LHCb 2009 - 2010 luminosity performance - rough estimate - 3.5 TeV

A path to the total integrated luminosity quoted at Chamonix 2009 while keeping the total intensity to a reasonable level. Necessarily approximate. Preliminary.

Month Comment

Turn
around
time

Energy
[TeV]

Max number bunches
Protons/Bunch
% nom.
intensity
Min beta*

Peak Luminosity
cm-2s-1

Integrated Luminosity
1
Beam commissioning
First collisions
2
Pilot physics, partial squeeze, gentle increase in bunch intensity, availability low
Long
3.5
19
3 x 1010
6 m
2.5 x 1029
100 - 200 nb-1
3
 
5
3.5
19
5 x 1010
3 m
1.4 x 1030
~ 0.7 pb-1
4
 
5
3.5
72
5 x 1010
2.5
3 m
5.3 x 1030
~2.5 pb-1
5a
No crossing angle - could at this stage push intensity see 5b
5
3.5
72
7 x 1010
3.4
3 m
1 x 1031
~5 pb-1
5b
No crossing angle - squeezing to beta* = 1m at this stage would double these lumi numbers (and the pile-up)
5
3.5
72
10 x 1010
4.8
3 m
2.1 x 1031
~10 pb-1
6
Possible shift to higher energy - would anticipate ~4 weeks to reestablish physics follow by a fairly gentle increase back up in intensity. Would aim to first provide a period of physics at the higher energy (4.5 TeV, say ) without crossing angle, this could be followed by a move to 50 ns with a limited number of bunches. Note that the total intensity limit will go down with the move to higher energy.
7

4 - 5 TeV (5 TeV luminosity quoted - doesn't make too much difference).
No crossing angle.

5
 4 -5
72
7 x 1010
3.4
4 m
1.1 x 1031
~6 pb-1
8
50 ns - nominal crossing angle - aperture restricts squeezing further - note limited complement of bunches.
5
4 -5
138
7 x 1010
3.1
4 m
2.2 x 1031
~10 pb-1
9
50 ns
5
4 -5
276
7 x 1010
6.2
4 m
4.2 x 1031
~20 pb-1
10
50 ns*
5
4 -5
414
7 x 1010
9.4
4 m
6.5 x 1031
~31 pb-1
(11)
50 ns*
5
4 -5
414
9 x 1010
11.5*
4 m
1 x 1032
~50 pb-1
   

Assuming:

Number of bunches, crossing angle and minimum beta* following Werner Herr at Chamonix 2009

ML September 09