EIC Science. Rik Yoshida, EIC-Center at Jefferson Lab Abhay Deshpande, Center for Frontiers in Nuclear Physics, BNL and Stony Brook

Similar documents
The Electron-Ion Collider: Exploring the science of Nuclear Femtography

Introduction to High Energy Nuclear Collisions I (QCD at high gluon density) Jamal Jalilian-Marian Baruch College, City University of New York

Electron-Ion Collider for Nuclear and Particle Physics. Hugh Montgomery Jefferson Lab

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

High Energy Physics. Lecture 9. Deep Inelastic Scattering Scaling Violation. HEP Lecture 9 1

erhic: Science and Perspective

I. Antoniadis CERN. IAS CERN Novice Workshop, NTU, 7 Feb 2014

Experimental results on nucleon structure Lecture I. National Nuclear Physics Summer School 2013

Nucleon Spin. Tyler Corbett

Laboratory for Nuclear Science

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

Electron Ion Collider: The next QCD frontier Understanding the Glue that Binds Us All

The Physics of Particles and Forces David Wilson

What is new about the Electron Ion Collider (EIC) in the US?

GPDs and TMDs at Electron-Ion Collider. Workshop on hadron tomography at J-PARC and KEKB January 6 th, 2017 KEK, Tsukuba, Japan Yuji Goto (RIKEN)

What does Dark Matter have to do with the Big Bang Theory?

What does Dark Matter have to do with the Big Bang Theory?

Physics at Hadron Colliders Partons and PDFs

Chapter 32 Lecture Notes

What does Dark Matter have to do with the Big Bang Theory?

Today. The nature of the Universe - Beyond the Standard Model

Today. The goals of science. The nature of the Universe - Beyond the Standard Model

Probing the Atomic Nucleus at Jefferson Lab

Evidence for the Strong Interaction

Experimental Aspects of Deep-Inelastic Scattering. Kinematics, Techniques and Detectors

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

Introduction to Quantum Chromodynamics (QCD)

Measurements with Polarized Hadrons

Particle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry

Jefferson Lab 12 GeV Science Program

Understanding the balance of matter and antimatter in the Universe

Frontier Particle Accelerators

INTERACTIONS. The science of matter, space and time. High-Energy Physics

New subatomic particle and the Electro-Strong and -Weak Interaction

AN OVERVIEW OF QUANTUM CHROMODYNAMICS UNIVERSITY OF WASHINGTON PHYS575 FARRAH TAN 12/10/2015

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

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

Hadronization with JLab 6/12 GeV

Particle + Physics at ATLAS and the Large Hadron Coillder

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

The Jefferson Lab 12 GeV Program

A Tour of the Standard Model of Elementary Particles and Fields

An Introduction to Particle Physics

REALIZING EINSTEIN S DREAM. Exploring Our Mysterious Universe

Chapter 22: Cosmology - Back to the Beginning of Time

Electron-Ion Collider Taking us to the next QCD Frontier

UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC. Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009

A Comparative Study of Quark-Gluon Plasma at the Core of a Neutron Star and in the Very Early Universe. Frikkie de Bruyn

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

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

The Electro-Strong Interaction

PHY357 Lecture 14. Applications of QCD. Varying coupling constant. Jets and Gluons. Quark-Gluon plasma. Colour counting

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

Introduction to Quantum ChromoDynamics and the parton model

Option 212: UNIT 2 Elementary Particles

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

An Assessment of U.S.-Based Electron-Ion Collider Science

Project. 1 Introduction. EPJ Web of Conferences 66, (2014)

In Pursuit of Discovery at The Large Hadron Collider

The first 400,000 years

A first trip to the world of particle physics

The Start of the LHC Era. Peter Wittich Laboratory of Elementary Particle Physics Cornell University

1. What does this poster contain?

High Energy Frontier Recent Results from the LHC: Heavy Ions I

The Detector Design of the Jefferson Lab EIC

Particles, Energy, and Our Mysterious Universe

Strong interaction physics with an Electron Ion Collider

Exciting opportunities at JLab GeV!

The Proton Radius Puzzle and the Electro-Strong Interaction

BRIEF INTRODUCTION TO HERA PHYSICS

Chapter 22 Back to the Beginning of Time

Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin

Overview of Science Goals, Golden Measurements and Implications for the Energy and Luminosity Reach of the EIC

THE NUCLEUS AS A QCD LABORATORY: HADRONIZATION, 3D TOMOGRAPHY, AND MORE

NUCLEAR FORCES. Historical perspective

Particles in the Early Universe

Status and Perspectives of Hadron Physics in Europe. Forschungszentrum Jülich in der Helmholtz-Gemeinschaft

PHL424: 4 fundamental forces in nature

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

THE NEUTRINOS. Boris Kayser & Stephen Parke Fermi National Accelerator Laboratory

Overview on the Future Electron-Ion Collider Projects

Lecture 36: The First Three Minutes Readings: Sections 29-1, 29-2, and 29-4 (29-3)

Welcome to DESY. What is DESY and what kind of research is done here?

High-energy ea scattering. Spectator nucleon tagging. Future facilities. Energy, luminosity, polarization. Physics objectives with light nuclei

Electron-Ion Collider for Nuclear and Particle Physics. Hugh Montgomery Jefferson Lab

arxiv: v1 [nucl-ex] 3 Sep 2018

v = H o d Hubble s Law: Distant galaxies move away fastest Velocity (v) is proportional to Distance (d):

Hunting for Quarks. G n M Co-conspirators: Jerry Gilfoyle for the CLAS Collaboration University of Richmond

Spin Structure with JLab 6 and 12 GeV

SPIN STRUCTURE OF THE NUCLEON AND POLARIZATION. Charles Y. Prescott Stanford Linear Accelerator Center Stanford University, Stanford CA 94309

11/19/08. Gravitational equilibrium: The outward push of pressure balances the inward pull of gravity. Weight of upper layers compresses lower layers

Nucleon Spin Structure from Confinement to Asymptotic Freedom

Nucleon Spin Structure: Overview

Lab Monday optional: review for Quiz 3. Lab Tuesday optional: review for Quiz 3.

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

Particle accelerators

Opportunities in low x physics at a future Electron-Ion Collider (EIC) facility

Phenomenology of Heavy-Ion Collisions

The Universe. Unit 3 covers the following framework standards: ES 8 and 12. Content was adapted the following:

Selected Topics from Modern Physics

Transcription:

EIC Science Rik Yoshida, EIC-Center at Jefferson Lab Abhay Deshpande, Center for Frontiers in Nuclear Physics, BNL and Stony Brook

Introduction Invited to give a talk EIC Science and JLEIC Status I will give 2 talks -This one EIC Science ~25 min - JLEIC status ~10 min After discussion with Abhay, we decided to give a different talk on EIC Science given the venue and audience. Abhay and I have been collaborating on a magazine article on EIC science. As EIC becomes more and more real, we will need to talk to people beyond nuclear physics, or even science. We thought it might be interesting to show what we have been thinking about to an expert audience. So this talk is co-authored by me and Abhay The second talk is a Jefferson Lab talk. EIC Science-INT Symposium 2018 2

Our Universe Observable universe contains about 10 53 kg of ordinary matter. Most of this mass is in about 10 80 protons and neutrons at the center of atoms. Where does the mass of the protons and neutrons come from? EIC Science-INT Symposium 2018 3

Higgs Boson Discovery In 2012, the Higgs Boson was discovered at the LHC at the CERN laboratory The Higgs mechanism gives mass to quarks, and protons (and neutrons) are made of quarks. BUT, it turns out that the quarks make up only about 1% of the proton mass. Where does the mass of the proton come from? EIC Science-INT Symposium 2018 4

Characteristics of the nucleons Quarks (and gluons) in protons are bound together by an interaction called Quantum Chromodynamics (QCD). The energy stored in the proton due to QCD interactions is responsible for the mass of the proton (E=mc 2, i.e. energy = mass times speed-of-light 2 ) But how exactly this happens is still a mystery! Spin In fact, we don t understand truly how any of the characteristics of the nucleon comes about from the fundamental QCD interactions. nucleon-nucleon forces EIC Science-INT Symposium 2018 5

Origin of Elements Characteristics of Protons and Neutrons (Nucleons), singly and collectively in Nuclei, in concert with EW and Gravity forms the visible Cosmos. Stellar Fusion Big Bang He through Fe Nova ~14 to 5 Billon Years ago H, He ~15 Billion Years ago Neutron stars ~250 Thousand Years ago Heavier than Fe EIC Science-INT Symposium 2018 6

Characteristics of Nucleons Nucleons Mass Spin Bulk NN interactions Arise out of quarks and gluons interacting through Quantum Chromodynamics (QCD) Nucleons are an emergent phenomena of QCD that we still don t really understand Fifty years after the discovery of the quarks, we are finally at the threshold of unraveling this mystery. This is the story of how we got here and where we re going next in this great adventure. EIC Science-INT Symposium 2018 7

Seeing Quarks and Gluons In the first part of the 20 th century we learned to see atoms using x-rays Double-Helix d ~ nanometers In the same way, we learned to see inside protons in the 1960 s using powerful electron beams. Electron acclerator at SLAC under construction femtometer EIC Science-INT Symposium 2018 8

Quantum Entanglement However, we have an immediate problem: Quantum Mechanics Atoms can be located at definite positions in space, with mostly empty space between them. Quarks and gluons are at a scale (1000000 smaller) which is deeply quantum mechanical: they exist only in superposition of infinite number of configurations. Worse: the tool that we use to probe the proton and the proton structure are quantum mechanically entangled and we can t tell them apart. How can we deal with this situation? EIC Science-INT Symposium 2018 9

Parton Model Feynman Imagine the proton is moving very (very) fast. Then the proton is flattened due to Lorenz contraction. Bjorken If the proton content ( partons ) is probed quickly enough then perhaps we can measure what fraction of the momentum the parton being probed (called Bjorken-x). We could then measure the x-distribution of partons? This turns out to be correct! EIC Science-INT Symposium 2018 10

Quantum Chromodynamics (QCD) Photons couple to electric charge. For QCD: electrons quarks photons gluons electric charge color gluons (unlike photons) carry charge and thus couple to gluons. EIC Science-INT Symposium 2018 11

Asymptotic Freedom and Confinement Gross, Politzer and Wilzcek (1973) Nobel Prize 2004 In high-energy interactions, quarks are weakly bound. QCD is a viable theory of quark interactions. partons = quarks is a viable hypothesis. Also implies quark-gluon plasma EIC Science-INT Symposium 2018 12

How and where we can solve QCD Protons Mass Spin Bulk NN interactions We still can t do the math! We can do the math! Lattice QCD sidebar EIC Science-INT Symposium 2018 13

Quantum Entanglement resolved (for Bjorken-x) As long as the the probe has small enough wavelength, the probe (the virtual photon) and the proton are not entangled. (factorization) This means we can measure the momentum distributions of quarks and gluons.. but in 1 direction only. The momentum distribution itself has its origins in the un-calculable part of QCD. So we gain an imperfect picture of the proton. EIC Science-INT Symposium 2018 14

Measuring x-distributions resolution smaller x How far can this rise go on? EIC Science-INT Symposium 2018 15

Large Hadron Collider Beam of quarks and gluons EIC Science-INT Symposium 2018 16

Learning to turn the proton Fast proton as seen from the side Fast proton seen head-on QCD Theory development in last 30 years New Factorization Old factorization EIC Science-INT Symposium 2018 17

First Transverse Structure Measurements worldwide DESY Laboratory, Germany CERN Laboratory, Switzerland HERMES experiment COMPASS experiment Brookhaven Laboratory, NY Brookhaven Laboratory, VA EIC Science-INT Symposium 2018 18

Advances in all areas means we are ready for the EIC Theory Accelerator Technologies Detector Technologies Computing Steady advances in all of these areas mean that EIC Science-INT Symposium 2018 19

US-Based EIC Proposals Jefferson Lab Newport News, VA 2002 JLab Concept Brookhaven Lab Long Island, NY EIC Science-INT Symposium 2018 20

EIC Science example: Spin Puzzle Try to gain dynamical understanding p b Momentum imaging (TMD s) Proton is transversely polarized Spatial Imaging (GPDs) Measure the quarks (and gluons) and relate this information to nucleon characteristics Imaging Measuring the correlations of position, momentum, spin, density: map the relationship between the parton state and the nucleon state. EIC Science-INT Symposium 2018 21

QCD at Extremes: Parton Saturation HERA discovered a dramatic rise in the number of gluons carrying a small fractional longitudinal momentum of the proton (i.e. small-x). This cannot go on forever as x becomes smaller and smaller: parton recombination must balance parton splitting. i.e. Saturation unobserved at HERA for a proton. (expected at extreme low x) In nuclei, the interaction probability enhanced by A ⅓ Will nuclei saturate faster as color leaks out of nucleons? EIC Science-INT Symposium 2018 22

Femtostructure vs. Nanostructure nanometers Highly relativistic Highly quantum mechanical Strongly coupled femtometers Unlike any other dynamical system we have studied. EIC Science-INT Symposium 2018 23

Modern Technology We live in a world that would have been unimaginable 100 years ago EIC Science-INT Symposium 2018 24

But 100 years ago William Henry Bragg (ca. 1915) We learned to map atoms inside matter using x-ray crystallography. This is where it all begins. The deep knowledge of atomic structures and electromagnetism is the basis of today s technology. Atomic- or nanotechnology. EIC Science-INT Symposium 2018 25

Limits of Nanotechnology: Atoms Microelectronics improve with reduction of the feature size We are now down to 10 nanometers. (about 100 atoms wide). Progress becomes more and more difficult. 2015 International Technology Roadmap for Semiconductors Can we go smaller? EIC Science-INT Symposium 2018 26

Structure of Matter Nanoworld (scale ~10-9 meters) A million times smaller Can we manipulate quarks and gluons? Femtoworld (scale ~10-15 meters) We have known for half a century that quarks (and gluons) and their interactions make up 99% of mass in the visible universe.. however.. no way to map quarks and gluons in the nucleus.. till now! EIC Science-INT Symposium 2018 27

Extra EIC Science-INT Symposium 2018 28

EIC Science: 3. Energy into Matter Investigate how energy turns into matter by using cold QCD matter as a detector Hadron Formation Color Neutralization Apply what is learned to HI EIC can scan through different configurations by changing the energy transfer. Understand, for the first time, time scales of hadronization. EIC Science-INT Symposium 2018 29