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Longitudinal Phase Space in MICE

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Tells us where to sit on the dE/dx curve for best cooling ... trec - ttrue [ns] s(E,dE) = 11.4 MeV2. s(dt,dE) = 1.97 ns MeV. Emittance at TRP vs Tof Res ... – PowerPoint PPT presentation

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Title: Longitudinal Phase Space in MICE


1
Longitudinal Phase Space in MICE
  • Chris Rogers
  • MICE CM
  • 2nd March 06

2
Overview
  • First look at longitudinal phase space in MICE
  • Magnetic lattice
  • Momentum acceptance of 200 MeV/c lattice
  • Emittance
  • Transverse emittance effects
  • Longitudinal phase space
  • RF bucket
  • Longitudinal emittance
  • Justification for TOF2 resolution
  • TOF2 is required primarily for longitudinal
    emittance measurement
  • Tells us where to sit on the dE/dx curve for best
    cooling
  • Gives us a comparison with ring coolers etc
  • Examine the time reconstruction resolution in
    tracker
  • Longitudinal emittance reconstruction resolution
  • Can we measure energy straggling

3
MICE VI Momentum Acceptance
MICE VI en12mm sx 52 mm spx 25 MeV
Stop band
Pass band
Pz MeV/c
Pz at start of channel
Pz MeV/c
  • Transmission of MICE magnetic lattice vs Pz
  • Particles matched for 200 MeV/c
  • Red is 10 MICE lattices, blue is 20 lattices, 1
    metre aperture
  • Left is histogram of Pz at various points in the
    channel
  • Particles seem to diffuse away from 180 MeV/c
    (3p/2)
  • Right plot show pz at beginning of the channel of
    particles that survive

4
Comparison with FS2
MICE VI en12mm sx 52 mm spx 25 MeV
Pz MeV/c
  • Left is transmission of MICE VI, right is FS2
    (1,1) lattice (Fernow, Muc-241)
  • FS2 (1,1) exhibits broader momentum acceptance in
    the 200 MeV/c region
  • FS2 (1,1) lattice has b280 mm in the absorbers
  • Both use 1 metre apertures
  • Not realistic

5
Stop-Bands
  • Decompose k2 (B2) into Fourier components qn
    where
  • Width of nth stop-band given by
  • Gives stop-bands at
  • 548 - 559 n1
  • 264 - 288 n2
  • 184.5 - 184.8 n3
  • 135 - 141 n4
  • Wider stop-bands comes from larger 2nth order
    Fourier modes
  • n1? From matching section?

Wang Kim, Phys Rev E 63 056502
6
Transport Matrix Approach
  • Can also get momentum acceptance using transport
    matrix formalism (Fernow, Muc-241)
  • Define transport matrix over 1 lattice R
  • Require transport matrix over n lattices, Rn, is
    finite for large n
  • Gives Dlt2 where Dtrace(R) (textbook result)
  • Calculate R(pz) using R P(MDrift(ds/2)MFocus(ds)
    MDrift(ds/2))

FS2 (1,1)
MICE VI
n3?
n1?
n4
n2
7
Comparison with tracking
FS2 (1,1)
  • Agreement is questionable
  • ICOOL acceptance is in 160/175 - 270/280
  • Tr(R) lt 2 between 146 - 253 MeV/c
  • Doesnt quite reach 2 at 184 MeV/c
  • Cross check using Wang and Kims scheme (141-264
    MeV/c)
  • Calculate Tr(R) using Fourier modes of k2
  • Better to use matched beams at each momentum?

8
Magnet Issues
  • Does the presence of LH2 change the momentum
    acceptance?
  • Diffusion into pass-band from energy straggling?
  • Change in pz from RF/LH2
  • Calculations and plots assumes constant pz
  • Other stuff
  • Strengthening of the transverse defocusing due to
    msc?
  • To what accuracy can we measure this?
  • To what accuracy is this desirable
  • What does it look like for other MICE settings?
  • This is all MICE VI, pz 200 MeV/c, b 420 mm
  • What are the effects of the matching section?
  • Can the beamline deliver a beam like this?
  • I would like a beam that fills the pass-band in
    each MICE case
  • Thats a lot of work!

9
Effect of Energy Spread on Cooling
1 MeV 90o
1 MeV/G4MICE
25 MeV 90o
25 MeV/G4MICE
25 MeV/RF 40o
25 MeV/ICOOL
  • Beta function for several different beams
  • Left hand plot has no RF/Absorbers, RH has full
    cooling
  • Energy spread gives a mismatch in the beam
  • Define 90o as on-crest

10
Transverse Emittance
25 MeV/RF 40o
25 MeV/G4MICE
25 MeV/ICOOL
25 MeV/RF 90o
1 MeV/G4MICE
1 MeV
1 MeV/RF 90o
  • Non-linear effects dominate with a small NuFact
    energy spread
  • Typical NuFact dE 25-100 MeV
  • Note blue red have same beam but with different
    scaping (1-5)
  • In ICOOL I killed particles at rgt250 mm, full
    aperture in G4MICE
  • Emittance growth originates from magnetic lattice
  • And is strong enough to kill all cooling

11
Emittance Growth vs Energy Spread
eout p mm rad
eout for E0-dE lt E lt E0dE
eout for E0lt E lt E0dE
dE MeV
  • Use a distn that is flat in momentum
  • Magnets only, ein12 p mm rad, taken over a 5.5 m
    MICE VI lattice
  • Clearly higher momentum spreads give more heating
  • Even for low momentum spreads eout gt 20 p mm rad
  • If we only take E gt E0 then we see no dependence
    on energy spread

12
Emittance Growth vs Energy
de p mm rad
Pz 177
Pz 200
n3
E0 MeV
  • Emittance growth is peaked around pz 180 MeV/c
  • Emittance growth over a single MICE lattice
    (-2750 to 2750) is 50 p mm rad!
  • Input beam has 12 p mm rad
  • This corresponds to the n3 resonance
  • The presence of this resonance seems a strong
    candidate for the emittance growth
  • It should be possible to remedy this by changing
    q0

13
Stop bands (Big)
14
Longitudinal Phase Space
  • MICE is scheduled to run on-crest
  • RF power too expensive to run off-crest
  • FS2 RF runs at 40o (relative to Ez0)
  • May be possible to run MICE V off-crest
  • Off-crest allows us to look at debunching due to
    Energy straggling
  • Longitudinal phase space at the centre of the 8th
    RF cavity

On crest
Off crest
15
Longitudinal Emittance
0.41 p ns rad
Un-normalised Trace Space (t,t), p ns/MeV
Normalised Phase Space (t, E) p ns rad
90 deg
40 deg
Heating associated with long drifts and magnets
Heating associated with magnetic lattice gtgt pz
normalisation
40 deg
90 deg
  • See large longitudinal emittance growth
  • Highly non-linear effects
  • Feeling is heating is mainly caused by the
    magnetic lattice
  • Also some particles dropping out of the RF
    bucket, some captured
  • Would like to see mainly heating from energy
    straggling
  • Why is there such a big difference between trace
    (x10) and phase (x2-4)?
  • It is crucial to understand what is going on here

16
Longitudinal Issues
  • Cov(E,t) is a free parameter?
  • I choose Cov(E,t)0 initially
  • Amplitude momentum correlation
  • Transverse emittance growth vs pz
  • Seems MICE VI baseline does not cool with an
    energy spread
  • The 3p/2 resonance is a good candidate for a
    cause
  • It would be interesting to look at general
    non-linear beam optics
  • We should be able to fix it by changing the
    magnetic lattice
  • In particular changing the q0 Fourier mode ltB2gt
  • But this needs to be verified
  • Longitudinal emittance growth
  • Longitudinal phase space is highly non-linear
  • Some particles in the RF bucket, some not
  • Emittance growth looks like it comes from the
    magnets here too
  • I havent gone into enough detail on this yet
  • There doesnt seem to be much literature on the
    subject

17
TOF, time and emittance
  • We need the timing measurements for certain tasks
    not related to PID
  • Longitudinal/6D emittance measurement
  • Longitudinal emittance growth tells us where to
    sit on the dE/dx curve for best cooling
  • Important for comparison with ring coolers, etc
  • Longitudinal-transverse correlations
  • As we have seen previously these are also
    important to MICE
  • Phasing of RF RF bucket
  • For these tasks
  • Timing measurement should be considered after any
    detector material
  • Timing measurement should be considered in the
    same plane as the other phase space variables
    (position, momentum, energy)
  • Think of MICE cooling channel as a black box
  • Measure phase space variables at each end of the
    cooling channel
  • Seek to understand what happens in between

18
Time at TRP
  • Seek to extrapolate TOF2 measurements into the
    tracker
  • Malcolm defines a Tracker Reference Plane (TRP)
    at the inside edge of the tracker
  • Seek to transport time measurement from TOF using
    energy measurement at SciFi
  • Track reconstructed particles from SciFi recon
    plane to TOF using G4MICE
  • Calculate time at TRP by t(z TRP) t(z TOF)
    dttracking
  • Tracking using reconstructed phase space
    variables from the downstream TRP to TOF2 (using
    G4MICE)
  • Expect to introduce an error from tracking s(t)
    s(dt/dz)Dz
  • I use standard beam matched to 4 T
  • Assume we have selected a beam with s(t) 500 ps
    upstream
  • In reality s(t) would grow in MICE but for
    convenience I assume it is 500 ps in the
    downstream tracker as well
  • s(E) 25 MeV

19
Detector Resolutions
Emeas - Etrue from SciFi
tmeas -ttrue from TOF
Full tracker
dElt10 MeV
  • Crucial variables are energy (dt/dz) resolution
    and time resolution
  • No TOF reconstruction yet so I assume a Gaussian
    distribution in t
  • No correlations with other phase space variables
  • Start with 70 ps resolution from TRD
  • Energy resolution looks rather large (rms21 MeV)
  • Malcolm informs me this is a bug
  • I will also try a cut dE lt 10 MeV gt (rms 5 MeV)

20
Error due to s(E)
dt(ztrp) ttrue - textr
textr (recon flight time from TRP to TOF)
Full tracker s(dt) 181 ps ltdtgt 27 ps
Full tracker
dElt10 MeV
dElt10 MeV s(dt) 93 ps ltdtgt 29 ps
  • Reconstructed flight time from TRP to TOF 7 ns
  • Track downstream to the TOF
  • Take out stochastic effects from the tracking,
    but still include ltdE/dzgt from the tracker
  • See 25 ps offset
  • Doesnt effect emittance measurement
  • Significant effect even without the larger
    momentum spread
  • Compare with TOF resolution 70 ps

21
Overall time resolution
dt(ztrp) tmeas - textr
Full tracker s(dt) 192 ps ltdtgt 26 ps
dElt10 MeV s(dt) 114 ps ltdtgt 28 ps
  • Time resolution at TRP roughly addition in
    quadrature of time resolution at TOF and time
    resolution from extrapolation
  • Calculated s(t) 194, 116 from addition in
    quadrature
  • Nb I define the 0 of time at the TRP

22
Time res at TRP vs Tof res
s(ttotal) ns
s(ttotal) ns
Full tracker
dElt10 MeV
s(ttof) ps
s(ttof) ps
  • Time resolution at TRP
  • Note the axes are different
  • 0.4-0.5 vs 0.1-0.2 ns
  • Compare with bunch length 500 ps
  • This answer is different to the one on the
    previous slide
  • I have made a mistake somewhere (ran out of time)

23
Correlations
Erec - Etrue MeV
Erec - Etrue MeV
s(dt,dE) 1.97 ns MeV
s(E,dE) 11.4 MeV2
trec - ttrue ns
dt ns
  • As expected, lots of correlations in the
    longitudinal phase space
  • Energy and time errors are highly correlated
  • E-dE correlation isnt as obvious
  • Remember

24
Emittance at TRP vs Tof Res
el ns
el ns
Full tracker
dElt10 MeV
s(ttof) ps
s(ttof) ps
  • Emittance resolution at TRP
  • Again the axes are different
  • Compare with true values
  • 0.116 inside cut
  • 0.119 outside cut

25
Time measurement issues
  • This is still preliminary
  • We need to measure time in MICE in order to
    measure longitudinal emittance
  • Also transverse-longitudinal correlations
  • Also RF bucket RF phase
  • A timing resolution of 70 ps is desirable to
    get a decent resolution on emittance
  • Timing at the TRP is crucially dependent on
    tracker resolution
  • Once the tracker bug is fixed, we should see an
    improvement in the resolution
  • With target tracker resolution 5MeV, we see of
    order 932 ps2 contribution to time resolution at
    TRP
  • I need to check the mistake in the time
    resolution calculation
  • The major hole really is understanding of the
    longitudinal emittance growth

26
Future
  • To write a MICE note on TOF II resolution
    requirement I need
  • To understand/resolve longitudinal emittance
    growth in MICE
  • Feeling is this means moving off the resonance
  • Need to check
  • Fall back use FS2 lattice (also has a notceable
    resonance)
  • To get a working reconstruction of pz
  • Fall back cut on pt or use a fitted
    reconstruction
  • To check/fix TOF resolution plots
  • These issues require input from other people
  • The time pressure is becoming more critical
  • Can we run on crest at MICE V?
  • What is the time scale for a decision if any?
  • What is the effect of a realistic RF field?
  • Is it reasonable to run without a central
    absorber?
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