Large Hadron Collider (LHC)

Slides:



Advertisements
Similar presentations
Particle Physics Chris Parkes Accelerators & Detectors
Advertisements

Transverse dynamics Selected topics, University of Oslo, Erik Adli, University of Oslo, August 2014,
The coldest and emptiest place in the solar system. The highest energies ever created. Cameras the size of cathedrals. A machine 27km long. LHC Overview.
Study of the Luminosity of LHeC, a Lepton Proton Collider in the LHC Tunnel CERN June F. Willeke, DESY.
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #8.
Note: most of the slides shown here are picked from CERN accelerator workshops. Please refer to those workshop for further understanding of the accelerator.
Synchrotron Radiation What is it ? Rate of energy loss Longitudinal damping Transverse damping Quantum fluctuations Wigglers Rende Steerenberg (BE/OP)
The Large Hadron Collider By Kathleen McKay. What is the LHC? The most powerful particle accelerator in the world. A synchrotron (ring-shaped particle.
M. LindroosNUFACT06 School Accelerator Physics Transverse motion Mats Lindroos.
Discovering the Unknown at the CERN Large Hadron Collider (LHC) Amy Gladwin University of Arizona.
Longitudinal motion: The basic synchrotron equations. What is Transition ? RF systems. Motion of low & high energy particles. Acceleration. What are Adiabatic.
A. Bay Beijing October Accelerators We want to study submicroscopic structure of particles. Spatial resolution of a probe ~de Broglie wavelength.
Luminosity Prospects of LHeC, a Lepton Proton Collider in the LHC Tunnel DESY Colloquium May F. Willeke, DESY.
1 Where to Search for the Higgs  A direct search for the Higgs was carried out by the four LEP experiments from CMS energy of GeV The.
Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Synchrotron radiation in LHC: spectrum and dynamics The Large Hadron Collider (LHC)
Accelerator Physics  Basic Formalism  Linear Accelerators  Circular Accelerators  Magnets  Beam Optics  Our Accelerator Greg LeBlanc Lead Accelerator.
Paul Derwent 30 Nov 00 1 The Fermilab Accelerator Complex o Series of presentations  Overview of FNAL Accelerator Complex  Antiprotons: Stochastic Cooling.
Introduction to Accelerators Eric Torrence University of Oregon QuartNet 2005 Special Thanks to Bernd Surrow
Eric Prebys Fermi National Accelerator Laboratory NIU Phy 790 Guest Lecture March 20, 2014 E.Prebys, NIU Phy 790 Guest Lecture 1.
Introduction to particle accelerators Walter Scandale CERN - AT department Roma, marzo 2006.
 Particle accelerators Particle accelerators are divided into two by the way they were built: 1-)Linear 2-)Circular.
The LHC: an Accelerated Overview Jonathan Walsh May 2, 2006.
March 2011Particle and Nuclear Physics,1 Experimental tools accelerators particle interactions with matter detectors.
Particle Accelerators
Chapter 2 Particle accelerators: From basic to applied research Rüdiger Schmidt (CERN) – Version E1.0.
Thomas Roser Snowmass 2001 June 30 - July 21, 2001 Polarized Proton Acceleration and Collisions Spin dynamics and Siberian Snakes Polarized proton acceleration.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
Particle Accelerators
880.P20 Winter 2006 Richard Kass 1 The Large Hadron Collider LHC is located at CERN CERN is located near Geneva Part of CERN is in France The LHC collides.
Rüdiger Schmidt1 The LHC collider project I Rüdiger Schmidt - CERN SUSSP Sumer School St.Andrews Challenges LHC accelerator physics LHC technology Operation.
Lecture 5 Damping Ring Basics Susanna Guiducci (INFN-LNF) May 21, 2006 ILC Accelerator school.
Particle physics experiments l Particle physics experiments: collide particles to  produce new particles  reveal their internal structure and laws of.
HST 2009 Introduction to AcceleratorsD. Brandt 1 The LHC: Physics without mathematics ! D. Brandt, CERN.
accelerator centers worldwide
By Verena Kain CERN BE-OP. In the next three lectures we will have a look at the different components of a synchrotron. Today: Controlling particle trajectories.
M. Garcia-Sciveres July 2002 ATLAS A Proton Collider Detector M. Garcia-Sciveres Lawrence Berkeley National Laboratory.
Chapter 10 Rüdiger Schmidt (CERN) – Darmstadt TU , version E 2.4 Acceleration and longitudinal phase space.
Steve Playfer University of Edinburgh 15th Novemebr 2008 Large Hadron Collider at CERN.
Backgrounds at FP420 Henri Kowalski DESY 18 th of May 2006.
Lattice design for FCC-ee Bastian Haerer (CERN BE-ABP-LAT, Karlsruhe Institute of Technology (KIT)) 1 8 th Gentner Day, 28 October 2015.
E. Todesco, Milano Bicocca January-February 2016 Unit 2 Magnets for circular accelerators: the interaction regions Ezio Todesco European Organization for.
Lecture 4 Longitudinal Dynamics I Professor Emmanuel Tsesmelis Directorate Office, CERN Department of Physics, University of Oxford ACAS School for Accelerator.
Optics with Large Momentum Acceptance for Higgs Factory Yunhai Cai SLAC National Accelerator Laboratory Future Circular Collider Kick-off Meeting, February.
Professor Philip Burrows John Adams Institute for Accelerator Science Oxford University ACAS School for Accelerator Physics January 2014 Longitudinal Dynamics.
HF2014 Workshop, Beijing, China 9-12 October 2014 Challenges and Status of the FCC-ee lattice design Bastian Haerer Challenges.
Research and development toward a future Muon Collider Katsuya Yonehara Accelerator Physics Center, Fermilab On behalf of Muon Accelerator Program Draft.
CERN’s Large Hadron Collider
Longitudinal Dynamics of Charged Particle
Beam-beam effects in eRHIC and MeRHIC
Large Booster and Collider Ring
Lecture 2 Live Feed – CERN Control Centre
High PT physics at LHC – Lecture I (Introduction and LHC accelerator)
Jeffrey Eldred, Sasha Valishev
The LHC Accelerator Complex
Hunting the Higgs Boson at the CERN Large Hadron Collider
Synchrotron Ring Schematic
Elementary particles Spring 2005, Physics /24/2018 Lecture XXV.
CASA Collider Design Review Retreat Other Electron-Ion Colliders: eRHIC, ENC & LHeC Yuhong Zhang February 24, 2010.
Lecture 3 - Magnets and Transverse Dynamics I
Jefferson Lab Student Seminar Series
LHC (SSC) Byung Yunn CASA.
Lecture 2: Invariants, cross-section, Feynman diagrams
Electron Rings Eduard Pozdeyev.
Explanation of the Basic Principles and Goals
Physics 417/517 Introduction to Particle Accelerator Physics
MEIC New Baseline: Luminosity Performance and Upgrade Path
Main Design Parameters RHIC Magnets for MEIC Ion Collider Ring
MEIC New Baseline: Performance and Accelerator R&D
MEIC Alternative Design Part III
Beam Synchronization in MEIC: The Problem, Scale and Prospect
Presentation transcript:

Large Hadron Collider (LHC) Dr. Venkat Kaushik 2016-01-15

Today’s Topic Introduction to Large Hadron Collider (LHC) How do justify the need for LHC? Why hadron? Why large ? Layout Design of LHC Important parameters of LHC Key Ideas of Colliding Particles Event Rate Center-of-mass energy (√s) Synchrotrons and Beams Cyclotron Frequency Betatron function β(s) Emittance (ε) Luminosity LHC 01/15/2016

Why Need An LHC? Probing smaller and smaller scale Is necessary to understand the structure of matter and what they are made of (constituents) To probe a distance 1000 times smaller than a proton Search for new types of matter (or new particles) Higher energies are needed to discover new particles Many theories predict particles with masses > 1 TeV Many of these processes are rare their rate of production (cross section) is small Surprising new results could be lurking. Need a probe like LHC De-Broglie wavelength of a proton is < 1.2 fm 01/15/2016 LHC

What’s Large About LHC ? 27 km circumference Hauling an ATLAS Magnet (toroid end cap) Lake Geneva 27 km circumference Highest energy collider ever built Superconducting, super cooled magnets ATLAS Our home (2008 – 2010) LHC 01/15/2016

High Energy Colliders Accelerator Particle Type, Laboratory Energy √s GeV Years of operation LEP-I e+e- collider, CERN 91 1989 – 1994 LEP-II 209 1995 – 2000 HERA-I e-p collider, DESY 27 + 800 1992 – 2000 HERA-II 27 + 920 2002 – 2007 Tevatron, Run I collider, Fermilab 1800 1987 – 1996 Tevatron Run II 1960 2002 – 2011 LHC, phase I pp collider, CERN 7000 2010 – 2012 LHC, phase II 14000 2014 – … HADRONS Highlights: Phase 1: Higgs boson -- discovered July 2012 Two year shutdown followed by Phase 2, which started in 2015 LHC 01/15/2016

LHC Layout 8 crossing interaction points (IP’s) ATLAS, ALICE, CMS, LHCb experiments Accelerator sectors go in between the IP’s Sector 23 goes between 2 and 3, sector 34 goes between 3 and 4 etc. 01/15/2016 LHC

LHC Parameters LHC 01/15/2016

Proton Bunches Each beam is made up of bunches of protons Each bunch is approximately a cylinder Bunch (n+1) Bunch n Bunch (n-1) Bunch spacing = 7.5 m Bunch length = 7.48 cm Effective Area (A) of a bunch A = 0.2 mm far away from collision points A = 16 μm at the collision or interaction point (IP) Bunches get squeezed by quadrupole magnets as they approach IP After doing some math Effective number of bunches around a 27 km ring = 2808 Since they are moving close to speed of light, the spacing between bunches arriving at IP is ~ 25 ns 01/15/2016 LHC

Event Rate Event Cross Section (σ) Luminosity = L Event Rate Any physical process that is allowed by nature and which obeys conservation laws (e.g., qq  Hγ) Cross Section (σ) Probability that an event occurs (units of 1b = 10-24 cm2) Rare processes have small cross sections Luminosity = L Ability of the particle accelerator to produce the required number of interactions (cm-2 s-1) Event Rate LHC 01/15/2016

Example 1 Find the rate of inelastic pp collisions at 14 TeV L = 1034 cm-2 s-1 σ ~ 80 mb = 80 x 10-3 x10-24 cm2 (at √s = 14 TeV) Event Rate = σL = 80 x 10(34-3-24) s-1 = 80 x 107/s LHC 01/15/2016

Example 2 Find the event rate for the process qq  Zh L = 1034 cm-2 s-1 σ ~ 50 fb = 50 x 10-15 x10-24 cm2 (at √s = 14 TeV) Event Rate = σL = 50 x 10(34-15-24) s-1 = 5 x 10-4/s At this rate, how long does it take to observe 100 events? t = 100/ (5 x 10-4/s) ~ 55 hours or > 2 days LHC 01/15/2016

Center of Mass Energy √s 2  2 collision (scattering) p1, p2 are the four momenta of incoming particles (a,b) p3, p4 are the four momenta of outgoing particles (c,d) Defined as s = (p1 + p2)2 = (p3 + p4)2 = 4E2 (Lorentz-invariant) √s = (E + E) which is the combined energy of the incoming particles as seen from the center-of-mass reference frame. For LHC a=proton, b=proton, E = 7 TeV, √s = 7+7 = 14 TeV LHC 01/15/2016

Cyclotron Frequency Cyclotron Synchrotron side view top view r Cyclotron For small values of velocity (β = v/c < 0.2) this is a perfectly valid Synchrotron We usually accelerate particles close to the speed of light β ~ .99 Relativistic correction to mass (replace m by γm0) As energy increases, fc is no longer a constant! fc becomes smaller, i.e., particles take longer to go around! 01/15/2016 LHC

Packing a Punch Bunches of Protons Radiofrequency (RF) Cavities We need protons to be in a close bunch. Why? in order to maximize collisions when the bunches “cross over” (i.e., collide) Radiofrequency (RF) Cavities Oscillating voltage at 400 MHz (radio frequency) Help keep the protons to remain closely packed “bunches” In addition, the bunches receive a “kick” in the forward direction every time they pass one of these cavities they gain additional 16 MeV At close to the speed of light, they complete 11245 laps in one second! To get from 0.45 TeV to 7 TeV, it takes about 37 seconds! 01/15/2016 LHC

Bending Using Dipoles B v F B v F The bending of protons occurs due to the transverse magnetic field The dipole magnet bends the protons and keeps them along the circular track just like a prism 01/15/2016 LHC

Focusing using Quadrupoles Imagine a bunch of protons Yellow line indicates the path First quadrupole magnet squeezes the bunch close together in the XY plane Second quadrupole magnet does the same in YZ plane This process continues to keep the bunch of protons within the vacuum tube in which they are circling around LHC has a total of 858 quadrupoles + +X +Y +Z 01/15/2016 LHC

Betatron Function Nominal Trajectory (s) Lateral Deviation (x) Is defined by the dipoles If we consider the protons in a bunch, they follow the nominal trajectory Lateral Deviation (x) There are deviations in the XY and XZ planes from nominal they oscillate around the nominal trajectory Beta function β(s) Describes the lateral shift and gives us a “beam envelope” which would contain the protons in the bunch. s Position along trajectory Lateral deviation x Nominal trajectory Particle trajectory Number of oscillations for one turn => TUNE 01/15/2016 LHC

Betatron Function Conceptual Understanding Normalized particle trajectory Trajectories over multiple turns Conceptual Understanding Betatron function is the bounding envelope of the beam You can think of it as the amplitude of the sine wave Strong closely spaced quadrupoles lead to Small β(s) , lots of wiggles Weak sparsely spaced quadrupoles lead to Large β(s) , fewer wiggles 01/15/2016 LHC

Emittance Definition x’ vs x is a “phase space” At any point along the trajectory, each particle can be represented by a position in this phase-space The collection (ensemble) of all the protons will be inside an ellipse with a certain area. This area is called “emittance” For a Gaussian distribution the RMS of emittance contains 39% of protons at LHC http://www.lhc-closer.es/taking_a_closer_look_at_lhc/0.complex_movement LHC 01/15/2016

Luminosity Luminosity is a function of number of protons in each bunch (N1, N2) Effective area of collision at interaction point (A) Bunch crossing frequency (f) LHC 01/15/2016

Luminosity at IP Accelerator physicists often express luminosity as a function of Betatron function and Emittance The bunches are squeezed / focused at IP Hourglass effect Crossing angle Betatron function β  β* LHC 01/15/2016

Increasing Luminosity Particles in a bunch Collision frequency Geometrical factor: - crossing angle - hourglass effect Transverse size (RMS) Normalized emittance Revolution frequency Number of bunches Betatron function at collision point 01/15/2016 LHC