The Proton Decay and Experiments

Similar documents
Option 212: UNIT 2 Elementary Particles

Lecture 18 - Beyond the Standard Model

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

XI. Beyond the Standard Model

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

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

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

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

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

Physics 4213/5213 Lecture 1

An Introduction to Particle Physics

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

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

Fundamental Particles and Forces

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

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

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

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

A first trip to the world of particle physics

Review Chap. 18: Particle Physics

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

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

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

FYS 3510 Subatomic physics with applications in astrophysics. Nuclear and Particle Physics: An Introduction

Physics 7730: Particle Physics

Elementary particles and typical scales in high energy physics

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

Fundamental Particles

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

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

Detectors for astroparticle physics

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

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

The Uncertainty Principle and the Quarks

PHYS 420: Astrophysics & Cosmology

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

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

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

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

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

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

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

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

CHAPTER 7 TEST REVIEW

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

Cosmology and particle physics

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

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

Measurement of 39 Ar in Underground Argon for Dark Matter Experiments

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

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

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

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

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

Lecture 2: The First Second origin of neutrons and protons

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

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

Weak Interactions. The Theory of GLASHOW, SALAM and WEINBERG

Physics Quarknet/Service Learning

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

Photon Coupling with Matter, u R

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

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

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

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

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

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

Chapter 32 Lecture Notes

Large Hadron Collider

Studies of the XENON100 Electromagnetic Background

First some Introductory Stuff => On The Web.

Dark matter and IceCube neutrinos

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

Unsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY

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

Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin

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

Is the Neutrino its Own Antiparticle?

Chapter 22: Cosmology - Back to the Beginning of Time

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

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 Dr. Rainer J. Fries

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

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

Particle + Physics at ATLAS and the Large Hadron Coillder

Study of the Scintillation Detector Efficiency and Muon Flux

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

Astronomy 182: Origin and Evolution of the Universe

A Tour of the Standard Model of Elementary Particles and Fields

Beyond the Standard Model

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

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

PHY-105: Introduction to Particle and Nuclear Physics

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

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

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

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

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

Phys 102 Lecture 28 Life, the universe, and everything

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

Transcription:

The Proton Decay and Experiments Astroteilchenphysik Vortrag Carlos Ayerbe Gayoso Ayerbe@kph.uni-mainz.de 18.12. 02

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

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

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?

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...

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 10 14 GeV

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

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

The Proton decay This means that the proton could decay to mesons and leptons!! p p e π + π + 0 + + 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

Detecting the proton decay One can t watch a proton for 10 30 years and see if it decay (is bored!!) But we can watch 10 30 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)

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

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 250-800 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

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

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

The Counting Test Facility at Grand Sasso Scintillator Containment Vessel

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%

The Counting Test Facility at Grand Sasso The Photomultiplier System

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 300 45 events/d 210 Po from the decay of 222 Rn 250 40 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

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

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