The Importance of Mass and How We Describe it

Similar documents
Activity 12: Energy from Nuclear Reactions

Instead, the probability to find an electron is given by a 3D standing wave.

1. What does this poster contain?

The Particle World. This talk: What is our Universe made of? Where does it come from? Why does it behave the way it does?

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

Fundamental Forces. Range Carrier Observed? Strength. Gravity Infinite Graviton No. Weak 10-6 Nuclear W+ W- Z Yes (1983)

A first trip to the world of particle physics

The Physics of Particles and Forces David Wilson

Particles in the Early Universe

Mass. Chris Quigg Fermi National Accelerator Laboratory

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

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

Photon Coupling with Matter, u R

THE NUCLEUS OF AN ATOM

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

The Higgs - Theory. The Higgs. Theory. Arthur H. Compton Lecture th. Martin Bauer. Oct. 26 Arthur H. Compton Lectures Oct 26th 2013

Introduction to Modern Physics Problems from previous Exams 3

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

TEACHER. The Atom 4. Make a drawing of an atom including: Nucleus, proton, neutron, electron, shell

The Exchange Model. Lecture 2. Quantum Particles Experimental Signatures The Exchange Model Feynman Diagrams. Eram Rizvi

cgrahamphysics.com Particles that mediate force Book pg Exchange particles

Bannerman High School Physics Department. Making Accurate Statements. Higher Physics. Quanta and Waves

Subatomic Particles. proton. neutron. electron. positron. particle. 1 H or 1 p. 4 α or 4 He. 0 e or 0 β

Chapter 32 Lecture Notes

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

Properties of Nuclei deduced from the Nuclear Mass

Quantum Numbers. Elementary Particles Properties. F. Di Lodovico c 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F.

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

The Quark-Gluon plasma in the LHC era

Unravelling the Mysteries of Matter with the CERN Large Hadron Collider An Introduction/Overview of Particle Physics

[1] (c) Some fruits, such as bananas, are naturally radioactive because they contain the unstable isotope of potassium-40 ( K.

Masses and binding energies

Astronomy 182: Origin and Evolution of the Universe

FUNDAMENTAL PARTICLES CLASSIFICATION! BOSONS! QUARKS! FERMIONS! Gauge Bosons! Fermions! Strange and Charm! Top and Bottom! Up and Down!

Bosons in the Zoo of Elementary Particles

Cosmology and particle physics

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

Physics 4213/5213 Lecture 1

Physics 1C. Lecture 29A. "Nuclear powered vacuum cleaners will probably be a reality within 10 years. " --Alex Lewyt, 1955

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

The symmetries of QCD (and consequences)

The Origin of the Visible Mass in the Universe

SUPERSYMETRY FOR ASTROPHYSICISTS

Section 2: Nuclear Fission and Fusion. Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

A Brief History of Modern Physics

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

THE STANDARD MODEL OF MATTER

Nuclear Physics and Nuclear Reactions

PHY 142! Assignment 11! Summer 2018

Electroweak and Higgs Physics

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

Ch(3)Matter & Change. John Dalton

Modern Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson XI November 19, 2015

Lecture 6: The Physics of Light, Part 1. Astronomy 111 Wednesday September 13, 2017

[2] State in what form the energy is released in such a reaction.... [1]

Lecture 4. The Bohr model of the atom. De Broglie theory. The Davisson-Germer experiment

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

THE NUCLEUS: A CHEMIST S VIEW Chapter 20

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

The Secret of Mass. Can we Evaporate the Vacuum at RHIC?

The Nucleus 1. The existence of a nucleus

1.1 The Fundamental Chemistry of life

Le Modèle Standard et ses extensions

The Building Blocks of Nature

- ~200 times heavier than the e GeV µ travels on average. - does not interact strongly. - does emit bremsstrahlung in

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

Particle Discovery at the LHC. Sally Seidel University of New Mexico 20 October 2017 APS Four Corners Meeting

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

Elementary particles and typical scales in high energy physics

Physics 102: Lecture 26. X-rays. Make sure your grade book entries are correct. Physics 102: Lecture 26, Slide 1

DISCRETE SYMMETRIES IN NUCLEAR AND PARTICLE PHYSICS. Parity PHYS NUCLEAR AND PARTICLE PHYSICS

Split SUSY and the LHC

Higgs boson may appear to be a technihiggs

The Positron Fraction in Primary Cosmic Rays and New Cosmological Problems

Elementary particles, forces and Feynman diagrams

Physics 142 Modern Physics 2 Page 1. Nuclear Physics

STANDARD MODEL and BEYOND: SUCCESSES and FAILURES of QFT. (Two lectures)

Introduction to Particle Physics. HST July 2016 Luis Alvarez Gaume 1

Phenomenology of Heavy-Ion Collisions

Atomic and nuclear physics

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

Wesley Smith, U. Wisconsin, January 21, Physics 301: Introduction - 1

2007 Section A of examination problems on Nuclei and Particles

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

PHY-105: Introduction to Particle and Nuclear Physics

Lecture 3: Big Bang Nucleosynthesis The First Three Minutes

Par$cles. Ma#er is made of atoms. Atoms are made of leptons and quarks. Leptons. Quarks. atom nucleus nucleon quark m m m m

Electric Dipole Moments and the strong CP problem

PHYS-1050 Hydrogen Atom Energy Levels Solutions Spring 2013

Thursday, April 23, 15. Nuclear Physics

Atomic emission & absorption spectra

Every atom has a nucleus which contains protons and neutrons (both these particles are known nucleons). Orbiting the nucleus, are electrons.

Quanta to Quarks. Science Teachers Workshop 2014 Workshop Session. Adrian Manning

NUCLEAR FORCES. Historical perspective

Particles. Constituents of the atom

Essentials of Particle Physics

Alpha Decay. Decay alpha particles are monoenergetic. Nuclides with A>150 are unstable against alpha decay. E α = Q (1-4/A)

Announcement. Station #2 Stars. The Laws of Physics for Elementary Particles. Lecture 9 Basic Physics

32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES

Transcription:

The Importance of Mass and How We Describe it Philip Bechtle SLAC 06/25/2005 Philip Bechtle p.1

Outline What does this concept of mass mean at all? Why the heck are masses so important? What would happen, if the fundamental masses would only slightly change? So, if we need to describe mass, how do we do it? What do we know about it and what can we learn in the future? Most importantly: Why particle physics really explains the everyday world! Philip Bechtle p.2

About this talk What it is: A discussion of why investigating fundamental properties of nature is interesting for our everyday life An introduction into the concepts behind our understanding of mass What it is not: A talk about the experimental techniques of searching and investigating the mass of elementary particles For that, please refer to previous (or future?) presentations about the LHC and the ILC Philip Bechtle p.3

What are we investigating? How are we influenced by the most tiny objects we know of? Philip Bechtle p.4

What are we investigating? The building blocks of all visible matter Philip Bechtle p.5

What is mass, after all?? Mass ist stored energy in an interaction in a motion not observed from outside (like temperature) Philip Bechtle p.6

What is the Universe made of? This discussion is only about the 4 % ordinary matter We hopefully are on the verge of finding out what the 21 % dark matter are made of Philip Bechtle p.7

Which Mass are we Talking About? The masses of the building blocks of matter: No idea yet why they look like that... But it is extremely important that they look like that! Philip Bechtle p.8

Influence of the Fundamental Mass For hydrogen (or any other atom): m p + m e = 938.8 MeV 2m u + m d + m e = 16.5 MeV 98% of all macroscopic mass is from interaction energy in the strong interaction kinetic energy of the quarks and gluons in the nucleus If the contribution of the fundamental mass is so small, why is it so important? Changing m u, m d or m e would have Small effects on macroscopic masses Small effects on Ω matter Huge effects on the behaviour of matter Let s see why... Philip Bechtle p.9

Protons and Neutrons The proton does not decay / +e + + ν e Stable neutrons exist only in heavy nuclei Heavy nuclei would be disrupted by the electromagnetic force if they had no neutrons Philip Bechtle p.10

What makes nuclei stable? The proton does not decay (thus there can be much hydrogen). p / n + e + + ν e, because m n m p = 939.6 938.8 MeV = 1.3 MeV (> m e : neutron decays) m mass = m d m u 3 4 MeV m elec = α em (q 2 d q2 u)/(r qq ) = 0.5 MeV/ r qq (fm) (2 3) MeV If the neutron decays, why does it exist in stable nuclei? In nucleus: n / p + e + ν e, because Neutron is stronger bound in nucleus than proton Binding energy difference E b (n) E b (p) some MeV > m d (m u + m e ) + m elec = 0.8 MeV is larger than energy gain from neutron decay Stability of nuclei is a delicate interplay between Strong force, electromagnetic force and masses Philip Bechtle p.11

What if m d changes? m d influences nuclei Consider small changes of m d (with respect to the total range of 1/10 14!) Increase m d by a factor of 2: m d = 16 MeV Allows n p + e ν e in nuclei, since E b (n) E b (p) some MeV < m d (m u + m e ) + m elec = 8.8 MeV Nuclei with Z = A, broken by electromagnetic force above 6 6C No oxygen, no water, no life as we know it Decrease m d by a factor of 2: m d = 4 MeV allows p n + e + + ν e, also in D, since m p m n = 934.3 931.6 MeV = 2.7 MeV forbids n + n D + e + ν e, since 2m n < m D + m e No protons, no stars, just neutrals n, γ, ν Philip Bechtle p.12

What if m e changes? m e and α em govern chemical processes Rydberg energy R = 1 2 α2 emm e Bohr radius a = 1/α em m e Decrease m e by factor 25: m e = 0.02 MeV Huge atoms, small binding energies Humans are giants, 130 feet tall covalent bindings in carbohydrates (CH 4 C + 2H 2 ) break at 140 o F Increase m e by factor 3: m e = 1.5 MeV K-capture in hydrogen: p + e n + ν e Star formation from stable n, D replaces hydrogen Humans are dwarfs, 2 feet tall Philip Bechtle p.13

Part 2: How does our concept of what fundamental mass is look like? Philip Bechtle p.14

The Higgs Mechanism Philip Bechtle p.15

The Higgs Mechanism Philip Bechtle p.16

The Higgs Mechanism Philip Bechtle p.17

The Higgs Boson Itself Philip Bechtle p.18

The Higgs Boson Itself Philip Bechtle p.19

The Higgs and its Interaction Dynamic generation of mass f 1/q (g f v/ 2 ) + + +... 1/q 1/q H H H 1 q/ + 1 q/ ( gf v 2 ) 1 q/ + = 1 q/ n=0 [( gf v 2 ) 1 q/ ] n = q/ 1 ( ) gf v 2 Philip Bechtle p.20

Why is there always a field? Philip Bechtle p.21

How to find the Higgs Boson? The heavier a particle, the stronger its coupling to the Higgs field in order to find the Higgs, produce heavy particles and see whether they emit a Higgs boson e + h Z 0 e Z 0 If such a particle is found: measure its properties If no such process is found at LHC and ILC: Higgs theory is wrong Philip Bechtle p.22

How to Measure its Properties? Philip Bechtle p.23

Outlook The fundamental pattern of masses is extremely important for the way the universe behaves We are just at the beginning of exploring the origins of mass Open question: How does the mechanism of the origin of fundamental particle masses work? Completely open question: What causes the mass hierarchies? An extremely interesting time lies ahead... to be studied at LHC and ILC Philip Bechtle p.24

Necessary Ingredients Need a non-vanishing background field with no preferred direction That means: The energy of the field must be at its lowest value, if there is a field, not if there is no field Potential Energy But: Theory must obey symmetries Field Strength Simplified example of a U(1) symmetry: E = φ Invariant under symmetry operation φ = φ + constant Philip Bechtle p.25

Rotational Symmetries Another symmetry defining the fundamental interactions: SU(2) Can be simplified as a rotation in 2 dimensions: Φ = φ 1 = cos α sin α φ 2 sin α cos α φ 1 φ 2 We can extend our simple potential from before to two dimensions φ 2 φ 2 φ 1 But the field in it moves over the 2D plane under symmetry operations! φ 1 Philip Bechtle p.26

Spontaneous Symmetry Breaking Clever Idea: Construct rotational symmetric potential: Result: Theory is symmetric under rotations, ground state is at φ 0 anyhow Philip Bechtle p.27