Weinberg UMass Astronomy astron100h-mdw@courses.umass.edu April 21, 2016 Read: Chap 23 04/26/16 slide 1 Early Final Exam: Friday 29 Apr at 10:30 am 12:30 pm, here! Emphasizes

More information

BROCK UNIVERSITY. Test 2, March 2018 Number of pages: 9 Course: ASTR 1P02, Section 1 Number of Students: 465 Date of Examination: March 12, 2018

BROCK UNIVERSITY. Test 2, March 2018 Number of pages: 9 Course: ASTR 1P02, Section 1 Number of Students: 465 Date of Examination: March 12, 2018 BROCK UNIVERSITY Page 1 of 9 Test 2, March 2018 Number of pages: 9 Course: ASTR 1P02, Section 1 Number of Students: 465 Date of Examination: March 12, 2018 Number of hours: 50 min Time of Examination:

More information

Chapter 17 Cosmology

Chapter 17 Cosmology Chapter 17 Cosmology Over one thousand galaxies visible The Universe on the Largest Scales No evidence of structure on a scale larger than 200 Mpc On very large scales, the universe appears to be: Homogenous

More information

Figure 19.19: HST photo called Hubble Deep Field.

Figure 19.19: HST photo called Hubble Deep Field. 19.3 Galaxies and the Universe Early civilizations thought that Earth was the center of the universe. In the sixteenth century, we became aware that Earth is a small planet orbiting a medium-sized star.

More information

Recall what you know about the Big Bang.

Recall what you know about the Big Bang. What is this? Recall what you know about the Big Bang. Most of the normal matter in the universe is made of what elements? Where do we find most of this normal matter? Interstellar medium (ISM) The universe

More information

The Milky Way Galaxy Guiding Questions

The Milky Way Galaxy Guiding Questions The Milky Way Galaxy Guiding Questions 1. What is our Galaxy? How do astronomers know where we are located within it? 2. What is the shape and size of our Galaxy? 3. How do we know that our Galaxy has

More information

The Milky Way Galaxy

The Milky Way Galaxy The Milky Way Galaxy Guiding Questions 1. What is our Galaxy? How do astronomers know where we are located within it? 2. What is the shape and size of our Galaxy? 3. How do we know that our Galaxy has

More information

Todays Topics 3/19/2018. Light and Telescope. PHYS 1403 Introduction to Astronomy. CCD Camera Makes Digital Images. Astronomical Detectors

Todays Topics 3/19/2018. Light and Telescope. PHYS 1403 Introduction to Astronomy. CCD Camera Makes Digital Images. Astronomical Detectors PHYS 1403 Introduction to Astronomy Light and Telescope Chapter 6 Todays Topics Astronomical Detectors Radio Telescopes Why we need space telescopes? Hubble Space Telescopes Future Space Telescopes Astronomy

More information

The Cosmic Microwave Background

The Cosmic Microwave Background The Cosmic Microwave Background Class 22 Prof J. Kenney June 26, 2018 The Cosmic Microwave Background Class 22 Prof J. Kenney November 28, 2016 Cosmic star formation history inf 10 4 3 2 1 0 z Peak of

More information

Dark Matter / Dark Energy

Dark Matter / Dark Energy Dark Matter / Dark Energy 2 different things! The first hints of Dark Matter arose with observations of large motions in clusters of galaxies in the 1930 s. The case became compelling in the 1970 s with

More information

I V E R S U N. The Hot Big Bang I T Y T H E O F E. Andrew Liddle R G. Image: NASA/WMAP Science Team

I V E R S U N. The Hot Big Bang I T Y T H E O F E. Andrew Liddle R G. Image: NASA/WMAP Science Team The Hot Big Bang Andrew Liddle T H E O F E U N D I I V E R S N U B R G I T Y H Image: NASA/WMAP Science Team The Standard Model The discovery of the Higgs particle completes the Standard Model of Particle

More information

Saturday Morning Physics (2007) Prof. Bhaskar Dutta and Prof. Teruki Kamon. Department of Physics Texas A&M University. Question

Saturday Morning Physics (2007) Prof. Bhaskar Dutta and Prof. Teruki Kamon. Department of Physics Texas A&M University. Question Dark Puzzles of the Universe Saturday Morning Physics (2007) Prof. Bhaskar Dutta and Prof. Teruki Kamon Department of Physics Texas A&M University Question March 24, 2007 Dark Puzzles of the Universe 2

More information

Dark Puzzles of the Universe

Dark Puzzles of the Universe Dark Puzzles of the Universe Saturday Morning Physics (2007) Prof. Bhaskar Dutta and Prof. Teruki Kamon Department of Physics Texas A&M University Question March 24, 2007 Dark Puzzles of the Universe 2

More information

Big Bang Theory How the Universe was Formed

Big Bang Theory How the Universe was Formed Big Bang Theory How the Universe was Formed Objectives Explain the Big Bang Theory. Give evidence to support the Big Bang Theory. Dispel misconceptions about the Big Bang Theory. Explain problems with

More information

LIFE CYCLE OF A STAR

LIFE CYCLE OF A STAR LIFE CYCLE OF A STAR First stage = Protostar PROTOSTAR Cloud of gas and dust many light-years across Gravity tries to pull the materials together Eventually, at the center of the ball of dust and gas,

More information

Brief Introduction to Cosmology

Brief Introduction to Cosmology Brief Introduction to Cosmology Matias Zaldarriaga Harvard University August 2006 Basic Questions in Cosmology: How does the Universe evolve? What is the universe made off? How is matter distributed? How

More information

Dark Matter and Dark Energy components chapter 7

Dark Matter and Dark Energy components chapter 7 Dark Matter and Dark Energy components chapter 7 Lecture 3 See also Dark Matter awareness week December 2010 http://www.sissa.it/ap/dmg/index.html The early universe chapters 5 to 8 Particle Astrophysics,

More information

A100 Exploring the Universe Big Bang Theory and the Early Universe. Martin D. Weinberg UMass Astronomy

A100 Exploring the Universe Big Bang Theory and the Early Universe. Martin D. Weinberg UMass Astronomy A100 Exploring the Universe and the Martin D. Weinberg UMass Astronomy astron100-mdw@courses.umass.edu December 02, 2014 Read: Chap 23 12/04/14 slide 1 Assignment on Chaps 22 23, at the end of next week,

More information

The Universe. But first, let s talk about light! 2012 Pearson Education, Inc.

The Universe. But first, let s talk about light! 2012 Pearson Education, Inc. The Universe But first, let s talk about light! Light is fast! The study of light All forms of radiation travel at 300,000,000 meters (186,000 miles) per second Since objects in space are so far away,

More information

What does Dark Matter have to do with the Big Bang Theory?

What does Dark Matter have to do with the Big Bang Theory? Gents of Texas A&M What does Dark Matter have to do with the Big Bang Theory? Prof. David Toback Texas A&M University Mitchell Institute for Fundamental Physics and Astronomy March 2018 Prologue We live

More information

FURTHER COSMOLOGY Book page T H E M A K E U P O F T H E U N I V E R S E

FURTHER COSMOLOGY Book page T H E M A K E U P O F T H E U N I V E R S E FURTHER COSMOLOGY Book page 675-683 T H E M A K E U P O F T H E U N I V E R S E COSMOLOGICAL PRINCIPLE Is the Universe isotropic or homogeneous? There is no place in the Universe that would be considered

More information