Electron Cooling in the Recycler Electron Cooling in the Recycler Ring Ring Alexander Shemyakin (Fermilab/AD) May 31, 2005
Jan 20, 2016
Electron Cooling in the Recycler RingAlexander Shemyakin (Fermilab/AD)May 31, 2005
Tevatron luminosity and antiprotonsThe Tevatron luminosity is linear with the total number of antiprotons available for the Tevatron store. The antiproton beam quality is characterized by the phase-space density. To achieve higher luminosity this density needs to be increased.
Fermilabs antiproton production chainInconel targetDebuncher (stochastic cooling)Accumulator (stochastic cooling)
8 GeV8 GeVUntil 2005Electron cooling in the Recycler Ring eliminates one of the bottlenecks in the long chain of the antiproton production. is the relative phase-space density
Idea of Electron coolingThe idea of electron cooling is a heat exchange through Coulomb scattering between hot heavy particles (antiprotons) and cold electrons while the beams are mixed in a cooling section.Was invented in 1967 by G.I. Budker (INP, Novosibirsk) as a way to increase luminosity of p-p and p-pbar colliders.
First tested in 1974 with 68 MeV protons at NAP-M storage ring at INP (Novosibirsk).CERN- ICE 1977 1979Fermilab 1979 - 1982
Low energy coolersWell established techniques for electron energies below 300 keV.A strong, continuous longitudinal magnetic field from the gun to the collectorAn electrostatic accelerator working in the energy- recovery modeExample of a 300 keV, 3 A cooler produced by Budker INP for IMP, Lanzhou (China). The voltage difference between the gun and collector ~ 3 kV.
Difficulties of implementing at relativistic energiesHigh electron beam power:4 MeV * 0.5 A = 2 MW DC!
Beam quality:The electron beam temperature (in the rest frame) should be comparable with the cathode temperature of 1200K (only a factor of ~10 increase is allowed for the transverse degree of freedom)
Design parameters of the RR ECool beam
Energy4.34 MeVBeam current0.5 Amps DC Angular spread0.2 mrad Effective energy spread 300 eV
History of relativistic electron coolingFermilab, 1983: D. Cline et al., Intermediate energy electron cooling for antiproton sources using a Pelletron acceleratorFor a pulsed electron beam in a Pelletron the beam quality is adequate for electron coolingNovosibirsk, 1987: successfully tested a prototype 1-MV, 1-A electron beam system.Continuous magnetic fieldAcceleration tubes are not sensitive to vacuum UVFermilab, UCLA, NEC, 1989: tested a 2-MV, 0.1-A DC recirculation system with a Pelletron.Poor stabilityFermilab, IUCF, NEC, 1995: started to work on a 2-MV Pelletron again- beginning of the RR ECool project
PremiseSolution for a high-power beam generator: use of a standard electrostatic accelerator (Pelletron) and non-standard focusing scheme Recirculation (energy/charge recovery) schemeNo continuous magnetic fieldA low-magnitude longitudinal magnetic field in the cooling section and at the cathode, but a lumped focusing in the remaining part of the beam line
Failure of the previous attempt was recognized to be caused by high losses in the acceleration tubesCurrent losses needs to be decreased below 0.01%
New solutions for the gun and collector were found. A gun with a negatively biased control electrode to suppress the beam halo and provide the beam transport at all currentsEffective suppressing of secondary electrons in the collector can be done by applying a transverse field in the collector cavity
Stage I - Test at NEC (Middleton, WI)GOALTo demonstrate a stable (~1 hour) generation of a 0.2 A relativistic beam using an existing 2 MV Pelletron at NEC
Nov. 95:project startedJan. 97:first recirculated current (10 A)Dec. 97:Max. recirculated current of 0.2 AMay. 98:0.2 A for 1 hours at 1.3 MeVDec. 98:Max. current of 0.7 AJan. 99:Gun solenoid (200 G) installedFeb. 99: 5 MeV Pelletron orderedMay.99:0.9 A with 200 G at the cathodeHow to scale the result for 1.3 MeV beam in a 2-MV tubes to a 4.3 MeV beam in a 5-MV accelerator ?
Stage II short line at WideBand Building (Fermilab)New means to improve stability: ion stoppers, crash scraper, closing the gun in 1 msDiagnostics: BPMs, scrapers, flying wireOperation was stable only at 3.5 MV. The tubes clearly needed to be extended. Now the main question was the beam quality.GOAL : To demonstrate a stable generation of a 0.5 A, 4.34 MeV beam in a short beam line
Feb 99: 5 MV Pelletron ordered.May 01: First beam of 30 A in the collector.Dec 01: 0.5 A at 3.5 MV Apr 02: NEC replaced acceleration tubesOct 02: 0.5 A at 4.34 MeVNov 02: Imax = 1.7 A at 3.5 MV Shut down to install the full beamline
Stage III full- length line at WideBandThe beam line was very similar to the final one at MI-31A novel type of the beam optics, angular momentum dominated Developed a technique of precise measurements of the solenoid field qualityBeam envelope measurements with movable orificesFinal version of BPM electronics
Jul- 03 - first DC beam in the full- scale lineDec-03- 0.5 A DC beamMay-04- 0.1 A beam with required properties in the cooling section
Final stage- Cooler in the RecyclerJun. 2004 Jan. 2005- assembling the cooler in MI-31/30Oct 2004- magnetic measurements in cooling sectionApr 2005- first DC beam in the collector passed through the cooling section
CoolingOne of the first indications of interaction between antiprotons and electrons. The plot shows evolution of antiproton energy distribution (log scale) after turning on an electron beam. Initially antiprotons occupy the entire momentum aperture of the Recycler.First interaction - July 9, 2005
First cooling- July 11, 2005
First electron cooling-assisted shot to Tevatron- July 12, 2005
Drag Force as a function of the antiproton momentum deviation100 mA, nominal cooling settings
First cooling rate measurements published
Electron cooling between transfers/extractionElectron beam is moved inStochastic coolingafter injectionElectron beam out (5 mm offset)Electron beam current 0.1 A/divTransverse emittance 1.5 p mm mrad/divElectron beam position 2 mm/divLongitudinal emittance (circle) 25 eVs/divPbar intensity (circle) 16e10/div~1 hour100 mA195e10~60 eVs254e10
Evolution of the number of antiprotons available from the RecyclerMixed mode operationEcool implementationRecycler only shots01/10/05 02/18/06
Chart1
42
47
85
90
91
54
56
78
67
74
89
37
37
45
45
49
49
91
91
72
71
71
69
70
71
71
86
86
81
81
68
16
57
48
78
64
85
92
98
91
43
76
65
70
63
56
124.1
113
166
51
74
58
39
108
60
116
90
138
124
121
143
144
44
66
138
94
56
69
58
14
16
59
7
33
32
42
45
49
47
65
52
128
85
51
59
74
43
71
95
30
90
32
62
106
83
53
100
81
58
61
60
94
109
51
46
92
137
116
111
Ecooling
59.5
90.7
30.6
85
48
100
60
100
143
126
59
59
89
85
92
81
97
116
112
137
111
182
46
41
98
110.5
143
60
109
64
70
136
70
113
165
129
134
141
142
216
241
90
55
69
77
225
280
235
257
183
153
209
117
197
228
111
168
191
219.57
223
285
247
266
320
220
256
89
171
248
204
200
300
248
252
174
99
132
77
181
72
55
163
219
288
236
137
270
255
273
260
354
326
323
289.7
284
198
154
115
127
182
30
107
176
201
139
209
181
334
258
258
418
197
131
150
283
166
243
Number of antiprotons (x 1010)
Sheet1
data
DateIntensityLong emittance 90%Long emittance 95%RMS mom spread90% mom spreadBucket lengthTrans emittanceNotes
2/14/041.88E+0114.018.215linear ramp, two bunches
4/7/041.60E+017.09.13.36linear ramp,single bunch
2/20/041.20E+0263.081.95.37Barrier bucket
3/12/043.50E+0121.027.32.37Barrier bucket
3/14/047.80E+0151.061.23.110.54.87Barrier bucket
3/25/043.57E+0131.938.32.89.23.33Barrier bucket
4/7/041.60E+017.09.23.511.70.36Barrier bucket
4/8/043.10E+0111.314.33.70.67Barrier bucket
4/12/045.20E+0120.625.6413.21.26Barrier bucket
4/23/049.70E+0149.058.83.110.34.64Barrier bucket
4/21/047.50E+0140.752.9
4/24/048.70E+0151.066.35.4
4/26/041.26E+0264.083.26
4/27/041.23E+0254.164.93105.33Before instability
4/30/041.17E+0250.060.03.110.34.74.2Barrier bucket
4/30/041.30E+0258.169.6310.25.73.6
5/3/041.45E+0263.876.53.210.65.854.3
5/28/044.33E+0116.319.72.58.41.855
6/9/046.70E+0130.837.23.311.12.65before mining for mixed mode
6/29/047.78E+0123.428.43.210.925Barrier bucket, before mining, after linear rf
7/6/047.50E+0123.028.03.411.61.85Barrier bucket, before mining, after linear rf
7/16/049.10E+0129.135.33.511.72.265Barrier bucket, before mining, after linear rf
7/20/046.04E+0122.327.23.310.81.825.4Barrier bucket, before mining, after linear rf
7/20/04626234.5
7/21/04505023.1
8/5/04424220.9
8/11/04303018.8
8/12/04404020.3
From This Time on we started
12/29/046.62E+0118.928.02.9101.85Barrier bucket, before mining, after linear rf
1/7/052.63E+0111.113.83.310.90.774.2Barrier bucket, before mining, after linear rf
1/10/054.23E+0114.717.72.68.61.574Barrier bucket, before mining, after linear rf
1/11/053.11E+0111.614.53.411.30.775Barrier bucket, before mining, after linear rf
1/15/05331414
1/17/058.57E+0125.931.32.99.72.545.3Barrier bucket, before mining, after linear rf
1/18/059.02E+0131.738.22.99.73.154Barrier bucket, before mining, after linear rf
1/25/055.40E+0118.322.02.79.31.94.3Barrier bucket, before mining, after linear rf
1/27/054016.0
1/26/054.04E+0112.416.24.2140.454.5Barrier bucket, before mining, after linear rf
1/28/055.61E+0118.022.13.511.91.294.1Barrier bucket, before mining, after linear rf
1/29/057.79E+0125.030.63.612.31.834.4Barrier bucket, before mining, after linear rf
1/31/057.01E+0122.427.33.411.51.754Barrier bucket, before mining, after linear rf
2/1/056.72E+0121.626.231024.2Barrier bucket, before mining, after linear rf
2/3/057.45E+0124.429.63.3511.11.974Barrier bucket, before mining, after linear rf
2/5/055.81E+0122.827.93.4411.51.763.3Barrier bucket, before mining, after linear rf
2/6/054.34E+0116.219.62.79.141.6663.7Barrier bucket, before mining, after linear rf
2/8/058.93E+0134.241.63.7612.42.464.5
TDR2.60E+0254.070.25538.547.75
6.50E+0254.070.25538.5125
1.80E+0254.070.25538.536.855
2.00E+016.07.85.854.0954.095
2.00E+010.00.0000
0.00E+000.0
1.80E+0296.0
6/30/047932
7/6/047728
7/16/049235.3
12/23/044120.9
12/29/046628
1/10/054220
1/12/054722
1/17/058536
1/18/059040
1/20/059143
1/24/055422.1
1/28/055627
1/30/057829
2/1/056726
2/3/057428
2/8/058941
2/13/053719
2/13/053718
2/17/0545
2/17/054522
2/22/054932
2/22/054932
2/23/059148
2/23/059144
2/24/057236
2/26/057130
2/26/057129
2/27/056939
2/27/057038
3/4/057135
3/4/057135
3/5/058640
3/5/058640
3/7/058140
3/7/058140
3/8/056837
3/9/05168.5
3/10/055728
3/12/0548
3/14/0578
3/15/056430
3/17/058543
3/18/059248
3/20/059847
3/21/059148
3/25/054323
3/26/057641
3/27/056530
3/29/057033
3/30/056328Started using ibs to help cool
4/2/055628
4/4/05124.147
4/7/05113.046.0
4/8/05166.059.3
4/10/0551.025.0
4/14/0574.031.0
4/17/0558.027.0
18-Apr39.019.0
4/20/05108.040.0
4/23/0560.028.0
4/24/05116.054.0
4/25/0590.035.0
4/27/05138.052.0
4/29/05124.045.0
4/30/05121.045.0
5/2/05143.052.0
5/4/05144.051.0
5/7/0544.020.0
5/9/0566.028.0
5/12/05138.051.0
5/13/0594.037.0
5/17/0556.022.0
5/18/0569.026.0
5/19/0558.024.0
5/19/0514.09.0
5/21/0516.010.0
5/23/0559.025.0
5/23/057.06.3
5/24/0533.014.0
5/26/0532.013.0
5/27/0542.018.0
5/28/0545.020.0
5/29/0549.024.0
5/31/0547.021.0
6/2/0565.028.0
6/4/0552.025.0
6/6/05128.051.0
6/7/0585.032.0
6/8/0551.035
6/10/0559.031.0
6/11/0574.030.0
6/17/0543.020.0
6/18/0571.030.0
6/19/0595.042.0
6/20/0530.014.0
6/22/0590.041.0
6/23/0532.014.0
6/24/0562.024.0
6/26/05106.045.0
6/28/0583.033.0
7/1/0553.023.0
7/5/05100.040.0
7/23/0581.026.0
7/26/0558.041.0
7/30/0561.025.0
7/31/0560.026.0
8/2/0594.041.0
8/7/05109.040.0
8/16/0551.025.0
8/18/0546.022.0
8/22/0592.044.0
8/26/05137.078.0
8/27/05116.078.5
8/29/05111.076.0
Ecooling
7/16/0559.515.9
7/18/0590.727.0
7/19/0530.68.5
7/21/0585.028.0
7/22/0548.019.0
7/25/05100.028.0
7/28/0560.020.0
8/1/05100.034.0
8/4/05143.051.0
8/6/05126.040.0
8/8/0559.018.0
8/10/0559.018.0
8/12/0589.024.0
8/13/0585.024.0
8/14/0592.028.0
8/18/0581.025.0
8/19/0597.035.0
8/23/05116.035.0
8/24/05112.031.0
8/26/05137.054.0
8/30/05111.037.0
9/1/05182.062.0
9/2/0546.018.0
9/3/0541.016.0
9/5/0598.030.0
9/6/05110.522.9
9/8/05143.036.0
9/9/0560.016.0
9/12/05109.028.0
9/13/0564.021.0
9/14/0570.021.0
9/16/05136.051.0
9/17/0570.027.0
9/18/05113.027.0
9/20/05165.067.0
9/22/05129.050.0
9/22/05134.047.5
9/24/05141.055.0
9/25/05142.049.0
9/26/05216.064.0
9/28/05241.065.0
9/28/0590.035.0
9/30/0555.020.0
10/1/0569.023.0
10/2/0577.028.0
10/4/05225.062.0
10/5/05280.060.0
10/8/05235.065.0
10/10/05257.066.0
10/12/05183.078.0
10/13/05153.051.0
10/15/05209.065.0
10/15/05117.032.0
10/16/05197.066.0
10/17/05228.066.0
10/19/05111.035.0
10/21/05168.057.0
10/22/05191.068.0
10/23/05219.657.0
10/25/05223.067.0
10/27/05285.067.0
10/29/05247.078.0
10/28/05266.066.0
10/31/05320.072.0
11/2/05220.071.0
11/3/05256.080.0
11/4/0589.045.0
11/5/05171.051.0
11/6/05248.065.0
11/7/05204.070.0
11/9/05200.070.0
11/10/05300.068.0
11/12/05248.065.0
11/13/05252.067.0
11/15/05174.055.0
12/12/0599.040.0
12/13/05132.060.0
12/14/0577.035.0
12/16/05181.058.0
12/17/0572.037.0
12/18/0555.028.0
12/19/05163.065.0
12/21/05219.063.0
12/22/05288.066.0
12/23/05236.064.0
12/25/05137.040.0
12/27/05270.065.0
12/28/05255.059.0
12/30/05273.065.0
1/2/06260.067.0
1/6/06354.072.0
1/7/06326.076.0
1/8/06323.070.0
1/10/06289.766.0
1/11/06284.068.0
1/14/06198.055.0
1/19/06154.061.0
1/23/06115.069.0
1/27/06127.074.0
1/28/06182.069.0
1/30/0630.049.0
2/2/06107.041.0
2/3/06176.041.0
2/4/06201.061.0
2/5/06139.040.0
2/6/06209.059.0
2/7/06181.090.0
2/9/06334.075.0
2/10/06258.055.0
2/12/06258.067.0
2/14/06418.066.0
2/17/06197.066.0
2/18/06131.054.0
2/19/06150.055.0
2/20/06283.058.0
2/21/06166.054.0
2/22/06243.059.0
2/1/06274.062.0
2/1/06240.043.0
Damper Test
8/23/0558.09.8
8/24/05112.024.0
now110.522.9
2.2222222222
7.5
data
00000
00000
00000
00000
0000
0000
0000
0000
0000
0000
0000
0000
0000
0000
0000
0000
0000
0000
000
000
000
000
00
00
00
00
00
00
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
Cons data
Pbar intensity, xE10
Long emittance (95%), eV-s
Recycler's best long. emittance as of 04/10/05
Plot
000000
000000
000000
000000
0000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
000
00
00
00
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00
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00
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00
00
00
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00
00
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00
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00
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00
00
00
00
00
00
00
00
00
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00
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00
00
00
00
0
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0
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0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
Pink Line
Post IBS Cooling (3/05 - 8/05)
blue Line
Ecool (7/05 - present)
'Feb/04 - Dec/04'
Last 5 to Tev
Pbar intensity, xE10
Long emittance (95%), eV-s
Recycler's Long. Emittance with Electron Cooling
Sheet3
000
000
000
000
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
blue Line
Pink Line
'Feb/04 - Dec/04'
Pbar intensity, xE10
Long emittance (95%), eV-s
Recycler's Long. Emittance Pre IBS Cooling
0000000
0000000
0000000
0000000
00000
0000
0000
0000
0000
0000
0000
0000
0000
0000
0000
0000
000
000
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000
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000
000
00
00
00
00
00
00
00
0
0
0
0
0
0
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0
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0
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0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
Pink Line
blue Line
Ecool (7/05 - present)
last 5
dec '05
Jan '06
Feb '06
Pbar intensity, xE10
Long emittance (95%), eV-s
Recycler's Long. Emittance as of 2/28/06
0000
0000
0000
0000
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
00
0
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0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
Pink Line
Post IBS Cooling (3/05 - 8/05)
blue Line
'Feb/04 - Dec/04'
Pbar intensity, xE10
Long emittance (95%), eV-s
Recycler's Long. Emittance Post IBS Cooling
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
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0
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0
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0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
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0
Mixed Mode Operations
EcoolImplementation
Recycler OnlyShots
Number of antiprotons (x 1010)
Long emittance
14
63
21
50.9913654065
31.908509866
7.0404649281
11.2891480685
48.9543515619
40.7
51
64
54.1471258502
50
49.9728362532
58.0912629581
63.8191827374
16.3045085162
30.7541904285
20.6061774981
7
Remaining questionsLife timeThe antiproton life time suffers at strong electron coolingEffect is not dramatic, but its removal will add additional percents to the number of antiprotons in Tevatron
Ultimate strength of coolingECool works at 3001010 , but additional work may be needed to cool effectively 6001010.
SummaryThe relativistic, non- magnetized electron cooling has been demonstratedAllows other laboratories to proceed with further developments:BNL- electron cooling at RHIC, Ee= 54 MeVGSI & TSL- fast cooling of antiprotons, Ee= 4 - 8 MeV
Fermilab has a world record electron cooling system that has allowed recent advances in luminosity
A hard limit on the maximum number of antiprotons in the Recycler has been removed. The road to higher luminosities is open.
The team (at the final stages)Beam studiesA.BurovK.CarlsonD.BroemmelsiekC.GattusoM.HuG.Kazakevich (BINP, guest scientist)T.KrocS.NagaitsevL.ProstS.PrussS.Seletskiy (U.of Rochester)A.ShemyakinC.SchmidtM.SutherlandV.TupikovA.Warner
Engineering supportB. KramperJ. LeibfritzL. NobregaG. SaewertK. Williams
Technical supportM. FrettR. KellettJ. NelsonJ. Simmons
International collaborationBINP (Novosibirsk, Russia)V. ParkhomchukV. RevaCOSY (Juelich, Germany)D. PrashunBNLA. FedotovPhysics discussions and modelingV. Lebedev
JINR(Dubna, Russia)I.N. MeshkovA. SidorinANLW. Gai