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LHC 2011, 2012 and 2015 Steve Myers

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LHC 2011, 2012 and 2015. Steve Myers. 2011. Last LHCC. 2011 Ions. Beam Current and Lumi Plots. 3.5e12. RF cavity. PS Scraper. PS Septum. 358 x 358 b. 400. 170 x 170 b. Stable Beams ~ 50 %. Peak and Integrated luminosity. 2010. 2010. In 2010: - PowerPoint PPT Presentation

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Page 1: LHC 2011, 2012 and 2015

LHC 2011, 2012 and 2015

Steve Myers

Page 2: LHC 2011, 2012 and 2015

S. Myers LHCC 2

2011

December 7, 2011

Page 3: LHC 2011, 2012 and 2015

S. Myers LHCC 3December 7, 2011

Last LHCC

Page 4: LHC 2011, 2012 and 2015

S. Myers LHCC 4December 7, 2011

Page 5: LHC 2011, 2012 and 2015

S. Myers LHCC 5December 7, 2011

Page 6: LHC 2011, 2012 and 2015

S. Myers LHCC 6

2011 Ions

December 7, 2011

Page 7: LHC 2011, 2012 and 2015

Beam Current and Lumi Plots

7S. Myers LHCCDecember 7, 2011

3.5e12

400

PS Scraper

PS Septum

RF cavity

170 x 170 b

358 x 358 b

Page 8: LHC 2011, 2012 and 2015

Stable Beams ~ 50 %

8S. Myers LHCCDecember 7, 2011

Page 9: LHC 2011, 2012 and 2015

9S. Myers LHCCDecember 7, 2011

In 2010:

Peak ~18E24; Integrated ~18ub-1 Max 137 bunches, larger *, smaller

bunch intensities

2010 2010

Peak and Integrated luminosity

356 bunches

Page 10: LHC 2011, 2012 and 2015

S. Myers LHCC 10

Using 2011 Data to Predict

),,,(4

**

2,1,sN

N

revbunchbunchbpeak R

fNNnL

𝐿𝑝𝑒𝑎𝑘¿𝐾 𝐿 ∙ (𝑁 h𝑏𝑢𝑛𝑐 ∙𝑛𝑏 ) ∙(𝑁 h𝑏𝑢𝑛𝑐

𝜀𝑁 )𝐾 𝐿 ∙𝑁𝑡𝑜𝑡𝑎𝑙 ∙𝐵

Peak Luminosity

𝐿𝑝𝑒𝑎𝑘𝐾 𝐿 ∙𝑁𝑡𝑜𝑡𝑎𝑙 ∙𝐵

December 7, 2011

Page 11: LHC 2011, 2012 and 2015

S. Myers LHCC 11

Peak LuminosityProcedureFrom the results of 2011

• Calculate the brightness (B) from the luminosity dataFor the first part of 2011 (until “mini Chamonix” at the end of July) the brightness was artificially decreased in the SPS before injection to the LHC. Only the data from the last period of 2011 is relevantIn the mini-Chamonix the presented maximum brightness parameters from the injectors were (at extraction of the SPS)

50ns: Nbunch = 1.55E11, with N= 2.0µm; i.e. Bmax = .775

25ns: Nbunch = 1.15E11, with N= 3.3µm; i.e. Bmax = .348

It was also observed that there was a reduction of the beam brightness when comparing collisions conditions with injection. The reduction was on average roughly 30%

𝐿𝑝𝑒𝑎𝑘𝐾 𝐿 ∙𝑁𝑡𝑜𝑡𝑎𝑙 ∙𝐵

December 7, 2011

Page 12: LHC 2011, 2012 and 2015

S. Myers LHCC 12

Brightness from Peak Luminosity

December 7, 2011

Page 13: LHC 2011, 2012 and 2015

S. Myers LHCC 13

From the Luminosity Data of the Last Period of 2011

The brightness in collision is fairly constant at 0.569 at intensities in the range 1.25 to 1.50E11 protons per bunch (colliding).Consequently the average measured loss of brightness from extraction at the SPS to collisions in LHC is 27%: i.e.

The brightness in the LHC (for 50ns bunch spacing) is given by

Or more generally (for different bunch spacings of 25 and 50ns)

December 7, 2011

Page 14: LHC 2011, 2012 and 2015

S. Myers LHCC 14

Evaluating Integrated Luminosity

• The Integrated Luminosity is influenced by• The peak luminosity• The luminosity loss rate (lifetime)• The lost time between fills

– Time to prepare stable beams– Technical problems causing beam dumps and inability to refill

• Try to get a statistical model from 2011 fills• Procedure

– Calculate Lave/Lpeak from the 2011 data (time weighted) as a function of Lpeak.

December 7, 2011

Page 15: LHC 2011, 2012 and 2015

The Average Luminosity

15S. Myers LHCCDecember 7, 2011

Lave = (Integrated luminosity)/(total time of fill)

Total time of fill

Stable Beams Time

Total time of fill

Stable Beams Time

Page 16: LHC 2011, 2012 and 2015

S. Myers LHCC 16

Lave /Lpeak is calculated for each fill

December 7, 2011

Page 17: LHC 2011, 2012 and 2015

S. Myers LHCC 17

Evaluating Integrated Luminosity from Peak

• Brightness– 50ns: B = 0.5694 + 0.0 (N∙ bunch - 1.35)

– 25ns: B = 0.2560 + 0.0 (N∙ bunch - 1.35)

• Average (Integrated) Luminosity– Lave/Lpeak = 0.231 + 0.0 (L∙ peak - 3300)

December 7, 2011

Page 18: LHC 2011, 2012 and 2015

S. Myers LHCC 18

Predicting 2011 Luminosities

December 7, 2011

Page 19: LHC 2011, 2012 and 2015

S. Myers LHCC 19

Lpeak 2011 Last period (50ns)

The fit is even better if the slope were to be included

December 7, 2011

Page 20: LHC 2011, 2012 and 2015

S. Myers LHCC 20

2011 Last Period (50ns)

The fit is even better if the slope were to be included

December 7, 2011

Page 21: LHC 2011, 2012 and 2015

S. Myers LHCC 21

2012 (Preparing for Chamonix)Assumptions• E=4TeV• β* = 0.7m (will be more difficult for 25ns)• 148 days of physics (5days scrubbing and 8

days special runs. N.B. more scrubbing would be needed for 25ns)

• no intensity limit for 25ns

December 7, 2011

Note on scalingEnergy: Peak, Integrated and µ scale linearlyβ*: Peak, Integrated and µ to first order scale inversely but R depends on β*, crossing angle and emittancesµ : linearly with Lpeak, inversely with nb.

Page 22: LHC 2011, 2012 and 2015

S. Myers LHCC 22

2012 Intensity Ramp Up

December 7, 2011

E= 4TeVBeta* = 0.7m148 days of physics

Page 23: LHC 2011, 2012 and 2015

S. Myers LHCC 23

Peak Luminosity with 50ns (2012)

December 7, 2011

E= 4TeVBeta* = 0.7m148 days of physics

Note on scalingEnergy: Peak, Integrated and µ scale linearlyβ*: Peak, Integrated and µ to first order scale inversely but R depends on β*µ : linearly with Lpeak, inversely with nb.

Page 24: LHC 2011, 2012 and 2015

S. Myers LHCC 24

Peak Luminosity with 25ns (2012)

December 7, 2011

Days since start of run

E= 4TeVBeta* = 0.7m148 days of physicsCertainly optimistic• Possible intensity limitation• Possible limitation to β*

Note on scalingEnergy: Peak, Integrated and µ scale linearlyβ*: Peak, Integrated and µ to first order scale inversely but R depends on β*µ : linearly with Lpeak, inversely with nb.

Page 25: LHC 2011, 2012 and 2015

S. Myers LHCC 25

2012 Integrated with 50ns

December 7, 2011

E= 4TeVBeta* = 0.7m148 days of physics

Note on scalingEnergy: Peak, Integrated and µ scale linearlyβ*: Peak, Integrated and µ to first order scale inversely but R depends on β*µ : linearly with Lpeak, inversely with nb.

Page 26: LHC 2011, 2012 and 2015

S. Myers LHCC 26

2012 Integrated with 25ns

December 7, 2011

Note on scalingEnergy: Peak, Integrated and µ scale linearlyβ*: Peak, Integrated and µ to first order scale inversely but R depends on β*µ : linearly with Lpeak, inversely with nb.

E= 4TeVBeta* = 0.7m148 days of physicsCertainly optimistic• Possible intensity limitation• Possible limitation to β*• More scrubbing needed

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S. Myers LHCC 27

Summary for 2012AssumptionsE=4TeV: beta* = 0.7m: 148 days of physics: no intensity limit for 25ns

December 7, 2011

𝐿𝑝𝑒𝑎𝑘𝐾 𝐿 ∙𝑁𝑡𝑜𝑡𝑎𝑙 ∙𝐵

Note on scalingEnergy: Peak, Integrated and µ scale linearlyβ*: Peak, Integrated and µ to first order scale inversely but R depends on β*, crossing angle and emittancesµ : linearly with Lpeak, inversely with nb.

Bunch Spacing

Peak Luminosity

Integrated Luminosity

(fb-1)

Pile Up N max

50ns 5.80E+33 ~16 ~27 1.55E+11

25ns 3.80E+33 ~10 ~9 1.15E+11

Page 28: LHC 2011, 2012 and 2015

S. Myers LHCC 28

What to do if Pile up is too high?

Three Possibilities

December 7, 2011

We must keep the maximum flexibility for 2012

Page 29: LHC 2011, 2012 and 2015

S. Myers LHCC 29

Using 2011 Data to Predict

),,,(4

**

2,1,sN

N

revbunchbunchbpeak R

fNNnL

𝐿𝑝𝑒𝑎𝑘¿𝐾 𝐿 ∙ (𝑁 h𝑏𝑢𝑛𝑐 ∙𝑛𝑏 ) ∙(𝑁 h𝑏𝑢𝑛𝑐

𝜀𝑁 )𝐾 𝐿 ∙𝑁𝑡𝑜𝑡𝑎𝑙 ∙𝐵

Peak Luminosity

𝐿𝑝𝑒𝑎𝑘𝐾 𝐿 ∙𝑁𝑡𝑜𝑡𝑎𝑙 ∙𝐵

December 7, 2011

Page 30: LHC 2011, 2012 and 2015

S. Myers LHCC 30

At 6.5TeV per beam

Assumptions• E=6.5TeV• β* = 0.5m• All other conditions as in 2012 i.e. no

improvement (yet) in injector brightness, LHC availability same etc

December 7, 2011

Page 31: LHC 2011, 2012 and 2015

S. Myers LHCC 31

6.5TeV per beam with 50ns

6.5Tev: 50 nsβ* = 0.5m148 days of physics

Lpeak ~10.5E33µ = ~50

December 7, 2011

Days since start of 2015 run

Page 32: LHC 2011, 2012 and 2015

S. Myers LHCC 32

6.5TeV: 25ns

6.5Tev: 25 nsβ* = 0.5m148 days of physics

Lpeak ~7.5E33µ = ~17

December 7, 2011

Days since start of 2015 run

Optimistic• Possible intensity limitation• Possible limitation to β*• More scrubbing needed

Page 33: LHC 2011, 2012 and 2015

S. Myers LHCC 33

Thank you for your attentionDecember 7, 2011