The Proton Decay and Experiments

Size: px
Start display at page:

Download "The Proton Decay and Experiments"

Transcription

1 The Proton Decay and Experiments Astroteilchenphysik Vortrag Carlos Ayerbe Gayoso

2 Contents 1- Summary of the Standard Model 2- Beyond Standard Model - Grand Unified Theories 3- The Proton Decay 4- Detecting the proton decay 5- The Counting Test Facility at Grand Sasso

3 Summary of the Standard Model Particles Spin 1 / 2 fermions and anti-fermions 3 Generations or families of quarks (d,u), (s,c), (b,t) 3 Generation of leptons ( e, νe),( µ, ν µ ),( τ, ντ ) Spin 1 gauge bosons 1 massless electronweak boson, the photon g + 3 massive electronweak bosons W, W, Z 8 massless coloured gluons, g Spin 0, Higgs boson, H 0 Interacctions Electromagnetic with coupling e (or α ΕΜ ) Weak with coupling G F Strong with coupling α S The first two are unified via two couplings g and g 0

4 BUT... Standard Model can t explain Values of the couplings e, g and α S Why there are 3 generations of quarks and leptons Why the quark generations are mixed but not the leptons The masses of the quarks and leptons And other open questions Is there a relationship between the strong force and the electroweak force? Is there a relationship between quarks and leptons? i.e. Why do the proton and electron have exactly opposite electrics charges but seem different in their properties What is the origin of CP violation? What about gravity?

5 Beyond Standard Model To answer some of these questions one needs to go beyond Standard Model to: Grand Unified Theories (GUTs) Composite Models Supersymmetry String Models...

6 Grand Unified Theories The basis of this theories is the behavior of the coupling constants: a EM increases with energy a S decreases with energy The couplings would come together at the so-called Unification Mass of about GeV

7 A little bit of mathematical foundation... Current theories are asociated with certain groups of the groups theory The Electromagnetic group U(1) has one gauge boson (the photon) The QCD group SU(3) has 3 colour charges and 8 gauge bosons (gluons) The electroweak interaction are represented by the product of the groups SU(2) U(1) So, the Standard Model is represented by the product of the groups SU(3) SU(2) U(1) The simplest GUT is labelled SU(5) and has 24 gauge bosons We have already 12 bosons There would also be: 3 bosons with electric charge 1/3 and color (Y R, Y G, Y B ) 3 bosons with electric charge 4/3 and color (X R, X G, X B ) And their 6 anti-particles These X and Y bosons are called leptoquarks

8 The Proton decay The bosons X, Y can change quarks into leptons and vice-versa It violates lepton (L) and baryon (B) conservation but still conserve B-L

9 The Proton decay This means that the proton could decay to mesons and leptons!! p p e π + π ν e With these desintegrations and assuming M X»10 14 GeV/c 2 this predicts a life time betweem 2x10 28 and 6x10 30 years

10 Detecting the proton decay One can t watch a proton for years and see if it decay (is bored!!) But we can watch protons for one year We need: A large mass (to provide the protons) A tracking capability for charged particles A way to mesure visible energy and identify particles Shielding against background (natural radiactive, cosmic rays)

11 The Counting Test Facility at Grand Sasso The CTF counting as a calorimetric liquid scintillator detector The active detector is 4.8 m 3 of a binary liquid scintillator (1,5 g PPO/L pseudocumene) The scintillator is held in a nylon vessel shielded by 1000 tons of purified water 100 PM surrounding the detector are used to mesure time and charge for each event

12 The Counting Test Facility at Grand Sasso The CTF is located at the Gran Sasso underground laboratories, it provides 3500 m water equivalent shielding from cosmic radiation It gives approximately 25/d/m 2 of muons flux Background radiation and shielding Inside the hall there is a g-rays flux of 10 8 /d/ m 2 from natural radiation The water shield provides 4,5 m of shielding from g-rays on all sides The phototubes contributes with additional g-rays of approx 2x10 6 d/ m 2 but they are 2,3 m away from scintillator Simulations suggest the water should reduce the external g-rays from natural radiation and PM to less than 100/d in the energy range of kev U, Th and K concentrations in the water contributes a BG of 100/d, those are the major sources of BG contribution (of the order os thousand scintillation events per day) BUT... With the PMT s and readout electronics they allow the identification of the excitation source for events and spatial reconstrucction, so we can identify those sources

13 The Counting Test Facility at Grand Sasso The CTF Subsystems The scintillator Scintillator Containment Vessel Scintillator Handling Scintillator Purification System Water Tank and Clean Room The Water Purification System The Photomultiplier System Data Acquisition Electronics Nitrogen System Ancillary Facilities

14 The Counting Test Facility at Grand Sasso Scintillator It consists of 1,5 g PPO (diphenyl oxazole) per liter of pseudocumene (1,2,4, trimethylbenzene) The density is 0,88 g/l at 15 C Refractive index is 1,5 at 420 nm Scintillator Containment Vessel The scintillator containmet vessel confines the scintillator within the water buffer It is made by a flexible ball of 0,5 mm thick and 1,05 m radius, made of an amorphous nylon from Bayer Chemicals It sustains the 570 kg bouyant force associated with the 12% density difference between water and scintillator It supports 3,5 MPa (but it was designated to support 14 MPa) In air, the wall have a optical trasmittance of 80% at 365nm It is attached by a system of 16 nylon strings

15 The Counting Test Facility at Grand Sasso Scintillator Containment Vessel

16 The Counting Test Facility at Grand Sasso The Photomultiplier System There are 100 PMT of 0,20 m of diameter (Thorn EMI 9351) They have a cathode eff of»25% (peak eff at 380nm) Transit time spread of 1 ns Dark noise of 500 Hz Low afterpulsing (»2,5%) Amplification of 10 7 They was choosed for their low radiactivity The dynodes are shielded against magnetic fields with mu-metall The PMT are coupled to truncated string cone light concentrators The Geometrical coverage of the active scintillator region is 21%

17 The Counting Test Facility at Grand Sasso The Photomultiplier System

18 The Counting Test Facility at Grand Sasso Background sources The main goal of the CTF is identify the radiactive sources of the scintillator to demostrate the feasibility of the facility The principal sources from scintillator are 85 Kr events/d 210 Po from the decay of 222 Rn events/d 210 Bi (events are expected in the energy window of interest, but its b-decay not have a monoenergetic signature to identify) Ra(U) < 4 x 10-9 Bq/kg and Th <10-9 Bq/kg 14 C» 3x10-4 Bq/kg (isotopic abundance 14 C/ 12 C 2x10-18 The 85 Kr is removed by nitrogen stripping Water extraction removed the 210 Po The internal radiactive BG was reduced to <40 events/d 14 C, U and Th remained stable for over a year. 85 Kr and 210 Po did not reappear Low intrisic BG was stable for several months

19 The Counting Test Facility at Grand Sasso Outlook and conclusions The CTF had demostrated the feasibility of a large scale low background liquid scintillator detector Online purification of a liquid scintillator achivied levels below detection and maintained the optical properties Radiopurity of a liquid scintillator at the level of 10-9 Bq/kg above 250 kev and 10-3 Bq/kg below 250 kev has been demostrated Since this facility main purpouse is not the detection of the proton decay, it have all the necesary for its detection

20 Conclusions The proton decay has not been detected yet, but there are a lot of facilities with the necesary to detect it Proton decay is a important piece in GUT but it is not the only Liquid scintillators detectors demostrated their capability to detect rare events as proton decay

21

Option 212: UNIT 2 Elementary Particles

Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy Option 212: UNIT 2 Elementary Particles SCHEDULE 26-Jan-15 13.00pm LRB Intro lecture 28-Jan-15 12.00pm LRB Problem solving (2-Feb-15 10.00am E Problem Workshop) 4-Feb-15

More information

Lecture 18 - Beyond the Standard Model

Lecture 18 - Beyond the Standard Model Lecture 18 - Beyond the Standard Model Why is the Standard Model incomplete? Grand Unification Baryon and Lepton Number Violation More Higgs Bosons? Supersymmetry (SUSY) Experimental signatures for SUSY

More information

Rivelazione di neutrini solari - Borexino Lino Miramonti 6 Giugno 2006 Gran Sasso

Rivelazione di neutrini solari - Borexino Lino Miramonti 6 Giugno 2006 Gran Sasso Rivelazione di neutrini solari - Borexino Lino Miramonti 6 Giugno 2006 Gran Sasso 1 RADIOCHEMICAL Integrated in energy and time CHERENKOV Less than 0.01% of the solar neutrino flux is been measured in

More information

XI. Beyond the Standard Model

XI. Beyond the Standard Model XI. Beyond the Standard Model While the Standard Model appears to be confirmed in all ways, there are some unclear points and possible extensions: Why do the observed quarks and leptons have the masses

More information

An Introduction to Modern Particle Physics. Mark Thomson University of Cambridge

An Introduction to Modern Particle Physics. Mark Thomson University of Cambridge An Introduction to Modern Particle Physics Mark Thomson University of Cambridge Science Summer School: 30 th July - 1 st August 2007 1 Course Synopsis Introduction : Particles and Forces - what are the

More information

Lecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli

Lecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli Lecture PowerPoint Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the

More information

Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013

Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013 Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013 1 Matter Particles Quarks: Leptons: Anti-matter Particles Anti-quarks: Anti-leptons: Hadrons Stable bound states of quarks Baryons:

More information

The Scale-Symmetric Theory as the Origin of the Standard Model

The Scale-Symmetric Theory as the Origin of the Standard Model Copyright 2017 by Sylwester Kornowski All rights reserved The Scale-Symmetric Theory as the Origin of the Standard Model Sylwester Kornowski Abstract: Here we showed that the Scale-Symmetric Theory (SST)

More information

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON FACULTY OF SCIENCE High Energy Physics WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON AIM: To explore nature on the smallest length scales we can achieve Current status (10-20 m)

More information

Physics 4213/5213 Lecture 1

Physics 4213/5213 Lecture 1 August 28, 2002 1 INTRODUCTION 1 Introduction Physics 4213/5213 Lecture 1 There are four known forces: gravity, electricity and magnetism (E&M), the weak force, and the strong force. Each is responsible

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

The first one second of the early universe and physics beyond the Standard Model

The first one second of the early universe and physics beyond the Standard Model The first one second of the early universe and physics beyond the Standard Model Koichi Hamaguchi (University of Tokyo) @ Colloquium at Yonsei University, November 9th, 2016. Credit: X-ray: NASA/CXC/CfA/M.Markevitch

More information

Most of Modern Physics today is concerned with the extremes of matter:

Most of Modern Physics today is concerned with the extremes of matter: Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large

More information

Fundamental Particles and Forces

Fundamental Particles and Forces Fundamental Particles and Forces A Look at the Standard Model and Interesting Theories André Gras PHYS 3305 SMU 1 Overview Introduction to Fundamental Particles and Forces Brief History of Discovery The

More information

Most of Modern Physics today is concerned with the extremes of matter:

Most of Modern Physics today is concerned with the extremes of matter: Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large

More information

Contents. Preface to the First Edition Preface to the Second Edition

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

More information

The God particle at last? Astronomy Ireland, Oct 8 th, 2012

The God particle at last? Astronomy Ireland, Oct 8 th, 2012 The God particle at last? Astronomy Ireland, Oct 8 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV I The Higgs boson

More information

The God particle at last? Science Week, Nov 15 th, 2012

The God particle at last? Science Week, Nov 15 th, 2012 The God particle at last? Science Week, Nov 15 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV Why is the Higgs particle

More information

A first trip to the world of particle physics

A first trip to the world of particle physics A first trip to the world of particle physics Itinerary Massimo Passera Padova - 13/03/2013 1 Massimo Passera Padova - 13/03/2013 2 The 4 fundamental interactions! Electromagnetic! Weak! Strong! Gravitational

More information

Review Chap. 18: Particle Physics

Review Chap. 18: Particle Physics Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material Review Chap. 18: Particle Physics Particles and fields: a new picture Quarks and leptons: the particle zoo

More information

9.2.E - Particle Physics. Year 12 Physics 9.8 Quanta to Quarks

9.2.E - Particle Physics. Year 12 Physics 9.8 Quanta to Quarks + 9.2.E - Particle Physics Year 12 Physics 9.8 Quanta to Quarks + Atomic Size n While an atom is tiny, the nucleus is ten thousand times smaller than the atom and the quarks and electrons are at least

More information

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Overview The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Our understanding is about to take a giant leap.. the Large Hadron Collider

More information

Discovery of the Neutrino Mass-I. P1X* Frontiers of Physics Lectures October 2004 Dr Paul Soler University of Glasgow

Discovery of the Neutrino Mass-I. P1X* Frontiers of Physics Lectures October 2004 Dr Paul Soler University of Glasgow -I P1X* Frontiers of Physics Lectures 19-0 October 004 Dr Paul Soler University of Glasgow Outline 1. Introduction: the structure of matter. Neutrinos:.1 Neutrino interactions. Neutrino discovery and questions.3

More information

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 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

More information

Physics 7730: Particle Physics

Physics 7730: Particle Physics Physics 7730: Particle Physics! Instructor: Kevin Stenson (particle physics experimentalist)! Office: Duane F317 (Gamow tower)! Email: kevin.stenson@colorado.edu! Phone: 303-492-1106! Web page: http://www-hep.colorado.edu/~stenson/!

More information

Elementary particles and typical scales in high energy physics

Elementary particles and typical scales in high energy physics Elementary particles and typical scales in high energy physics George Jorjadze Free University of Tbilisi Zielona Gora - 23.01.2017 GJ Elementary particles and typical scales in HEP Lecture 1 1/18 Contents

More information

Lecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model

Lecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model Lecture 03 The Standard Model of Particle Physics Part III Extensions of the Standard Model Where the SM Works Excellent description of 3 of the 4 fundamental forces Explains nuclear structure, quark confinement,

More information

Fundamental Particles

Fundamental Particles Fundamental Particles Standard Model of Particle Physics There are three different kinds of particles. Leptons - there are charged leptons (e -, μ -, τ - ) and uncharged leptons (νe, νμ, ντ) and their

More information

Beyond the standard model? From last time. What does the SM say? Grand Unified Theories. Unifications: now and the future

Beyond the standard model? From last time. What does the SM say? Grand Unified Theories. Unifications: now and the future From last time Quantum field theory is a relativistic quantum theory of fields and interactions. Fermions make up matter, and bosons mediate the forces by particle exchange. Lots of particles, lots of

More information

Physics Beyond the Standard Model. Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare

Physics Beyond the Standard Model. Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare Physics Beyond the Standard Model Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare Increasingly General Theories Grand Unified Theories of electroweak and strong interactions Supersymmetry

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

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

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS Class Mechanics My office (for now): Dantziger B Room 121 My Phone: x85200 Office hours: Call ahead, or better yet, email... Even better than office

More information

The Uncertainty Principle and the Quarks

The Uncertainty Principle and the Quarks The Uncertainty Principle and the Quarks Andrei Gritsan Johns Hopkins University August, 2007 JHU Quarknet Meeting Outline The Uncertainty Principle quantum mechanics with elementary particles The Quarks

More information

PHYS 420: Astrophysics & Cosmology

PHYS 420: Astrophysics & Cosmology PHYS 420: Astrophysics & Cosmology Dr Richard H. Cyburt Assistant Professor of Physics My office: 402c in the Science Building My phone: (304) 384-6006 My email: rcyburt@concord.edu My webpage: www.concord.edu/rcyburt

More information

Particle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes.

Particle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes. Particle Physics 12.3.1 Outline the concept of antiparticles and give examples 12.3.2 Outline the concepts of particle production and annihilation and apply the conservation laws to these processes. Every

More information

Origin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean?

Origin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean? Origin of the Universe - 2 ASTR 2120 Sarazin What does it all mean? Fundamental Questions in Cosmology 1. Why did the Big Bang occur? 2. Why is the Universe old? 3. Why is the Universe made of matter?

More information

The Discovery of the Higgs Boson: one step closer to understanding the beginning of the Universe

The Discovery of the Higgs Boson: one step closer to understanding the beginning of the Universe The Discovery of the Higgs Boson: one step closer to understanding the beginning of the Universe Anna Goussiou Department of Physics, UW & ATLAS Collaboration, CERN Kane Hall, University of Washington

More information

Lecture 02. The Standard Model of Particle Physics. Part I The Particles

Lecture 02. The Standard Model of Particle Physics. Part I The Particles Lecture 02 The Standard Model of Particle Physics Part I The Particles The Standard Model Describes 3 of the 4 known fundamental forces Separates particles into categories Bosons (force carriers) Photon,

More information

Electron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron.

Electron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron. Particle Physics Positron - discovered in 1932, same mass as electron, same charge but opposite sign, same spin but magnetic moment is parallel to angular momentum. Electron-positron pairs can be produced

More information

1. Introduction. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 1. Introduction 1

1. Introduction. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 1. Introduction 1 1. Introduction Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 1. Introduction 1 In this section... Course content Practical information Matter Forces Dr. Tina Potter 1. Introduction 2 Course

More information

1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles

1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles 1 Introduction The purpose of this chapter is to provide a brief introduction to the Standard Model of particle physics. In particular, it gives an overview of the fundamental particles and the relationship

More information

The Standard Model. 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories

The Standard Model. 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories The Standard Model 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories Bosons (force carriers) Photon, W, Z, gluon, Higgs Fermions (matter particles) 3 generations

More information

CHAPTER 7 TEST REVIEW

CHAPTER 7 TEST REVIEW IB PHYSICS Name: Period: Date: # Marks: 94 Raw Score: IB Curve: DEVIL PHYSICS BADDEST CLASS ON CAMPUS CHAPTER 7 TEST REVIEW 1. An alpha particle is accelerated through a potential difference of 10 kv.

More information

Intro to Particle Physics and The Standard Model. Robert Clare UCR

Intro to Particle Physics and The Standard Model. Robert Clare UCR Intro to Particle Physics and The Standard Model Robert Clare UCR Timeline of particle physics Ancient Greeks Rutherford 1911 Rutherford Chadwick Heisenberg 1930 s Hofstader Gell-Mann Ne eman 1960 s Timeline

More information

Cosmology and particle physics

Cosmology and particle physics Cosmology and particle physics Lecture notes Timm Wrase Lecture 5 The thermal universe - part I In the last lecture we have shown that our very early universe was in a very hot and dense state. During

More information

Physics 214 Experimental Particle Physics. Lecture 1 What to expect.

Physics 214 Experimental Particle Physics. Lecture 1 What to expect. Physics 214 Experimental Particle Physics Lecture 1 What to expect. We ll start with a grand tour. I do not expect you to understand this tour in detail. Instead, think of it as an orientation to which

More information

Precision Tests of the Standard Model. Yury Kolomensky UC Berkeley Physics in Collision Boston, June 29, 2004

Precision Tests of the Standard Model. Yury Kolomensky UC Berkeley Physics in Collision Boston, June 29, 2004 Precision Tests of the Standard Model Yury Kolomensky UC Berkeley Physics in Collision Boston, June 29, 2004 Motivation Experiments (not covered by previous speakers ) Atomic Parity Violation Neutrino

More information

Measurement of 39 Ar in Underground Argon for Dark Matter Experiments

Measurement of 39 Ar in Underground Argon for Dark Matter Experiments Measurement of 39 Ar in Underground Argon for Dark Matter Experiments Jingke Xu Princeton University June 7 th, 2013 1 Evidences for Dark Matter Rotation Curve Gravitational Lensing CMB Power Spectrum

More information

The Collider Detector at Fermilab. Amitabh Lath Rutgers University July 25, 2002

The Collider Detector at Fermilab. Amitabh Lath Rutgers University July 25, 2002 The Collider Detector at Fermilab Amitabh Lath Rutgers University July 25, 2002 What is Fermilab? A user facility with the Tevatron: 4 mile ring with superconducting magnets. Collides protons with antiprotons.

More information

Physics 214 Experimental Particle Physics. Lecture 1 What to expect.

Physics 214 Experimental Particle Physics. Lecture 1 What to expect. Physics 214 Experimental Particle Physics Lecture 1 What to expect. We ll start with a grand tour. I do not expect you to understand this tour in detail. Instead, think of it as an orientation to which

More information

Matter: it s what you have learned that makes up the world Protons, Neutrons and Electrons

Matter: it s what you have learned that makes up the world Protons, Neutrons and Electrons Name The Standard Model of Particle Physics Matter: it s what you have learned that makes up the world Protons, Neutrons and Electrons Just like there is good and evil, matter must have something like

More information

Physics 129 LECTURE 6 January 23, Particle Physics Symmetries (Perkins Chapter 3)

Physics 129 LECTURE 6 January 23, Particle Physics Symmetries (Perkins Chapter 3) Physics 129 LECTURE 6 January 23, 2014 Particle Physics Symmetries (Perkins Chapter 3) n Lagrangian Deductions n Rotations n Parity n Charge Conjugation Gauge Invariance and Charge Conservation The Higgs

More information

Outline: Introduction Search for new Physics Model driven Signature based General searches. Search for new Physics at CDF

Outline: Introduction Search for new Physics Model driven Signature based General searches. Search for new Physics at CDF PE SU Outline: Introduction Search for new Physics Model driven Signature based General searches R Search for new Physics at CDF SUperSYmmetry Standard Model is theoretically incomplete SUSY: spin-based

More information

Lecture 2: The First Second origin of neutrons and protons

Lecture 2: The First Second origin of neutrons and protons Lecture 2: The First Second origin of neutrons and protons Hot Big Bang Expanding and cooling Soup of free particles + anti-particles Symmetry breaking Soup of free quarks Quarks confined into neutrons

More information

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM Lecture 03 The Standard Model of Particle Physics Part II The Higgs Boson Properties of the SM The Standard Model So far we talked about all the particles except the Higgs If we know what the particles

More information

Physics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1

Physics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1 Physics 662 Particle Physics Phenomenology February 21, 2002 Physics 662, lecture 13 1 Physics Beyond the Standard Model Supersymmetry Grand Unified Theories: the SU(5) GUT Unification energy and weak

More information

Weak Interactions. The Theory of GLASHOW, SALAM and WEINBERG

Weak Interactions. The Theory of GLASHOW, SALAM and WEINBERG Weak Interactions The Theory of GLASHOW, SALAM and WEINBERG ~ 1959-1968 (Nobel 1979) Theory of the unified weak and electromagnetic interaction, transmitted by exchange of intermediate vector bosons mass

More information

Physics Quarknet/Service Learning

Physics Quarknet/Service Learning Physics 29000 Quarknet/Service Learning Lecture 3: Ionizing Radiation Purdue University Department of Physics February 1, 2013 1 Resources Particle Data Group: http://pdg.lbl.gov Summary tables of particle

More information

Today. From Last Time. Fundamental Matter Particles. Similar particles. Exchange Bosons (force carriers) And several different interactions

Today. From Last Time. Fundamental Matter Particles. Similar particles. Exchange Bosons (force carriers) And several different interactions From Last Time Discussed the weak interaction All quarks and leptons have a weak charge They interact through the weak interaction Weak interaction often swamped by electromagnetic or strong interaction.

More information

Photon Coupling with Matter, u R

Photon Coupling with Matter, u R 1 / 16 Photon Coupling with Matter, u R Consider the up quark. We know that the u R has electric charge 2 3 e (where e is the proton charge), and that the photon A is a linear combination of the B and

More information

Introduction to Particle Physics and the Standard Model. Robert Clare UCR

Introduction to Particle Physics and the Standard Model. Robert Clare UCR Introduction to Particle Physics and the Standard Model Robert Clare UCR Timeline of particle physics Ancient Greeks Rutherford 1911 Rutherford Chadwick Heisenberg 1930 s Hofstader Gell-Mann Ne eman 1960

More information

Particles and Interactions. Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014

Particles and Interactions. Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014 Particles and Interactions Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014 What is the world made of? In the ancient time: 4 elements 19 century atoms Beginning 20 th century

More information

Nuclear and Particle Physics 3: Particle Physics. Lecture 1: Introduction to Particle Physics February 5th 2007

Nuclear and Particle Physics 3: Particle Physics. Lecture 1: Introduction to Particle Physics February 5th 2007 Nuclear and Particle Physics 3: Particle Physics Lecture 1: Introduction to Particle Physics February 5th 2007 Particle Physics (PP) a.k.a. High-Energy Physics (HEP) 1 Dr Victoria Martin JCMB room 4405

More information

PHY492: Nuclear & Particle Physics. Lecture 24. Exam 2 Particle Detectors

PHY492: Nuclear & Particle Physics. Lecture 24. Exam 2 Particle Detectors PHY492: Nuclear & Particle Physics Lecture 24 Exam 2 Particle Detectors Exam 2 April 16, 2007 Carl Bromberg - Prof. of Physics 2 Exam 2 2. Short Answer [4 pts each] a) To describe the QCD color quantum

More information

Fundamental Forces. David Morrissey. Key Concepts, March 15, 2013

Fundamental Forces. David Morrissey. Key Concepts, March 15, 2013 Fundamental Forces David Morrissey Key Concepts, March 15, 2013 Not a fundamental force... Also not a fundamental force... What Do We Mean By Fundamental? Example: Electromagnetism (EM) electric forces

More information

The Four Fundamental Forces. The Four Fundamental Forces. Gravitational Force. The Electrical Force. The Photon (γ) Unification. Mass.

The Four Fundamental Forces. The Four Fundamental Forces. Gravitational Force. The Electrical Force. The Photon (γ) Unification. Mass. The Four Fundamental Forces What are the four fundamental forces? The Four Fundamental Forces What are the four fundamental forces? Weaker Stronger Gravitational, Electromagnetic, Strong and Weak Nuclear

More information

Chapter 32 Lecture Notes

Chapter 32 Lecture Notes Chapter 32 Lecture Notes Physics 2424 - Strauss Formulas: mc 2 hc/2πd 1. INTRODUCTION What are the most fundamental particles and what are the most fundamental forces that make up the universe? For a brick

More information

Large Hadron Collider

Large Hadron Collider Large Hadron Collider Himadri Barman TSU, JNCASR September 18, 2008 0-0 Large Hadron Collider (LHC): Plan We ll see 4 short videos. In between I ll give you a little guideline. Purpose is to understand

More information

Studies of the XENON100 Electromagnetic Background

Studies of the XENON100 Electromagnetic Background Studies of the XENON100 Electromagnetic Background Daniel Mayani Physik-Institut University of Zurich PhD Seminar PSI, August 26-27, 2015 Searching for elusive particles The main challenge for experiments

More information

First some Introductory Stuff => On The Web.

First some Introductory Stuff => On The Web. First some Introductory Stuff => On The Web http://hep.physics.utoronto.ca/~orr/wwwroot/phy357/phy357s.htm PHY357 = What is the Universe Made Of? Is the Universe Made of These? Proton = (u u d) held

More information

Dark matter and IceCube neutrinos

Dark matter and IceCube neutrinos IL NUOVO CIMENTO 38 C (2015) 31 DOI 10.1393/ncc/i2015-15031-4 Colloquia: IFAE 2014 Dark matter and IceCube neutrinos R. Biondi Dipartimento di Scienze Fisiche e Chimiche, Università degli Studi di L Aquila,

More information

Search for a Z at an e + e - Collider Thomas Walker

Search for a Z at an e + e - Collider Thomas Walker Search for a Z at an e + e - Collider Thomas Walker Significance: Many theories predict that another neutral gauge boson (Z ) may exist. In order to detect this Z, I would use an e + e - linear collider

More information

Unsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY

Unsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY Unsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY 1 I am going to go through some of the major unsolved problems in theoretical physics. I mean the existing theories seem

More information

Particle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden

Particle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden Particle Physics Tommy Ohlsson Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden International Baccalaureate T. Ohlsson (KTH) Particle Physics 1/

More information

Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin

Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin Outline The Four Fundamental Forces The Strong Force History of the Strong Force What These People Did Experimental Support 1 Fundamental Forces

More information

November 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model

November 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model Scalar from November 24, 2014 1 2 3 4 5 What is the? Gauge theory that explains strong weak, and electromagnetic forces SU(3) C SU(2) W U(1) Y Each generation (3) has 2 quark flavors (each comes in one

More information

Is the Neutrino its Own Antiparticle?

Is the Neutrino its Own Antiparticle? Is the Neutrino its Own Antiparticle? CENPA REU Summer Seminar Series University of Washington, Seattle, WA July 22, 2013 Outline What s a neutrino? The case for Majorana neutrinos Probing the nature of

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

Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material. From last time

Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material. From last time Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material From last time Quantum field theory is a relativistic quantum theory of fields and interactions. Fermions

More information

Saturday Morning Physics -- Texas A&M University. What is Matter and what holds it together? Dr. Rainer J. Fries. January 27, 2007

Saturday Morning Physics -- Texas A&M University. What is Matter and what holds it together? Dr. Rainer J. Fries. January 27, 2007 Saturday Morning Physics -- Texas A&M University Particles and Forces What is Matter and what holds it together? Dr. Rainer J. Fries January 27, 2007 Zooming in on the World around us Particles and Forces

More information

Saturday Morning Physics -- Texas A&M University Dr. Rainer J. Fries

Saturday Morning Physics -- Texas A&M University Dr. Rainer J. Fries Saturday Morning Physics -- Texas A&M University Particles and Forces What is Matter and what holds it together? Dr. Rainer J. Fries January 27, 2007 Zooming in on the World around us Particles and Forces

More information

PH5211: High Energy Physics. Prafulla Kumar Behera Room: HSB-304B

PH5211: High Energy Physics. Prafulla Kumar Behera Room: HSB-304B PH5211: High Energy Physics Prafulla Kumar Behera E-mail:behera@iitm.ac.in Room: HSB-304B Information Class timing: Wed. 11am, Thur. 9am, Fri. 8am The course will be graded as follows: 1 st quiz (20 marks)

More information

Remainder of Course. 4/22 Standard Model; Strong Interaction 4/24 Standard Model; Weak Interaction 4/27 Course review 5/01 Final Exam, 3:30 5:30 PM

Remainder of Course. 4/22 Standard Model; Strong Interaction 4/24 Standard Model; Weak Interaction 4/27 Course review 5/01 Final Exam, 3:30 5:30 PM Remainder of Course 4/22 Standard Model; Strong Interaction 4/24 Standard Model; Weak Interaction 4/27 Course review 5/01 Final Exam, 3:30 5:30 PM Practice Final on Course Web Page See HW #12 (not to be

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

Study of the Scintillation Detector Efficiency and Muon Flux

Study of the Scintillation Detector Efficiency and Muon Flux Study of the Scintillation Detector Efficiency and Muon Flux Ali Al-dulaimi 1, Areeg Al-hamadany 1, Mohammed Al-Gherairy 1, Rafid Al-Zuhairi 1 and Amar Al-timimi 1 Department of Physics, College of Science/University

More information

Cosmogenic background for the GERDA experiment. Luciano Pandola INFN, Laboratori del Gran Sasso, Italy

Cosmogenic background for the GERDA experiment. Luciano Pandola INFN, Laboratori del Gran Sasso, Italy Cosmogenic background for the GERDA experiment Luciano Pandola INFN, Laboratori del Gran Sasso, Italy Cosmogenic Activity and Background Workshop, Berkeley April 15 th, 2011 GERDA experiment at LNGS The

More information

Astronomy 182: Origin and Evolution of the Universe

Astronomy 182: Origin and Evolution of the Universe Astronomy 182: Origin and Evolution of the Universe Prof. Josh Frieman Lecture 12 Nov. 18, 2015 Today Big Bang Nucleosynthesis and Neutrinos Particle Physics & the Early Universe Standard Model of Particle

More information

A Tour of the Standard Model of Elementary Particles and Fields

A Tour of the Standard Model of Elementary Particles and Fields A Tour of the Standard Model of Elementary Particles and Fields What Do We Know About the Fundamental Structure of Nature and How Do We Know It? Dr. Michael G. Strauss The University of Oklahoma Elementary

More information

Beyond the Standard Model

Beyond the Standard Model Beyond the Standard Model The Standard Model Problems with the Standard Model New Physics Supersymmetry Extended Electroweak Symmetry Grand Unification References: 2008 TASI lectures: arxiv:0901.0241 [hep-ph]

More information

Design, Construction, Operation, and Simulation of a Radioactivity Assay Chamber

Design, Construction, Operation, and Simulation of a Radioactivity Assay Chamber Design, Construction, Operation, and Simulation of a Radioactivity Assay Chamber Wesley Ketchum and Abe Reddy EWI Group, UW REU 2006 Outline Neutrino Physics Background Double Beta Decay and the Majorana

More information

Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo

Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo Particle Physics Fall 2015 1 Course Overview Lecture 1: Introduction, Decay Rates and Cross Sections Lecture 2: The Dirac Equation and Spin

More information

PHY-105: Introduction to Particle and Nuclear Physics

PHY-105: Introduction to Particle and Nuclear Physics M. Kruse, Spring 2011, Phy-105 PHY-105: Introduction to Particle and Nuclear Physics Up to 1900 indivisable atoms Early 20th century electrons, protons, neutrons Around 1945, other particles discovered.

More information

DarkSide. Bianca Bottino Università di Genova and INFN Sezione di Genova on behalf of the DarkSide collaboration 1

DarkSide. Bianca Bottino Università di Genova and INFN Sezione di Genova on behalf of the DarkSide collaboration 1 DarkSide Bianca Bottino Università di Genova and INFN Sezione di Genova on behalf of the DarkSide collaboration 1 DARKSIDE MAIN FEATURES Dark Matter direct detection WIMP induced nuclear recoils Double

More information

A brief history of neutrino. From neutrinos to cosmic sources, DK&ER

A brief history of neutrino. From neutrinos to cosmic sources, DK&ER A brief history of neutrino Two body decay m 1 M m 2 Energy-momentum conservation => Energy of the decay products always the same 1913-1930: Puzzle of decay Continuous spectrum of particles Energy is not

More information

Guest Lecture PHY 7361: Harnessing Cherenkov Radiation SteveSekula, 13 April 2010 (created 9 April 2010)

Guest Lecture PHY 7361: Harnessing Cherenkov Radiation SteveSekula, 13 April 2010 (created 9 April 2010) Physics Notebook - 2010 Steve Sekula's Analysis Notebook Physics Notebook - 2010 Steve Sekula's Analysis Notebook Guest Lecture PHY 7361: Harnessing Cherenkov Radiation SteveSekula, 13 April 2010 (created

More information

Neutrino Physics. Neutron Detector in the Aberdeen Tunnel Underground Laboratory. The Daya Bay Experiment. Significance of θ 13

Neutrino Physics. Neutron Detector in the Aberdeen Tunnel Underground Laboratory. The Daya Bay Experiment. Significance of θ 13 Neutrino Physics Neutron Detector in the Aberdeen Tunnel Underground Laboratory John K.C. Leung Department of Physics, HKU On behalf of CUHK, LBL & IHEP Presented to HKRPS on June 21, 2007 Neutrinos have

More information

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course?

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course? Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course? Contents: Review of the Standard Model! What we know! What we don

More information

Phys 102 Lecture 28 Life, the universe, and everything

Phys 102 Lecture 28 Life, the universe, and everything Phys 102 Lecture 28 Life, the universe, and everything 1 Today we will... Learn about the building blocks of matter & fundamental forces Quarks and leptons Exchange particle ( gauge bosons ) Learn about

More information

The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today. M. Herndon, Phys

The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today. M. Herndon, Phys The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today M. Herndon, Phys 301 2018 1 The Periodic Table: The early 20 th century understanding of the

More information