Strategy for Nuclear Physics Scope and Range of Physics Current Projects Future Projects Other issues Balance of Programme, Theory.

Slides:



Advertisements
Similar presentations
Update from NSAC NuPECC Long Range Planning Meeting Susan J. Seestrom NSAC Chair U.S. Department of Energy Office of Science.
Advertisements

The Physics of Nuclei, Nuclear Matter and Nucleosynthesis Report of the Nuclear Physics Advisory Panel.
Supported by DOE 11/22/2011 QGP viscosity at RHIC and LHC energies 1 Huichao Song 宋慧超 Seminar at the Interdisciplinary Center for Theoretical Study, USTC.
What is QCD? Quantum ChromoDynamics is the theory of the strong force –the strong force describes the binding of quarks by gluons to make particles such.
Electromagnetic Force QED Strong Force QCD Gravitational Force General Relativity galaxy m matter m crystal m atom m atomic nucleus.
The Phase Diagram of Nuclear Matter Oumarou Njoya.
University of Surrey Nuclear Physics Research Group Nuclear theory group (2 Professors (Al-Khalili & Tostevin) ; 2 Senior Lecturers (Stevenson & Barbieri),
GSI and FAIR - EPICS status report - Peter Zumbruch Experiment control systems group GSI (KS/EE)
LRP- WG3 Nuclear structure and dynamics NuPECC Liaisons: Angela Bracco, Maria Borge Convener: Rauno Julin Navin Alahari Thomas Aumann Yorick Blumenfeld.
NSAC Long Range Plan Report Donald Geesaman Argonne National Laboratory Chair, US Department of Energy/National Science Foundation Nuclear Science Advisory.
Age, Evolution, and Size of the Cosmos Szydagis and Lunin.
Early Universe Chapter 38. Reminders Complete last Mallard-based reading quiz before class on Thursday (Ch 39). I will be sending out last weekly reflection.
The Science of an EIC Nuclear Science Goals: How do we understand the visible matter in our universe in terms of the fundamental quarks and gluons of QCD?
24/04/2007ALICE – Masterclass Presentation1 ALICE Hannah Scott University of Birmingham.
Smashing the Standard Model: Physics at the CERN LHC
EJB April 2006 Nuclear Science: The Mission Understand the origin, evolution, and structure of the baryonic matter of the Universe Cosmic accelerationRotation.
Modern Physics LECTURE II.
Introduction to Radiochemistry NUSC Forces in Matter and the Subatomic Particles Chapter 1.
Opportunities for low energy nuclear physics with rare isotope beam 현창호 대구대학교 과학교육학부 2008 년 11 월 14 일 APCTP.
Electron-Ion Collider and the NSAC Long Range Plan Robert Tribble December 7, 2007 Texas A&M University.
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
quarks three families Standard - Theory III II I.
Christina Markert Physics Workshop UT Austin November Christina Markert The ‘Little Bang in the Laboratory’ – Accelorator Physics. Big Bang Quarks.
Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion.
Discovery of the Higgs Boson Gavin Lawes Department of Physics and Astronomy.
Long Range Plan (LRP) & EDM Nuclear Physics LRP is prepared every 5- 6 years Provides guidance to funding agencies w.r.t. scientific and funding priorities.
My Chapter 30 Lecture.
Atomic Structure Basic and Beyond. What are the 3 major parts of an atom? Protons Electrons Neutrons.
Standard Model A Brief Description by Shahnoor Habib.
Subatomic Physics Chapter Properties of the Nucleus The nucleus is the small, dense core of an atom. Atoms that have the same atomic number but.
The Big Bang!. “To make an apple pie from scratch, you must first invent the universe” Carl Sagan 1980.
Quarks, Leptons and the Big Bang particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
06-20,2005UH Teacher Workshop What’s New in Nu-clear Physics Ed V Hungerford University of Houston According to Pogo: “Nuclear Physics is not so new, and.
What is Higgs theory anyway? The search for the Higgs boson was the top priority in Particle Physics for years – but why? The 'Standard Model' describes.
Recreating the Big Bang with the World’s Largest Machine Prof Peter Watkins Head of Particle Physics Group The University of Birmingham Admissions Talk.
Today: “Nucleosynthesis… another phase change in early universe… and why is the Universe so Flat?” HW for next time: Onion, “the nucleus and forces of.
Axel Drees, Stony Brook University, Lectures at Trento June 16-20, 2008 Electromagnetic Radiation form High Energy Heavy Ion Collisions I.Lecture:Study.
High Energy Nuclear Physics and the Nature of Matter Outstanding questions about strongly interacting matter: How does matter behave at very high temperature.
Chiral phase transition and chemical freeze out Chiral phase transition and chemical freeze out.
Particles and how they interact
General Discussion some general remarks some questions.
Chapter 17 The Beginning of Time. Running the Expansion Backward Temperature of the Universe from the Big Bang to the present (10 10 years ~ 3 x
The FAIR* Project *Facility for Antiproton and Ion Research Outline:  FAIR layout  Research programs Peter Senger, GSI USTC Hefei Nov. 21, 2006 and CCNU.
Anthropology Series In the Beginning How did the Universe begin? Don’t know!
Inorganic Chemistry May 12, Describe how the strong force attracts nucleons Relate binding energy and mass defect Predict the stability of a nucleus.
UK Research in Nuclear Physics P J Nolan University of Liverpool.
SYNTHESIS The Standard Model 1.Elementary particles 2.Strong nuclear force 3.Weak nuclear force 4.The Standard Model.
What is the Standard Model of Particle Physics ???? 1. A theory of three of the four known fundamental interactions and the elementary particles that.
PPAN perspective and the Science Roadmap Jordan Nash PPAN Chair.
Quark Gluon Plasma Presented by: Rick Ueno Welcome to the presentation of:
Axel Drees, University Stony Brook, PHY 551 S2003 Heavy Ion Physics at Collider Energies I.Introduction to heavy ion physics II.Experimental approach and.
The outlook for Nuclear Theory Niels Walet School of Physics and Astronomy University of Manchester.
Standard Model of Particle Physics
Nuclear Physics -- Today and Tomorrow From the infinitely strong –
Elemental Composition of the Universe
CHAPTER 12 The Atomic Nucleus
What do you know about the Big Bang Theory? List anything 
Unit 11 - Nuclear Chemistry
The Beginning of Time (Birth Of The Universe)
Chapter 13 Nuclear Chemistry.
Unit 13 Nuclear Chemistry.
Unit 11 - Nuclear Chemistry
SPH4U Elementary Particles.
Early Universe.
Lecture 2: The First Second origin of neutrons and protons
Atomic Structure Basic and Beyond.
Atomic Structure Basic and Beyond.
Physics 4 – April 18, 2019 Agenda:
Particle Physics and The Standard Model
Presentation transcript:

Strategy for Nuclear Physics Scope and Range of Physics Current Projects Future Projects Other issues Balance of Programme, Theory

Nuclear Structure Advisory Committee (NSAC) Dec [US] Organisation for Economic Co-operation and Development (OECD) May 2008 [World] NuPECC 2004 [EU] Context:

Nuclear Structure Advisory Committee (NSAC) Dec [US] Organisation for Economic Co-operation and Development (OECD) May 2008 [World] Quantum Chromodynamics What are the phases of strongly interacting matter, and what roles do they play in the cosmos? What is the internal landscape of the nucleons? What does QCD predict for the properties of strongly interacting matter? What governs the transition of quarks and gluons into pions and nucleons? What is the role of gluons and gluon self-interactions in nucleons and nuclei? What determines the key features of QCD, and what is their relation to the nature of gravity and spacetime? Nuclei and Nuclear Astrophysics What is the nature of the nuclear force that binds protons and neutrons into stable nuclei and rare isotopes? What is the origin of simple patterns in complex nuclei? What is the nature of neutron stars and dense nuclear matter? What is the origin of the elements in the cosmos? What are the nuclear reactions that drive stars and stellar explosions? Fundamental Symmetries and Neutrinos What is the nature of the neutrinos, what are their masses, and how have they shaped the evolution of the universe? Why is there now more visible matter than antimatter in the universe? What are the unseen forces that were present at the dawn of the universe but disappeared from view as the universe evolved? Is QCD the complete theory of the strong interaction? What are the phases of nuclear matter? What is the structure of nuclear matter? What is the role of nuclei in shaping the evolution of the universe? What physics is there beyond the Standard Model?

Nuclear Physics Forum:  How do the properties of atomic nuclei emerge from the forces between the nucleons?  What is the origin of the chemical elements?  What is the nature of strongly interacting matter?

What is the Nature of Nuclear Matter? What are the limits of nuclear existence? How does the ordering of quantum states change in dilute or neutron-rich matter? Are there new forms of nuclear matter in very loosely bound systems and beyond the limits of stability? How do simple patterns arise in complex nuclei? Are there new symmetries describing nuclei far from stability? Can nuclei be described in terms our understanding of the strong interaction? What is the equation-of-state of nuclear matter? Is QCD the Complete Theory of the Strong Interaction? What is the nature of the quark-quark interaction? What is the structure of the proton and neutron? How do the neutron and proton get their spin? What are the phases of strongly interacting matter? What was the nature of matter an instant after the Big Bang? How do quarks and gluons transform into baryons? What is the Origin of the Elements? How are the elements and isotopes found in the Universe formed? Where is the site of the r-process of nuclear synthesis? What is the nuclear equation-of-state for neutron stars?

1) Nuclear (not nucleon) Physics is seen as incremental, study of trends, building up systematics evolving theory. Not answering big questions. Not really understood the questions we are asking. PPAN Perception Issues: 2) Nucleon (not nuclear) Physics is seen as picking up old particle physics, tackling issues which particle physics left behind as too complex or less interesting. 3) Link between Facilities, Projects and Physics: Not easy for them to say “at FAIR we will discover X” as “at ATLAS we will discover the Higgs” 4) Impact of a small group of scientists (~60) / criticality of field.

A Possible Strategy…………………. Fundamental Symmetries and Neutrinos What is the nature of the neutrinos, what are their masses, and how have they shaped the evolution of the universe? Why is there now more visible matter than antimatter in the universe? What are the unseen forces that were present at the dawn of the universe but disappeared from view as the universe evolved? A Physics Programme Based on developing areas of present expertise Not: Rationale: In UK particle physics community have already stolen a march, NP community limited numbers not realistic to lead such endeavours.

A Possible Strategy…………………. A. Richter INPC 2004 Building an understanding of the nucleon: QCD o nucleon spin and moments o meson and baryon resonances o Quark Gluon Plasma o Temperature – density phase diagram o Freeze out of the QGP: from “plasma” to baryons Effective Field Theory

A Possible Strategy………………….

A Possible Strategy: Nuclear Astrophysics

What is the Nature of Nuclear Matter? Is QCD the Complete Theory of the Strong Interaction? What is the Origin of the Elements? A Possible Strategy………………….

What is the Nature of Nuclear Matter? What are the limits of nuclear existence? How does the ordering of quantum states change in dilute or neutron-rich matter? Are there new forms of nuclear matter in very loosely bound systems and beyond the limits of stability? How do simple patterns arise in complex nuclei? Are there new symmetries describing nuclei far from stability? Can nuclei be described in terms our understanding of the strong interaction? What is the equation-of-state of nuclear matter? Is QCD the Complete Theory of the Strong Interaction? What is the nature of the quark-quark interaction? What is the structure of the proton and neutron? How do the neutron and proton get their spin? What are the phases of strongly interacting matter? What was the nature of matter an instant after the Big Bang? How do quarks and gluons transform into baryons? What is the Origin of the Elements? How are the elements and isotopes found in the Universe formed? Where is the site of the r-process of nuclear synthesis? What is the nuclear equation-of-state for neutron stars?

Connecting Physics, Facility and Projects

Projects Timelines ~1/3 of Nuclear Physics funding is project based (NUSTAR, AGATA, PANDA) Is profile right? Is balance of programme right? Are travel grants a good thing? Financial Year

What can we do to support theory? Other Strategic Issues How to include Applied Nuclear Science in the Strategy? What to input into the Review? Student Destinations (124) PDRA Destinations (58) Permanent

Birmingham Masters (PTNR) (2 years) [62 students]