Mark Neubauer Kevin Pitts University of Illinois MAY 29, 2009

Similar documents
BOB KOWALEWSKI UNIVERSITY OF VICTORIA MAY 24, 2011

Antimatter Mysteries. Rolf Landua CERN. Antimatter Mysteries 1. Research physicist

Angels & Demons: Physics, Antimatter, and Armageddon

ANTIMATTER. A beam of particles is a very useful tool. Antimatter! 1

ANTIMATTER PROPULSION

Antimatter: It Matters 1. Antimatter: It Matters. Alex Elizabeth Heart. University of Cincinnati

CERN-TE-EPC. Aug-14 TE-EPC Presentation 2

CERN collision course

2016 IN PICTURES 20 JANUARY 15 FEBRUARY 23 JANUARY 24 MARCH

Instructions for gg Coincidence with 22 Na. Overview of the Experiment

A GAME ABOUT RADIOACTIVE DECAY

versiondog on the trail of the Big Bang versiondog on the trail of the Big Bang

Antimatter, the Ultimate Mirror

Astronomy 230 Section 1 MWF B6 Eng Hall. Outline. E=mc 2. Fuel Efficiency. Alternative fuels for space travel. Warp Drives?

Picturing. gallery: physics photowalk. the world s particle physics laboratories. By Katie Yurkewicz. Top Three Global Jury Winners

APRIL When Matter Meets ANTIMATTER. Battling Zits Forget gold... think platinum

Education and Outreach in Particle Physics

Accelerators for health

Sharing the Research Process with the Public

Technology Transfer at CERN

Astronomy 330. Final Papers. Presentation. Final

Astronomy 230 Section 1 MWF B1 Eng Hall. Outline. Fuel Efficiency

Herwig Schopper CERN 1211 Geneva 23, Switzerland. Introduction

STPA FOR LINAC4 AVAILABILITY REQUIREMENTS. A. Apollonio, R. Schmidt 4 th European STAMP Workshop, Zurich, 2016

Commercial Production and Use of Antiprotons

SCIENCE. Curated by CAROL SQUIRES. March 12 through May 30, International Center of Photography Avenue of the Americas. New York, NY 10036

Mitigating high energy anomalous signals in the CMS barrel Electromagnetic Calorimeter

Princeton University

Electromagnetic Radiation Worksheets

Organisation for Economic Co-operation and Development Global Science Forum

CERN AND INNOVATION. The Heart of the Matter

Scintillators as an external trigger for cathode strip chambers

The CMS Silicon Strip Tracker and its Electronic Readout

By Nicholas Bock. symmetry volume 06 issue 06 december 09. Photos: Reidar Hahn, Fermilab

Particle Physics labs in UTFSM Hayk Hakobyan (Physics department & CCTVal)

Future Perspectives. Maria Grazia Pia, INFN Genova in rappresentanza del gruppo Geant4-INFN.

ELECTROMAGNETIC WAVES AND THE EM SPECTRUM MR. BANKS 8 TH GRADE SCIENCE

Investigate Antimatter

The Earth s Atmosphere

Chair of the CERN Council Professor Michel Spiro

Data acquisition and Trigger (with emphasis on LHC)

Learning Objectives. Understand how light is generated in a scintillator. Understand how light is transmitted to a PMT

The Australian Curriculum Science

INTRODUCTION. 5. Electromagnetic Waves

ESS 7 Lectures 15 and 16 November 3 and 5, The Atmosphere and Ionosphere

National 4. Waves and Radiation. Summary Notes. Name:

Development and tests of a large area CsI-TGEM-based RICH prototype

Layout and prototyping of the new ATLAS Inner Tracker for the High Luminosity LHC

A novel solution for various monitoring applications at CERN

SLAC National Accelerator Laboratory

Data acquisition and Trigger (with emphasis on LHC)

Plans for RPC DHCAL Prototype. David Underwood Argonne National Laboratory

TEST AND CALIBRATION FACILITY FOR HLS AND WPS SENSORS

CMS Conference Report

Strategic Plan for a Scientific Software Innovation Institute (S 2 I 2 ) for High Energy Physics DRAFT

Strategic Plan for a Scientific Software Innovation Institute (S 2 I 2 ) for High Energy Physics DRAFT

Materials Monthly May 2006

Ask yourself: Yerkes Summer Institute 2002 Resonance

Positron Emission Tomography

Q&A with Sean Carroll Interviewed by Joelle Seligson

Development of n-in-p Active Edge Pixel Detectors for ATLAS ITK Upgrade

arxiv: v1 [physics.pop-ph] 16 Nov 2017

Some great Ideas in Physics

Conceptual Physics Fundamentals

Thoughts about SLAC s Role for HEP Theory in the LHC Era. Tim M.P. Tait. University of California, Irvine

The Use of OpenSource in the Grid Computing and Data Acquisition System in High Energy and Particle Physics Research Projects

European Strategy for Particle Physics and its Update Plan

LHC Experiments - Trigger, Data-taking and Computing

APAC 2007, Raja Ramanna Centre for Advanced Technology(RRCAT), Indore, India LHC STATUS. Lyndon Evans, CERN, Geneva, Switzerland

LHC: CONSTRUCTION AND COMMISSIONING STATUS

Photos: Reidar Hahn, Fermilab; Bradley Plummer, SLAC; Sandbox Studio Photo-illustration: Sandbox Studio 18

Medical Imaging. X-rays, CT/CAT scans, Ultrasound, Magnetic Resonance Imaging

HCERES report on research unit:

KEK Archives, 11 August Why are social scientists interested in HEP?

PET Detectors. William W. Moses Lawrence Berkeley National Laboratory March 26, 2002

explore space Texas Alliance for Minorities in Engineering, Trailblazer I -

ANTICOINCIDENCE LOW LEVEL COUNTING

ORIENTATION LAB. Directions

PoS(EPS-HEP 2009)150. Silicon Detectors for the slhc - an Overview of Recent RD50 Results. Giulio Pellegrini 1. On behalf of CERN RD50 collaboration

Lesson 24 Electromagnetic Waves

Final Exam. Sunday, 5/12, 7:45 am Van Vleck B115

The Radio Ice Cerenkov Experiment : RICE. Jenni Adams and Suruj Seunarine

ndex Gemini project, 96 R&D expenditures, 114, science goals, Brookhaven National Laboratory, 122

MPGDs: a tool for progress in HEP

Accelerator science. Talk to prospective students. 30 November Andrei Seryi John Adams Institute for Accelerator Science

LAB 1 Linear Motion and Freefall

UC Santa Cruz Tesla Coil Show at Aptos High School

Behind the scenes of Big Science. Amber Boehnlein Department of Energy And Fermi National Accelerator Laboratory

Relevant KS2 Links: SC1 1b, 2a, 2d, 2e, 2f, 2g, 2h, 2i, 2j, 2k, 2l, 2m; SC3 1a; MA2 1k; MA3 4b; MA4 1a, 1c, 2a, 2b, 2c, 2e;

DQW HOM Coupler for LHC

Explain what is meant by a photon and state one of its main properties [2]

Plasma in the ionosphere Ionization and Recombination

Illustrations: Sandbox Studio

arxiv: v2 [physics.ins-det] 13 Oct 2015

Trigger Algorithms for the SuperCDMS Dark Matter Search

Recall Argument Against Travel!

The design and performance of the ATLAS jet trigger

EKA Laboratory Muon Lifetime Experiment Instructions. October 2006

LHCb Preshower(PS) and Scintillating Pad Detector (SPD): commissioning, calibration, and monitoring

High-Speed Mobile Communications in Hostile Environments

Transcription:

Mark Neubauer Kevin Pitts University of Illinois MAY 29, 2009

THE MOVIE

Antimatter is stolen from CERN s Large Hadron Collider (LHC) and hidden in Vatican City. THE PLOT Countdown to Vatican annihilation begins. Race through Rome to avert death and destruction.

"The most incomprehensible thing about the world is that it is comprehensible."

ATOMS & THE SUBATOMIC WORLD Everything familiar to us is made of billions and billions of atoms. Atoms consist of protons, neutrons and electrons. Our job is to peer inside the atom, and even inside the proton! particle accelerators are big microscopes!

We need BIG tools for this job!

We need BIG tools for this job!

ANTIMATTER REALLY EXISTS All material familiar to us (Earth, people, atmosphere) is matter (made up of protons, neutrons and electrons) For every type of matter particle, there is also an antimatter particle. It has the same mass and opposite charge as matter.

Matter: p + = proton e = electron Antimatter Antiproton Antineutron antielectron Antimatter: p = antiproton e + = antielectron (positron)

CAN WE MAKE ANTIMATTER? We can, and do in particle accelerators

ANTIMATTER QUESTIONS How much of it occurs naturally? Answer: tiny, tiny, tiny amounts (more on this later) How do you make it and why did you let the illuminati steal it? Can you really make an antimatter bomb?

Professor Einstein had it right E=mc 2 energy mass Speed of light = constant!! Use a large particle accelerator to give particles enormous energy. (big, big E) Smash those particles into other particles (convert E to m!!) Some of the mass created is matter, some is antimatter!

HOW MUCH CAN WE MAKE? At Fermilab, we make about antiprotons per hour. 200,000,000,000 That sounds like a lot, but it takes: 150,000,000,000,000,000,000,000,000,000 antiprotons to make ¼ gram of antimatter (i.e. the antimatter bomb)

ANTIMATTER S NO THREAT We make very little antimatter Fermilab creates 2 nanograms of antiprotons per year It would take 100 million years to make ¼ gram

MATTER VS. ANTIMATTER Anti-Tom Hanks Tom Hanks Would look very much like

MATTER VS. ANTIMATTER But were they to meet E=mc 2

ANGELS & DEMONS & ANTIMATTER Rome is threatened by ¼ gram of antimatter Annihilation of: ¼ g matter + ¼ g antimatter = 10,000 kilotons of TNT More than enough to destroy the Vatican ¼gram

It s not portable ANTIMATTER S NO THREAT

ANTIMATTER CAN T BE USED FOR: Power Have to make every single antiparticle Not an energy source: much more energy goes in than is produced Bombs Spaceships

BUT ANTIMATTER CAN BE (& IS BEING) USED FOR: Medicine & Diagnostic Imaging Positron Emission Tomography (PET) Particle accelerators routinely used in cancer treatment Solving some of the biggest mysteries of the Universe Why do we exist? Why do we have mass? What is most of the Universe made of?

SEARCHING FOR ANSWERS At high energy physics laboratories around the world TRIUMF CERN Fermilab SLAC Brookhaven DESY IHEP KEK

CERN CERN is a real-life laboratory near Geneva, Switzerland Not top secret!

LARGE HADRON COLLIDER (LHC) Located at CERN The world s most powerful particle accelerator 16.8 miles around, 330 feet underground

ATLAS ALICE France CMS LHCb Switzerland

HOLLYWOOD S LHC CONTROL ROOM

real scientists, no lab coats!

ANTIMATTER & LHC Antimatter will be produced at the LHC Half of everything produced in the collisions is antimatter! but, amount will be tiny (0.000000002 grams / year) 125 million years to create ¼ gram and it annihilates almost immediately in the detector

ANTIMATTER: WHERE ELSE? Cosmic ray showers In fact, how antimatter was discovered 75 years ago e + e - Not a recent discovery

ANTIMATTER: WHERE ELSE? You! Radioactive decay of atoms (e.g. 40 K) in your body produce antimatter (positrons) This antimatter annihilates into photons (light) in your body We have all have faint antimatter glow! In PET scans, similar radioactive atoms are placed in you to enhance this glow so that it can be analyzed

A WINDOW INTO THE EVOLUTION OF OUR UNIVERSE particle accelerators allow us to look back in time! You are here

SEARCHING FOR ANSWERS IN Champaign/Urbana University of Illinois high energy physics group 9 experimentalists, 6 theoreticians We participate in world-wide collaborations at laboratories in the U.S., Europe and South America Contact us or visit our web page to learn more http://www.hep.uiuc.edu/hepg/index.html

THANK YOU For more information: www.hep.uiuc.edu/hepg/index.html www.uslhc.us www.fnal.gov www.cern.ch

SUPPLEMENTAL SLIDES

THE MYSTERY OF ANTIMATTER We exist because there is almost no antimatter around It wasn t always that way

THE BIG BANG 14 billion years ago, the Big Bang produced equal amounts of matter and antimatter Everything should have annihilated Instead

WHAT HAPPENED TO THE ANTIMATTER? After 40 years of research we know: Some particles behave differently from their antiparticles The difference is very slight not enough to explain vast dominance of matter over antimatter There must be another explanation Lots of ideas, but Nature gets the last word Active area of current research at labs around the world, including Fermilab and CERN

GOD PARTICLE?!? Both Matter and Antimatter have mass But what is the origin of that mass? Why do different particles have such different masses? We believe that its due to an allpervasive Higgs field that interacts with matter/antimatter particles

Imagine that a room full of physicists chattering quietly is like space filled with the Higgs field HIGGS FIELD?

this increases his resistance to movement, in other words, he acquires mass! A well-known scientist walks in, attracting a cluster of admirers with each step

Black Holes? According to some speculative theories, tiny black holes could be produced in collisions at the LHC. They would then very quickly decay and be detected by experiments (the tinier the black hole, the faster it evaporates). 41

Simulation of a Microscopic-Black Hole Event 42

Would Microscopic-Black Holes be Dangerous? Cosmic rays are continuously bombarding Earth's atmosphere with far more energy than protons will have at the LHC They have done so throughout the 4.5 billion years of the Earth's existence, and the Earth is still here! So nobody should loose sleep over this 43

Extra Dimensions of Space!?! 44

Are There Extra Dimensions? To understand why extra dimensions were proposed, consider: Which is weaker: Gravity or Electromagnetism? Which is more powerful: A small magnet or The entire massive Earth? So gravity is extremely weak! Why? 45

Why Is Gravity so Weak? Electromagnetism is confined to our usual three dimensions of space electromagnetism Maybe Gravity sees the other dimensions of space. As the force is spread out, it is weakened. gravity 46

How can there be extra dimensions? Think about an acrobat and a flea on a tight rope. The acrobat can move forward and backward along the rope. But the flea can also move sideways around the rope. If the flea keeps walking to one side, it goes around the rope and winds up where it started. 47

How can there be extra dimensions? So the acrobat has one dimension, and the flea has two dimensions, but one of these dimensions is a small closed loop. The acrobat can only detect the one dimension of the rope, just as we can only see the world in three dimensions, even though it might well have more. This is impossible to visualize, precisely because we can only visualize things in three dimensions! 48

But there is More than just Matter and Antimatter Looking at our Universe we see much more than ordinary matter (or antimatter) We call this extra stuff dark matter because we cannot see it. But what is it? Composition of our Universe Ordinary matter 49

Dark Matter Dark matter Not dark matter except that s not really true 50

Much Evidence for its Existence In galaxies and galaxy clusters There is not enough visible mass in rotating spiral galaxies to hold them together Separation of dark matter and ordinary matter in the collision of two clusters of galaxies Photos courtesy of NASA 51

What is Dark Matter? We don t know! But we have ideas If the constituents of dark matter are new particles, the LHC should discover them and elucidate the mystery of dark matter. Dark Matter produced in the laboratory! 52

CERN European Laboratory for Particle Physics Founded in 1954 20 member countries More than 9,000 scientists Over 100 nationalities More than 1,000 from U.S. universities and labs