the path to an international linear collider barry barish triumpf seminar 15-april-05
TRANSCRIPT
The Path to an International Linear Collider
Barry BarishTRIUMPF Seminar
15-April-05
15-April-05 TRIUMPF 2
Features of e+e- Collisions
• elementary particles
• well-defined
– energy,
– angular momentum
• uses full COM energy
• produces particles democratically
• can mostly fully reconstruct events
15-April-05 TRIUMPF 3
A Rich History as a Powerful Probe
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The Energy Frontier
15-April-05 TRIUMPF 5
2001: The Snowmass Workshop participants produced the statement recommending construction of a Linear Collider to overlap LHC running.
2001: HEPAP, ECFA, ACFA all issued reports endorsing the LC as the next major world project, to be international from the start
2002: The Consultative Group on High-Energy Physics of the OECD Global Science Forum executive summary stated as the first of its Principal Conclusions:
“The Consultative Group concurs with the world-wide consensus of the scientific community that a high-energy electron-positron collider is the next facility on the Road Map.
“There should be a significant period of concurrent running of the LHC and the LC, requiring the LC to start operating before 2015. Given the long lead times for decision-making and for construction, consultations among interested countries should begin at a suitably-chosen time in the near future.”
The Linear Collider
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Understanding Matter, Energy, Space and Time:The Case for the Linear Collider
A summary of the scientific case for the e+ e- Linear Collider, representing a broad consensus of the particle
physics community.
April 2003: signed now by ~2700 physicists worldwide.:
“Consensus Document”
http://sbhepnt.physics.sunysb.edu/~grannis/ilcsc/lc_consensus.pdf )(To join this list, go to http://blueox.uoregon.edu/~lc/wwstudy/ )
15-April-05 TRIUMPF 7
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 LC and the LHC science.
15-April-05 TRIUMPF 8
Electroweak Precision Measurements
LEP results strongly point to a low mass Higgs and an energy scale for new physics < 1TeV
0
2
4
6
10020 400
mH GeV
Excluded Preliminary
had =(5)
0.027610.00036
0.027470.00012
Without NuTeV
theory uncertainty
Winter 2003
15-April-05 TRIUMPF 9
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 LC and the LHC science.
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The 500 GeV Linear Collider Spin Measurement
LHC should discover the Higgs
The linear collider will measure the spin of any Higgs it can produce.
The process e+e– HZ can be used to measure the spin of a 120 GeV Higgs particle. The error bars are based on 20 fb–1 of luminosity at each point.
LHC/ILC Complementarity
The Higgs must have spin zero
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Extra Dimensions
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
LHC/ILC Complementarity
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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
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main linacbunchcompressor
dampingring
source
pre-accelerator
collimation
final focus
IP
extraction& dump
KeV
few GeV
few GeVfew GeV
250-500 GeV
Linear Collider Concept
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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
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Which Technology to Chose?
– 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.
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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.
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TESLA Cavity
• RF accelerator structures consist of close to 21,000 9-cell niobium cavities operating at gradients of 23.8 MV/m (unloaded as well as beam loaded) for 500 GeV c.m. operation.
• The rf pulse length is 1370 µs and the repetition rate is 5 Hz. At a later stage, the machine energy may be upgraded to 800 GeV c.m. by raising the gradient to 35 MV/m.
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TESLA Single Tunnel Layout
• The TESLA cavities are supplied with rf power in groups of 36 by 572 10 MW klystrons and modulators.
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• The JLC-X and NLC are essentially a unified single design with common parameters
• The main linacs are based on 11.4 GHz, room temperature copper technology.
GLCGLC/NLC Concept
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GLC GLC/NLC Concept
• The main linacs operate at an unloaded gradient of 65 MV/m, beam-loaded to 50 MV/m.
• The rf systems for 500 GeV c.m. consist of 4064 75 MW Periodic Permanent Magnet (PPM) klystrons arranged in groups of 8, followed by 2032 SLED-II rf pulse compression systems
15-April-05 TRIUMPF 21
GLC / NLC Concept
NLC
• Two parallel tunnels for each linac.
• For 500 GeV c.m. energy, rf systems only installed in the first 7 km of each linac.
• Upgrade to 1 TeV by filling the rest of each linac, for a total two-linac length of 28 km.
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The Report Validates the Readiness of L-band and X-
band Concepts
ICFA/ILCSC Evaluation of the Technologies
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TRC R1 Issues
L-Band: Feasibility for 500 GeV operation had been demonstrated, but 800 GeV with gradient of 35 MV/m requires a full cryomodule (9 or 12 cavities) and shown to have acceptable quench and breakdown rates with acceptable dark currents.
X-band: Demonstrate low group velocity accelerating structures with acceptable gradient, breakdown and trip rates, tuning manifolds and input couplers. Demonstrate the modulator, klystron, SLED-II pulse compressors at the full power required.
R1 issues pretty much satisfied by mid-2004
15-April-05 TRIUMPF 24
The Charge to the International Technology Recommendation Panel
General Considerations The International Technology Recommendation Panel (the Panel) should recommend a Linear Collider (LC) technology to the International Linear Collider Steering Committee (ILCSC).
On the assumption that a linear collider construction commences before 2010 and given the assessment by the ITRC that both TESLA and JLC-X/NLC have rather mature conceptual designs, the choice should be between these two designs. If necessary, a solution incorporating C-band technology should be evaluated.
Note -- We interpreted our charge as being to recommend a technology, rather than choose a design
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International Technology Review Panel
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ITRP Schedule of Events • Six Meetings
– RAL (Jan 27,28 2004)
– DESY (April 5,6 2004)
– SLAC (April 26,27 2004)
– KEK (May 25,26 2004)
– Caltech (June 28,29,30 2004)
– Korea (August 11,12,13)
– ILCSC / ICFA (Aug 19)– ILCSC (Sept 20)
Tutorial & Planning
Site Visits
Deliberations
Exec. Summary Final Report
Recommendation
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Evaluating the Criteria Matrix
• We analyzed the technology choice through studying a matrix having six general categories with specific items under each:– the scope and parameters specified by the ILCSC; – technical issues; – cost issues; – schedule issues; – physics operation issues; – and more general considerations that reflect the impact of the
LC on science, technology and society
• We evaluated each of these categories with the help of answers to our “questions to the proponents,” internal assignments and reviews, plus our own discussions
15-April-05 TRIUMPF 28
Our Process• We studied and evaluated a large amount of
available materials
• We made site visits to DESY, KEK and SLAC to listen to presentations on the competing technologies and to see the test facilities first-hand.
• We have also heard presentations on both C-band and CLIC technologies
• We interacted with the community at LC workshops, individually and through various communications we received
• We developed a set of evaluation criteria (a matrix) and had each proponent answer a related set of questions to facilitate our evaluations.
• We assigned lots of internal homework to help guide our discussions and evaluations
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What that Entailed
– We each traveled at least 75,000 miles
– We read approximately 3000 pages
– We had constant interactions with the community and with each other
– We gave up a good part of our “normal day jobs” for six months
– We had almost 100% attendance by all members at all meetings
– We worked incredibly hard to “turn over every rock” we could find.
from Norbert Holtkamp
15-April-05 TRIUMPF 30
The 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).
– The superconducting technology has several very nice features for application to a linear collider. They follow in part from the low rf frequency.
15-April-05 TRIUMPF 31
Some Features of SC Technology
• The large cavity aperture and long bunch interval reduce the complexity of operations, reduce the sensitivity to ground motion, permit inter-bunch feedback and may enable increased beam current.
• The main linac rf systems, the single largest technical cost elements, are of comparatively lower risk.
• The construction of the superconducting XFEL free electron laser will provide prototypes and test many aspects of the linac.
• The industrialization of most major components of the linac is underway.
• The use of superconducting cavities significantly reduces power consumption.
15-April-05 TRIUMPF 32
Technology Recommendation
• The recommendation was presented to ILCSC & ICFA on August 19 in a joint meeting in Beijing.
• ICFA unanimously endorsed the ITRP’s recommendation on August 20
15-April-05 TRIUMPF 33
What’s Next
• Organize the ILC effort globally
– Coordinate worldwide R & D efforts, in order to demonstrate and improve the performance, reduce the costs, attain the required reliability, etc.
– Undertake making a “global design” over the next few years for a machine that can be jointly implemented internationally.
– These goals are within reach and we fully expect to have an optimized design within a few years, so that we can undertake building the next great particle accelerator.
15-April-05 TRIUMPF 34
Fall 2002: ICFA created the International Linear Collider Steering Committee (ILCSC) to guide the process for building a Linear Collider. Asia, Europe and North America each formed their own regional Steering Groups (Jonathan Dorfan chairs the North America steering group).
Physics and Detectors Subcommittee (AKA WWS) Jim Brau, David Miller, Hitoshi Yamamoto, co-chairs (est. 1998 by ICFA as free standing group)
International Linear Collider Steering CommitteeMaury Tigner, chair
ParametersSubcommitteeRolf Heuer, chair
(finished)
Accelerator SubcommitteeGreg Loew, chair
Comunicationsand OutreachNeil Calder et al
Technology Recommendation Panel
Barry Barish, chair (finished)
Global Design Initiative
organization Satoshi Ozaki, chair (finished)
GDI central team site
evaluation Ralph Eichler,
chair
GDI central team director
search committee Paul Grannis,
chair
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Starting Points for the ILC Design
33km47 km
TESLA TDR500 GeV (800 GeV)
US Options Study500 GeV (1 TeV)
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Experimental Test Facility - KEK
• Prototype Damping Ring for X-band Linear Collider
• Development of Beam Instrumentation and Control
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Evaluation: Technical Issues
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TESLA Test Facility Linac
laser driven electron gun
photon beam diagnostics
undulatorbunch
compressor
superconducting accelerator modules
pre-accelerator
e- beam diagnostics
e- beam diagnostics
240 MeV 120 MeV 16 MeV 4 MeV
15-April-05 TRIUMPF 39
Attendees: Son (Korea); Yamauchi (Japan); Koepke (Germany); Aymar (CERN); Iarocci (CERN Council); Ogawa (Japan); Kim (Korea); Turner (NSF - US); Trischuk (Canada); Halliday (PPARC); Staffin (DoE – US); Gurtu (India)
Guests: Barish (ITRP); Witherell (Fermilab Director,)
“The Funding Agencies praise the clear choice by ICFA. This recommendation will lead to focusing of the global R&D effort for the linear collider and the Funding Agencies look forward to assisting in this process.
The Funding Agencies see this recommendation to use superconducting rf technology as a critical step in moving forward to the design of a linear collider.”
FALC is setting up a working group to keep a close liaison with the Global Design Initiative with regard to funding resources.
The cooperative engagement of the Funding Agencies on organization, technology choice, timetable is a very strong signal and encouragement.
Statement of Funding Agency (FALC) 17-Sept-04 @ CERN
The Birth of the
Global Design Effort
Linear Collider Workshop
Stanford, CAMarch-05
15-April-05 TRIUMPF 41
ILC Design Issues
First Consideration : Physics Reach
ILC Parameters
Energy Reach
2cm fill linac RFE b L G
Luminosity RF AC BS
cm y
PL
E
15-April-05 TRIUMPF 42
Parameter Space
nom low N lrg Y low P
N 1010 2 1 2 2
nb2820 5640 2820 1330
ex,ymm, nm 9.6, 40 10,30 12,80 10,35
bx,ycm, mm 2, 0.4 1.2, 0.2 1, 0.4 1, 0.2
sx,ynm 543, 5.7 495, 3.5 495, 8 452, 3.8
Dy18.5 10 28.6 27
dBS% 2.2 1.8 2.4 5.7
szmm 300 150 500 200
PbeamMW 11 11 11 5.3
L 1034 2 2 2 2
Range of parametersdesign to achieve 21034
15-April-05 TRIUMPF 43
Achieving Maximum Luminosity
nom low N lrg Y low P High L
N 1010 2 1 2 2 2
nb 2820 5640 2820 1330 2820
x,y m, nm 9.6, 40 10,30 12,80 10,35 10,30
x,y cm, mm 2, 0.4 1.2, 0.2 1, 0.4 1, 0.2 1, 0.2
x,y nm 543, 5.7 495, 3.5 495, 8 452, 3.8 452, 3.5
Dy 18.5 10 28.6 27 22
BS % 2.2 1.8 2.4 5.7 7
z m 300 150 500 200 150
Pbeam MW 11 11 11 5.3 11
L 1034 2 2 2 2 4.9!
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Towards the ILC Baseline Design
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e- Beam Transport XFEL
e- Damping Ring
HEP & XFEL Experiments
e- Main LINAC e+ Beam delivery e+ Main LINAC
e+ Damping Ringe- Sources e+ Beam Transport
e- Beam delivery
e+ Source
e- Switchyard XFEL
PreLinac
PreLinac
Beam DumpsDESY site Westerhorn
TESLA machine schematic view
Power Water & Cryogenic Plants
Machine cost distribution
Main LINAC Modules
Main LINAC RF System
Civil Engineering
MachineInfrastructure
X FELIncrementals
Damping Rings
HEP Beam Delivery
AuxiliarySystems
Injection System
1131
~ 33 km
587 546
336241 215
124 101 97
Million Euro
TESLA Cost Estimate3,136 M€ (no contingency, year 2000) + ~7000 person years
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Gradient
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(Improve surface quality -- pioneering work done at KEK)
BCP EP
• Several single cell cavities at g > 40 MV/m
• 4 nine-cell cavities at ~35 MV/m, one at 40 MV/m
• Theoretical Limit 50 MV/m
Electro-polishing
15-April-05 TRIUMPF 48
Gradient
Results from KEK-DESY collaboration
must reduce spread (need more statistics)
single
-cell
measu
rem
ents
(in
nin
e-c
ell
cavit
ies)
15-April-05 TRIUMPF 49
New Cavity Shape for Higher Gradient?
TESLA Cavity
• A new cavity shape with a small Hp/Eacc ratio around35Oe/(MV/m) must be designed. - Hp is a surface peak magnetic field and Eacc is the electric field gradient on the beam axis.
- For such a low field ratio, the volume occupied by magnetic field in the cell must be increased and the magnetic density must be reduced.
- This generally means a smaller bore radius. - There are trade-offs (eg. Electropolishing, weak cell-to-cell
coupling, etc)
Alternate Shapes
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Gradient vs Length
• Higher gradient gives shorter linac – cheaper tunnel / civil engineering– less cavities – (but still need same # klystrons)
• Higher gradient needs more refrigeration– ‘cryo-power’ per unit length scales as G2/Q0
– cost of cryoplants goes up!
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Klystron Development
THALUS
CPITOSHIBA
10MW 1.4ms Multibeam Klystrons~650 for 500 GeV+650 for 1 TeV upgrade
15-April-05 TRIUMPF 52
Towards the ILC Baseline Design
Not cost drivers
But can be L performancebottlenecks
Many challenges!
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Damping Rings
bunch train compression300km 20km
smaller circumference(faster kicker)
higher Iav
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Beam Delivery System
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Strawman Final Focus
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Parameters of Positron Sources
rep rate# of bunches per pulse
# of positrons per bunch
# of positrons per pulse
TESLA TDR 5 Hz 2820 2 · 1010 5.6 · 1013
NLC 120 Hz 192 0.75 · 1010 1.4 · 1012
SLC 120 Hz 1 5 · 1010 5 · 1010
DESY positron source
50 Hz 1 1.5 · 109 1.5 · 109
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Positron Source
• Large amount of charge to produce
• Three concepts:– undulator-based (TESLA TDR baseline)
– ‘conventional’ – laser Compton based
15-April-05 TRIUMPF 61
Remarkable progress in the past two years toward realizing an international linear collider:
important R&D on accelerator systems
definition of parameters for physics
choice of technology
start the global design effort
funding agencies are engaged
Many major hurdles remain before the ILC becomes a reality (funding, site, international organization, detailed design, …), but there is increasing momentum toward the ultimate goal --- An International Linear Collider.
Conclusions