Richard E. Hughes lastClass p.1 “The most incomprehensible thing about the universe is that it is comprehensible” - Albert Einstein.

Slides:



Advertisements
Similar presentations
ICECUBE & Limits on neutrino emission from gamma-ray bursts IceCube collaboration Journal Club talk Alex Fry.
Advertisements

That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov
The largest contribution to the mass of the atom is: 1.Higgs field providing fundamental particle mass by interacting with quarks 2.Einstein’s E = mc 2.
Fermilab E = Mc 2 Opening Windows on the World Young-Kee Kim Fermilab and the University of Chicago June 1, 2010.
Gravitation Newton’s Law of Gravitation Superposition Gravitation Near the Surface of Earth Gravitation Inside the Earth Gravitational Potential Energy.
The Dark Energy Survey The Big Questions The Discovery of Dark Energy The Dark Energy Survey – The telescope – The camera – The science Expected Results.
A Short Introduction to Particle Physics What do we know? How do we know? What next? “Is there physics beyond the Standard Model?”
1 Dark Energy and How to Find It: The SNAP Experiment Stuart Mufson IU Astronomy June 2007.
2011 Nobel Prize in Physics Awarded to Saul Permutter Brian Schmidt Adam Riess "for the discovery of the accelerating expansion of the Universe through.
PRESENTATION TOPIC  DARK MATTER &DARK ENERGY.  We know about only normal matter which is only 5% of the composition of universe and the rest is  DARK.
Objectives Distinguish the different models of the universe.
1 Extreme Astronomy and Supernovae Professor Lynn Cominsky Department of Physics and Astronomy Sonoma State University.
SPECIAL RELATIVITY -Postulates of Special Relativity -Relativity of time –> time dilation -Relativity of length –> length contraction © 2005.
March 24, 2007Dark Puzzles of the Universe1 Prof. Bhaskar Dutta and Prof. Teruki Kamon Department of Physics Texas A&M University Saturday Morning Physics.
Gamma-Ray Astronomy Dana Boltuch Ph. D
Announcements Homework 14 due Wednesday (5 questions) Monty Python Challenge offer good through this Wednesday! Final exam in SL 228 next Monday or Tuesday.
The Extreme Universe of Gamma-ray Astronomy Professor Lynn Cominsky Department of Physics and Astronomy Sonoma State University.
Survey of the Universe Greg Snow U Nebraska Lincoln CROP.
Particle Physics at UCI Probing the most fundamental structure of matter of matter and energy –From the Standard Model to String Theory –Search for the.
J. Goodman – May 2003 Quarknet Symposium May 2003 Neutrinos, Dark Matter and the Cosmological Constant The Dark Side of the Universe Jordan Goodman University.
The latest experimental evidence suggests that the universe is made up of just 4% ordinary matter, 23% cold dark matter and 73% dark energy. These values.
Stellar Kinematics Astronomy 315 Professor Lee Carkner Lecture 18.
Review for Exam 3.
Dr. Michael Cooke Dr. David Schmitz Fermilab. Newton’s Laws of Motion o o 1. Objects in motion want to stay in motion and objects at rest want to stay.
A superconducting proton collider Kevin Stenson University of Colorado – Boulder July 31, 2008.
Olbers Paradox Why is the sky dark? Possible answers:
Dark Matter Masses of Galaxies Gravity and Light Black Holes What is Dark Matter?
A long baseline neutrino oscillation search - MINOS Reinhard Schwienhorst School of Physics and Astronomy University of Minnesota.
DARK MATTER. DARK MATTER: It is called dark matter because it can’t be seen due to the fact it does not reflect light. Dark matter is made up of atoms,
Exploring the Cosmos with Neutrinos Aart Heijboer …all of them. nm
 Named after Edwin Hubble, the astronomer who discovered the expansion of the universe. Launched in 1990 and contains a 2.4 m (95 in) mirror with which.
The Origin, Expansion, & Dark Side of the Universe Lecture 25 “The Planets” Lecture 25 “The Planets” Not included on the final exam. Relax! Enjoy!
Monitoring of FHEP Teacher Research Internship Fermilab – Summer 2011.
Telescopes Science 9. Telescopes The main purpose of a telescope is to gather light Images that form can be recorded by taking a picture or a video.
GRAVITY AND MOTION. WHAT IS GRAVITY?? Gravity- the force that pulls objects towards one another This causes all objects in the universe with a mass to.
The Energy in our Universe Dr. Darrel Smith Department of Physics.
The Dark Side of the Universe
Finishing things up. So what’s with that 14 C? Masses of isotopes (not “natural” stuff) truly are multiples of basic hydrogen. Hydrogen is positively.
Presented by Laura Johnson, Catherine Jones, Catherine Cutts and Victoria Green.
Engineering Mechanics
H.5.1Discuss muon decay as experimental evidence to support special relativity. H.5.2Solve some problems involving the muon decay experiment. H.5.3Outline.
The Fate of the Universe
Monday, Feb. 24, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #11 Monday, Feb. 24, 2003 Dr. Jae Yu 1.Brief Review of sin 2  W measurement 2.Neutrino.
ANTARES  Physics motivation  Recent results  Outlook 4 senior physicists, ~5 PhD students, ~5 technicians M. de Jong RECFA 23 September 2005.
What is the Higgs??? Prof Nick Evans University of Southampton.
The Dark Energy Survey The Big Questions The Discovery of Dark Energy
Monday, Feb. 19, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #7 Monday, Feb. 19, 2007 Dr. Jae Yu 1.Neutrino Oscillation Experiments 2.Long.
What IS Matter ? Matter is all the “stuff” around you! Here’s the picture we’re going to uncover (not all today though) Hadrons Matter Leptons Baryons.
©2004 Richard E. Hughes Fermilab; p.1 Studying the Fundamental Particles  Particle physicists see the world as made up of a small number of fundamental.
Dr. Michael Cooke Dr. David Schmitz Fermilab
Ghosts in the Universe Jordan A. Goodman Department of Physics University of Maryland The world we don’t see around us.
CERN, 8 February, 2001 Egil Lillestøl, CERN & Univ. of Bergen Lectures recorded at :
Astroparticle physics with large neutrino detectors  Existing detectors  Physics motivation  Antares project  KM3NeT proposal M. de Jong.
High Energy Accelerators Dennis Silverman Physics and Astronomy U. C. Irvine.
Fermilab: Present and Future Young-Kee Kim Data Preservation Workshop May 16, 2011.
Birth of Neutrino Astrophysics
The cosmic connection There is a very close connection between particle physics and astrophysics. I’m going to show two examples: Type II supernovas Dark.
1 The Standard Model of Particle Physics Owen Long U. C. Riverside March 1, 2014.
A black hole: The ultimate space-time warp Ch. 5.4 A black hole is an accumulation of mass so dense that nothing can escape its gravitational force, not.
Neutrino. Game Board FERMILABHAPPENINGSFIRSTSNEUTRINOSDETECTION.
Dark Matter, Dark Energy
The Dark Universe Susan Cartwright.
January 29, 2003 Science Center 308 3:00 p.m.
Chapter 30 Section 4 Big Bang Theory.
The Antares Neutrino Telescope
Neutrinos and the Evolution
Building ICECUBE A Neutrino Telescope at the South Pole
Building ICECUBE A Neutrino Telescope at the South Pole
Dark matter and dark energy
Neutrino JEOPARDY!.
Presentation transcript:

Richard E. Hughes lastClass p.1 “The most incomprehensible thing about the universe is that it is comprehensible” - Albert Einstein

Richard E. Hughes lastClass p.2 Why is the universe ~100% Matter?

Richard E. Hughes lastClass p.3 Study Matter/AntiMatter with BaBar

Richard E. Hughes lastClass p.4 SuperK Sees that Neutrinos have Mass. Why?  481 MeV muon neutrino (MC) produces 394 MeV muon which later decays at rest into 52 MeV electron.  Size of PMT corresponds to amount of light seen by the PMT. PMTs are drawn as a flat squares even though in reality they look more like huge flattened golden light bulbs. Muon neutrino muon electron

Richard E. Hughes lastClass p.5 Study Neutrino Mass with MINOS Near Detector: 980 tons Far Detector: 5400 tons Det. 2 Det. 1

Richard E. Hughes lastClass p.6 What is accelerating Cosmic Rays?

Richard E. Hughes lastClass p.7 Study cosmic rays with The Auger Observatory

Richard E. Hughes lastClass p.8 What is the Dark Energy Accelerating the Expansion of the Universe?

Richard E. Hughes lastClass p.9 Study Dark Energy with SNAP! Super Nova Acceleration Probe Proposed space-based telescope that seeks to discover several extremely distant supernovae Lawrence Berkeley National Lab & University of California at Berkeley SNAP would orbit a 3-mirror, 2-meter reflecting telescope in a high orbit over the Earth’s poles, circling the globe every 1 or 2 weeks.  By repeatedly imaging just one or two large patches of sky, SNAP could gather 2,000 type Ia supernovae in a single year, 20 times the number from a decade of ground-based search. Because of enhanced sensitivity to infrared light above the atmosphere, many of these new supernovae would be at distances and redshifts far greater than any yet found.

Richard E. Hughes lastClass p.10 Why do The Fundamental Particles have mass?

Richard E. Hughes lastClass p.11 Use ATLAS and CMS to search for the Higgs.

Richard E. Hughes lastClass p.12 Why is the top quark so different?  Since the top quark is so massive, maybe it can tell us about mass itself.  Theorist Chris Hill of Fermilab claims that an understanding of the origin of mass would rank as "an achievement on a par with the greatest scientific strides in history, like Newton's establishing the universal law of gravitation or Einstein's connection of energy to mass and the speed of light."

Richard E. Hughes lastClass p.13 Study the top quark using the CDF Detector Fermilab; p.13 ©2004 Richard E. Hughes

Richard E. Hughes lastClass p.14

Richard E. Hughes lastClass p.15

Richard E. Hughes lastClass p.16

Richard E. Hughes lastClass p.17

Richard E. Hughes lastClass p.18 What is Dark Matter?

Richard E. Hughes lastClass p.19 Look for Dark Matter with GLAST