SPL-Fréjus Collection partkirkmcd/mumu/target/...+ ATM ν:see Th. Schwetz Machines R. Garoby & M....

31
ISS-CERN 22-24/9/05 SPL-Fréjus Collection part J.E Campagne Thanks to S. Gilardoni, A. Cazes

Transcript of SPL-Fréjus Collection partkirkmcd/mumu/target/...+ ATM ν:see Th. Schwetz Machines R. Garoby & M....

Page 1: SPL-Fréjus Collection partkirkmcd/mumu/target/...+ ATM ν:see Th. Schwetz Machines R. Garoby & M. Lindroos TRE CERN SPL LSM-Fréjus Near detector 1 3 0 km Related talks ISS CERN 05

ISS-CERN 22-24/9/05

SPL-Fréjus

Collection part

J.E Campagne

Thanks to S. Gilardoni, A. Cazes

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ISS CERN 05 J.E Campagne (LAL) 2

New optimization questioned @ MMW04*

Particle production

Horn design optimisation

Decay tunnel parameter optimisation

Flux computation at Fréjus

θ13 and δCP sensitivity.LAL – 04-102 submitted to EPJC

p

π,Κ

π,Κ ν

*: Multi MegaWatt Workshop at CERN 26-28 May 04

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ISS CERN 05 J.E Campagne (LAL) 3

Particle productionProton beam :

1. Pencil like2. Ek=2.2GeV, 3.5GeV,…, 8GeV

Target : 1. 30cm long cylinder, ∅15mm in Liq. Hg2. FLUKA 2002.4

Normalized to 4MW beam power:1.10 1023 pot/yr @ 2.2GeV0.69 1023 pot/yr @ 3.5GeV0.30 1023 pot/yr @ 8.0GeV

Pion+ production

0,25

0,26

0,27

0,28

0,29

0,30

0,31

0,32

0,00 2,00 4,00 6,00 8,00 10,00

Beam Energy

yiel

d (1

e23)

Max. π yield ≠

Max. Phys. sensitivity

5GeV

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SuperBeam vs νFact Optics

px/pz

x20 mrad

2 m

Super Beam

Spot size @ 130kmDecay tunnel size

px/pz

x

½ rad

30cm

νFact

Decay channel solenoidsAperture and B strength

Thanks S. Gilardoni

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ISS CERN 05 J.E Campagne (LAL) 5

Pion production p (2.2GeV)π+

Hg

νFact SB

at the exit of the target

Horn optimisation by S. Gilardoni

This new optimisation

2 105 pot

Rule of thumb: Eπ/3~ Eν (MeV) > 2.L(km)

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Kaon production?

at 2.2GeV : 0.26 π+/s 0.8 10-3 K+/s

see BENE meeting 11/09/03

at 3.5GeV : 0.29 π+/s 2.8 10-3 K+/s

at 4.5GeV : 0.32 π+/s 5.2 10-3 K+/s

Ep(GeV) Ep(GeV)

π+

π-

K+

K-

K0Not physical dip !!!Not Used…

3.52.2

For

500

000

pot

Rate x 1016

New Fluka will be tested

HARP ???

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Horn style of collection

Bφ(r) ∝ Icur/rIcur ~ (300 ÷ 600) kA

rmin limited by Target size π+

IN

OUT

“Ideal”

shape

20cm

4cm1m 2m

40cm

The wrong sign pionsare eliminated locally

JEC NuFact-Note-138

Fixed momentum focalisation~800 MeV/c

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Comparison Solenoid vs Horn

S. Gilardoni thesis

capt

ure

Dec

ay s

olen

oid

~3m

20T →1.2

5T30cm

0,3m ~1m

The collection yield is identical ~1.4 10-3 π/pot

νFact

Solenoid

Horn x 2MARS

Cut : 1.5 cm.rad

In µRLA

Dec

ay s

olen

oid

~0.5m~1m ~1m

E

Horn ≈ Solenoid

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Horn design parameter for Super Beam

140 cm 220 cm

80 cm

140cmtotal length

220cmtotal length40cmouter radius

REFLECTOR

20.5cmouter radius40cmneck length3.4cminner radius

HORNHORN

Eν~300MeVEπ~800MeV

Conductor thickness : 3mmhorn : 300kAmps

reflector : 600kAmpsChallenging!!!

Using Geant 3.2.1NuFact-Note 138

Drawing from the horn built at CERNOptimized for Super Beam

+ or - focusing

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Decay Tunnel Parameters

• Lengths: 1. Modify beam purity2. Tested: 10m …→ 40m …→ 60m3. Optimum @ 40m

• Radius: 1. modify acceptance2. 1m …→ 2m3. No optimum found: larger is better (we just keep

“reasonable” radius)

This results have been checked on sensitivity to θ13 and δCP

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Fluxes comparison @ 130km

<Eν> ~ 275 MeV, 4.5 1011/m2/yrOld νFact optimum

<Eν> ~ 300 MeV, 1.2 1012/m2/yr3.5GeV SPL optimum

~95 νµCC/kT/yr*

*: Lipari x-sect. (see later)Reflector: 50% of the Flux

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π+π−

~1/2 µ− & 1/2 K0e3

µ+

Flux @ 130km: compositionhttp://opera.web.lal.in2p3.fr/horn/Simu/index.htm

3.5GeV Kinetic p beam~800MeVπ focusing40m decay tunnel length2m decay tunnel radius

+ Focusing

− Focusingπ−π+

~1/3 µ+ & 1/3 K0e3 & 1/3 K+

e3

µ−

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The X-sections

βB is an ideal tool to measure these cross-sections and a 2% systematic error on both signal and background are used.

---: Lipari et al.PRL74(95)4384

on H20

νµ SPL

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Some physics performances440kT water Č, 4MW SPL, GLoBES

2% syst. on signal & bkg

(χ2(2dof)=4.6 or 11.83)*: 5 bins [0.08,1.08] GeV

Sin22θ13(90%CL) = 610-3 (0.7°)

5yrs (+)δCP=0

preliminary

90%CL

New Opt.Old Opt.

True values: (∆m23, sin22θ13)

sin22θ12=0.82, θ23=π/4, ∆m221=8.1 10-5eV2

5% external precision on θ12 and ∆m221 and

use SPL disappearance channel and spectrum analysis*

sizeable improvement

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Beam Energy comparison

hep-ex/0411062 with an early version of analysis

10-310-4 10-310-4

5y+ 2y+8y-

2.2GeV3.5GeV4.5GeV8GeV

-100

-50

0

50

-150

3.5GeV is an optimum

Eν~260MeV

δCP = 010-3 sin22θ13

10-3

∆m

2 23 (e

V2)

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CNGS vs SB/νFact HORN

SB/νFact CERN proto

CNGS Horn

Pbeam = 4MW / 2÷3GeV, Target inside300÷600kA/50Hz/100µs200 M pulses/6 weeks

Neck: PJ = 7kW, PB = 63kW (8mm eq. Alu)1022 fast neutron/cm2/6 months

Pbeam = 0,4MW / 400GeV, Target outside150kA/2pulses 10µs-6s20 M 2pulses/5 years

IC: PJ = 13kW, PB = 5kW (2mm Alu)

Every parameter is critical

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CERN prototype (2001-2002)

Neck

Inner Cond. Double skin

S. GilardoniS.Rangod, J.M Mauguin…

1 m

42 c

m

Water cooling

(NUFACT-NOTE : 4, 28, 42, 80, 81, 126, 129)

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Energy deposition in the horn (induced by protons)

34.0 kW47kW

A. Cazes + JECNufact-Note-134

4MW, 2GeV proton beam

+7kW fromJoule effect

13.6kW

Solution ?: reduce Al thickness (3mm Al) + strength rings

63kW(8mm Al)

Page 19: SPL-Fréjus Collection partkirkmcd/mumu/target/...+ ATM ν:see Th. Schwetz Machines R. Garoby & M. Lindroos TRE CERN SPL LSM-Fréjus Near detector 1 3 0 km Related talks ISS CERN 05

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Horn cooling (CERN schema)

Round shape thread inside the waist

The gain in surface exchange is somewhatlost by the thickness increase and then the heat load increase…

Double skin 20kW/surface exchange275kW/m2

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R&D: water cooling is still ok?

Aluminum alloy cylinder80 mm ext. diameter300 mm length

Heat load ~ 30 kW

Water curtainor other water jets

configuration

At LAL

Sprinkler

Contact me if you plan to do it

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Power Supply (basic)

500 (180 Horn) µΩR1500µFC

0.6 (0.4 Horn)µHL

100µsτo

300kA (14,5 rms)IM

7kVUo

50Hz thyristors

50Hz: 20 x « µ life time »

The main trouble

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Power Supply

• CERN had successfully tested the Horn at 100kA/(0.5)Hz• mid-June 03: a schedule of conditions have been written by LAL

(13p) for a (300kA/100µs/50Hz) power supply.• 1st industrial price feed back:

1. Main power supply (7kV/130A): HAZEMEYER co.: ~ 160k€2. Switches (300kA/100µs/50Hz): ABB co: ~ 3x2x50k€* = 300k€

But we think that a 300kA/1Hz may be a good next step to push the present CERN power supply prototype..

A solution exists for ~ 460k€ (700kCH)

*: factor 2 for # of switches, factor 3 for 1Hz -> 50Hz

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Al alloy property modifications

6082 (CNGS) or 6061 (MiniBOONE)

Précipitation (Mg2Si) par nThermique

Défauts par nRapide

Flux (n/cm2)

Rp ou Rm

1021 61022

Cavités

(n,p) et (n,α) reactions produce hydrogen and helium cavities

J.E.C NuFact-Note-130

Non irradiated Al can stand more than 108 pulses

And also MiniBOONE…

108 pulses

Max. stress ~ 14MPa to be confirmed

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Other problems…

• Integration of the Target• Compatibility with Hg• Radioactive water cooling treatment • Water Cooled Striplines• Fabrication cost issues if the life time of

a horn is < 1y• Fast Coupling (cooling & electric) remotely

controlled (see US/Japan example)

• Nuclear waste management...

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Summary

An optimized version of the Horn-like collection/focusing and SuperBeam energy is availablewith the present knowledge of the π/K production x-sections and the detector performances.The Horn R&D has been interrupted more or less in 2002 at CERN and not revived yet elsewhere.The Horn-like collection has been demonstrated in the past to be equivalent to a Solenoid-like collection for a NuFact. The SB-Horn and the NF-Horn are different simply because they have different purposes, but they share a lot of design parameters, so a SB-Horn is a prototype for a NF-Horn.

Thank you

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ISS-CERN 22-24/9/05

END

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A possible schema

+ BetaBeam: see M. Mezzetto+ ATM ν: see Th. Schwetz

MachinesR. Garoby & M. Lindroos

TRE

CERN SPLLSM-Fréjus

Near detector

130km

Related talks

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ISS CERN 05 J.E Campagne (LAL) 28

SPL block diagram (CDR 1)Characteristics (Conceptual Design Report 1):

are “optimized” for a neutrino factoryassume the use of LEP cavities & klystrons up to the

highest energy

2.2GeV

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Gradients at 700 MHz

Last test performed in CryHoLab (July 04):5-cells 700 MHz ß=0.65 Nb cavity A5-01from CEA/Saclay and IPN-Orsay

from Stephane Chel, HIPPI04, Frankfurt, sep04

LEP cavities may have worked 350MHz & 3.6MV/m effective gradientNuFact Note 040

1E+08

1E+09

1E+10

1E+11

0 2 4 6 8 10 12 14 16 18 20Eacc ( MV/m )

Q0

Vertical Cryostat (Fast Cooling)

Horizontal Test in CryHoLab (B1)

quench

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Choice of the EnergyNeglecting Matter effect (Ok CERN-Frejus), for δCP = 0°

Maximum of probability is obtained for

2famillies formula

∆m221=810-5eV2, ∆m2

31=2.410-3eV2, L=130km

Eν = 250MeV

c23=s23=1/√2,tan2θ12=0.4

sin22θ13=10-2, Eν =320MeV sin22θ13=10-3, Eν =390MeV

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Decay Tunnel ParametersLengthLength

1. modify purity2. L=10m, 20m, 40m and

60m have been tested.

3. 10m→40mνµ , νµ + 50% to 70%νe , νe + 50% to 100%

4. 40m→60mνµ , νµ + 5%νe , νe + 20%

40m seems better40m seems better

RadiusRadius1. modify acceptance2. R=1m, 1.5m and 2m

have been Tested3. 1m →2m (L=40)

νµ , νµ +50%νe , νe +50% to 70%

Larger is better (2m)…Larger is better (2m)…

This results have been checked on sensitivity to θ13 and δCP