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 |
Energy |
Max number bunches |
Protons/Bunch |
% nom. intensity |
Min beta* |
Peak Luminosity |
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). |
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