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Radioactive Ion Beams, 1

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Title: Radioactive Ion Beams, 1


1
Radioactive Ion Beams
  • A. Fabich, CERN
  • on behalf of the Beta-beam Study Group
  • http//cern.ch/beta-beam
  • NuFact06, UCIrvine

2
Outline
  • Beta-beam concept
  • EURISOL DS scenario
  • Layout
  • Main issues on acceleration scheme
  • Physics reach
  • Other scenarios
  • High-energy Beta-beams
  • Monochromatic beams with electron capture
  • Summary

3
Beta-beam principle
  • Aim production of (anti-)neutrino beams from the
    beta decay of radio-active ions circulating in a
    storage ring
  • Similar concept to the neutrino factory, but
    parent particle is a beta-active isotope instead
    of a muon.
  • Beta-decay at rest
  • n-spectrum well known from electron spectrum
  • Reaction energy Q typically of a few MeV
  • Accelerated parent ion to relativistic gmax
  • Boosted neutrino energy spectrum En?2gQ
  • Forward focusing of neutrinos ???1/g
  • Pure electron (anti-)neutrino beam!
  • NB Depending on b- or b--decay we get a
    neutrino or anti-neutrino
  • Two (or more) different parent ions for neutrino
    and anti-neutrino beams
  • Physics applications of a beta-beam
  • Primarily neutrino oscillation physics and
    CP-violation

4
Production chain
  • n-factory uses beam of 4th generation.
  • Beta-beam uses 3rd generation beam.
  • Beta-beam is technically closer to existing/used
    accelerator technology.
  • .

n-factory
and charge conjugated
beta-beam
Ion source
Acceleration
Storage
Neutrino beam
5
Choice of ion species
  • Beta-active isotopes
  • Distance from stability
  • Production rates
  • Life time
  • Reasonable lifetime at rest
  • If too short decay during acceleration
  • If too long low neutrino production
  • Optimum life time given by acceleration scenario
    and neutrino rate optimization
  • In the order of a second
  • Low Z preferred
  • Minimize ratio of accelerated mass/charges per
    neutrino produced
  • One ion produces one neutrino.
  • Reduce space charge problems

EURISOL DS
6
Baseline and detector
  • Neutrino physics similar as in n-factory, but at
    different n-energies.
  • Baseline distance
  • Relativistic gamma in the range of 100 400
  • Q-value of MeV ?? En in the range of GeV
  • Baselines in the range of 100-1500 km
  • Only one detector ? one baseline
  • Location available for detector underground area?
  • E.g. Fermilab-Soudan 730 km
  • Suitable for g6He350.
  • Detector technology
  • No magnetized detector necessary
  • Water Cherenkov is the standard choice.
  • Technically considerable in the Megaton class
  • Energy resolution of 250 MeV

CERN-Frejus 130 km
7
Guideline to n-beam scenarios based on
radio-active ions
  • Low-energy beta-beam relativistic g lt 20
  • Physics case neutrino scattering
  • Medium energy beta-beam g 100
  • E.g. EURISOL DS
  • Today the only detailed study of a beta-beam
    accelerator complex
  • High energy beta-beam g gt350
  • Take advantage of increased interaction
    cross-section of neutrinos
  • Monochromatic neutrino-beam
  • Take advantage of electron-capture process
  • Accelerator physicists together with neutrino
    physicists defined the accelerator case of
    g100/100 to be studied first (EURISOL DS).

8
The EURISOL scenario
  • Based on CERN boundaries
  • Ion choice 6He and 18Ne
  • Relativistic gamma100/100
  • SPS allows maximum of 150 (6He) or 250 (18Ne)
  • Gamma choice optimized for physics reach
  • Based on existing technology and machines
  • Ion production through ISOL technique
  • Post acceleration ECR, linac
  • Rapid cycling synchrotron
  • Use of existing machines PS and SPS
  • Achieve an annual neutrino rate of either
  • 2.91018 anti-neutrinos from 6He
  • Or 1.1 1018 neutrinos from 18Ne
  • Once we have thoroughly studied the EURISOL
    scenario, we can easily extrapolate to other
    cases. EURISOL study could serve as a reference.

9
Ion production ISOL method
  • 6He production
  • converter technology using spallation neutrons
  • Nominal production rate 51013 ions/s can be
    achieved.
  • 18Ne production
  • Spallation of close-by target nuclides 18Ne from
    MgO
  • 24Mg12 (p, p3 n4) 18Ne10
  • Direct target the beam hits directly the oxide
    target
  • Required production rate of 51013 ions/s
  • (for 200 kW dc, few GeV proton beam)
  • Estimated production rate more than one order of
    magnitude too low!
  • Novel production scenarios required.

10
Low-energy accumulation
  • Optional scenario to overcome short-fall in
    production rate
  • Target operated in DC mode
  • Not 100 of production is used
  • Dead time during acceleration
  • Simultaneous accumulation in low-energy ring
  • Design of a low-energy accumulation ring
    dedicated for isotope accumulation.
  • Possible solution. Yet not all technical issues
    addressed and solved.

11
Production with re-circulating ions
  • Production of unstable isotopes
  • Primary ions circulate in the beam until they
    undergo nuclear processes in the thin target
    foil.
  • Injection
  • Permanent accumulation of primary ions Single
    ionized ions are fully stripped by a thin foil.
  • Compensating ionization losses
  • Acceleration at each turn by an adequate
    RF-cavity
  • Ion channel
  • E.g. 7Li D ? 8Li p
  • 8Li t1/20.8 s, ltEngt6.7MeV
  • Rate gt 1014 ions/s
  • C. Rubbia et al. (see talk this week)

12
Use of existing accelerators
  • Use of CERN PS and SPS
  • Difficulties
  • Not designed for high intensity operation of
    radioactive ions
  • No collimation, non-baked vacuum system, ...
  • Slow cycling
  • Allows no optimization on machine design
  • Large ion loss
  • Considerable activation
  • Vacuum degradation
  • Space charge
  • Advantages
  • Possible cost reduction
  • Maximize use of well-known machines

13
Intensity evolution during acceleration
Bunch 20th 15th 10th 5th 1st
total
  • Cycle optimized for neutrino rate towards the
    detector
  • 30 of first 6He bunch injected are reaching
    decay ring
  • Overall only 50 (6He) and 80 (18Ne) reach decay
    ring
  • Normalization
  • Single bunch intensity to maximum/bunch
  • Total intensity to total number accumulated in RCS

14
Power losses - Activation
Power loss per unit circumference of a machine
Ploss/l ions Beta-beam Beta-beam
CNGS 6He 18Ne
RCS - 0.17 0.14
PS 3.3 2.2 2.8
SPS 0.25 0.4 0.25
  • Nucleon losses compared
  • PS and SPS comparable for CNGS and bb operation
  • PS exposed to highest power losses

15
Dynamic vacuum
  • Decay losses cause degradation of the vacuum due
    to desorption from the vacuum chamber
  • The current study includes the PS, which does not
    have an optimized lattice for unstable ion
    transport and has no collimation system
  • The dynamic vacuum degrades to 310-8 Pa in
    steady state (6He)
  • An optimized lattice with collimation system
    would improve the situation by more than an order
    of magnitude.

C. Omet et al., GSI
P. Spiller et al., GSI
16
Decay ring
A. Chance et al., CEA Saclay
  • Geometrical considerations
  • Maximize straight section
  • Shortest arcs possible
  • High magnetic field
  • SC magnets
  • For EURISOL scenario (g100)
  • Circumference 6900 m
  • Length of straight section 2500m
  • Ratio straight section/circumference 0.36
  • Geometric sizing for other gamma ranges just by
    linear scaling ? ratio always about 36
  • Neutrino rate

17
Stacking process
  • Longitudinal merging
  • Mandatory for success of the Beta-beam concept
  • Lifetime of ions (minutes) is much longer than
    cycle time (seconds) of a beta-beam complex

1) Injection
  1. Injection off-momentum
  2. Rotation
  3. Merging oldest particles pushed outside
    longitudinal acceptance ? momentum collimation

3a) Single merge
2) Rotation
3b) Repeated merging
18
Particle turnover
  • 1 MJ beam energy/cycle injected
  • ? equivalent ion number to be removed
  • 25 W/m average
  • Momentum collimation 51012 6He ions to be
    collimated per cycle
  • Decay 51012 6Li ions to be removed per cycle
    per meter

bb
19
Collimation and absorption
  • Merging
  • increases longitudinal emittance
  • Ions pushed outside longitudinal acceptance
  • ? momentum collimation
  • in straight section
  • Decay product
  • Daughter ion occurring continuously along decay
    ring
  • To be avoided
  • magnet quenching reduce particle deposition
    (average 10 W/m)
  • Uncontrolled activation
  • Arcs Lattice optimized for absorber system OR
    open mid-plane dipoles

s (m)
Straight section Ion extraction et each end
A. Chance et al., CEA Saclay
20
Physics reach
  • EURISOL scenario
  • g100
  • each 6He and 18Ne with a 5-year run
  • 2.91018 6He decays/year or 1.11018 6Ne
    decays/year
  • Physics reach
  • Sensitivity on Q13 down to 1o

21
Towards high-energy beta-beams
  • Beta-beam operation at higher relativistic g
    reduces the annual rate Rn due to
  • Extended acceleration time
  • Simple analytical approximation
  • Boosted life time
  • Average neutrino rate R at decay ring
  • at fixed ion rates from production.
  • Physics reach on neutrino beam side PR ? R g

R ? 1/g
22
Using existing HE hadron machines
Machine tramp (including injector chain) s Gmax(proton) gmax (6He2) gmax (18Ne10)
Tevatron 18 1045 349 581
RHIC 101 (41) 268 89 149
LHC 1200 7600 2500 3500
  • Tevatron most realistic scenario
  • Comparable fast acceleration in all energy
    regimes
  • gtop350
  • About 70 survival probability for 6He
  • Compare with 45 in the EURISOL DS
  • (2 seconds accumulation time considered)
  • Reduced decay losses and activation during
    acceleration
  • Several studies on the physics reach exist, but
    annual neutrino rates have to be reviewed.

23
n-Spectra
  • Wide spectra from super- and Beta-beams
  • Requires energy reconstruction in detectors
  • solution EC monochromatic beam
  • Electron capture
  • pe-?? nn
  • Sharp energy spectrum of the neutrino beam

24
Monochromatic n-beam
Decay t1/2 BRn EC/b En MeV DEn MeV
148Dy?148Tb 3.1m 1 0.96 2.1
150Dy?150Tb 7.2m 0.64 1 1.4
152Tm?152Er 8.0s 1 0.45 4.4 0.52
150Tm?1508Dy 72s 1 0.77 3.0 0.4
  • Disentangle measurement of q13 and dCP running at
    two different g
  • Ion species 150Dysprosium
  • Physics reach for 1018 neutrinos/year at DR, each
    5-year run at two different g

25
Special aspects of a EC n-beam
  • Requires acceleration of partly stripped ions
  • Vacuum lifetime comparable to half-life
  • Particle losses due to charge state change
    negligible
  • Most promising candidate 150Dysprosium
  • Main characteristics
  • Heavy and exotic isotope
  • Long lifetime
  • Production required gt1015 150Dy atoms/second
  • Production achievable 1011 150Dy atoms/second
  • 50 microAmps primary proton beam with existing
    technology (TRIUMF)
  • Acceleration demanding
  • Balance for charge state between high magnetic
    rigidity and space charge

Decay t1/2 BRn EC/b En MeV DEn MeV
150Dy?150Tb 7.2m 0.64 1 1.4
26
Physics reach in comparison
  • For q13gt1O a Beta-beam scenario is useful.
  • Improved situation in combination with
  • Super-beam
  • Simultaneous analysis of atmospheric neutrinos

27
Summary
  • Beta-beam accelerator complex is a very high
    technical challenge due to high ion intensities
  • Activation
  • Space charge
  • So far it looks technically feasible.
  • The physics reach for technically achievable
    scenarios is competitive for q13gt1O.
  • Usefulness depends on the short/mid-term findings
    by other neutrino search facilities.
  • Acknowledgment of the input given by M. Benedikt,
    A. Jansson, M. Lindroos, M. Mezzetto, beta-beam
    task group and related EURISOL tasks
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