Future HERA High Luminosity Performance

Post on 14-Jan-2016

21 views 1 download

Tags:

description

Future HERA High Luminosity Performance. H1. Georg H. Hoffstaetter and Ferdinand Willeke (DESY, Hamburg). 778 m. 29 March 2001. HERMES. HERA. HERA-B. Protons Electrons. 6336 m long 920 GeV protons 27.5 GeV electrons / positrons. PETRA. ZEUS. HERA: Improvements 1999/2000. - PowerPoint PPT Presentation

Transcript of Future HERA High Luminosity Performance

Georg.Hoffstaetter@DESY.de

Future HERA High Luminosity Performance

Georg H. Hoffstaetter and Ferdinand Willeke

(DESY, Hamburg)

29 March

2001

H1

ZEUS

HERMES

HERA-B HERA

PETRA

ProtonsElectrons

778 m

6336 m long

920 GeV protons

27.5 GeV electrons/positrons

Georg.Hoffstaetter@DESY.de

pe

HERA: Improvements 1999/2000Start luminosityandBeam currents:

Efficiency%

Average over month

mA

Georg.Hoffstaetter@DESY.de

Development of the Luminosity

Inte

grat

ed L

umin

osity

(1/

pb)

HERA Luminosity 1993-2000

Linear increase of the integrated Luminosity

The time for a luminosity upgrade of HERA has come

Days after start of run

Georg.Hoffstaetter@DESY.de

Th e Detec to r R

e gion

courtesy B.Holzer courtesy B.Holzer

Geo

rg.Hoffstae

tter@D

ES

Y.de

Georg.Hoffstaetter@DESY.de

Superconducting Magnet GO

Geo

rg.H

offs

tae

tter

@D

ES

Y.d

e

Georg.Hoffstaetter@DESY.de

Potential Problems

Dynamic Aperture OK? Polarization OK?, Luminosity OK? Can HERA be handled well?

Polarization OK?, Luminosity OK?

Too strong beam-beam force on p? Too strong beam-beam force on e?

Focusing:

fRF increase:

Georg.Hoffstaetter@DESY.de

The Luminosity was initially too small: Lumiscan

Emittance and Lumi for 72° Optic

)60( sL

)60( sL )72( sL

)72( sL

)(mmx )(mmx)(mmy )(mmy

Bunch has no product distribution: )()( yx coupling

)72( sL

)72( sL

x

y

Luminosity with 72° is large as expected

Georg.Hoffstaetter@DESY.de

Dynamic Aperture for 72° Optic

The kick where half the current is lost leads to a satisfactory dynamic aperture.

Kickx

x´ V2(kV)

Georg.Hoffstaetter@DESY.de

Polarization was in the spin matched 72° optic quickly brought to 63% (one day).

Harmonic bumps were immediately effective Decoupling bumps worked well

60%

PolarizationIe

Polarization for 72° Optic

Georg.Hoffstaetter@DESY.de

6 more measurements indicate For the center frequency , the

luminosity is increased as expected

Luminosity for fRF IncreaseLL

RFf RFf

HzfZentrum 175

HzfZentrum 175

HzfZentrum 175HzfZentrum 0

Georg.Hoffstaetter@DESY.de

Ls is independent of e-current Tp depends on e-current Tails depend on

e-current

Too Strong Beam-Beam Force on p?16mA 73mACorresponding e-current after upgrade

Georg.Hoffstaetter@DESY.de

Too Strong Beam-Beam Force on e?

No reduction of Ls by the second experiment

No reduction of Ls by a larger -funktionen

Ls

Ippb

So far no reduction of Ls by the

bunch current

Georg.Hoffstaetter@DESY.de

)(mey

measureds,L

Where are the Beam-Beam Limits?

Upgrade and Ip=140mA: emittance starts to grow

)(mey

yQ2

xQ2

)(mey

emeasuredx,

emeasuredy ,

)(mey

)( ,ecalcys L

measureds,L

)( ,emeasuredys L

Georg.Hoffstaetter@DESY.de

Lumi Reduction by Hourglass Effect

)(cmpy

ep

75.1)5.12(

0L

L cmpyLength 19cm:

12cm: 9.1)5.12(

0L

L cmpy

Luminosity ( )3210

20cm

bunch length: 6cm

30cm

Georg.Hoffstaetter@DESY.de

Tune Shift with Bunch Length Effect

How will the tune shift parameters change and have these been analyzed by accelerator experiments ?

Georg.Hoffstaetter@DESY.de

Resonances with Bunch Length EffectHow will the resonance strength change and have these been analyzed by accelerator experiments ?

All large resonance strength are due to the proton bunch length

Georg.Hoffstaetter@DESY.de

Nominal and Ultimate Parameters

The performance goal of HERA is not unrealistic and should not be too hard to achieve.

A shortfall of beam intensity in the short term can be compensated.