PHY313 - CEI544 The Mystery of Matter From Quarks to the Cosmos Fall 2005

Size: px
Start display at page:

Download "PHY313 - CEI544 The Mystery of Matter From Quarks to the Cosmos Fall 2005"

Transcription

1 PHY313 - CEI544 The Mystery of Matter From Quarks to the Cosmos Fall 2005 Peter Paul Office Physics D PHY313 Peter Paul 10/20/05 PHY313-CEI544 Fall-05 1

2 What have we learned last time I The elements up to the tightest bound one, 56 Fe, are formed during the burning process in the star as it uses its primordial fuel, 75% hydrogen (protons) and 25% Helium. In the first step the star burns four protons into 4 He. Once sufficed 4 He is produced, 3 4 He will combine to yield 12 C. This process produces more heat. In the next step the star uses 12 C and the available hydrogen to go through the CNO cycle which produces the elements between 12 C and 16 O. This heats the star up further. One there is sufficient 16 O around the star will produce still heavier elements by using available H and 4 He to fuse with the 16 O. The process continues until the elements that are produced reach the peak of the nuclear binding energy, at Fe/Ni. Then the star cools (Red Giant). Gravitation compresses the star. The heaviest elements accumulate at the core in layers of density. Compression reheats the star. It explodes as a Supernova. Nuclear reactions occurring during this violent phase produce many neutrons. These are rapidly captured into the Fe/Ni core to produce the heavier nuclei (rprocess). Beta decay changing n p inside the nuclei moves the neutronrich nuclei toward the valley of stability. The final explosive phase spews these heavy elements into the interstellar medium. There they are incorporated into new stellar objects Peter Paul 10/20/05 PHY313-CEI544 Fall-05 2

3 What have we learned last time II The known zoo of strongly interacting particles (hadrons) was found divided into very heavy particles (Baryons) and medium heavy particles (Mesons). It became clear from the formation and decay of these particles that several hidden quantum numbers must play a role, in addition to the conservation of electric charge, such as S and B. Strangeness S and Baryon number B are always conserved in reactions that involve the strong interaction. A concept of elemental building blocks, called up, down and strange quarks, u,d,s, could explain all properties of the construction of the observed hadrons. The quarks have electric changes in units of 1/3 of the electron charge, Baryon number 1/3. and spin 1/2. All known Baryons could be constructed combining 3 quarks; all Mesons could be constructed with pairs of one quark and an anti-quark. The discovery of the predicted Ω particle, a combination of 3 s quarks, showed that there was reality behind the quark concept. Later, three heavier quarks, the charm, top and bottom quarks were discovered. The total of 6 quarks and 6 antiquarks can be grouped into three families. Quarks are bound to each other by a force that becomes stronger as the quarks are pulled apart (Confinement). Peter Paul 10/20/05 PHY313-CEI544 Fall-05 3

4 The three quark families Today we know 3 families of quarks, and 3 antiquark families. Spin Charge First family Second family Third family 1/2 +2/3 up charm top (3 MeV) (1300 MeV) (175,000 MeV) 1/2-1/3 down strange bottom (6 MeV) (100 MeV) (4,300 MeV) Note that the neutron and proton and the light mesons are all build up of the lightest quarks, the u and d quarks (and their anti-quarks in the meson case). The strange particles contain the s-quark which is much heavier Peter Paul 10/20/05 PHY313-CEI544 Fall-05 4

5 Reminder: Particles from quarks Mesons are made from quarks and anti-quarks u and anti-d = π+ d and anti-up = π- u and anti-s = K+ and so on, making hundreds of particles. Baryons are made from 3 quarks uud = proton udd = neutron uds = lambda (Λ) and so on, making hundreds of baryons Note: Anti-quarks have the opposite charge of the quarks Peter Paul 10/20/05 PHY313-CEI544 Fall-05 5

6 Quark Confinement (Repeat) The interaction between quarks binds them such that no single quark can ever be free. This is different from two charged bodies bound by the Coulomb force, which becomes weaker as the charges are separated It is similar to the binding of a magnetic northpole and a south-pole. Thus any quark that emerges from a proton will dress itself with other quarks or anti-quarks and emerge as a jet. The binding force between quarks is weak when they are close together but grows stronger as they are pulled apart. At close distances they can almost be treated as free: Asymptotic freedom Peter Paul 10/20/05 PHY313-CEI544 Fall-05 6

7 Peter Paul 10/20/05 PHY313-CEI544 Fall-05 7

8 Color in the Strong Interaction Some particles are made up of 3 identical quarks, like the Ω-: s s s This contradicts Pauli Principle because two would have the same QN. Therefore, in addition to their regular quantum properties, like spin and electric charge, quarks must have another property that differentiates them from each other. This property is called Color. There are 3 colors : Red, Green and Blue (these are just stand-in names). Thus the proton could look like this uud or any other color combination. A particle in the real world, like a proton (u-u-d) cannot show any color. It must appear white, i.e. it must be made of quark combinations that contain all 3 colors equally. The colored Quarks interact with each other through the exchange of gluons, which exchange color between the quarks (Color interaction). The Theory that describes the Color interaction iscalled Quantum Chromo Dynamics (QCD) Peter Paul 10/20/05 PHY313-CEI544 Fall-05 8

9 The Force Carriers of the Strong Interaction The Strong Interaction involves the exchange of gluons The Gluons, which are mass less, exchange color between quarks There are 9 color-anti-color combinations, but only 8 quarks, since the 9 th combination contains all colors and thus is white. greenanti-green redanti-red blueanti-blue greenanti-red redanti-blue blueanti-red greenanti-blue redanti-green blueanti-green Peter Paul 10/20/05 PHY313-CEI544 Fall-05 9

10 Can we ever set quarks free? Setting a quark free means breaking the connection to its partner quarks. This cannot happen in free space, but it could happen in a medium. This is analogous to the situation in Water: In ice the molecules are strictly bound and ordered into a crystal. Even in liquid form the molecules feel an interaction between each other. Only when we evaporate the water are the molecules free. Can we evaporate quark matter? Peter Paul 10/20/05 PHY313-CEI544 Fall-05 10

11 Example: The Phases of Water As water changes from Ice to Vapor, the binding between molecules is first weakened, then broken Peter Paul 10/20/05 PHY313-CEI544 Fall-05 11

12 Evolution of the Universe ~ 10 µs after Big Bang T = K (~ 170 MeV) T = 10 9 K Hadron Synthesis strong force binds quarks and gluons in massive objects: p & n; mass ~ 1 GeV ~ 100 s after Big Bang Nucleon Synthesis strong force binds protons and neutrons into nuclei QCD: Quantum Chromo Dynamics Two puzzles: Confinement & Chiral Symmetry Can we undo confinement? Unbound quark ~1 MeV (Higgs mass) Constituent quarks ~ 300 MeV Peter Paul 10/20/05 PHY313-CEI544 Fall-05 12

13 Explore QCD (Nuclear) Matter at High Temperature and Density nuclear matter p, n density or temperature Quark-Gluon Plasma q, g QCD potential: in vacuum: linear increase with distance from color charge strong attractive force confinement of quarks to hadrons : baryons (qqq) and mesons (qq-bar) in dense and hot matter screening of color charges; Debye screening potential vanishes for large distance deconfinement of quarks QGP Peter Paul 10/20/05 PHY313-CEI544 Fall-05 13

14 QCD predictions for the Phase Transition Results from lattice QCD establish the QCD phase transition and chiral symmetry transition. Karsch, Laermann, Peikert (99) ε C = 0.6 GeV/fm 3 T C ~ 170 MeV jump in energy density predicted at: T C ~ 170 MeV ε C = 0.6 GeV/fm 3 T ~ 220 MeV ε = 3.5 GeV/fm 3 Peter Paul 10/20/05 PHY313-CEI544 Fall-05 14

15 Phase Diagram for Quark Matter Phase transition temperature T = 170 MeV ~ Kelvin Peter Paul 10/20/05 PHY313-CEI544 Fall-05 15

16 Use energetic Gold collisions to. Create nuclear matter in the combined volume of the 2 Gold ions (2x 200 nucleons!) to create the medium in which quarks could be deconfined. Bring in enough energy to compress the nuclear matter and to heat it to several 100 MeV in temperature. In the parlance of the scientists: Create QGP as transient state in heavy ion collisions up to 400 nucleons in close proximity verify experimentally existence of QGP study QCD confinement of quarks to hadrons study how hadrons get their masses Retrace spontaneous breaking of chiral symmetry Turn free quarks ( ~ 5 MeV for u,d ) into constituent quarks ( ~ 300 MeV for u,d) Peter Paul 10/20/05 PHY313-CEI544 Fall-05 16

17 Schematic View of a Heavy Ion Collision projectile J/ψ p several 1000 particles produced in central collision π π b ~ 0 cc Κ π π π target p e e + hadrons π, K, p -lots, produced late when particles stop to interact (freezeout) thermal equilibrium and collective behavior ( flow ) strangeness equilibration Correlated systems from dense system(j/ψ, Jets) electro-magnetic radiation γ, e + e, µ + µ -few, emitted any time ; black body radiation π π Peter Paul 10/20/05 PHY313-CEI544 Fall-05 17

18 Violent collisions produce lots of particles Amazingly, these particles can all be recorded simultaneously Peter Paul 10/20/05 PHY313-CEI544 Fall-05 18

19 The Relativistic Heavy Ion Collider at BNL Peter Paul 10/20/05 PHY313-CEI544 Fall-05 19

20 Gold Ion Collisions in RHIC PHOBOS 10:00 o clock High Int. Proton Source Pol. Proton Source PHENIX 8:00 o clock LINAC BAF (NASA) BOOSTER µ g-2 12:00 o clock RHIC STAR 6:00 o clock U-line AGS 9 GeV/u Q = +79 HEP/NP 4:00 o clock BRAHMS 2:00 o clock Six collision regions Four detectors Design Parameters: Beam Energy = 100 GeV/u No. Bunches = 57 No. Ions /Bunch = T store = 10 hours L ave = cm -2 sec -1 1 MeV/u Q = +32 TANDEMS Peter Paul 10/20/05 PHY313-CEI544 Fall-05 20

21 Basic Principle of Acceleration: Use Electric Force Voltage - Two charged particles electrons Battery + Voltage In ~1920 s Cockcroft and Walton invented the first particle accelerator: The electrostatic accelerator. It uses the fact that bodies with electric charges interact with each other: They feel a force. 1. Equally charged particles repel each other, 2. Oppositely charged particles attract each other. Peter Paul 10/20/05 PHY313-CEI544 Fall-05 21

22 Acceleration with DC or AC Electric Fields Acceleration is done by the Coulomb force acting on the positive or negative charge of the accelerated particle. Acceleration principle is very simple: E= q V where q = n x e. V can be a positive or negative voltage. Typical voltages can be 1 MV/m or even 70 MV/m Acceleration in a DC field produces a steady beam. Acceleration in an AC or rf field produces bunches of accelerated particles. Particle beam Peter Paul 10/20/05 PHY313-CEI544 Fall-05 22

23 The Van de Graaf Accelerator Van de Graaf invented a simple electrostatic aacacelerator: It was the first accelerator to reach large energies by the use of very high voltages. It uses an insulated conveyor belt to shuffle positive (or negative) charges into an insulated dome. This builds up voltage as high as 20 Million Volts (20 MV). If the dome is positively charged, protons will be accelerated downward; if the dome is negatively charged, electrons can be accelerated downward. Today thousands of these accelerators from a few 100 kv to 20 MV are used all over the world. Positive Protons accelerated downward Peter Paul 10/20/05 PHY313-CEI544 Fall-05 23

24 Modern Tandem at Oak Ridge Peter Paul 10/20/05 PHY313-CEI544 Fall-05 24

25 Circular Accelerators: The Cyclotron The Cyclotron was invented at Berkeley in the 1930 s by E. Lawrence. It runs particle bunches in circles many time through the same electric field. The electric field is timed so that each time a bunch enters into one of two gaps, it gets an accelerating kick. This requires a resonance condition between the path of the beam bunch and the accelerating wave. Peter Paul 10/20/05 PHY313-CEI544 Fall-05 25

26 The latest stage: Sector focusing superconducting cyclotrons Peter Paul 10/20/05 PHY313-CEI544 Fall-05 26

27 Synchrotrons One can cut out the center of the cyclotron magnet if the particles can be made to stay on a fixed orbit as they get accelerated. This requires that the Magnetic Field be increased linearly with the velocity gain of the beam during acceleration. Removing the center part of the magnet eliminates huge amount of weight and cost for steel. Most modern particle accelerators are synchrotrons. Extracted beam Circling beam RF voltage Peter Paul 10/20/05 PHY313-CEI544 Fall-05 27

28 Beam deflection in magnets Lorentz Force F L = qbv A magnetic field deflects but does not accelerate. The force acts perpendicular to the direction of flight. It bends a charge beam. The bending power is directly proportional to the magnetic field strength B This can be used in particle accelerators to bend and/or focus beams It is also used to deflect beams in detectors Peter Paul 10/20/05 PHY313-CEI544 Fall-05 28

29 Electrostatic fields and beam focusing Electric fields widely used for beam focusing (TV picture tubes!), similar to the use of lenses for light focusing. Charged particles follow trajectories that are perpendicular to the line of equal voltage It is weak focusing because one cannot achieve very high electric DC fields: ~ 1 MV/m Peter Paul 10/20/05 PHY313-CEI544 Fall-05 29

30 Strong focusing with magnetic quadrupoles Magnetic quadrupole lens focuses in one direction but defocuses in the other. However, a sequence of two lenses with a drift space in between has a net focus on two dimensions Focusing strength of a single lens is proportional to the magnetic field f = p qbl = x f y X-focusing Y-focusing Peter Paul 10/20/05 PHY313-CEI544 Fall-05 30

31 Strong focusing of particle beams Magnetic Quadrupole fields have a strong focusing action. They are the work horse of all modern machines. A single quadrupole focuses in one direction, defocuses in the orthogonal direction. Thus two lenses must always be paired Strongest lenses can be made with superconductors and with very mall dimensions Beam system for CEBAF accelerator Peter Paul 10/20/05 PHY313-CEI544 Fall-05 31

32 Radiofrequency waves E z c z Electromagnetic waves are electromagnetic fields that change with time. They can travel in free space or in resonator cavities that contain them. E z ct = λ 2 c c A charged particle can ride on this wave like a surfer, either at the peak or a little in front of it. Staying a bit ahead of the wave is more stable. z Peter Paul 10/20/05 PHY313-CEI544 Fall-05 32

33 The skill of the Surfer By staying ahead of the peak of the wave the surfer makes sure he does not fall off the wave backwards. He cannot fall forward since the wave will catch up with him. The stability of his position requires that his/her speed is matched to the speed of the wave. The same synchronization condition applies to the particle beam (=surfer) and the electromagnetic wave. In free space the EM wave would travel with the speed of light. But in a resonator cavity it can be slowed down to match the changing speed of the particle beam. Peter Paul 10/20/05 PHY313-CEI544 Fall-05 33

34 Linear accelerators Resonators filled with such traveling waves are used in linear Accelerators. The particle bunches travel on a linear path through a series of resonators, being pushed forward in each resonator. Linear accelerators are used for very high particle currents, e.g. in neutron spallation sources They are the basis for the most modern proposed accelerator, the International Linear Collider (ILC). RF power supply Particle beam Resonators Peter Paul 10/20/05 PHY313-CEI544 Fall-05 34

35 Superconducting resonators made from Nb have achieved the highest quality and highest electric field. Superconducting resonators Since electric currents experience almost no resistive losses in superconducting materials, such cavities can achieve large accelerating fields with little electric power. The preparation of these resonators requires ultimate cleanliness and surface smoothness Peter Paul 10/20/05 PHY313-CEI544 Fall-05 35

36 Particle Colliders When a beam has been accelerated in a synchrotron ring, it can be stored and let to coast for many hours. The beams of 2 rings can then be crossed and made to collide If both beams have the same energy the collision of 2 particles, one from each ring, brings them to a stop. This is a very efficient transformation of beam energy into reaction energy (or heat of the reaction zone). All modern HEP accelerators are colliders. Look at for more information The Large Hadron Collider (LHC) at CERN carries two beams in one magnet ring and collides them in 4 crossings. It will begin operation in Peter Paul 10/20/05 PHY313-CEI544 Fall-05 36

37 Energy Frontier of Colliders LHC at CERN, E cm = 14 TeV Peter Paul 10/20/05 PHY313-CEI544 Fall-05 37

38 Gold Ion Collisions in RHIC PHOBOS 10:00 o clock High Int. Proton Source Pol. Proton Source PHENIX 8:00 o clock LINAC BAF (NASA) BOOSTER µ g-2 12:00 o clock RHIC STAR 6:00 o clock U-line AGS 9 GeV/u Q = +79 HEP/NP 4:00 o clock BRAHMS 2:00 o clock Six collision regions Four detectors Design Parameters: Beam Energy = 100 GeV/u No. Bunches = 57 No. Ions /Bunch = T store = 10 hours L ave = cm -2 sec -1 1 MeV/u Q = +32 TANDEMS Peter Paul 10/20/05 PHY313-CEI544 Fall-05 38

39 RHIC Pictures (1) Blue and yellow rings Injection arcs to blue and yellow rings Peter Paul 10/20/05 PHY313-CEI544 Fall-05 39

40 RHIC Pictures (2) Rf storage cavities Installation of final focussing triplets Peter Paul 10/20/05 PHY313-CEI544 Fall-05 40

41 Bringing beams precisely into collision Beam in blue ring Beam in yellow ring 200 ns (60 m) Beams in collision at the interaction regions 200 ns (60 m) Peter Paul 10/20/05 PHY313-CEI544 Fall-05 41

42 Stored beams in a Collider (RHIC) Coll. rate / Blue Ions / Yellow Ions [Hz/10 18 ] Beams in a collider die because of scattering of the particles within each bunch and the scattering of the bunches with rest gas in the beam pipe Peter Paul 10/20/05 PHY313-CEI544 Fall-05 42

43 The PHENIX Detector at RHIC This detector surrounds the collision point and tracks all particles coming from the center. It can track several thousand particles simultaneously and identify their energy and charge. A good fraction of it was built by students at Stony Brook. Peter Paul 10/20/05 PHY313-CEI544 Fall-05 43

44 East carriage Installation of PHENIX Drift Chambers West carriage and Magnet in IR Drift chamber + Pad chamber 1 Peter Paul 10/20/05 PHY313-CEI544 Fall-05 44

45 Detection of charged particles Charged particlesnize gases. The degree of ionization depends on the charge of the particle and its velocity. The particle ionizes throughout its path, but most heavily at the end of its path. The ionization products than be deflected by an electric or a magnetic field toward sensors Such detectors are wire chambers or time projection chambers (TPC). Bragg Curve of an Iron beam Peter Paul 10/20/05 PHY313-CEI544 Fall-05 45

46 Operation of gas drift chamber Peter Paul 10/20/05 PHY313-CEI544 Fall-05 46

47 Combined Identification of different particle species Tracking Beam-Beam Counter Time-of-Flight array provides excellent hadron identification over broad momentum band: Peter Paul 10/20/05 PHY313-CEI544 Fall-05 47

48 The Power of Modern Tracking Peter Paul 10/20/05 PHY313-CEI544 Fall-05 48

49 The STAR TPC Detector Peter Paul 10/20/05 PHY313-CEI544 Fall-05 49

50 First events in STAR: Big Time Projection Chamber First Events June first Au-Au collisions at STAR June 12 Brookhaven Science Associates U.S. Department of Energy 44 Peter Paul 10/20/05 PHY313-CEI544 Fall-05 50

51 Detention of Gamma rays Gamma rays can be detected with very high efficiency and resolution by use of semiconductor detectors, such as Germanium crystals. Peter Paul 10/20/05 PHY313-CEI544 Fall-05 51

52 Seventh Homework, due Oct. 27, The Lambda particle has a mass of about 1,200 MeV/c2 and zero electric charge. It behaves strangely. 1. Is it a Baryon or a Lepton: Explain your answer. 2. What combination of quarks does it contain. 2. Describe how one attempts to free up (deconfine) individual quarks and what temperatures are required to achieve that goal. 3. How long after the initial Big Bang did the quarks freeze into nucleons and mesons? 4. What force is used to accelerate charged particles? Can we build accelerators for both negatively charged particles (electrons) and for positively charge particles (protons)? 5. Describe the principle of a Synchrotron and explain the basis for its name. 6. How do we detect charged particles is used to detected them and measure their charge and velocity? Peter Paul 10/20/05 PHY313-CEI544 Fall-05 52

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

High Energy Frontier Recent Results from the LHC: Heavy Ions I High Energy Frontier Recent Results from the LHC: Heavy Ions I Ralf Averbeck ExtreMe Matter Institute EMMI and Research Division GSI Helmholtzzentrum für Schwerionenforschung Darmstadt, Germany Winter

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

Short Introduction to CLIC and CTF3, Technologies for Future Linear Colliders

Short Introduction to CLIC and CTF3, Technologies for Future Linear Colliders Short Introduction to CLIC and CTF3, Technologies for Future Linear Colliders Explanation of the Basic Principles and Goals Visit to the CTF3 Installation Roger Ruber Collider History p p hadron collider

More information

Why do we accelerate particles?

Why do we accelerate particles? Why do we accelerate particles? (1) To take existing objects apart 1803 J. Dalton s indivisible atom atoms of one element can combine with atoms of other element to make compounds, e.g. water is made of

More information

Little bang.. On earth experiments emulating time between second after the BIG_Bang. PartI : actors (particles) Tools (accelerators)

Little bang.. On earth experiments emulating time between second after the BIG_Bang. PartI : actors (particles) Tools (accelerators) Little bang.. On earth experiments emulating time between 0.001-1 second after the BIG_Bang PartI : actors (particles) Tools (accelerators) Can we restore creation of matter in experiments on Earth? Structure

More information

Particle physics experiments

Particle physics experiments Particle physics experiments Particle physics experiments: collide particles to produce new particles reveal their internal structure and laws of their interactions by observing regularities, measuring

More information

Section 4 : Accelerators

Section 4 : Accelerators Section 4 : Accelerators In addition to their critical role in the evolution of nuclear science, nuclear particle accelerators have become an essential tool in both industry and medicine. Table 4.1 summarizes

More information

The Origin of the Visible Mass in the Universe

The Origin of the Visible Mass in the Universe The Origin of the Visible Mass in the Universe Or: Why the Vacuum is not Empty Ralf Rapp Cyclotron Institute + Physics Department Texas A&M University College Station, USA Cyclotron REU Program 2007 Texas

More information

Modern Accelerators for High Energy Physics

Modern Accelerators for High Energy Physics Modern Accelerators for High Energy Physics 1. Types of collider beams 2. The Tevatron 3. HERA electron proton collider 4. The physics from colliders 5. Large Hadron Collider 6. Electron Colliders A.V.

More information

QGP event at STAR. Patrick Scott

QGP event at STAR. Patrick Scott QGP event at STAR Patrick Scott Overview What is quark-gluon plasma? Why do we want to study quark-gluon plasma? How do we create quark-gluon plasma? The past and present SPS and RHIC The future LHC and

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

Particles and Universe: Particle accelerators

Particles and Universe: Particle accelerators Particles and Universe: Particle accelerators Maria Krawczyk, Aleksander Filip Żarnecki March 24, 2015 M.Krawczyk, A.F.Żarnecki Particles and Universe 4 March 24, 2015 1 / 37 Lecture 4 1 Introduction 2

More information

PHY397K - NUCLEAR PHYSICS - 2

PHY397K - NUCLEAR PHYSICS - 2 PHY397K - NUCLEAR PHYSICS - 2 PHY397K - NUCLEAR PHYSICS Spring 2015, Unique numbers: 57115 RLM 5.116, TTH 12:30-2:00 pm Christina Markert Office: RLM: 10.305 Phone: 512 471 8834 Email: cmarkert@physics.utexas.edu

More information

Big Bang to Little Bang ---- Study of Quark-Gluon Plasma. Tapan Nayak July 5, 2013

Big Bang to Little Bang ---- Study of Quark-Gluon Plasma. Tapan Nayak July 5, 2013 Big Bang to Little Bang ---- Study of Quark-Gluon Plasma Tapan Nayak July 5, 2013 Universe was born through a massive explosion At that moment, all the matter was compressed into a space billions of times

More information

Direct-Current Accelerator

Direct-Current Accelerator Nuclear Science A Teacher s Guide to the Nuclear Science Wall Chart 1998 Contemporary Physics Education Project (CPEP) Chapter 11 Accelerators One of the most important tools of nuclear science is the

More information

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

The Secret of Mass. Can we Evaporate the Vacuum at RHIC? : Can we Evaporate the Vacuum at RHIC? Texas A&M University February 24, 2007 Outline The Beauty of Nature: Symmetries The Beauty of Nature: Symmetries What is a symmetry? Geometry: Certain operations

More information

Exam Results. Force between charges. Electric field lines. Other particles and fields

Exam Results. Force between charges. Electric field lines. Other particles and fields Exam: Exam scores posted on Learn@UW No homework due next week Exam Results F D C BC B AB A Phy107 Fall 2006 1 Particles and fields We have talked about several particles Electron,, proton, neutron, quark

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

Particles and Waves Final Revision Exam Questions Part 1

Particles and Waves Final Revision Exam Questions Part 1 Particles and Waves Final Revision Exam Questions Part 1 Cover image: cutaway diagram of CERN, CERN Version 2013 P&W: Exam Questions Part 1 Version 2013 Contents Section 1: The Standard Model 1 Section

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

PARTICLE PHYSICS :Higher Level Long Questions

PARTICLE PHYSICS :Higher Level Long Questions PARTICLE PHYSICS :Higher Level Long Questions Particle Accelerators (including Cockcroft and Walton experiment) 2013 Question 10 (a) In 1932 J.D. Cockroft and E.T.S. Walton accelerated protons to energies

More information

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

Wesley Smith, U. Wisconsin, January 21, Physics 301: Introduction - 1 Wesley Smith, U. Wisconsin, January 21, 2014 Physics 301: Introduction - 1 Physics 301: Physics Today Prof. Wesley Smith, wsmith@hep.wisc.edu Undergraduate Physics Colloquium! Discussions of current research

More information

CfE Higher Physics. Particles and Waves

CfE Higher Physics. Particles and Waves Wallace Hall Academy CfE Higher Physics Particles and Waves Exam Questions Part 1 Cover image: cutaway diagram of CERN, CERN P&W: Exam Questions Part 1 Version 2013 Contents Section 1: The Standard Model

More information

At this time the quark model consisted of three particles, the properties of which are given in the table.

At this time the quark model consisted of three particles, the properties of which are given in the table. *1 In 1961 Murray Gell-Mann predicted the existence of a new particle called an omega (Ω) minus. It was subsequently discovered in 1964. At this time the quark model consisted of three particles, the properties

More information

X = Z H + N n TBE. X = d 1 Z 2 + d 2 Z d 3 + d + d 4, where d i = f (Ci, A) 75 Se 75 Br. 75 Zn. 75 Ga. 75 Kr. 75 Ge 75 As

X = Z H + N n TBE. X = d 1 Z 2 + d 2 Z d 3 + d + d 4, where d i = f (Ci, A) 75 Se 75 Br. 75 Zn. 75 Ga. 75 Kr. 75 Ge 75 As 1 Lecture 4 : Beta stability, the LD Mass Formula, and Accelerators Simplest form of LD Mass Formula TBE = C 1 A C 2 A 2/3 C 3 Z 2 /A 1/3 C 4 (N-Z) 2 /A 2 + C 6 /A 1/2 = C 1 C 2 A 1/3 C 3 Z 2 /A 4/3

More information

Particles in the Early Universe

Particles in the Early Universe Particles in the Early Universe David Morrissey Saturday Morning Physics, October 16, 2010 Using Little Stuff to Explain Big Stuff David Morrissey Saturday Morning Physics, October 16, 2010 Can we explain

More information

PHYS 3446 Lecture #15

PHYS 3446 Lecture #15 PHYS 3446 Lecture #15 Monday, Oct. 30, 2006 Dr. 1. Particle Accelerators Electro-static Accelerators Cyclotron Accelerators Synchrotron Accelerators 2. Elementary Particle Properties Forces and their relative

More information

Introduction to accelerators for teachers (Korean program) Mariusz Sapiński CERN, Beams Department August 9 th, 2012

Introduction to accelerators for teachers (Korean program) Mariusz Sapiński CERN, Beams Department August 9 th, 2012 Introduction to accelerators for teachers (Korean program) Mariusz Sapiński (mariusz.sapinski@cern.ch) CERN, Beams Department August 9 th, 2012 Definition (Britannica) Particle accelerator: A device producing

More information

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

Introduction to Particle Accelerators & CESR-C

Introduction to Particle Accelerators & CESR-C Introduction to Particle Accelerators & CESR-C Michael Billing June 7, 2006 What Are the Uses for Particle Accelerators? Medical Accelerators Create isotopes tracers for Medical Diagnostics & Biological

More information

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

Particle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry Particle Physics JJ Thompson discovered electrons in 1897 Rutherford discovered the atomic nucleus in 1911 and the proton in 1919 (idea of gold foil expt) All science is either physics or stamp collecting

More information

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

A Comparative Study of Quark-Gluon Plasma at the Core of a Neutron Star and in the Very Early Universe. Frikkie de Bruyn A Comparative Study of Quark-Gluon Plasma at the Core of a Neutron Star and in the Very Early Universe By Frikkie de Bruyn Introduction 1 Study of quark-gluon plasma fluid is of mutual Interest to both

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

Linear and circular accelerators

Linear and circular accelerators Linear and circular accelerators Ion Accelerator Physics and Technology Oliver Boine-Frankenheim, Gesellschaft für Schwerionenforschung (GSI), Darmstadt Tel. 06159 712408, O.Boine-Frankenheim@gsi.de o

More information

Looking for strange particles in ALICE. 1. Overview

Looking for strange particles in ALICE. 1. Overview Looking for strange particles in ALICE 1. Overview The exercise proposed here consists of a search for strange particles, produced from collisions at LHC and recorded by the ALICE experiment. It is 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

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

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS LSN 7-3: THE STRUCTURE OF MATTER Questions From Reading Activity? Essential Idea: It is believed that all the matter around us is made up of fundamental

More information

Heavy-Ion Physics Lecture 1: QCD and the Quark-Gluon Plasma

Heavy-Ion Physics Lecture 1: QCD and the Quark-Gluon Plasma Heavy-Ion Physics Lecture 1: QCD and the Quark-Gluon Plasma Professor David Evans The University of Birmingham Nuclear Physics Summer School Queen s University, Belfast XX th August 2017 Outline of Lectures

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

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

Fundamental Forces. Range Carrier Observed? Strength. Gravity Infinite Graviton No. Weak 10-6 Nuclear W+ W- Z Yes (1983) Fundamental Forces Force Relative Strength Range Carrier Observed? Gravity 10-39 Infinite Graviton No Weak 10-6 Nuclear W+ W- Z Yes (1983) Electromagnetic 10-2 Infinite Photon Yes (1923) Strong 1 Nuclear

More information

Appendix A2. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France.

Appendix A2. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France. Appendix A. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France. Prepared by: Arash Akbari-Sharbaf Why Build Accelerators? Probe deeper From

More information

Today in Astronomy 142

Today in Astronomy 142 Today in Astronomy 142! Elementary particles and their interactions, nuclei, and energy generation in stars.! Nuclear fusion reactions in stars TT Cygni: Carbon Star Credit: H. Olofsson (Stockholm Obs.)

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

The Building Blocks of Nature

The Building Blocks of Nature The Building Blocks of Nature PCES 15.1 Schematic picture of constituents of an atom, & rough length scales. The size quoted for the nucleus here (10-14 m) is too large- a single nucleon has size 10-15

More information

The Quark-Gluon Plasma and the ALICE Experiment

The Quark-Gluon Plasma and the ALICE Experiment The Quark-Gluon Plasma and the ALICE Experiment David Evans The University of Birmingham IoP Nuclear Physics Conference 7 th April 2009 David Evans IoP Nuclear Physics Conference 2009 1 Outline of Talk

More information

The first 400,000 years

The first 400,000 years The first 400,000 years All about the Big Bang Temperature Chronology of the Big Bang The Cosmic Microwave Background (CMB) The VERY early universe Our Evolving Universe 1 Temperature and the Big Bang

More information

The Electro-Strong Interaction

The Electro-Strong Interaction The Electro-Strong Interaction Taking into account the Planck Distribution Law of the electromagnetic oscillators, we can explain the electron/proton mass rate and the Weak and Strong Interactions. Lattice

More information

Phenomenology of Heavy-Ion Collisions

Phenomenology of Heavy-Ion Collisions Phenomenology of Heavy-Ion Collisions Hendrik van Hees Goethe University Frankfurt and FIAS October 2, 2013 Hendrik van Hees (GU Frankfurt/FIAS) HIC Phenomenology October 2, 2013 1 / 20 Outline 1 Plan

More information

Overview* of experimental results in heavy ion collisions

Overview* of experimental results in heavy ion collisions Overview* of experimental results in heavy ion collisions Dipartimento di Fisica Sperimentale dell Universita di Torino and INFN Torino * The selection criteria of the results presented here are (to some

More information

Physics 736. Experimental Methods in Nuclear-, Particle-, and Astrophysics. - Accelerator Techniques: Introduction and History -

Physics 736. Experimental Methods in Nuclear-, Particle-, and Astrophysics. - Accelerator Techniques: Introduction and History - Physics 736 Experimental Methods in Nuclear-, Particle-, and Astrophysics - Accelerator Techniques: Introduction and History - Karsten Heeger heeger@wisc.edu Homework #8 Karsten Heeger, Univ. of Wisconsin

More information

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

New subatomic particle and the Electro-Strong and -Weak Interaction New subatomic particle and the Electro-Strong and -Weak Interaction Named Ds3*(2860), the particle, a new type of meson, was discovered by analyzing data collected with the LHCb detector at CERN's Large

More information

EP228 Particle Physics

EP228 Particle Physics EP8 Particle Physics Topic 3 Department of Engineering Physics University of Gaziantep Course web page www.gantep.edu.tr/~bingul/ep8 Dec 01 Page 1 Outline 1. Introduction. Electrostatic (DC) Accelerators

More information

Chapter test: Probing the Heart of Matter

Chapter test: Probing the Heart of Matter PRO dditional sheet 5 Chapter test: Probing the Heart of Matter 40 marks total nswer LL the questions. Write your answers in the spaces provided in this question paper. The marks for individual questions

More information

Hour Exam 3 Review. Quantum Mechanics. Photoelectric effect summary. Photoelectric effect question. Compton scattering. Compton scattering question

Hour Exam 3 Review. Quantum Mechanics. Photoelectric effect summary. Photoelectric effect question. Compton scattering. Compton scattering question Hour Exam 3 Review Hour Exam 3: Wednesday, Apr. 19 In-class (2241 Chamberlin Hall) Twenty multiple-choice questions Will cover: Basic Quantum Mechanics Uses of Quantum Mechanics Addl. Lecture Material

More information

Historical developments. of particle acceleration

Historical developments. of particle acceleration Historical developments of particle acceleration Y.Papaphilippou N. Catalan-Lasheras USPAS, Cornell University, Ithaca, NY 20 th June 1 st July 2005 1 Outline Principles of Linear Acceleration Electrostatic

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

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

The Particle World. This talk: What is our Universe made of? Where does it come from? Why does it behave the way it does? The Particle World What is our Universe made of? Where does it come from? Why does it behave the way it does? Particle physics tries to answer these questions. This talk: particles as we understand them

More information

Ultra-relativistic nuclear collisions and Production of Hot Fireballs at SPS/RHIC

Ultra-relativistic nuclear collisions and Production of Hot Fireballs at SPS/RHIC Ultra-relativistic nuclear collisions and Production of Hot Fireballs at SPS/RHIC Benjamin Dönigus 03.12.2009 Seminar WS 2009/2010 Relativistische Schwerionenphysik Interface of Quark-Gluon Plasma and

More information

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

PHY357 Lecture 14. Applications of QCD. Varying coupling constant. Jets and Gluons. Quark-Gluon plasma. Colour counting PHY357 Lecture 14 Applications of QCD Varying coupling constant Jets and Gluons Quark-Gluon plasma Colour counting The proton structure function (not all of section 5.8!) Variable Coupling Constants! At

More information

Theory English (Official)

Theory English (Official) Q3-1 Large Hadron Collider (10 points) Please read the general instructions in the separate envelope before you start this problem. In this task, the physics of the particle accelerator LHC (Large Hadron

More information

Particle Acceleration

Particle Acceleration Nuclear and Particle Physics Junior Honours: Particle Physics Lecture 4: Accelerators and Detectors February 19th 2007 Particle Beams and Accelerators Particle Physics Labs Accelerators Synchrotron Radiation

More information

1. What does this poster contain?

1. What does this poster contain? This poster presents the elementary constituents of matter (the particles) and their interactions, the latter having other particles as intermediaries. These elementary particles are point-like and have

More information

Tools of Particle Physics I Accelerators

Tools of Particle Physics I Accelerators Tools of Particle Physics I Accelerators W.S. Graves July, 2011 MIT W.S. Graves July, 2011 1.Introduction to Accelerator Physics 2.Three Big Machines Large Hadron Collider (LHC) International Linear Collider

More information

Particle physics: what is the world made of?

Particle physics: what is the world made of? Particle physics: what is the world made of? From our experience from chemistry has told us about: Name Mass (kg) Mass (atomic mass units) Decreasing mass Neutron Proton Electron Previous lecture on stellar

More information

PHYS 3446 Lecture #18

PHYS 3446 Lecture #18 PHYS 3446 Lecture #18 Monday, Nov. 7, 2016 Dr. Jae Yu Particle Accelerators Electro-static Accelerators Cyclotron Accelerators Synchrotron Accelerators Elementary Particle Properties Forces and their relative

More information

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

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

More information

Introduction to Elementary Particle Physics I

Introduction to Elementary Particle Physics I Physics 56400 Introduction to Elementary Particle Physics I Lecture 9 Fall 2018 Semester Prof. Matthew Jones Particle Accelerators In general, we only need classical electrodynamics to discuss particle

More information

Quarkonia physics in Heavy Ion Collisions. Hugo Pereira Da Costa CEA/IRFU Rencontres LHC France Friday, April

Quarkonia physics in Heavy Ion Collisions. Hugo Pereira Da Costa CEA/IRFU Rencontres LHC France Friday, April Quarkonia physics in Heavy Ion Collisions Hugo Pereira Da Costa CEA/IRFU Rencontres LHC France Friday, April 5 2013 1 2 Contents Introduction (QGP, Heavy Ion Collisions, Quarkonia) Quarkonia at the SPS

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

Particle Accelerators. The Electrostatic Accelerators

Particle Accelerators. The Electrostatic Accelerators Particle Accelerators The Electrostatic Accelerators References K. Wille The Physics of Particle Accelerator, Oxford University press pag 1-29 H. Wiedeman Particle accelerator physics volume 1, chapter

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

3. Particle accelerators

3. Particle accelerators 3. Particle accelerators 3.1 Relativistic particles 3.2 Electrostatic accelerators 3.3 Ring accelerators Betatron // Cyclotron // Synchrotron 3.4 Linear accelerators 3.5 Collider Van-de-Graaf accelerator

More information

Stellar Astronomy Sample Questions for Exam 4

Stellar Astronomy Sample Questions for Exam 4 Stellar Astronomy Sample Questions for Exam 4 Chapter 15 1. Emission nebulas emit light because a) they absorb high energy radiation (mostly UV) from nearby bright hot stars and re-emit it in visible wavelengths.

More information

Lecture 8. CPT theorem and CP violation

Lecture 8. CPT theorem and CP violation Lecture 8 CPT theorem and CP violation We have seen that although both charge conjugation and parity are violated in weak interactions, the combination of the two CP turns left-handed antimuon onto right-handed

More information

Chapter 22. Preview. Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem. Section 1 The Nucleus

Chapter 22. Preview. Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem. Section 1 The Nucleus Section 1 The Nucleus Preview Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem Section 1 The Nucleus Objectives Identify the properties of the nucleus of an atom. Explain

More information

Accelerators Ideal Case

Accelerators Ideal Case Accelerators Ideal Case Goal of an accelerator: increase energy of CHARGED par:cles Increase energy ΔE = r 2 F dr = q ( E + v B)d r The par:cle trajectory direc:on dr parallel to v ΔE = increase of energy

More information

CLASS 32. NUCLEAR BINDING ENERGY

CLASS 32. NUCLEAR BINDING ENERGY CLASS 3. NUCLEAR BINDING ENERGY 3.. INTRODUCTION Scientists found that hitting atoms with alpha particles could induce transformations in light elements. (Recall that the capture of an alpha particle by

More information

Introduction to Accelerator Physics Part 1

Introduction to Accelerator Physics Part 1 Introduction to Accelerator Physics Part 1 Pedro Castro / Accelerator Physics Group (MPY) Introduction to Accelerator Physics DESY, 27th July 2015 Pedro Castro / MPY Introduction to Accelerator Physics

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

Frontier Science: The mystery of Antimatter

Frontier Science: The mystery of Antimatter Frontier Science: The mystery of Antimatter Cristina Lazzeroni Professor in Particle Physics STFC Public Engagement Fellow ASE Frontier Science Lecture University of Birmingham Poynting Physics S02 7th

More information

Laboratory for Nuclear Science

Laboratory for Nuclear Science The Laboratory for Nuclear Science (LNS) provides support for research by faculty and research staff members in the fields of particle, nuclear, and theoretical plasma physics. This includes activities

More information

Particle physics today. Giulia Zanderighi (CERN & University of Oxford)

Particle physics today. Giulia Zanderighi (CERN & University of Oxford) Particle physics today Giulia Zanderighi (CERN & University of Oxford) Particle Physics Particle Physics is fundamental research, as opposed to many applied sciences (medicine, biology, chemistry, nano-science,

More information

Lectures on accelerator physics

Lectures on accelerator physics Lectures on accelerator physics Lecture 3 and 4: Examples Examples of accelerators 1 Rutherford s Scattering (1909) Particle Beam Target Detector 2 Results 3 Did Rutherford get the Nobel Prize for this?

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

Accelerator Physics, BAU, First Semester, (Saed Dababneh).

Accelerator Physics, BAU, First Semester, (Saed Dababneh). Accelerator Physics 501503746 Course web http://nuclear.bau.edu.jo/accelerators/ edu or http://nuclear.dababneh.com/accelerators/ com/accelerators/ 1 Grading Mid-term Exam 25% Projects 25% Final Exam 50%

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

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

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES Q1. The figure below shows what scientists over 1000 years ago thought the solar system was like. Give one way that the historical model of the solar

More information

Quantum Mechanics. Exam 3. Photon(or electron) interference? Photoelectric effect summary. Using Quantum Mechanics. Wavelengths of massive objects

Quantum Mechanics. Exam 3. Photon(or electron) interference? Photoelectric effect summary. Using Quantum Mechanics. Wavelengths of massive objects Exam 3 Hour Exam 3: Wednesday, November 29th In-class, Quantum Physics and Nuclear Physics Twenty multiple-choice questions Will cover:chapters 13, 14, 15 and 16 Lecture material You should bring 1 page

More information

Introduction to the Standard Model of elementary particle physics

Introduction to the Standard Model of elementary particle physics Introduction to the Standard Model of elementary particle physics Anders Ryd (Anders.Ryd@cornell.edu) May 31, 2011 Abstract This short compendium will try to explain our current understanding of the microscopic

More information

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

Unravelling the Mysteries of Matter with the CERN Large Hadron Collider An Introduction/Overview of Particle Physics Unravelling the Mysteries of Matter with the CERN Large Hadron Collider An Introduction/Overview of Particle Physics Introductory Lecture August 3rd 2014 International Centre for Theoretical Physics and

More information

QCD Matter under Extreme Conditions

QCD Matter under Extreme Conditions Physics Colloquium QCD Matter under Extreme Conditions Neda Sadooghi Department of Physics Sharif University of Technology Tehran-Iran October 2006 How everything began? How everything will end? The Big

More information

PARTICLE ACCELERATORS

PARTICLE ACCELERATORS VISUAL PHYSICS ONLINE PARTICLE ACCELERATORS Particle accelerators are used to accelerate elementary particles to very high energies for: Production of radioisotopes Probing the structure of matter There

More information

A few thoughts on 100 years of modern physics. Quanta, Quarks, Qubits

A few thoughts on 100 years of modern physics. Quanta, Quarks, Qubits A few thoughts on 100 years of modern physics Quanta, Quarks, Qubits Quanta Blackbody radiation and the ultraviolet catastrophe classical physics does not agree with the observed world Planck s idea: atoms

More information

(a) (b) Fig. 1 - The LEP/LHC tunnel map and (b) the CERN accelerator system.

(a) (b) Fig. 1 - The LEP/LHC tunnel map and (b) the CERN accelerator system. Introduction One of the main events in the field of particle physics at the beginning of the next century will be the construction of the Large Hadron Collider (LHC). This machine will be installed into

More information

FXA Candidates should be able to :

FXA Candidates should be able to : 1 Candidates should be able to : MATTER AND ANTIMATTER Explain that since protons and neutrons contain charged constituents called quarks, they are therefore, not fundamental particles. Every particle

More information

What is a heavy ion? Accelerator terminology: Any ion with A>4, Anything heavier than α-particle

What is a heavy ion? Accelerator terminology: Any ion with A>4, Anything heavier than α-particle Outline Introduction to Relativistic Heavy Ion Collisions and Heavy Ion Colliders. Production of particles with high transverse momentum. Collective Elliptic Flow Global Observables Particle Physics with

More information

THE STANDARD MODEL OF MATTER

THE STANDARD MODEL OF MATTER VISUAL PHYSICS ONLINE THE STANDARD MODEL OF MATTER The "Standard Model" of subatomic and sub nuclear physics is an intricate, complex and often subtle thing and a complete study of it is beyond the scope

More information