Agenda News CERN EP DT MARS AOB UNIT1 BENDOTTI Jerome DIXON Neil DUMPS Raphael GONGALVES Antonio KOTTELAT LucJoseph KRISTIC Robert LAHU Gregory LOOS Robert PIEDIGROSSI Didier VERGAIN Maurice ID: 804881
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Slide1
DT-EF Section meeting 29/1/2016
Agenda
News CERN, EP, DT
MARS
AOB
Slide2UNIT1
BENDOTTI Jerome
DIXON Neil
DUMPS RaphaelGONGALVES AntonioKOTTELAT Luc-JosephKRISTIC RobertLAHU GregoryLOOS RobertPIEDIGROSSI DidierVERGAIN MauriceVOGEL A (Fell)UNIT2ANSTETT Didier HenriBOUVIER Philippe JacquesIJZERMANS PieterLESENECHAL YannickVAN BEELEN Jacob Bastiaan
Detector Construction & Operations(DT-CO)Antti ONNELADeputy: F.PEREZ
PH-DT Detector Technologies
Group leader: Mar CAPEANSDeputies: Andrea CATINACCIO & Michael MOLL Secretariat: Veronique WEDLAKESafety Linkperson: Isabelle MARDIROSSIAN
Design roomBAULT Christophe (PL)DEGRANGE JordanJAMET OlivierLENOIR PhilippeDesign and AnalysisALVAREZ DiegoBATISTA Joao CarlosDUARTE Fernando GARGIULO Corrado HATCH MarkWERTELAERS PietMARTENSSON O (Tech)Composite LabBOYER F (TRN VIA)
Engineering Office
(DT-EO)Andrea CATINACCIO
Silicon det R&D
MAPELLI AlessandroHONMA AlanMCGILL IanMANOLESCU FlorentinaBONNAUD J (Fell)GALLRAPP C (Fell)BRONUZZI I (Doct)CURRAS E (Doct)MATEU I (TRN FTEC)NEUGEBAUER H (Doct)OTERO Sofia (Doct)PITAES C (TRN Pt) Gas Det R&DROPELEWSKI Leszek (PL)OLIVERI EraldoRESNATI F (Fell)THUINER P (Doct) Irradiation FacilitiesRAVOTTI Federico (PL)GLASER MauriceFORTIN Richard GGORINE G (Doct)GOTKSE B (Doct)
Detector Development(DT-DD) Petra RIEDLER
GUIDA Roberto (Gas PL)PETAGNA (Cooling PL)CARRIE PatrickDAGUIN JeromeD'AURIA AndreaDE MENEZES Louis-PhilippeMERLET FredericNOEL JeromePAVIS StevenVERLAAT Bart WASEM AlbinZWALINSKI LukaszGIAKOUMI K (Fell EU)MANDELLI B (Fell)MOUSSY Y (Fell)OSTREGA M (Fell)PIMENTEL T (TRN Pt)HELLENSCHMIDT A (Doct)ROMAGNOLI G (Doct)SPADAVECHIA N (Tech)
Fluidic Systems
(DT-FS)Paola TROPEA
Engineering Facilities(DT-EF)Hans DANIELSSONDeputy: PA.GIUDICI
Thin Film & GlassSCHNEIDER Thomas (PL)DAVID ClaudeVAN STENIS MirandaMicro-Pattern TechDE OLIVEIRA Rui (PL)FERRY SergeGRIS AlexandraPIZZIRUSSO OlivierRANCHIN DavidRODRIGUES AlexisTEIXEIRA AntonioCHAMLEY C (Tech)Machine ShopsBODE AlainBRENDLEN RomainBRUNEL BernardCANTIN BernardGARNIER Francois Magnets supportBERGSMA Felix (PL)
DAVENPORT Martyn
GYS Thierry HAHN Ferdinand HAIDER StefanJORAM Christian KLEMPT Wolfgang MARTINENGO PaoloSROKA S (Fell)KOSTOGLOU S (Tech)
Technology & Physics(DT-TP)Burkhard SCHMIDT
PONS XavierBLANC PascalBOURGEOIS NicolasDERONT LaurentMAIRE GillesRAVAT SylvainRIGAUT Y.A. (PA)
Detector Interface
(DT-DI)Giovanna LEHMANN
Projects
Services
Contact Persons for Experiments and Projects
FSU PH40
FSU PH02
14/10/2015
2
Slide3Slide4MARS schedule
I have no date for my MARS yet but it is after 6/2
We should try to finish the
interviews in February, but the absolute deadline is March 11MARS form completed by GL and sent to the staff member by April 22.
Slide5Slide62015 at a glance: International Relations
ICA signature with USA at White House, 7-5-2015:
R.-D. Heuer with DOE Secretary E.J. Moniz and
NSF Director F. A. Córdova. ICA formalises US participation in HL-LHC and CERN participation in neutrino programme at FermilabAssociate Member States: Pakistan, Turkey, Serbia (in the pre-stage to membership)
Candidate to Membership accession: RomaniaApplicants for Membership or Associate Membership: Azerbaijan, Brazil, Croatia, Cyprus, India, Russia, Slovenia, Ukraine
International Cooperation Agreements (ICA): Lebanon, Palestine, USA, ESO, IRENA
Geographical enlargementYellow: 2015Protocol visits in 2015: 126Member States: 57Non-Member States: 39Observers: 17
Candidates for accession: 3Associates: 1Miscellaneous: 9
Slide71.2M CERN mentions
on social media
1.3M followers on Twitter
Awarded best Twitter page in Switzerland7M unique visitors to CERN’s core websites
2015 at a glance: Communications and Outreach
2015 media coverage:
180k press cuttings worldwide
New Microcosm exhibition openCERN guided tours 107000 visitors in 2015> 300000 visit requests/yr
Slide88
Why is the Higgs boson so light
(so-called “naturalness” or “hierarchy” problem)
?What is the origin of the matter-antimatter asymmetry in the Universe ?Why 3 fermion families ? Why do neutral leptons, charged leptons and quarks behave differently ? What is the origin of neutrino masses and oscillations ?What is the composition of dark matter (23% of the Universe) ?What is the cause of the Universe’s accelerated expansion (today: dark energy ?primordial: inflation ?)Why is Gravity so weak ? However: there is NO direct evidence for new particles (yet…) from the LHC or other facilitiesi.e. at what E scale(s) will we find the answers to these questions ?Main questions in today’s particle physics (a non-exhaustive list ..)Where is the New Physics ?
Slide99
With the discovery of the Higgs boson,
we have completed the Standard Model
(> 50 years of theoretical and experimental efforts !)However: the SM is not a complete theory of particle physics, as several outstanding questions remain (raised also by precise experimental observations) that cannot be explained within the SM. These questions require NEW PHYSICSNote: fermions (c, b, t, τ) discovered at accelerators in the US, bosons (g, W, Z, H) in Europe !
We have tested the Standard Model with very highprecision (wealth of measurements since early ‘60s,in particular at accelerators)it works BEAUTIFULLY (puzzling …)no significant deviations observed (but difficult to accommodate non-zero neutrino masses) Scientific strategy
Slide10Future Circular Colliders (FCC)
International conceptual design study of a ~100 km ring:
pp collider (FCC-hh): ultimate goal
defines infrastructure requirements
√s ~ 100 TeV, L~2x1035; 4 IP, ~20 ab-1/expt
e+e- collider (FCC-ee): possible first step
√s = 90-350 GeV, L~200-2 x 1034; 2 IPpe collider (FCC-he): option √s ~ 3.5 TeV, L~1034Also part of the study: HE-LHC: FCC-hh dipole technology (~16 T) in LHC tunnel √s ~ 30 TeV
GOAL: CDR in time for next ES
90-100 km ring fits geology
Machine studies are site-neutral.
However, FCC at CERN would greatly benefit from existing laboratory infrastructure and accelerator complexInternational Collaboration: ~ 70 Institutes
Slide111/28/16
FCC-hh: a ~100 TeV pp collider is expected to:
explore directly the 10-50 TeV E-scale
conclusive exploration of EWSB dynamics
say the final word about heavy WIMP dark matter FCC-ee: 90-350 GeVmeasure many Higgs couplings to few permill
indirect sensitivity to E-scale up to O(100 TeV) by improving by ~20-200 times the precision of EW parameters measurements, ΔMW < 1 MeV, Δmtop ~ 10 MeV
Many huge technological, design and operationalchallenges: e.g. ~16 T Nb3Sn magnets
Demonstrator (16 T, 50 mm gap)~ 1m, end 2018, 1980
1985
1990
1995
20002005
20102015
202020252030
2035
Physics
Construction
ProtoDesign
FCCConstruction
PhysicsProtoLHCConstructionPhysicsDesign
HL-LHC
DesignFCC
The two machines arecomplementary and synergetic
Slide12SAFETY
http://cds.cern.ch/journal/CERNBulletin/2015/49/Official News/2105551?ln=en
New safety rules:
Slide13AOB
AOB
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