Neutrino. Game Board FERMILABHAPPENINGSFIRSTSNEUTRINOSDETECTION.

Slides:



Advertisements
Similar presentations
Neutrinos Beck Róbert Fizikus MSc II. ELTE TTK.
Advertisements

Recent Discoveries in Neutrino Physics: Understanding Neutrino Oscillations 2-3 neutrino detectors with variable baseline 1500 ft nuclear reactor Determining.
Neutrino emission =0.27 MeV E=0.39,0.86 MeV =6.74 MeV ppI loss: ~2% ppII loss: 4% note: /Q= 0.27/26.73 = 1% ppIII loss: 28% Total loss: 2.3%
 Rafael Sierra. 1) A short review of the basic information about neutrinos. 2) Some of the history behind neutrinos and neutrino oscillations. 3) The.
By Miriam Aczel. What are neutrinos? They are almost massless— hardly feel the force of gravity They have no electric charge— don’t feel the electromagnetic.
Is B s 0 production by neutrino interactions interesting? Presented at the Super-B factory workshop as an alternative approach Nickolas Solomey 21 April.
Calorimetry and Showers Learning Objectives Understand the basic operation of a calorimeter (Measure the energy of a particle, and in the process, destroy.
An accelerator beam of muon neutrinos is manufactured at the Fermi Laboratory in Illinois, USA. The neutrino beam spectrum is sampled by two detectors:
Massive Neutrino – a search over 50 years April 14 th, 2003 at Palm desert Gang Li, IGPP, UCR.
Neutrino Physics Pedro Ochoa May 15th 2006.
“The Story of the neutrino” Does the missing matter matter? or.
The MINOS Experiment Andy Blake Cambridge University.
Neutrinos Jason Cook. Topics of Interest Neutrinos  History  Sources  Detection  Solar Neutrino Problem  Neutrino Oscillation  Practicality of Neutrinos.
Atmospheric Neutrino Anomaly
Solar Neutrinos and the SNO Experiment JJ Anthony April 11, 2006 Astronomy 007.
8/5/2002Ulrich Heintz - Quarknet neutrino puzzles Ulrich Heintz Boston University
1 Neutrinos: Past, Present and Future Robert C. Webb Physics Department Texas A&M University Robert C. Webb Physics Department Texas A&M University.
Neutrino Mass By Ben Heimbigner.
Peggy Norris, Black Hills State Univ/Sanford Underground Laboratory at Homestake.
Neutrino emission =0.27 MeV E=0.39,0.86 MeV =6.74 MeV ppI loss: ~2% ppII loss: 4% note: /Q= 0.27/26.73 = 1% ppIII loss: 28% Total loss: 2.3%
P461 - particles VIII1 Neutrino Physics Three “active” neutrino flavors (from Z width measurements). Mass limit from beta decay Probably have non-zero.
6. Atomic and Nuclear Physics Chapter 6.6 Nuclear Physics.
UPRM Center Rafael Aramis López LEAD TEACHER. The Universe is made of Quarks and Leptons Everything from galaxies to mountains, to molecules is made from.
A Summer at Fermi National Laboratory In which one math teacher struggles to do pretty much anything…
A long baseline neutrino oscillation search - MINOS Reinhard Schwienhorst School of Physics and Astronomy University of Minnesota.
What we did: ★ Inquiry based calibration data analysis of J/psi meson, W and Z bosons ★ Tours: webtour of CMS, LINAC, Accelerator Control room, DØ, MINOS,
(insert Star Wars video here). Neutrinos Group C June 29, 2014 ESHEP2014.
The Solar Neutrino Problem Barbara Sylwester Zakład Fizyki Słońca CBK PAN.
Making a neutrino beam The neutrinos detected in the MINOS experiment are produced in the Neutrinos at the Main Injector (NuMI) beam line at Fermi National.
My Chapter 30 Lecture.
1. THE GHOSTLY NEUTRINOS Hate them or love them, neutrinos do exist. Vector Particle Physics (VPP) automatically gives the correct structures and characteristics.
The Elementary Particles. e−e− e−e− γγ u u γ d d The Basic Interactions of Particles g u, d W+W+ u d Z0Z0 ν ν Z0Z0 e−e− e−e− Z0Z0 e−e− νeνe W+W+ Electromagnetic.
0 Neutrino Conversations Boris Kayser NeutrinoFest April 18, 2005.
Richard E. Hughes lastClass p.1 “The most incomprehensible thing about the universe is that it is comprehensible” - Albert Einstein.
The Little Neutral One (The neutrino and it’s detection) Presented by: André M. Gagnier For: Questions contemporaines en physiques (PHY3903)
O n t h e T r a c k o f M o d e r n P h y s i c s Wolfgang Pauli was a scientist with "NO" in his mind. Pauli's exclusion principle, that two electrons.
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.
More Nuclear Physics Neutrons and Neutrinos. More Nuclear Physics Neutrons and Neutrinos Nucleon – particles that can be found in the nucleus of an atom.
Fermilab Neutrino Program Jim Strait Neutrino Discussion at CERN 26 November 2013.
Wednesday, Feb. 14, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #6 Wednesday, Feb. 14, 2007 Dr. Jae Yu 1.Neutrino Oscillation Formalism 2.Neutrino.
Neutrino Nobel Prize overview
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.
Analysis of Alpha Background in SNO Data Using Wavelet Analysis
Beta Decay Contents: What it is (Maximum) Energy of radiation from mass defect Beta-(Maximum) Energy of radiation from mass defect Beta- Whiteboard (Maximum)
Kamiokande = Kamioka Nucleon Decay Experiment
Nuclear Physics. The famous Geiger-Marsden Alpha scattering experiment (under Rutherford’s guidance) In 1909, Geiger and Marsden were studying how alpha.
Soudan Underground Laboratory. The Soudan Underground Laboratory is located at the Soudan Underground Mine State Park, Soudan Minnesota.
On 4 December 1930, Austrian theorist Wolfgang Pauli (pictured here in 1933) wrote a famous letter in which he dared to hypothesise the existence of new.
Neutrinos: What we’ve learned and what we still want to find out Jessica Clayton Astronomy Club November 10, 2008.
Quarks and Leptons Announcements 1.Recitation this week in lab. BRING QUESTIONS ! 2.See my by Wed. if you have any grading issues with your exam. 3.Reading.
More Nuclear Physics Neutrons and Neutrinos. More Nuclear Physics Neutrons and Neutrinos Nucleon – particles that can be found in the nucleus of an atom.
High Energy Accelerators Dennis Silverman Physics and Astronomy U. C. Irvine.
Michel Gonin – Ecole Polytechnique – France : SUPER NOVA SN1987A Super-Kamiokande Introduction neutrino oscillations mixing matrices Introduction.
Super-Kamiokande and Neutrino Oscillation
Particle Physics Timeline 1895 X-rays discovered by W. Roentgen 1897 Electron discovered by J.J. Thompson 1905 Photons proposed by A. Einstein 1911 Nucleus.
Solar Neutrinos By Wendi Wampler. What are Neutrinos? Neutrinos are chargeless, nearly massless particles Neutrinos are chargeless, nearly massless particles.
60 27 Co Ni +  - + e Beta Decay: 13 7 N 13 6 C +  + + e Conservation of charge Beta minus - electron “As if” neutron -> proton + electron Beta.
Soudan Underground Laboratory MINOS and the Based on notes by Michael Nordstrom and MINOS collaborators.
Monday, Mar. 3, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #12 Monday, Mar. 3, 2003 Dr. Jae Yu 1.Neutrino Oscillation Measurements 1.Atmospheric.
Particle Physics Kihyeon Cho *Transparency from Prof. Young-Kee Kim.
What are the Elementary Constituents of Matter? What are the forces that control their behaviour at the most basic level?
CHAPTER 14 Elementary Particles
Neutrinos and the Evolution
HCP: Particle Physics Module, Lecture 4
Pauli´s new particle * nt nm ne e m t Beta-Decay Pa 234 b (electron)
Neutrinos in the Standard Model and Beyond
Neutrino Physics & Astrophysics : Overview
1930: Energy conservation violated in β-decay
Modern Studies of the Atom
Neutrino JEOPARDY!.
Presentation transcript:

Neutrino

Game Board FERMILABHAPPENINGSFIRSTSNEUTRINOSDETECTION

Fermi 100 THE PERSON THIS LAB IS NAMED AFTER

Fermi 100 WHO IS ENRICO FERMI

Fermi 200 THE ACCELERATOR FIRING THE PROTONS THAT MAKE THE NEUTRINO BEAM

Fermi 200 WHAT IS THE MAIN INJECTOR

Fermi 300 THE MOST POWERFUL PARTICLE ACCELERATOR IN THE WORLD

Fermi 300 WHAT IS THE TEVATRON

Fermi 400 THIS DIMENSION OF THE TEVATRON IS FOUR MILES

Fermi 400 WHAT IS THE CIRCUMFERENCE

Fermi 500 FERMILAB IS LOCATED HERE

Fermi 500 WHERE IS BATAVIA, ILLINOIS (CHICAGO, ILLINOIS)

Happenings 100 MINOS IS THE ACRONYM FOR THIS

Happenings 100 WHAT IS MAIN INJECTOR NEUTRINO OSCILLATION SEARCH

Happenings 200 CDMS IS THE ACRONYM FOR THIS

Happenings 200 WHAT IS CRYOGENIC DARK MATTER SEARCH

Happenings 300 KAMIOKANDE’S BIGGER BROTHER

Happenings 300 WHAT IS SUPER KAMIOKANDE

Happenings 400 SUPER KAMIOKANDE’S NON-NEUTRINO GOAL

Happenings 400 WHAT IS PROTON DECAY

Happenings 500 SNO IS THE ACRONYM FOR THIS

Happenings 500 WHAT IS SUDBURY NEUTRINO OBSERVATORY

Firsts 100 Slide 23 ORIGINALLY THOUGHT TO BE ZERO

Firsts 100 WHAT IS THE MASS OF THE NEUTRINO

Firsts 200 NEUTRINOS WERE FIRST SEEN IN THIS TYPE OF DECAY

Firsts 200 WHAT IS BETA (  ) DECAY

Firsts 300 THE MAN WHO FIRST PROPOSED NEUTRINO OSCILLATIONS

Firsts 300 WHO IS RAY DAVIS

Firsts 400 THE PLACE WHERE NEUTRINO OSCILLATIONS WERE FIRST OBSERVED

Firsts 400 WHAT IS THE SUPER KAMIOKANDE

Firsts 500 THE FIRST OBSERVATION OF A NEUTRINO WAS HERE

Firsts 500 WHERE IS THE SAVANNAH RIVER NUCLEAR REACTOR

Neutrinos 100 

WHAT IS THE MUON NEUTRINO

Neutrinos 200 

WHAT IS THE TAU NEUTRINO

Neutrinos 300 NEUTRINO MEANS “LITTLE NEUTRAL ONE” IN THIS LANGUAGE

Neutrinos 300 WHAT IS ITALIAN

Neutrinos 400 THIS MAN FIRST PROPOSED THE NEUTRINO

Neutrinos 400 WHO IS WOLFGANG PAULI

Neutrinos 500 MUON, TAU, AND ELECTRON ARE EXAMPLES OF THESE

Neutrinos 500 Slide 42 WHAT ARE FLAVORS OF NEUTRINOS

Detection 100 THE PARTICLE THAT IS ACTUALLY DETECTED AT MINOS

Detection 100 Slide 44 WHAT IS A PHOTON

Detection 200 5,500 TONS

Detection 200 Slide 46 WHAT IS THE WEGHT OF THE FAR DETECTOR

Detection 300 THERE ARE 486 OF THESE AT THE FAR DETECTOR

Detection 300 Slide 48 WHAT ARE THE DETECTOR PLATES

Detection 400 TO GET AWAY FROM COSMIC RAYS

Detection 400 Slide 50 WHY IS THE LAB UNDERGROUND

Detection 500 ABOUT THREE TIMES A DAY

Detection 500 HOW OFTEN MINOS DETECTS A NEUTRINO INTERACTION

DAILY DOUBLE 1 Slide 53

DAILY DOUBLE 2