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DIS06 Tsukuba April 23 rd 2006 John Dainton THE COCKCROFT INSTITUTE of ACCELERATOR SCIENCE and TECHNOLOGY Large Hadron electron Collider LHeC … 1.Introduction 2. LHeC: “energy, precision and luminosity 3. The Physics Horizon 4. Experiment 5. Onwards ? John Dainton * Cockcroft Institute, Daresbury Science and Innovation Centre, GB http:// www.lancs.ac.uk/cockcroft -institute/ … indisputably the next step Deep-Inelastic Lepton Scattering at the LHC * with M Klein (DESY Zeuthen) P Newman (Univ Birmingham), E Perez (CE Saclay) F Willeke (DESY Hamburg) ep-ex/0603016 DESY 06-006 Cockcroft-06-05

THE COCKCROFT INSTITUTE of ACCELERATOR SCIENCE and TECHNOLOGY DIS06 Tsukuba April 23 rd 2006 John Dainton Large Hadron electron Collider LHeC … 1.Introduction

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DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Large Hadron electron Collider

LHeC …

Large Hadron electron Collider

LHeC …

1. Introduction2. LHeC: “energy, precision and luminosity”3. The Physics Horizon4. Experiment5. Onwards ?

John Dainton*

Cockcroft Institute,Daresbury Science and Innovation Centre, GB

http://www.lancs.ac.uk/cockcroft-institute/

… indisputably the next step

… indisputably the next step

Deep-Inelastic Lepton Scattering

at the LHC

Deep-Inelastic Lepton Scattering

at the LHC

*with M Klein (DESY Zeuthen)P Newman (Univ Birmingham),

E Perez (CE Saclay)F Willeke (DESY Hamburg)

hep-ex/0603016 DESY 06-006 Cockcroft-06-05

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

1.Introduction1.Introduction

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

2007: a vintage year for Physics2007: a vintage year for Physics

●July 2007: final HERA data samplee± p chiral probe @ 0.001 fm

●July 2007: first collisions @ LHCpp @ 14000 GeV @ 1033 cm-2 s-1

●July 2007: hitherto unique p and A beam7 TeV per nucleon, high intensitynew opportunities ?

LR

20??: 70 GeV e± in LHC tunnele± p chiral probe @ 0.00014 fm

LR?

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGYKinematic ReachKinematic Reach

●70 7000 GeV e± p cm energy 1400 GeV

Z W

e

RL

quark structure@ ≥ 0.0001 fmquark structure@ ≥ 0.0001 fm

space-like >TeV

?

?

eq >TeV

3×10-7

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Structure of MatterStructure of Matter

dstructure q = 2/

electron point-like “source”

Z0 W

nu

cle

us

nu

cle

on

qu

ark

NC

+C

C+

glu

on

●LHeC

glu

on

s E

W

?

●unique chiral probe @ 0.0001 fm ?

●precision

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

SM

-0.0001

-0.0003

-0.001

-0.003

-0.01

-0.03

-0.1

e+e-.

Progress … ?Progress … ? (fm)

1960 1970 1980 1990 2000 2010 ….?

.ep p SLAC+CERNquarks in proton NC P

ep

QPM

HERA

QCD+EW

EW QCD .. LQ

l*

q*

SU

SY

?Q

CD

+EW

un

ificati

on

HF+

EW

ep eA

QCD spin gluon

leptons+ quarks

hadronic mass in Universe

Higgs mass

CKM

?

?

?.p p A

beyond?

CERN+FNALHERA

epeA

LH

eC

?

epeA

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

2. LHeC: “energy, 2. LHeC: “energy, 2. LHeC: “energy, precision

2. LHeC: “energy, precision

2. LHeC: “energy, precision

and luminosity”

2. LHeC: “energy, precision

and luminosity”

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGYProton beamProton beam

●”standard” LHC protons

protons

antiprotons

protons

Np

εpN

… with electrons?

protonselectrons?

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGYep Luminosityep Luminosity

●few 10s GeV electrons (LEP = 70 GeV!) ●RF power = 50 MW = 0.86 LEP = 28% CERN site

●RF power = synchrotron radiation Ie = 74 mA

luminosity

74×10-3×1.67×1011×7000/.9384π×1.6×10-19×3.75×10-6×=

L = 1.15×1033/ (m2) cm-2 s-1

L ~ 1033 cm-2s-1 for reasonable p-beam β ~ 1 m

“per

fect

bunch x-

ing

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

●LLHeC e±p@ 0.00014 fm

●LLHeC e±p@ 0.00014 fm

e±p Luminositye±p Luminosity

●astounding !

●×102 LNMC

@ 0.01 fm

●×102 LNMC

@ 0.01 fm

●LeRHIC

@ 0.007 fm

●LeRHIC

@ 0.007 fm

indisputably the next step … is it feasible ?

●×102 LHERA

@ 0.001 fm

●×102 LHERA

@ 0.001 fm

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Feasible Luminosity ?Feasible Luminosity ?

●bunch matching βeεe = βpεp = βpγp

●electron βe constrained by depth of focus for p-bunches σp ~ 7 cm

●electron emittance εe constrained by- dynamic aperture- geometric aperture- beam-beam tune shifts

feasible match with tolerable “hour-glass” loss

σp

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGYLHeC SpecificationLHeC Specification

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Lepton RingLepton Ring

●in LEP tunnel so like LEP- FODO in eight arcs β-tron phase advance φH=108o φV=90o

- bending radius 3005.3 m- (δE/Ebeam)rms = 1.1×10-3

- SR 26 W/cm (Ec=254 KeV)- scRF @ 1GHz resonators @ 12 MV/m 100 m structure = 670 cells

sync. Phase 31o

bucket takes 10× (δE/Ebeam)rms - unlikely e-beam instability single bunch current modest impedance << LEP

LEP=9 W/cmHERA=13.5 W/cm

scRF proven@ 6 MV/m

1

2

3 4

5

6

78

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGYLepton RingLepton Ring

LHeC

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGYep Collisionsep Collisions

●after B physics @ LHC

during pp pA AA data-taking @ LHC

p

e

civil engineeringtunnel 2×250m×2m Ø @IP

civil engineeringtunnel 2×250m×2m Ø @IP

LHeC

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Interaction RegionInteraction Region

●highest lumi

- low βe

close sc quads

- low x-ing angle“hard” bend

SR fan sc p-beam « HERA

- “crab” RF cavity p-bunch rotation

3.5 mrad0.5 mrad

V-displaced

top elevation

11.4 kW

3.4 kW 3.2 kW

●1o beam access = low-lumi/low-x option (cf HERA)

“crabbed”(rotated)p-bunch

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Interaction RegionInteraction Region

●high luminosity operation

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

●beam-beam- “hour-glass”- dynamic β: < HERA- long range beam-beam (parasitic interactions):

marginal

Operational Luminosity

Operational Luminosity

operational luminosity

!

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

IR and ExperimentIR and Experiment

●IR ±many m

●IR ≥9.4o around beam

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

LHeCLHeC

●tunnel exists (LEP, LHC)

●injection once existed (LEP)

●operating p-beam (from 2007)

●operating A-beam (from 2007)

●ep operating alongside pp pA AA

●LHC upgrade●cost ?

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

3.The Physics Horizon

3.The Physics Horizon

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

New Kinematic Reach in Lepton-Hadron

New Kinematic Reach in Lepton-Hadron

space-like >TeV

eq >TeV

3×10-7

●Q2LHEC 102Q2

HERA

●xLHEC 10-2xHERA

●sLHEC 20sHERAeq eq

●extrapolation … …or interpolation ?

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Lepton-Parton and Parton-Parton

Lepton-Parton and Parton-Parton

●sLHC 102×sLHeC70 GeV

●for target parton

xprobe/proton =

= 0.01 @ LHC

sLHeC

sLHC

●LHC probe - confused LHC>LHeC - complementary for LHC~LHeC gluon @ low-x

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Energy FrontierEnergy Frontier

LQe

q …

e

q

Z

e

q

e

2

+

LQ+q

e

●leptoquarks

100 fb-1

10 fb-1 (1 year @ LHeC)

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Energy FrontierEnergy Frontier

LQe

q …

e

q

Z

e

q

e

2

+

LQ+q

e

●leptoquarks

- formation and decay-e±qNC,CC

- fermion number

- branching ratios

- spin-parity

- chirality ?

- flavourcoupling

●if LQ spectroscopy discovered precision tools to understand it

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Dense Chromodynamics

Dense Chromodynamics

●relentless low-x rise of F2 for x ≥ 10-4

- saturation? partons must someday recombine

- LHeC: precision for x > 3×10-7: extreme nuclei ?(∂F2/∂ lnx)Q2

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Precision Chromodynamics

Precision Chromodynamics

●short distance structure of QCD

- 2006 @ 10-9

- 2006 GF @ 10-5

- 2006 G @ 0.1%

- 2006 S @ 1-2%

- LHeC precision S

few/mil

●discovery + precisionprobe new chromodynamic physics ?

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Comprehensive Physics HorizonComprehensive Physics Horizon

●energy foreq discoveryextreme chromodynamics

●precision foreq discoveryeq understandingextreme chromodynamics

●luminosity foreq discovery

LHeC and LHC

LHeC and ILC

LHeC and LHC

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

4. Experiment

4. Experiment

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

Acceptance and Measurement

Acceptance and Measurement

e

!

●70 7000 GeV

●high lumi quads (±10o bp) Q2 > 100 GeV2 x > 3×10-5

●few GeV ≤ Eh,e ≤ few TeV

●low lumi for low x (no quads) 1 < Q2 < 100 GeV2

x < 3×10-5

“forward” hadrons:

“forward rapgap” instrumentation precision e/had-measurement

170 < θe < 179o 170 < θh < 179o

jete

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGYRateRate

●100/10 fb-1

= 100/LHeC y-1

@ Q2 = 1 TeV2

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

8. Onwards ?8. Onwards ?

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

NowNow

●LHeC 70e 7000p GeV

- can be built

- has startlingly good luminosity 1033 cm-2s-1

grows with LHC pp luminosity

- adds substantially, uniquely and with synergy to LHCTeV energy physics

- probes chromodynamics@ new density frontier in uniquely comprehensive mannerwith unchallengable precisionsynergetically with LHC pp pA AA

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

NowNow

●CERN: Engelen “work it out!” Fall 2005

●hep-ex/0603016CERN Council (CC) Strategy group - emphasised by speakers - encouraging individual response●hep-ex/0603016 noted in the US DoE strategy: meeting now on lepton-hadron

●strong interest in LHeC @ DIS2006 … to be carried to CERN Strategy group by its members @ DIS2006 - implies global support - confirms importance of breadth in future HEP

CC Strategy Group “interesting to work it out”

??

Jan 2006Jan 2006

April 2006April 2006

May 2006May 2006

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

NextNext

●begin preparation of detailed evaluation- establish global working group (CERN pivotal)

1. machinee± injectione± ringLHC impact and modifications

2. experiment3. physics

●look for any remaining “showstoppers”●prepare CERN “white book”

●LoI to LHCC

●cost

2009 ?

other LHC upgrades ?

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGYCoordinating GroupCoordinating Group

●organisation ?

●coordinator(s) ?

●first meeting where ?

●first meeting when ?

●first meeting to organise work + schedule

DIS06TsukubaApril 23rd 2006John Dainton THE COCKCROFT INSTITUTE of

ACCELERATOR SCIENCE and TECHNOLOGY

In case you were wondering … ?

In case you were wondering … ?

Sir John Cockcroft …

doing accelerator physics ca 1950 …

… with 1950 DAQ – pencil and paper!

… with 1950 graphics – ammeter! voltmeter!