!

CERN

LHC ring:
27 km circumference

Pisa Meeting 20091

TFJ
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IJOU TDBQF
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UBPS

nTOF

AD

11/13 May ‘09

Main Auditorium
Isoldecontinuation forrunning experiments,
new proposals,
accelerator(s),test beams,
impressions...

SPS
Workshop to preview anddiscuss plans to diversify thescientific programme for non-LHC
experiments
Sessionst SPS Deep-Inelastic Scattering, including polarized targetst SPS Rare K-decays and CNGSt SPS Hadrons & Ionst PS and Non-accelerator experimentst Isoldet nTOFt Test Beams & Irradiation facilitiest Antiproton Decelerator (AD)t Possible future developmentst Other facilitiest New Proton drivers at CERN

Organizing Committee

Ewa Rondio, CERN Directorate Office

KAON09 , Tsukuba 12 June 2009

I. Bejar Alonso, S. Bertolucci, P. Bloch, J. Dainton, M. Doser, J. Ellis, M. Huyse, P. Mage, E. Rondio, E. Tsesmelis

Contact new-physics@cern.ch / http://indico.cern.ch/event/51128

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“New Opportunities in the Physics Landscape at CERN”• took place at CERN on May 10-13,• a starting point to assess new ideas for uniqueexperiments, which can be performed at CERN,
outside the LHC programme.
http://indico.cern.ch/conferenceDisplay.py?confId=51128

Large interest in the community
 attendance (> 500),
 more than 100 abstract received,
 very lively community.

All abstracts, talks and recording of presentation on ,the summaries by the conveneors will appear their soonmore activities on non LHC physics
will follow soon
• A neutrino workshop, co-organized with the SPC
Study Group, will be held on October 1-3, 2009,
to focus the discussion on the European
Strategy on ν physics• A stronger connection among the CLIC and ILC
accelerator and detector R&D is being realized.
• A technical review of the LHC new injection
chain (LINAC4,SPL,PS2) is underway4due to “Austrian crisis”
replaced by Sergio Bertolucci

SPSC chair
INTC chair: short address by Rolf Heuer
new SPSC chair
new INTC chair5

sessions divided by subject and“accelerator requirements”• SPS:– Deep inelastic scattering, including polarized targets – E.Aschenauer– Rare K-decays and CNGS – C. Touramanis– Hadrons and Ions – K. Peters••••••PS and Non-accelerator Experiments – T. Sloan
ISOLDE – Y. Blumenfeld
n-ToF – F. Gunsing
Test beams and Irradiation facilities – C. Rembser
Antiproton decelerator (AD) – H. Abramowicz
Possible future developments – M. Mangano6

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Accelerators8•Correct size(~100m x 30m).

-Easy connection
to existing
Linac2-PSB line.

-Orientation
allowing future
extension to theSPL.

-Natural (earth)shielding.

•Linac4 because
the 4th ion linac tobe built at CERNPSLINAC49(possibly at 2020)

study group is working on PS2 ﬁxed target experimental area opLons, intensity upgrade
report in June 2009.

10SteveMyers

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The particle physics landscape• I

now and next 5-10 years
from conclusionsof SPSC and INTC chairsn‐ToF

s‐processes, cross sec*ons,
ﬁssion, neutron‐neutron int.
high brightness

ISOLDE

isotopes He to Ra
10‐6eV – 3MeV/ushell evolu*on, shapes,
exo*c nucl.,tests of SM12

13• Hadronic matter•  deconfinement•search for critical point,understanding of phasetransition
SPS gives an uniquepossibility for a scan
option of light ion in parallel with
Pb for LHC being checked14• hadron structure physics tries:– to understand the phenomenology resulting from QCD– provide input for searches for New Physics• improvements in precision and kinematic coverage forparton distributions is still needed– COMPASS short, medium and longterm plans:• spin structure, GPD, D-Y on pol. nucleon• exotic states, central production– DIRAC – now PS, 2011SPS (πK,KK,πµ)15new16

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needed synchronizaLon with FLAIR @ GSI/FAIR (>2015)

19

CAST search for solar axions
ISOLDE, n‐TOF ↔ nuclear
NA‐61 ↔

detector R&D for
DM search and otherexperiments can largely
proﬁt form CERN experLseand resources

astrophysics

air showers

Christian Spiering… are examples for CERN experiments

on astroparLcle physics or closely related
to astroparLcle physics

A European Centre for AstroparAcle Theory
could be established either in oneof the European countries or at CERN.
Given the synergy between LHC
physics and astroparLcle physics,
CERN would be a natural host,parLcularly in view of several
astroparLcle experiments
being CERN recognized experiments.

• search for neutral lepton (PS,SPS..)• study of “MiniBoone anomaly” (neutrino beam from PS)• MODULAR – very massive Liquide argon detector on CNGS beam

• charm baryons magnetic moment (extr. LHC beams)• charm production (fixed target with LHC protons)• mono energetic gammas, electrons in LHC• Proton Driven Plasma Wakefield Acceleration• measurement of u/d quarks distribution inside proton(for interpretation of LHC results)• novel axion helioscope - axion detection in thegradient of magnetic field21

presently considered at BNL (start 2017)at CERN can be done in half Lme if polarized beams get priority
22Light exoLc nuclei

ab‐ini*o from nucleon‐nucleon forcesshell evoluLon …………………………..
shell model interac*on

nuclear shapes at low spin
density‐func*onal theories

r‐process and rp‐process………………
nucleosynthesis and stellar energy genera*on

Vud, e‐ν correlaLons, etc.
tests of SM

580 parAcipants in 73 acAve experiments

research with RIB

s‐process and stellarcross‐secLon rates
neutron‐neutroninteracLon

σa, σf, of acLnides, ﬁssion,structure, of ADS/EA
77 parAcipants in 5 acAve experiments

~ 2000 researchers in low‐energy NP require both in‐ﬂight
and ISOL faciliLes (NuPECC LRP)
Complementarity (Europe)(i) SPIRAL‐2 – range of radionuclides(ii) FAIR – in‐ﬂight facility
CompeAAon (North America & Japan)
HIE‐ISOLDE + SPIRAL2 well placed to compete:
ISAC‐2 (TRIUMF) and FRIB (MSU) –Lmeline for technological development
RIBF(RIKEN) – in‐ﬂight facility

EU programmes
ExisLng: (‐2010) NUDATRA and EFNUDAT
new proposal ANDES (2010‐)
Complementarity/ CompeAAon(Europe)(i) GELINA (Geel) – electron linac(ii) NFS (GANIL) – cold ﬁssion(North America & Japan)
LANSCE (Los Alamos) spallaLon source
ORELA (Oak Ridge) electron linac
JPARC – spallaLon source
n_TOF advantages: brightness and energy resoluLon

North Area
SPS Test Beams

East Area
PS Test Beams

13 Mai 2009

E. Gschwendtner, CERN

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NorthArea
7 beam lines
total length 5.8 km
SPS
Test Beams

Three experimental halls :EHN1, EHN2, ECN3

East Area
PS Test Beams
5 beam lines
total length 300m
13 Mai 2009

E. Gschwendtner, CERN28

Test Beam Needs for Neutrino Detector R&D Projects

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Some test detectors exisLng or underconstrucLon

MEMPHYNO‐ Prototype forof Megaton
Mass PHYSics
Totally acLve ScinLllator

INO‐BABY‐MIND
E.g. magneLzed iron interleaved by acLve
detector elements

Liquid Argon R&D(Glacier Collab.)ePiLAr proposal
E. Gschwendtner, CERN

13 Mai 2009

• CERN has worldwide unique opportunity for detector and physics tests– PS and SPS beam-lines– Technical support and infrastructure provided by CERN• Facilities are heavily used
– Always fully booked• Future requests– Interest in Heavy Ions
• Needs additional preparation: e.g. radiation safety issues• Short-medium term (up to 2012)– R&D for Neutrino Detectors••••

Large objects
Looking for more permanent installation
Additional infrastructure (magnets, cryogenics)
High-Power targets

 Exciting new ideas for future experiments New technologies
 All experiments need test beams
13 Mai 2009

E. Gschwendtner, CERN30• many interesting ideas to follow up• expect several LoI or proposals soon work for scientiffic committees– running experiments have plans to continue• proposed upgrades in infrastructure need discussion and commitments• strong need for test beams will continue• more synergies with astroparticle community
thank you !
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