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Collimation Issues for the Phase 1 Insertion Upgrade

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Title: Collimation Issues for the Phase 1 Insertion Upgrade


1
Collimation Issues for the Phase 1 Insertion
Upgrade
  • R. Assmann, CERN, AB/ABP
  • Acknowledgements to the colleagues in the LHC
    Collimation Working Group which worked out and
    presented most of the results shown here
  • http//www.cern.ch/lhc-collimation
  • Acknowledgements to the colleagues in AB/ABP and
    AT for discussions and help in understanding the
    upgrade ideas.
  • CERN, Switzerland
  • November 1st, 2007

2
1) Why Talk About Collimation?
  • Collimation protects the machine aperture against
    damage and quenches.
  • Any significant change in aperture must be
    revisited also from the collimation and machine
    protection view possible impact on protection,
    loss distribution, activation, quench
    limitations, experimental background.
  • Critical issues The HERA insertion upgrade was
    heavily affected by unforeseen problems with beam
    loss and background after the upgrade. Loss in
    overall integrated luminosity with insertion
    upgrade.
  • Goal of this talk Give collimation input to the
    ongoing discussions for the phase 1 triplet
    upgrade such that it will be fully successful.
  • Note MP and dump issues only mentioned as far as
    collimation is affected ? for additional input
    see presentations at LUMI06 by B. Goddard and R.
    Schmidt.

3
System Design
Phase 1
Momentum Cleaning
Betatron Cleaning
Final system Layount is 100 frozen!
? Outcome of accelerator physics energy
deposition optimization
4
Multi-Stage Cleaning Protection
Beam axis
Beam propagation
Impact parameter
Collimator
Core
Particle
Unavoidable losses
Primary halo (p)
Secondary halo
p
p
Shower
p
Tertiary halo
Impact parameter 1 mm
p
e
p
Primary collimator
Secondary collimator
Shower
e
SC magnets and particle physics exp.
Absorber
Super-conducting magnets
Absorber
W/Cu
CFC
W/Cu
CFC
5
Functional Description
  • Two-stage cleaning (robust CFC primary and
    secondary collimators).
  • Catching the cleaning-induced showers (Cu/W
    collimators).
  • Protecting the warm magnets against heat and
    radiation (passive absorbers).
  • Local cleaning and protection at triplets (Cu/W
    collimators).
  • Catching the p-p induced showers (Cu
    collimators).
  • Intercepting mis-injected beam (TCDI, TDI, TCLI).
  • Intercepting dumped beam (TCDQ, TCS.TCDQ).
  • Scraping and halo diagnostics (primary
    collimators and thin scrapers).

6
Setting Strategy for Collimation and Protection
Elements
  • Clear requirements for settingsLHC ring
    aperture sets scale aring? tight LHC
    apertureProtection devices must protect ring
    aperture aprot lt aring ? protect against
    injected beam take into account
    accuraciesSecondary collimators tighter than
    protection asec lt aprot ? avoid too much
    secondary halo hitting protection
    devicesPrimary collimators tighter than
    secondary aprim lt asec ? primary collimators
    define the aperture bottleneck in the LHC
    for cleaning of circulating beam!
  • These conditions should always be fulfilled
    Not allowed to use protection devices (or warm
    aperture limits) as a single-stage cleaning
    system!

R. Assmann, Chamonix 2005
7
7 TeV Settings at (in sb ,d0, nominal b)
aabs 20.0 s Active absorbers in IR3 asec3
18.0 s Secondary collimators IR3 (H) aprim3
15.0 s Primary collimators IR3 (H) aabs
10.0 s Active absorbers in and IR7 aring 8.4
s Triplet cold aperture aprot 8.3 s TCT
protection and cleaning at triplet aprot 7.5
s TCDQ (H) protection element asec 7.0 s
Secondary collimators IR7 aprim 6.0 s
Primary collimators IR7 ? Canonical 6/7 s
collimation settings are achievable!
R. Assmann, Chamonix 2005
8
2) Insertion Aspects for Collimation
  • Chamonix 2003 (R. Assmann)
  • Only way to open collimator gaps Increase
    triplet aperture! Still true but lots of things
    understood since 2003!

9
2004 Addition of Tertiary Collimators
  • Collimator settings defined with required
    hierarchy.
  • Detailed loss maps for beam 1 and beam 2
    produced.
  • Problem Halo losses in triplets (standard
    optics, 0.55m) up to 25 times above quench limit.
  • Solution Addition of tertiary collimators
  • Make use of large aperture until D1.
  • Placed before D1 such that all losses are
    intercepted before the triplet is hit.
  • Completely solves loss issue.
  • Improves machine protection (allowing feasible
    requirements in local dump protection in IR6).
  • Checked for experimental background in CMS and
    ATLAS Beneficial effect.

10
System Design
Phase 1
Momentum Cleaning
Betatron Cleaning
11
7 TeV Proton Loss Distribution
p losses inefficiency
G. Robert-Demolaize et al
12
Beam1 and Beam 2 Asymmetry
Beam1, 7 TeV Betatron cleaning Ideal performance
TCDQ
Quench limit (nominal I, t0.2h)
Local inefficiency 1/m
Beam2, 7 TeV Betatron cleaning Ideal performance
TCDQ
Quench limit (nominal I, t0.2h)
Local inefficiency p lost in bin over total p
lost over length of aperture bin!
13
Asymmetry IR1/IR5
  • Beam 1 betatron halo losses on TCT left sides of
    IP
  • IR1 5e-4 of total halo loss
  • IR5 5e-6 of total halo loss
  • Beam 2 betatron halo losses on TCT right sides of
    IP
  • IR1 2e-5 of total halo loss
  • IR5 3e-4 of total halo loss
  • Halo losses in experimental insertions are
    asymmetric. Detailed losses depend on collimator
    settings, phase advance and halo phase space
    properties.
  • Above settings assume IR2 and IR8 collimators
    present and at same setting as IR1/IR5 teriary
    collimators. We might open them and losses in
    IR1/IR5 will increase (small gaps not needed in
    IR2/8 trapped mode issues with higher b, small
    gaps in IR2/8).? In worst case increase losses
    by a factor 2.

14
Interim Summary I
  • Phase 1 collimation system fully shadows the
    IR1/5 at 7 TeV.
  • Three components to reach this goal
  • IR3/IR7 collimators set to shadow the triplet
    (depends on beta and triplet aperture) against
    the primary and secondary halo.
  • Local tertiary collimators TCT (58 mm full
    maximum gap) to clean tertiary halo which would
    otherwise be 20 times above quench limit 4 per
    IR.
  • Local copper absorbers TCL/TCLP to catch showers
    from IP before the arc.
  • Insertion upgrade (ignoring cleaning efficiency
    limitations in IR7)
  • An increased minimum normalized aperture in
    IR1/IR5 can in principle be used to open the
    IR3/IR7 collimators ? reduced impedance.
  • Even if n1 is increased it is expected that the
    stringent aperture bottle-necks (including new
    and earlier bottle-necks) in IR1/IR5 must be
    protected with tertiary collimators (new types,
    more TCT 4 ? 6).
  • Opening gaps can affect other issues (efficiency,
    protection, ).

15
2003 Reduce Impedance with Increased Gaps!
Typical collimator half gap
104
103
102
LHC impedance without collimators
Transverse Impedance MO/m
10
factor 1.6
1
10-1
0 2 4
6 8 10
Half Gap mm
F. Ruggiero, L. Vos
2007 E. Metral ? stable beam with 50 larger
gaps from detailed analysis
16
2) Limitation in Cleaning Efficiency
  • As just shown, cleaning efficiency in IR1/5 is no
    issue any more.
  • Fundamental limitation arises at the end of IR7
    (single-diffractive scattering tertiary halo)
    after betatron cleaning.
  • Nuclear physics routine cross-checked between 3
    different programs.
  • Independent studies at CERN, SLAC and IHEP agree
    on the predicted limitations.
  • Outside experts usually think we are even
    optimistic
  • Loss assumptions.
  • Only partial errors included (loss of factor 2
    seen).
  • Uncertainties in diffusion and halo models.
  • SNS has just published a paper with 5-6 times
    higher fractional losses in magnets than
    predicted in simulations. Absolute losses locally
    up to 20 times above specifications!

17
Preventing Quenches
  • Quench limits of SC magnets given by design.
  • Overall criterion for preventing quenches

Fractional Leakage Dilution Fractional
quench loss rate rate length limit (w/o BLM
threshold)
Minimize Minimize Spread losses inefficiency losse
s
Example 0.1 per s 1/5,000 1/(10 m) ? 2.0 10-8
(ms)-1
18
Performance Prediction
19
Uncertainties
  • Many uncertainties do affect results
  • Uncertainty in loss assumptions. Supported by
    external collimation review in 2004. However,
    some find the loss rates too low, other too high.
  • Impact from imperfections Almost always drives
    efficiency down.
  • Required margin from BLM thresholds Factor 3
    announced ? beam abort 3 times below quench
    limit.
  • Impact from showers Dilutes losses ? gain
    somewhat.
  • Quench limits Any reduction/increase in quench
    limit will reduce/improve the performance reach.
  • We try to do the best possible simulations, given
    the available resources.
  • Extensive cross-checks with other ongoing
    efforts in the field agreement on the predicted
    efficiency limitation (not a single published
    result with a different conclusion).
  • Approach Being fully aware of the uncertainties,
    use the predictions to guide us towards achieving
    LHC performance goals.

20
7 TeV Proton Loss Prediction
Ideal case
G. Robert-Demolaize et al
With design orbit error
21
Peak Inefficiency Versus Gap
C. Bracco et al
Phase 1 upgrade possibility (n19)
LHC nominal
BLM threshold?
Quench limit
0 5 10
15 20
25
Aperture primary collimator s
22
Other Possible Impacts from Larger Collimation
Gaps in IR7
  • Machine Protection For example, in case of
    magnet trips (for example affecting x) with
    larger gaps (1) the first losses are seen later.
    (2) dx/dt when are seen is increased. ? R.
    Schmidt and MPWG.
  • Momentum collimation gaps must be opened as well
    ? impact on abort gap population (synchrotron
    radiation) and abort gap cleaning.
  • Increased impact of off-momentum beta-beat (if
    retraction distance between primary and
    secondary jaws is kept constant).

23
Interim Summary 2
  • Cleaning efficiency in IR7 is predicted to be the
    driving limitation from LHC collimation, more
    severe than impedance.
  • Reducing collimator-induced impedance issue will
    not affect the overall limit (limitations must
    not be added, only the bigger counts).
  • Small gaps are required to maximize cleaning
    efficiency in IR7.
  • Gaps can still be opened but will lead to a
    decrease in the allowable intensity and such to a
    decrease in performance.
  • Efficiency must be addressed in addition to
    impedance.
  • With this in mind, an increased aperture in IR1/5
    and the phase 1 upgrade are fully supported
    from collimation, as it will provide the basic
    possibility of opening gaps after the phase 2
    upgrade.
  • Other side effects of increased gaps must not be
    forgotten!

24
3) Off-Momentum Beta Beat
  • Off-momentum beat beat mixes up the 6D phase
    space and can corrupt collimation performance
    (secondary collimator becomes a primary
    collimator for off-momentum particles).
  • Studies by C. Bracco and myself complete for
    nominal optics.
  • Presentation by C. Bracco next Monday in LCU
    meeting.
  • Here, first glance at preliminary results on
    upgrade optics that we got from R. de Maria.

25
Upgrade optics nominal setting (TCP_at_6s,
TCSG_at_7s....) Horizontal Collimators
Allowed phase (yellow area) space should always
be defined by primary collimators (red lines). It
is not below d1e-3! Could lead to break-down
of cleaning efficiency for off-momentum particles!
C. Bracco, R. Assmann
26
Upgrade optics nominal setting (TCP_at_6s,
TCSG_at_7s...) - Vertical collimators
Secondary collimators become primary collimators!
27
Upgrade optics nominal setting (TCP_at_6s,
TCSG_at_7s....) IR7 collimators retraction
Nominal retraction
Secondary collimator becomes primary collimator
28
Upgrade optics new setting(TCP.IR7_at_9s,
TCSG.IR7_at_10s,TCLA.IR7_at_13s) IR7 collimators
Retraction
Nominal retraction
Secondary collimator becomes primary collimator
29
Interim Summary 3
  • We see noticeable but still acceptable effects
    from off-momentum beta-beat for the nominal LHC
    optics 30 loss in retraction.
  • Preliminary results show much stronger effects
    for upgrade optics, up to the point where
    multi-stage cleaning is corrupted.
  • Importance will depend on longitudinal beam
    lifetime, synchrotron losses and equilibrium beam
    distribution in off-momentum.
  • Remedy Use larger retraction ? increased
    aperture would be used (at least partially) for
    increased retraction (reduced gain in impedance).
  • Here we only show primary and secondary
    collimators. All collimator families must
    analyzed for this effect.
  • Preliminary results further work needed and
    optics might be adapted to minimize impact.

30
4) Input and Proposals
  • The upgraded triplets should include fixed masks
    for the incoming beam. This provides the best
    possible triplet protection and cleaning. These
    fixed masks should allow for easy exchange in
    case of damage.
  • The upgrade optics should be compatible with the
    58 mm full aperture of the existing tertiary
    collimators, which are located between the D1 and
    the D2 magnets.
  • In case that requirement 2) cannot be fulfilled,
    limited local background control for ATLAS and
    CMS must either be abandoned or new tertiary
    collimators must be developed, tested and
    constructed. This affects up to eight tertiary
    collimators installed in IR1 and IR5.
  • The goal of providing room for opening primary
    collimators in IR7 to 9 s is supported (50
    increased collimator aperture as indicated by
    studies from E. Metral). This corresponds to n1
    10.5 (up from n1 7) if we just scale n1.
  • For ultimate intensity a factor 2 increase in gap
    (compared to today) is needed to remove the
    impedance limit. This means n114. Stick to
    nominal in the next slides.

31
Input and Proposals continued
  • To respect the specified hierarchy of collimator
    and protection settings minimal available IR
    aperture after upgrade must be 2.4 s to 3.6 s
    larger than the assumed setting of the primary
    collimators. Required 12.6 s (this corresponds
    to n1 10.5). If we take a constant 3s increase
    of all gaps 11.4 s. Will provide less
    reduction on impedance!
  • The feasibility of any reduction in available
    aperture in adjacent magnets to the triplets must
    be checked with full evaluations of beam halo,
    beam loss maps, energy deposition, impedance and
    experimental background. The placement of
    additional tertiary collimators might be
    required.
  • The showers from the IP must be tracked into the
    arc to verify that the foreseen TCL/TCLP
    collimators are still fully adequate.
  • The performance reach of the LHC after the
    insertion upgrade must be calculated, taking into
    account also performance limitations in other
    areas of the machine. This concerns in particular
    the predicted limitations due to cleaning
    efficiency.

32
Input and Proposals continued
  • If it is assumed that the betatron collimators
    are opened after a triplet upgrade, then various
    secondary effects must be considered. In
    particular, it might be required to open also the
    momentum collimators with resulting effects on
    losses of off-momentum particles (synchrotron
    radiation losses), abort gap cleaning etc.
  • The compatibility of an additional
    triplet-induced off-momentum beta-beat with
    collimation must be verified.
  • All warm and cold aperture limits must be in the
    shadow of machine protection collimators,
    independently of the fact that warm elements
    cannot quench!
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