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The International Linear Collider Barry Barish Caltech 5-Jan-06
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The International Linear Collider

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The International Linear Collider. Barry Barish Caltech 5-Jan-06. Particle Physics Inquiry Based Science. Are there undiscovered principles of nature: New symmetries, new physical laws? How can we solve the mystery of dark energy? Are there extra dimensions of space? - PowerPoint PPT Presentation
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Page 1: The International Linear Collider

The International Linear Collider

Barry BarishCaltech 5-Jan-06

Page 2: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 2

Particle Physics Inquiry Based Science

1. Are there undiscovered principles of nature:New symmetries, new physical laws?

2. How can we solve the mystery of dark energy?

3. Are there extra dimensions of space?

4. Do all the forces become one?

5. Why are there so many kinds of particles?

6. What is dark matter?How can we make it in the laboratory?

7. What are neutrinos telling us?

8. How did the universe come to be?

9. What happened to the antimatter?from the Quantum Universe

Page 3: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 3

Answering the QuestionsThree Complementary Probes

• Neutrinos as a Probe– Particle physics and astrophysics using a weakly

interacting probe

• High Energy Proton Proton Colliders– Opening up a new energy frontier ( ~ 1 TeV scale)

• High Energy Electron Positron Colliders– Precision Physics at the new energy frontier

Page 4: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 4

Why a TeV Scale e+e- Accelerator?

• Two parallel developments over the past few years (the science & the technology)

– The precision information from LEP and other data have pointed to a low mass Higgs; Understanding electroweak symmetry breaking, whether supersymmetry or an alternative, will require precision measurements.

– There are strong arguments for the complementarity between a ~0.5-1.0 TeV ILC and the LHC science.

Page 5: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 5

Electroweak Precision Measurements

What causes mass??

0

2

4

6

10020 400

mH GeV

Excluded Preliminary

had =(5)

0.027610.00036

0.027470.00012

Without NuTeV

theory uncertainty

Winter 2003

The mechanism – Higgs or alternative appears around the corner

Page 6: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 6

Accelerators and the Energy FrontierLarge Hadron Collider

CERN – Geneva Switzerland

Page 7: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 7

LHC and the Energy FrontierSource of Particle Mass

The Higgs FieldDiscover the Higgs

or variants or ???

fb-1

LEP

FNAL

Page 8: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 8

LHC and the Energy FrontierA New Force in Nature

Discover a new heavy particle, Z’

Can show by measuring the couplings with the ILC how it relates to other particles and forces

Page 9: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 9

This led to higher energy machines: Electron-Positron Colliders

Bruno Touschek built the first successful electron-positron collider at Frascati, Italy (1960)

Eventually, went up to 3 GeV

ADA

Page 10: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 10

But, not quite high enough energy ….

DiscoveryOf

CharmParticles

and

3.1 GeV

Burt RichterNobel Prize

SPEAR at SLAC

Page 11: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 11

The rich history for e+e- continued as higher energies were achieved …

DESY PETRA Collider

Page 12: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 12

Electron Positron CollidersThe Energy Frontier

Page 13: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 13

Why e+e- Collisions ?

• elementary particles

• well-defined – energy,

– angular momentum

• uses full COM energy

• produces particles democratically

• can mostly fully reconstruct events

Page 14: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 14

The linear collider will measure the spin of any Higgs it can produce by measuring the energy dependence from threshold

How do you know you have discovered the Higgs ?

Measure the quantum numbers. The Higgs must have spin zero !

Page 15: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 15

What can we learn from the Higgs?

•Straight blue line gives the standard model predictions.

• Range of predictions in models with extra dimensions -- yellow band, (at most 30% below the Standard Model

• The red error bars indicate the level of precision attainable at the ILC for each particle

Precision measurements of Higgs coupling can reveal extra dimensions in nature

Page 16: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 16

New space-time dimensions can be mapped by studying the emission of gravitons into the extra dimensions, together with a photon or jets emitted into the normal dimensions.

Linear collider

Direct production from extra dimensions

?

Page 17: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 17

Bosons Fermions

Virtues of Supersymmetry:– Unification of Forces– The Hierarchy Problem– Dark Matter

Is There a New Symmetry in Nature? Supersymmetry

Page 18: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 18

Parameters for the ILC

• Ecm adjustable from 200 – 500 GeV

• Luminosity ∫Ldt = 500 fb-1 in 4 years

• Ability to scan between 200 and 500 GeV

• Energy stability and precision below 0.1%

• Electron polarization of at least 80%

• The machine must be upgradeable to 1 TeV

Page 19: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 19

A TeV Scale e+e- Accelerator?

• Two parallel developments over the past few years (the science & the technology)

– Two alternate designs -- “warm” and “cold” had come to the stage where the show stoppers had been eliminated and the concepts were well understood.

– A major step toward a new international machine requires uniting behind one technology, and then make a unified global design based on the recommended technology.

Page 20: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 20

• The JLC-X and NLC essentially a unified single design with common parameters

• The main linacs based on 11.4 GHz, room temperature copper technology.

GLC GLC/NLC Concept

Page 21: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 21

TESLA Concept

• The main linacs based on 1.3 GHz superconducting technology operating at 2 K.

• The cryoplant, is of a size comparable to that of the LHC, consisting of seven subsystems strung along the machines every 5 km.

Page 22: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 22

CLIC Concept

The main linac rfpower is produced by decelerating a high-current (150 A) low-energy (2.1 GeV) drive beam

Nominal accelerating gradient of 150 MV/m

GOALProof of concept ~2010

Drive Beam

Main Accelerator

Page 23: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 23

International Technology Review Panel

Page 24: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 24

SCRF Technology Recommendation

• The recommendation of ITRP was presented to ILCSC & ICFA on August 19, 2004 in a joint meeting in Beijing.

• ICFA unanimously endorsed the ITRP’s recommendation on August 20, 2004

Page 25: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 25

The ITRP Recommendation

• We recommend that the linear collider be based on superconducting rf technology

– This recommendation is made with the understanding that we are recommending a technology, not a design. We expect the final design to be developed by a team drawn from the combined warm and cold linear collider communities, taking full advantage of the experience and expertise of both (from the Executive Summary).

Page 26: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 26

The Community Self-Organized

Nov 13-15, 2004

Page 27: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 27

Global Design Effort (GDE)

• February 2005, at TRIUMF, ILCSC and ICFA endorsed the search committee choice for GDE Director

• On March 18, 2005

I officially accepted

the position at

the opening of

LCWS 05 meeting

at Stanford

Page 28: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 28

Global Design Effort

– The Mission of the GDE • Produce a design for the ILC that includes a

detailed design concept, performance assessments, reliable international costing, an industrialization plan , siting analysis, as well as detector concepts and scope.

• Coordinate worldwide prioritized proposal driven R & D efforts (to demonstrate and improve the performance, reduce the costs, attain the required reliability, etc.)

Page 29: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 29

GDE Begins at Snowmass

670 Scientists attended two week

workshopat

Snowmass

GDE MembersAmericas 22 Europe 24 Asia 16

Page 30: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 30

main linacbunchcompressor

dampingring

source

pre-accelerator

collimation

final focus

IP

extraction& dump

KeV

few GeV

few GeVfew GeV

250-500 GeV

Designing a Linear Collider

Superconducting RF Main Linac

Page 31: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 31

GDE Organization for Snowmass

•W

G1

LE

T b

dy

n.

•W

G2

Ma

in L

ina

c

•W

G3

a S

ou

rces

•W

G3

b D

R

•W

G4

BD

S

•W

G5

Ca

vity• GG1 Parameters• GG2 Instrumentation• GG3 Operations & Reliability• GG4 Cost & Engineering• GG5 Conventional Facilities• GG6 Physics Options

Technical sub-systemWorking Groups

Global Group

Provide input

Page 32: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 32

rf bands:

L-band (TESLA) 1.3 GHz = 3.7 cm

S-band (SLAC linac) 2.856 GHz 1.7 cm

C-band (JLC-C) 5.7 GHz 0.95 cm

X-band (NLC/GLC) 11.4 GHz 0.42 cm

(CLIC) 25-30 GHz 0.2 cm

Accelerating structure size is dictated by wavelength of the rf accelerating wave. Wakefields related to structure size; thus so is the difficulty in controlling emittance growth and final luminosity.

Bunch spacing, train length related to rf frequency

Damping ring design depends on bunch length, hence frequency

Specific Machine Realizations

Frequency dictates many of the design issues for LC

RF Bands

Page 33: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 33

Design Approach

• Create a baseline configuration for the machine– Document a concept for ILC machine with a complete

layout, parameters etc. defined by the end of 2005– Make forward looking choices, consistent with attaining

performance goals, and understood well enough to do a conceptual design and reliable costing by end of 2006.

– Technical and cost considerations will be an integral part in making these choices.

– Baseline will be put under “configuration control,” with a defined process for changes to the baseline.

– A reference design will be carried out in 2006. We are using a “parametric” design and costing approach.

– Technical performance and physics performance will be evaluated for the reference design

Page 34: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 34

The Key Decisions

Critical choices: luminosity parameters & gradient

Page 35: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 35

Making Choices – The Tradeoffs

Many decisions are interrelated and require input from several WG/GG groups

Page 36: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 36

ILC Baseline Configuration

• Configuration for 500 GeV machine with expandability to 1 TeV

• Some details – locations of low energy acceleration; crossing angles are not indicated in this cartoon.

Page 37: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 37

Cost Breakdown by Subsystem

cf31%

structures18%rf

12%

systems_eng8%

installation&test7%

magnets6%

vacuum4%

controls4%

cryo4%

operations4%

instrumentation2%

Civil

SCRF Linac

Page 38: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 38

How Costs Scale with Gradient?

Relative

Co

st

Gradient MV/m

2

0

$ lincryo

a Gb

G Q

35MV/m is close to optimum

Japanese are still pushing for 40-45MV/m

30 MV/m would give safety margin

C. Adolphsen (SLAC)

Page 39: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 39

Superconducting RF Cavities

High Gradient Accelerator35 MV/meter -- 40 km linear collider

Page 40: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 40

Improved Fabrication

Page 41: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 41

Improved ProcessingElectropolishing

Chemical Polish

Electro Polish

Page 42: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 42

Gradient

Results from KEK-DESY collaboration

must reduce spread (need more statistics)

single

-cell

measu

rem

ents

(in

nin

e-c

ell

cavit

ies)

Page 43: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 43

Baseline Gradient

Page 44: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 44

Large Grain Single Crystal Nb Material

Page 45: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 45

The Main Linac Configuration

• Klystron – 10 MW (alternative sheet beam klystron)

• RF Configuration – 3 Cryomodules, each with 8 cavities

• Quads – one every 24 cavities is enough

Page 46: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 46

Other Features of the Baseline

• Electron Source – Conventional Source using a DC gun

Page 47: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 47

Other Features of the Baseline

• Positron Source – Helical Undulator with Polarized beams

Primary e-

source

e-

DR

Target e- Dump

Photon Beam Dump

e+

DR

Auxiliary e- Source

Photon Collimators

Adiabatic Matching

Device

e+ pre-accelerator

~5GeV

150 GeV 100 GeV

HelicalUndulatorIn By-Pass

Line

PhotonTarget

250 GeV

Positron Linac

IP

Beam Delivery System

Page 48: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 48

Damping Ring Options

3 Km6 Km

3 or 6 km rings can be built in independent tunnels

“dogbone” straight sections share linac tunnel

Two or more rings can be stacked in a single tunnel

Page 49: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 49

ILC Siting and Conventional Facilities

• The design is intimately tied to the features of the site– 1 tunnels or 2 tunnels?– Deep or shallow?– Laser straight linac or follow earth’s curvature in

segments?

• GDE ILC Design will be done to samples sites in the three regions – North American sample site will be near Fermilab– Japan and Europe are to determine sample sites by the

end of 2005

Page 50: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 50

1 vs 2 Tunnels

• Tunnel must contain– Linac Cryomodule– RF system– Damping Ring Lines

• Save maybe $0.5B

• Issues– Maintenance– Safety– Duty Cycle

Page 51: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 51

Possible Tunnel Configurations

• One tunnel of two, with variants ??

Page 52: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 52

Americas Sample Site

• Design to “sample sites” from each region– Americas – near Fermilab– Japan– Europe – CERN & DESY

• Illinois Site – depth 135m– Glacially derived deposits

overlaying Bedrock. The concerned rock layers are from top to bottom the Silurian dolomite, Maquoketa dolomitic shale, and the Galena-Platteville dolomites.

Page 53: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 53

Parametric Approach

• A working space - optimize machine for cost/performance

Page 54: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 54

Beam Detector Interface

TauchiLCWS05

Page 55: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 55

• Large Scale 4detectors with solenoidal magnetic fields.

• In order to take full advantage of the ILC ability to reconstruct, need to improve resolutions, tracking, etc by factor of two or three

• New techniques in calorimetry, granularity of readout etc being developed

Detectors for the ILC

Page 56: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 56

Accelerator Physics Challenges• Develop High Gradient Superconducting RF systems

– Requires efficient RF systems, capable of accelerating high power beams (~MW) with small beam spots(~nm).

• Achieving nm scale beam spots – Requires generating high intensity beams of electrons and

positrons– Damping the beams to ultra-low emittance in damping rings– Transporting the beams to the collision point without significant

emittance growth or uncontrolled beam jitter– Cleanly dumping the used beams.

• Reaching Luminosity Requirements– Designs satisfy the luminosity goals in simulations– A number of challenging problems in accelerator physics and

technology must be solved, however.

Page 57: The International Linear Collider

The GDE Plan and Schedule 2005 2006 2007 2008 2009 2010

Global Design Effort Project

Baseline configuration

Reference Design

ILC R&D Program

Technical Design

Expression of Interest to Host

International Mgmt

LHCPhysics

CLIC

Page 58: The International Linear Collider

5-Jan-06 Caltech Physics Research Conference 58

Conclusions

• We have determined a number of very fundamental physics questions to answer, like ….– What determines mass?– What is the dark matter?– Are there new symmetries in nature?– What explains the baryon asymmetry?– Are the forces of nature unified

• We are developing the tools to answer these questions and discover new ones– Neutrino Physics– Large Hadron Collider– International Linear Collider

• Prospects for next era of particle physics are very bright!