tevatron status

54
Tevatron Status Mike Martens V. Shiltsev, J. Annala, K. Bishofberger, B. Hanna, P. Ivanov, R. Moore, V. Ranjbar, J. Steimel, D. Still, C.Y. Tan, R. Tokarek, J. Volk, A. Xiao, X. Zhang, M. Syphers, Y. Alexahin, V. Lebedev, J. Johnstone, M. Xiao, N. Gelfand, L. Michelotti, D. Edwards, T. Sen, B. Erdelyi, A. Drozhdin, N. Mokov, P. Bauer UTev Seminar June 6, 2003

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Tevatron Status. UTev Seminar June 6, 2003. Mike Martens - PowerPoint PPT Presentation

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Page 1: Tevatron Status

Tevatron Status

Mike Martens

V. Shiltsev, J. Annala, K. Bishofberger, B. Hanna, P. Ivanov, R. Moore, V. Ranjbar, J. Steimel, D. Still, C.Y. Tan, R. Tokarek, J. Volk, A. Xiao, X. Zhang, M. Syphers, Y. Alexahin, V. Lebedev, J. Johnstone, M. Xiao, N. Gelfand, L. Michelotti, D. Edwards, T. Sen, B. Erdelyi, A. Drozhdin, N. Mokov, P. Bauer

UTev Seminar June 6, 2003

Page 2: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 2

Talk Outline

Introduction to luminosity and the Tevatron.

Recent performance of the Tevatron.

Tevatron physics issues.

Plans for the near future.

Page 3: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 3

Luminosity

Pint = Nprotint /A

Rate = L int

A

int

pbars

protons

L = frevNpbar Nprot/A

Page 4: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 4

Low Beta Lattice

Page 5: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 5

Hourglass shape

Beta x in the IR

0

200

400

600

800

-150 -100 -50 0 50 100 150

S in cm

beta

x i

n c

mx = x

* + (s-s0)2/ x*

x2 = xx(s)

Protons Pbars

For 20 mm-mrad emittance,xm (rms).

Page 6: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 6

Luminosity Integral

L = 2 frev 1 2 dx dy dz d(ct)

(x,y,z,ct) =

exp[- (y+y/2)2/ 2y2]

Hourglass shape: Cogging offset: Separated Orbits:x

2 = xx(z) center of beams x = z tan(x) + xo

y2 = yy(z) collide at z = ct0/2 y = z tan(y) + y0

exp[- (x+x/2)2/ 2 x2]

exp[ -(z+ct-ct0)2/ 2z2]

N1

2 x

12 y

12 z

Page 7: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 7

Luminosity Formula

L = F(z / *, x, y)frev BNp Np

2 * (1 + 2 )-

Major limitations: Np/ 1 = Protons beam brightness (Beam-beam tune shift.) BNp = Total number of antiprotons (Stacking rate.)

* = 35 cm is fixed by lattice. 20 mm-mrad (95%, normalized).z = Bunch length.B = Number of bunches.x, y = Crossing angles (during 132 nsec operations.)

F = Form factor 1 for 36 x 36 = ~0.5 for 132 nsec.

Page 8: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 8

• Beam IntensitiesNprot, Npbar

• Beam Emittancesx, y, z, ,p/p (Proton)

x, y, z, p/p (Pbar)

• Lattice Functions*

x, *x, *

x, ’x*

y, *y, *

y, ’y

• Separated orbitsx, x, y, y

• Cogging offset, revolution frequencyct0, frev

24 factors in the luminosity integral!

Factors in the luminosity integral:

Page 9: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 9

Run II Bunch Configuration

36 x 36 configuration

396 nsec bunch spacing

3 x 12 proton bunches

3 x 12 pbar bunches

Page 10: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 10

Beam-beam tune shifts

Horizontal tune shift

Ver

tical

tun e

sh i

ft

Tune Shift of a pbar bunch from 2 head on collisions

Tune shift becomes too large with more than 2 head-on collisions.

Solution is electrostatic separators.

Page 11: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 11

Tevatron Separators

Protons

C0

B0

A0

D0

F0

E0 Antiprotons

H,V

H,V

H,VH,V

H

H

V

VElectrostatic separators are used to separate the proton and pbar orbits transversely …except at the IPs where the protons and pbars collide head-on.

Page 12: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 12

Tevatron Efficiencies

protoninjections

pbarinjections

rampOpen helix

poor lifetimes

10% bunchedbeam loss in ramp

and squeeze

Page 13: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 13

Luminosity Since June 2002

• 225 HEP stores

• 212 pb-1 to each detector

• Increase in luminosity from 15e30 to 40.5e30

• Run I record of 25.0e30 broken on 7/26/2002

• Run II record of 44.8e30 set on 5/17/2003

Peak LuminosityAverage of CDF and Dzero at start of store

0.0

10.0

20.0

30.0

40.0

50.0

J un-02 Aug-02 Nov-02 Feb-03 May-03

Date

Peak

Lum

(e3

0)

Avg lumi (e30)

20x running average

Pbar

coa

lesc

ing

fixe

d

BLT

Shu

tdow

n

Page 14: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 14

Beam Intensities

Number of antiprotons

Increase factor of 2.5 Oct March

from 9e9 25e9 per bunch

Number of protons

Mostly steady

in the 200e9 range 250e9 max

Protons at start of HEP

0

2000

4000

6000

8000

10000

J un-02 Aug-02 Nov-02 Feb-03 May-03

Date

Tot

al p

roto

ns (

E9)

Pbars at start of HEP

0

200

400

600

800

1000

J un-02 Aug-02 Nov-02 Feb-03 May-03

Date

Tot

al p

bar

s (e

9)

250e9/bunch

25e9/bunch

Linac, Booster, MI

improvements

Page 15: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 15

Tevatron Emittance

General comments on emittance blow-up from Flying Wire measurement**

(95%, normalized emittances):

• < 1 - 2 at proton injection • ~ 5 - 6 at pbar injection• < (negative) 2 - 3 protons at 150 (scraping)• ~ (negative) 0 -3 pbars at 150 (scraping)• 4 -7 blowup on ramp (prots and pbars)• occasional instability, 5 – 50, at 980 Gev** There remains uncertainty of FW emittance measurements. (See later slides)

Page 16: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 16

Reasons for L-progress Since Jun’02

• “Shot lattice” AA x 1.40• Pbar emittance at injection Tev/Lines x 1.20• Pbar coalescing improvement MI x 1.15 • Shoot from larger stacks x 1.10• Improved Tev Pbar efficiency x 1.10• More Protons at Low Beta x 1.10

totaltotal x 3.3 x 3.3

….plus additional improvements in the Tevatron:• Tunes/coupling/chromaticities at 150/ramp/LB• Orbit smoothing• Longitudinal dampers to stop s blowup• Transverse dampers improves 150 Gev lifetime• F11 vacuum

Page 17: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 17

Goals and Current Performance

Current Record FY03 Parameter Status Store Goal Typical Luminosity 3.5e31 4.5e31 6.6e31 cm-2sec-1

Integrated Luminosity 6.0 12.0 pb-1/weekProtons/bunch 200e9 240e9 240e9Antiprotons/bunch 22e9 25e9 31e9

Higher intensity Fundamental physics limitations– Beam-Beam Effects– Instabilities– Beam Halo and Lifetimes

Understanding/Solving these issues requires …– Stable Tevatron Lattice– Diagnostics– Study Time

Page 18: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 18

Integrated Luminosity FY 2003

150 pb-1 to each detector

Record integratedluminosity

9.1pb-1/week

Page 19: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 19

Beam-beam Interaction As Major Factor

• Pbar transfer efficiency strongly depends on N_p, helix separation,

orbits, tunes, coupling, chromaticity and beam emittances at injection

• Summary of progress with beam-beam since March 2002:

Mar’02 * Oct’02 ** Jan’03 ***

Protons/bunch 140e9 170e9 180e9

Pbar loss at 150 GeV 20% 9% 4%

Pbar loss on ramp 14% 8% 12%

Pbar loss in squeeze 22% 5% 3%

Tev efficiency Injlow beta 54% 75% 75%

Efficiency AAlow beta 32% 60% 62%

* average in stores #1120-1128 ** average in stores #1832-1845*** average in stores #2114-2153 (9 stores)

Page 20: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 20

Beam-beam Effects: Pbar Only

8% loss on ramp – DC beam (depends

on MI tuneup)

Page 21: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 21

Attacking the Beam-beam Effects

• Smaller emittances from AA (“AA shot lattice” )

• Reduced injection errors

– Beam Line Tuner

• Better control of orbits / tunes / coupling

– Tunes up the ramp

– Tune and coupling drift at 150 Gev

– Orbit smoothing

• Larger injection helix

– C0 Lambertson replacement

– New Separator settings

Page 22: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 22

Beam-beam @ Injection Vs Emittance

Lifetime of 12 pbar bunches: A1-A4 are injected first with emittances of 32 pi mm mrad – lifetime is 0.95 hr2.4 hrs; the second set of bunches A13-16 with emittance of 12pi had 4 hours lifetime; and the 3rd train A25-28 with emittances of about 18 pi mm mrad had some 3.2 hr lifetime.

M.Martens

Page 23: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 23

Antiproton Lifetime at 150 Gev

@ 150 GeV

Pbar losses depend strongly on pbar emittances and N_p

A

Proton

bunches

Proton Beam as Proton Beam as “Soft Donut “Soft Donut Collimator”Collimator”

Page 24: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 24

Injection Oscillations in Tevatron

Bunch 1 Bunch 2 Bunch 3 Bunch 4

__________________Antiprotons_______________

• Turn-by-turn position monitor, (and bunch-by-bunch for pbar)• Use to tune up injection closure• 1 mm corresponds to roughly 3-4 emittance blowup

• Improved Pbar emittance blowup by ~3-5

Turn number0 256

Hor

z (m

m)

Ver

t (m

m)

3 m

m

Page 25: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 25

Tune/coupling/chromaticity/orbits

• Tune up is essential for consistent operations … – Much effort during “Studies Periods” is actually

maintenance (orbit smoothing and tune/coupling/chromaticity adjustments)

• … and for understanding more complicated physics– Beam-beam effects, instabilities and dampers, beam

lifetimes, beam halo rates, etc. are more difficult to understand when machine parameters drifting.

• Some troubles:

– Tune/coupling drifts at 150 Gev. (Now compensated.)

– Tune/coupling snapback on the ramp. (Now compensated.)

– Chromaticity snapback? (Was measured. Is OK.)

– Orbit drifts. (Started BPM and smoothing improvements)

Page 26: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 26

Tune Drift @ 150 Gev

M.Martens, J.Annala

Page 27: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 27

Coupling Drift @ 150 Gev

M.Martens, J.Annala

Page 28: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 28

Tune Variations on Ramp/squeeze

• Near start of ramp (150 153 Gev): large tune/coupling excursions• Tune/coupling changes of (0.02 tune units, 0.02 minimum tune split)• Variations fixed with additional breakpoint at 153 Gev and tune/coupling snapback correction at start of ramp.

0.02

tune units

After fixes

Desired tunes (red lines) at

0.575 and 0.583

153 Gev

Page 29: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 29

Measured b2 in the Tevatron dipolesat start of the ramp after 20 minute front porch

-5

-4.5

-4

-3.5

-3

-2.5

-2

0 5 10 15 20 25

Time from start of ramp (sec)

Mea

sure

d b

2

Measured b2, w ith snapback

Measured b2, no snapback

3rd order f it of b2, no snapback

Chromaticity Snapback Measurements

M.Martens, J.Annala, P. Bauer

Measured b2

Estimated b2 without snapback

Page 30: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 30

Comparison of measured and applied snapback for 20 min and 120 min front porch

-0.5

0

0.5

1

1.5

2

0 2 4 6 8 10 12

Time from start of ramp (sec)

b2

sn

ap

ba

ck

Meas b2 - 3rd order f it, 120 min FP

Applied b2 snapback, 120 min FP

Meas b2 - 3rd order f it, 20 min FP

Applied b2 snapback, 20 min FP

Chromaticity Snapback Compensation

M.Martens, J.Annala, P. Bauer

b2 snapback is correctly compensated (for shot setup conditions.)

15

0 G

ev

19

5 G

ev

Page 31: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 31

Orbit Drifts

Tunes, coupling, vary with closed orbits distortions

“Rule of thumb” -- keep orbit drifts under 0.5 mm rms from “silver orbit”

Orbit drifts of that scale occur in 1-2 weeks (see picture) Requires routine orbit smoothing at 150 Gev, ramp, flat-top, squeeze, and low-beta.

 

“orbit – reference” at low beta after about 2 weeks in

September’02

Page 32: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 32

Motion of Tevatron Dipole

Newly added a tiltmeter to a Tevatron dipole.

Observed 10 urad roll after a quench

Still watching!!

Larger rolls on other dipoles?

Long term drifts?

 

Roll of E35-1 dipole after a

Tevatron quench.

Measu

red r

oll

(ura

d)

-75

-70

-65

-60

-55

Tevatr

on

qu

en

ch

1 day

Page 33: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 33old helix opened vertically 130%

current helix

proposed helix

Helix Improvement

Current helix

Proposed helix

Distance from B0 Distance from B0

Dia

gonal se

para

tion S

Aperture limitation at

C0

Increasing proton/pbar helix separation

• Replace C0 Lambertson with MI magnets

• Increase vertical aperture at C0 from ~15mm -> 40 mm (but only ~30% larger helix due to other aperture limitations.)

• Modify helix to increase min separation, Smin, from 5.5 to 6.6

22 )/()/( yx yxS

Page 34: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 34

C0 Lambertson Replacement

Pbar lifetime depends on emittances and helix size.

C0 Lambertson is severest aperture restriction. (See picture)

Design injection helix modified and optimized to fit tight C0 aperture (“new-new helix”)

(Jan 2003) Replace C0 LambertsonsGain 25 mm vertically

Vertical aperture 13-16 m

m

Protons 1 and 3 sigma

Pbars 1 and 3 sigma

7mm

Proton and pbar beam position and sizes on the helix at the location of C0 Lambertson

Page 35: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 35

Beam-beam Tune Shift Reduction

Calculated Pbar tune shift (by bunch)

0

0.0005

0.001

0.0015

0.002

0.0025

-0.001 0 0.001 0.002 0.003

Horz tune shift

Ver

t tu

ne

shif

t

Current Helix Proposed Helix

Proposed injection helix (with larger C0 aperture) will reduce small amplitude tune shift of pbars

Page 36: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 36

Proton Lifetime Issues at 150 Gev

• Poor proton lifetime on helix ~ 2 hr

– depends on chromaticity

– Instability prevents lower chromaticity (now 8)

– Orbits/size of helix affect lifetime

– Tunes/coupling are a factor

Page 37: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 37

Loss rates (LOSTP) versus chromaticity

0400800

120016002000

0 2 4 6 8

Horizontal Chromaticity

Loss

rat

es (

Hz)

Lifetime and Chromaticity at 150 Gev

Loss rates (LOSTP) versus chromaticity

0

400

800

1200

1600

0 2 4 6 8

Vertical Chromaticity

Loss

rat

es (

Hz)

• Lower chromaticity is better for lifetime

• Instabilities appear < 3-4

• Run with H = 8, V=8 to avoid instabilities

• Dampers allow us to lower chromaticity and improve lifetime

Measured loss rates as function of chromaticity (with protons on the pbar helix)

Page 38: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 38

0 200 400 600 800 1000 1200 1400 1600 1800 20004

2

0

2

43.213

3.4

xj 10

A j 10

A j 10

1.964 1031 j

Turn Number

Am

plitu

de

Unstable Head-tail Motion

Developing head-tail instability with monopole configuration Beam is unstable for x 6, y -3Longitudinal and transverse dampers OFFNp= 260E9

5725.0,5857.0,3,6,106.2 11 yxyxN

Page 39: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 39

Transverse Instability

• Beam remnants point to coherent betatron mode with l=2

beamremainppb

Nbeaminitppb

N .111003.1.11106.2

P.Ivanov, A.Burov

Page 40: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 40

0 200 400 600 800 1000 1200 1400 1600 1800 20001

0.5

0

0.5

10.606

0.636

xj 10

A j 10

A j 10

1.964 1031 j

Turn Number

Am

plitu

de

Unstable Head-tail Motion

Observed transverse oscillation for stable conditionsBeam is stable for x 8, y 8Longitudinal and transverse dampers OFFNp= 260E9

5736.0,5850.0,2,8,106.2 11 yxyxN

Page 41: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 41

TeV Transverse Damper

AutoZero

Δ

VCO

NotchFilter

1.9 MHz

GainControl

VCO

Δ

To 5kWInjectionDamper

Power Amps

From pbar damper signal

Page 42: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 42

Mountain Range DisplayMountain Range Display

19 ns

Longitudinal Impedance – “Dancing Bunches”

• Beam in 30 buckets

• 100 Tevatron turns (~2 ms) between traces

• Synch freq ~ 85 Hz

• Oscillation amplitude depends on bunch, changes slowly with time (minutes at 150 GeV, seconds at 980 GeV)

• Model needs inductive impedance Z/n2 Ohm interplaying with cavity impedance

• Coalesced bunches have dancing bumps

R.Moore

Page 43: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 43

TeV Longitudinal Damper Block

Digital Delay

Digital Delay

-To FanoutPhase Shifter

1 turn

53 turns

90° Delay

Beam In

VCO

100 MHz

30 MHz

I

Q

GainControl

1.5 MHz

CavityCompensation

Page 44: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 44

Bunch Length Blowup During Stores

Before damperBefore damper With damperWith damper

blow up ~10%

Bunchlength

(ns)

DCIntensity

(E12)

no sudden jumps over entire store

• Intensity-dependent, leads to significant CDF background rise• Usually only one or a few bunches would suffer• Problem solved by bunch-by-bunch longitudinal damper

J.Steimel, C.Y.Tan

Page 45: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 45

Diagnostics Progress: SyncLite Monitor

H.Cheung

Bunch #1 Bunch #8

•Works >800 GeV

•Significant progress since March’02

•Reports rms, mean, N, tilt bunch-by-bunch for both protons and pbars

•Invaluable instrument

Page 46: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 46

Diagnostics: Flying Wires

• Proton channels tuned up in March

• Still some (15% ?) calibration needed

• Pbar channels data are subject of correction

• “Jumping” emittances

• (improper dP/P?)

• Recalibration of both p and pbar channels is due

• Need raw data

#1828, injection

Page 47: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 47

Tev Scraping Studies

ma

eB

yt

is

ne

ts

nI

T:

VB

AA

LS

Vertical prot emittance measurement (95%, normalized)

Use scrapers to measure emittance. Then compare to FW and Sync. Lite

Scraping: 24-27 Flying Wire: 30 Sync. Lite: 34

Intensity versus collimator position assuming Gaussian beam (1D scraping):

)1(2

2)0(

20

xx

eNN

220 240 260 280 300 320Collimator Position mils

0

0.05

0.1

0.15

0.2

T:

MA

EB

I

Collimator position (mils)

B

eam

Inte

nsi

ty

Need to know function at monitors!

Page 48: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 48

700 720 740 760Colimator position mils0

1000

2000

3000

4000

5000

maeBytisnetnIC:

GNPIBF

Tev Scraping Studies

Dispersion is an issue !!!

Horizontal protonScraping: 31-33 Flying Wire: 22-28 Sync. Lite: 34

Vertical pbar

Scraping: 20-24 Flying Wire: 42 Sync. Lite: 44

Collimator position (mils)

B

eam

In

tensi

ty

Collimator position (mils)-220 -200 -180 -160 -140 -120

0

2

4

6

8

10

Beam

In

tensi

ty

Page 49: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 49

Progress on Tevatron Physics Issues

• Lattice Measurements• F0 Lambertson major impedance source• Smart bolts and coupling• 1st indication of Beam-beam comp. (TEL)• Dancing bunches analyzed• New 1.5 GHz Schottky tune detector• SBD/FBI calibration• Work on the new helix• Octupole studies to improve beam

stability

Page 50: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 50

Beam-beam Effects at 980 Gev

• Pbar bunches near abort gaps have better emittances and live longer • Emittances of other bunches are being blown up to 40% over the first 2 hours – see scallops over the bunch trains • The effect is (and should be) tune dependent - see on the right• Recently, serious effects of pbars on protons – completely unexpected

0.585 0.590 0.595 0.600 0.605 0.610

0.575

0.580

0.585

0.590

0.595

0.600

0.585 0.590 0.595 0.600 0.605 0.610

0.575

0.580

0.585

0.590

0.595

0.600

Yu.Alexahin

Page 51: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 51

Beam-beam Tune Shift Measurement

• Measured and predicted pbar tune shift as function of bunch number at collisions.• Used gated “tickler” to excite individual pbar bunches and measured tunes with schottky pickup

pbar tunes in collision

0.57

0.575

0.58

0.585

0.59

0.595

0 10 20 30 40bunch number

QH

,V

QH lower

QV lower

prediction H (Alexahin)

prediction V(Alexahin)

Page 52: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 52

Working Point Tune Scans

Measured pbar halo loss rate during collisions as function of pbar tunes

Page 53: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 53

Goals for near future

• Deliver 200 – 300 pb-1 to each detector by end October 2003

• Steadier running (less studies)

• Reach peak luminosities of 45-50e30 be end of summer.

• 5-10% more protons– From MI, better in Tev

• 5-10% more pbars– Larger stacks– New helix

• 5-10% smaller emittances– Scallops tuned– Injection matching– Dampers

Page 54: Tevatron Status

UTeV Talk June 5, 2003 Mike Martens, Page 54

Tevatron Beam Physics Issues

• New helix• MI -> Tev injection mismatch• Octupoles or dampers on the ramp• Beam-beam studies and compensation• Tevatron BPMs, orbit smoothing• Tevatron alignment (smart bolts and rolls) • Lattice measurements