tevatron status
DESCRIPTION
Tevatron Status. UTev Seminar June 6, 2003. Mike Martens - PowerPoint PPT PresentationTRANSCRIPT
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
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.
UTeV Talk June 5, 2003 Mike Martens, Page 3
Luminosity
Pint = Nprotint /A
Rate = L int
A
int
pbars
protons
L = frevNpbar Nprot/A
UTeV Talk June 5, 2003 Mike Martens, Page 4
Low Beta Lattice
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).
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
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.
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:
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
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.
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.
UTeV Talk June 5, 2003 Mike Martens, Page 12
Tevatron Efficiencies
protoninjections
pbarinjections
rampOpen helix
poor lifetimes
10% bunchedbeam loss in ramp
and squeeze
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
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
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)
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
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
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
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)
UTeV Talk June 5, 2003 Mike Martens, Page 20
Beam-beam Effects: Pbar Only
8% loss on ramp – DC beam (depends
on MI tuneup)
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
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
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”
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
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)
UTeV Talk June 5, 2003 Mike Martens, Page 26
Tune Drift @ 150 Gev
M.Martens, J.Annala
UTeV Talk June 5, 2003 Mike Martens, Page 27
Coupling Drift @ 150 Gev
M.Martens, J.Annala
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
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
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
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
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
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
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
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
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
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)
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
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
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
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
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
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
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
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
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
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!
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
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
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
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)
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
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
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