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The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

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Page 1: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

The Energy Frontier and a Lepton Collider

Barry BarishCaltech

Neutrino Oscillations in Venice13-April-08

Page 2: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 2

Answering the Questions

Three 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

• Increasing connections to Astrophysics/Cosmology

Page 3: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 3

Exploring the Terascalethe tools

• The LHC– It will lead the way and has large reach– Quark-quark, quark-gluon and gluon-gluon collisions at

0.5 - 5 TeV– Broadband initial state

• The ILC– A second view with high precision– Electron-positron collisions with fixed energies,

adjustable between 0.1 and 1.0 TeV– Well defined initial state

• Together, these are our tools for the terascale

Page 4: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 4

Three Generations of e+e- CollidersThe Energy Frontier

FourthGeneration?

SPEAR

PETRA

LEP

EN

ER

GY

YEAR 2020

1 Te

V

ILC

1970

1 Ge

V

Page 5: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 5

Possible TeV Scale Lepton Colliders

ILC < 1 TeVTechnically possible

~ 2019

QUADQUAD

POWER EXTRACTIONSTRUCTURE

BPM

ACCELERATINGSTRUCTURES

CLIC < 3 TeVFeasibility?

ILC + 5-10 yrsMain beam – 1 A, 200 ns from 9 GeV to 1.5 TeV

Drive beam - 95 A, 300 nsfrom 2.4 GeV to 240 MeV

Muon Collider < 4 TeV

FEASIBILITY??ILC + 15 yrs?

Much R&D Needed• Neutrino Factory R&D +• bunch merging• much more cooling• etc

ILC

CLIC

Muon Collider

Page 6: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 6

Why e+e- Collisions ?

• Elementary particles

• Well-defined

– energy,

– angular momentum

• Uses full COM energy

• Produces particles democratically

• Can mostly fully reconstruct events

Page 7: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 7

LHC: Low mass Higgs: H MH < 150 GeV/c2

Rare decay channel: BR ~ 10-3

Requires excellent electromagnetic calorimeter performance

acceptance, energy and angle resolution,

g/jet and g/p0 separation Motivation for LAr/PbWO4

calorimeters for CMS

Resolution at 100 GeV: 1 GeV

Background large: S/B 1:20, but can estimate from non signal areas

CMS

Page 8: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 8

ILC: Precision Higgs physics

Model-independent Studies

• mass

• absolute branching ratios

• total width

• spin

• top Yukawa coupling

• self coupling

Precision MeasurementsGarcia-Abia et al

Page 9: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 9

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 10: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 10

What can we learn from the Higgs?

Precision measurements of Higgs coupling

Higgs Coupling strength is proportional to Mass

Page 11: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 11

e+e- : Studying the Higgsdetermine the

underlying model

SM 2HDM/MSSM

Yamashita et al Zivkovic et al

Page 12: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 12

Top Quark Measurements

Bounds on axial ttbarZ and left handed tbW for LHC and ILC compared to deviations in various models

Page 13: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 13

- Measure quantum numbers

- Is it MSSM, NMSSM, …?

- How is it broken?

ILC can answer these questions!

- tunable energy

- polarized beams

Supersymmetry at ILC

e+e- production crosssections

Page 14: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 14

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 15: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 15

– E ~ (E4 /m4 R)– Cost ~ a R + b E

~ a R + b (E4 /m4 R)– Optimization : R ~ E2 Cost ~ c E2

• Circular Machine

Why Linear?cost

Energy

CircularCollider Linear

Collider

– Cost (linear) ~ a L – where L ~ E

R

m,E

SynchrotronRadiation

R

~ 200 GeV

Page 16: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 16

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 17: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 17

ILC – Underlying Technology

• Room temperature copper structures

OR

• Superconducting RF cavities

Page 18: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 18

Superconducting RF Technology

• Forward looking technology for the next generation of particle accelerators: particle physics; nuclear physics; materials; medicine

• The ILC R&D is leading the way Superconducting RF technology– high gradients; low noise; precision optics

Page 19: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 19

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 20: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 20

Luminosity & Beam Size

• frep * nb tends to be low in a linear collider

• Achieve luminosity with spot size and bunch charge

Dyx

repb HfNn

L

2

2

L frep [Hz] nb N [1010] x [mm] y [mm]

ILC 2x1034 5 3000 2 0.5 0.005

SLC 2x1030 120 1 4 1.5 0.5

LEP2 5x1031 10,000 8 30 240 4

PEP-II 1x1034 140,000 1700 6 155 4

Page 21: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 21

• Low emittance machine optics• Contain emittance growth• Squeeze the beam as small as possible

Achieving High Luminosity

~ 5 nmInteraction Point (IP)

e- e+

Page 22: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 22

– 11km SC linacs operating at 31.5 MV/m for 500 GeV– Centralized injector

• Circular damping rings for electrons and positrons

• Undulator-based positron source

– Single IR with 14 mrad crossing angle– Dual tunnel configuration for safety and availability

ILC Reference Design

Reference Design – Feb 2007

Documented in Reference Design Report

Page 23: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 23

RDR Design Parameters

Max. Center-of-mass energy 500 GeV

Peak Luminosity ~2x1034 1/cm2s

Beam Current 9.0 mA

Repetition rate 5 Hz

Average accelerating gradient 31.5 MV/m

Beam pulse length 0.95 ms

Total Site Length 31 km

Total AC Power Consumption ~230 MW

Page 24: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 24

RDR Complete

• Reference Design Report (4 volumes)

ExecutiveSummary

Physicsat theILC

AcceleratorDetectors

Page 25: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 25

US/UK Funding and Future Prospects

• UK ILC R&D Program– About 40 FTEs.  Leadership roles in Damping Rings and

Positron Source, as well as in the Beam Delivery System and Beam Dumps. 

– All of this program is generic accelerator R&D, some of which will be continued outside the specific ILC project.

• US Program– ILC R&D was basically terminated for FY08, but a reduced

level ($42M FY07 ~$35M) program proposed for FY09.

– Presently a broad based U.S. program. Future??

– Generic SCRF also terminated in FY08, but expected to be restored in FY09: broad applications (e.g. Project X at Fermilab; fulure particle accelerators). Primary focus is to build US SCRF capability ($25M proposed for FY09)

Page 26: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 26

The Context

• THE SCIENCE !!!– Nothing has changed. A linear collider remains the consensus

choice as the highest priority long term investment for particle physics

• The Technology– Key technical, design & cost issues must be resolved before a

serious project could be proposed

• Increased Coordination with CERN CLIC R&D Program– A program to work together on areas of mutual interest was

initiated last fall, before the funding problems. – Major areas of cooperative work identified in February

• Conventional Facilities -- Civil, Cooling, Industry, etc• Non main linac technology – Particle sources, beam delivery• Detectors and simulations

Page 27: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 27

Technical Design Phase 1 -- 2010

• Technical risk reduction:– Gradient

• Results based on re-processed cavities• Reduced number 540 390 (reduced US program)

– Electron Cloud (CesrTA)

• Cost risks (reductions) – Main Cost Drivers– Conventional Facilities (water, etc)– Main Linac Technology

• Technical progress (global design)– Cryomodule baseline design is a being developed (e.g.

plug compatible parts)

Page 28: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 28

Technical Design Phase 2 - 2012

• RF unit test – 3 CM + beam (KEK)

• Complete the technical design and R&D needed for project proposal (exceptions*)– Documented design– Complete and reliable cost roll up

• Project plan developed by consensus– Cryomodule Global Manufacturing Scenario– Siting Plan or Process

Page 29: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

ILC – Global Design Phase

2005 2006 2007 2008 2009 2010 2012 ?????

Global Design Effort

Baseline configuration

Reference Design

R&D Program

Technical Design

Siting Studies

International Mgmt

LHCPhysics

Omnibus

Omnibus

Project

Page 30: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 30

ILC Reference Design and Plan

Producing Cavities

Cavity Shape

Obtaining Gradient

Page 31: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 31

Cavity Gradient – Results

KEK single cell results:2005 – just learning2006 – standard recipe2007 – add final 3 μm fresh acid EPNote: multi-cells are harder than singles

2005

2007

2006

Page 32: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 32

Superconducting RF Cryomodule

Page 33: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 33

ILC Reference Design and Plan

Making Positrons6km Damping Ring

10MW Klystrons

Beam Delivery and Interaction Point

Page 34: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 34

Electron cloud – Goal

• Ensure the e- cloud won’t blow up the e+ beam emittance.– Do simulations (cheap)– Test vacuum pipe coatings, grooved

chambers, and clearing electrodes effect on e- cloud buildup

– Do above in ILC style wigglers with low emittance beam to minimize the extrapolation to the ILC.

Page 35: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 35

E Cloud – Results

SLAC

Page 36: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 36

~30 km long tunnel

Particle Detector

Main Research Center

Two tunnels • accelerator units• other for services - RF power

Linear Collider Facility

Page 37: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 37

Conventional Facilities

72.5 km tunnels ~ 100-150 meters underground

13 major shafts > 9 meter diameter

443 K cu. m. underground excavation: caverns, alcoves, halls

92 surface “buildings”, 52.7 K sq. meters = 567 K sq-ft

Page 38: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 38

Detector Concepts Report

Page 39: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 39

Detector Performance Goals

Page 40: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 40

Detector Performance Goals

Page 41: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 41

Detector Performance Goals

• ILC detector performance requirements and comparison to the LHC detectors:○ Inner vertex layer ~ 3-6 times closer to IP

○ Vertex pixel size ~ 30 times smaller

○ Vertex detector layer ~ 30 times thinner

Impact param resolution Δd = 5 [μm] + 10 [μm] / (p[GeV] sin 3/2θ)

○ Material in the tracker ~ 30 times less

○ Track momentum resolution ~ 10 times better

Momentum resolution Δp / p2 = 5 x 10-5 [GeV-1] central region

Δp / p2 = 3 x 10-5 [GeV-1] forward region

○ Granularity of EM calorimeter ~ 200 times better

Jet energy resolution ΔEjet / Ejet = 0.3 /√Ejet

Forward Hermeticity down to θ = 5-10 [mrad]

Page 42: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 42

detectorB

may be accessible during run

accessible during run Platform for electronic and

services (~10*8*8m). Shielded (~0.5m of concrete) from five sides. Moves with detector. Also provide vibration isolation.

Concept of IR hall with two detectors

The concept is evolving and details being worked out

detectorA

Page 43: The Energy Frontier and a Lepton Collider Barry Barish Caltech Neutrino Oscillations in Venice 13-April-08

11-Feb-08 Harvard Colloquium

The International Linear Collider 43

Conclusions

• The energy frontier continues to be a primary tool to explore the central issues in particle physics

• The LHC at CERN will soon open the 1 TeV energy scale and we anticipate exciting new discoveries

• A companion lepton collider appears to be the logical next step, but such a machine has technical challenges and needs significant R&D and design now

• LHC results will inform the final design and even whether a higher energy options is needed, If so, this may also be possible, but on a longer time scale.