Fast ground motion will cause independent orbit movements
in the two linacs of a linear collider such, that the beams may
miss each other at the interaction point (IP). But even at rather
large vertical beam-beam separations at the IP, beams will deflect
each other through their electromagnetic fields. By measuring
the position of a beam, which has just passed the IP and compare
in it the position of a first pilot bunch -which does not have
a partner in the opposing beam- with that of the following bunches
in the same bunch train, the opposing beam can be steered with
ultra fast kicker magnets for optimum collision at the IP. A feed-back
system based on this principle will make the necessary steering
corrections within a time short compared to the duration of the
bunch train.
Fast beam steering at the interaction point, which relies on the beam-beam effect of colliding bunches, is a powerful tool to relax nanometer tolerances for final focus quadrupoles in linear colliders. Even betatron amplitude growth excited by vibrating quadrupoles further upstream in the linac, which is not filamented by the time the beam reaches the IP, can be corrected with fast beam steering. From Tracking calculations we expect only 30% filamentation over the entire length of the linac 1.
One stringent requirement for a feedback, which corrects the bunch train offset in the IP is, that the beam pulse is long compared to the overall processing time of the detected signal from the beam position measurement (BPM) to the kicker magnet. Parameters that influence this delay are the distance of the beam position monitor to the IP, the processing time of the feedback loop and the required magnetic field strength compared to the available peak power of the amplifier (compare Figure 1). The amplitude of pulse to pulse ground motion which can be expected from measurements done in the HERA tunnel, which is a tunnel under the city of Hamburg with an colliding beam facility, [2, 3] is approximately 70 nm rms for Frequencies below 1 Hz which is roughly six times the design vertical beam size. In order to limit the Luminosity reduction to 5%, the jitter at the IP should be smaller than 30% of the beam size, which is 5 nm in our case. A list of the interaction region parameters is extracted [4] from the complete list and given in Table 1.
One possibility to achieve this tolerance is to design a passive
support system that keeps the final doublets at a given position
over a time scale much larger than the repetition rate of the
accelerator. This is certainly a challenging task for the technical
design of the quadrupole supports which are part of the experiment
of a linear collider. Vibrations from the linac quadrupoles are
not correctable by this method with resonable effort.
Ne per bunch | ||
vert. beam size (no pinch) | ||
horiz. beam size (no pinch) | ||
Disruption (vertical) | ||
Disruption (horizontal) | ||
y at IP | ||
x at IP | ||
bunch length | ||
crossing angle | ||
bunch train length | ||
bunch to bunch distance | ||
distance: BPM to IP |
Table 1:
Interaction region parameters for the 500 GeV S-band Linear Collider
Study
For the S-Band Linear Collider study two feedback loops are foreseen
to relax this tolerance well beyond the measured value of 100 nm
which was mentioned before. One loop relies on a direct measurement
of the quadrupole vibration in combination with a mechanical (or
correction magnet) feedback. Such a loop has been tested already
and a suppression of a factor of 4 in amplitude for the rms value
at 2 Hz has been proven 5. This feedback loops have mainly
been developed to correct the linac quadrupole vibration. The
second loop will be described in more detail in the following
text.
For a round beam the beam-beam force of two colliding bunches is proportional to the separation of the two bunches over approximately one . Operating with an aspect ratio(=x/y) of 20 (or more), as it is foreseen in Linear Colliders to reduce the beamstrahlung, produces an almost linear beam-beam force over approximately 10 y. According to the beam-beam simulations using the parameters from Table 1, the kick angle per y separation of the two colliding beams is given to within a good approximation by:
Let us assume that the BPM next to the IP is located at the position of the first quadrupole of the final doublet, which is 2 meters away. At this position the beam offset in the monitor according to formulae (1) would be 120 m per y separation at the IP, which is easy to measure as compared to the 4 micrometer resolution being required for the rest of the linac BPM's.
A method based on beam-beam deflections to measure precisely the
offset of the two colliding beams has been used for single bunch
operation in the SLC from pulse to pulse already 6. On the other
hand, a bunch to bunch measurement of the beam position, as being
proposed for the TESLA Linear Collider study for both outgoing
beams within one pulse can not be used, because of the delay time
for signal processing as compared to the overall pulse length
and bunch to bunch distance (compare Table 1). Therefore, in case
of the S-Band Linear Collider study, a combination of both methods
is proposed which uses a pilot bunch in one of the two colliding
beam pulses and only a single BPM in combination with a single
kicker magnet. Using such a scheme has the significant advantage,
that almost no mechanical disturbance with an amplitude larger
than a nanometer (vibration, girder resonance etc) can separate
the colliding beams on the time scale of one bunch train length
(2 sec -> 500 kHz), once they are colliding.
The location of the beam position monitor and the
kicker has to be as close as possible to the IP in order to reduce
the processing time of the feedback loop. Because the quadrupole
next to the IP will have an integrated BPM the shortest distance
is 2.2 meters from the IP. If the delays on cables, the response
time of the feedback amplifier and the finite rise time of the
kicker are added up, an overall delay of 50 nsec is expected.
If we assume in addition that one bunch train will have a pilot
bunch, the delay will increase to about 60 nsec. Therefore
3% of the 2 sec long beam pulse will not be corrected and,
if far enough separated between pulses, will not contribute to
Luminosity. In case of SLED operation with a 500 nsec long
beam pulse, as foreseen for the energy upgrade to 800 GeV,
the potential loss will increase to 12%. A continu-ous measurement
of the beambeam separation during the pulse will be done
to correct even displacements which change along the bunch train.
The beam-beam force with flat beam operation is approximately linear over 10 y.
In order to allow orbit corrections at the IP for a value of 150 nm,
the required kick is only 0.07 rad, if a distance from the
kicker to the IP as close as the BPM position is assumed. For
the 250 GeV beam a magnetic field of 6
10-5 T is sufficient. The kicker will be a stripline
type kicker fed by two broad band amplifiers which can excite
a maximum magnetic field of 1.1 104. The parameters
are given in Table 2.
aperture radius | ||
effective length | ||
magetic field (max. possib.) | ||
pulse duration | ||
bandwidth of amplifier | ||
peak power /amplifier | ||
pulse current | ||
rise time | ||
repetition rate |
The power amplifiers deliver a peak power of 2.5 kW each and have
a bandwidth of more than 50 MHz to power each strip. A sketch
of the kicker is shown in Figure 2.
In order to measure the beam position of the pilot
bunch with respect to the colliding bunches an analogue delay
will be used to subtract the two signals from the pilot bunch
and the first colliding bunch directly. In addition the bunch
intensity must be determined as well because the beam-beam kick
is proportional to the bunch charge in the opposite beam. The
resolution of the beam position measurement is 5 m 7 which
is 4% of effect of a one y separation and the bunch
intensity measurement should be of the some order of magnitude.
A sketch of the BPM set-up and the readout electronics design
is shown in Figure 3.
Figure 3:
Schematics for the beam position monitor and the readout electronics.
Acknowledgment
The authors would like to thank S. Ptzold,
J. R¸mmler, and M. Wendt from DESY for their support
and their contributions to the discussion on the possibilities
to realize the required hardware for the feedback which is proposed
in this paper.