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DT-EF Section meeting 29/1/2016 DT-EF Section meeting 29/1/2016

DT-EF Section meeting 29/1/2016 - PowerPoint Presentation

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DT-EF Section meeting 29/1/2016 - PPT Presentation

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

doct fell fcc 2015 fell doct 2015 fcc amp tev lhc cern physics 100 tech detector membership questions collider

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Slide1

DT-EF Section meeting 29/1/2016

Agenda

News CERN, EP, DT

MARS

AOB

Slide2

UNIT1

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

Slide3

Slide4

MARS 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.

Slide5

Slide6

2015 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

Slide7

1.2M 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

Slide8

8

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 ?

Slide9

9

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

Slide10

Future 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

Slide11

1/28/16

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

Slide12

SAFETY

http://cds.cern.ch/journal/CERNBulletin/2015/49/Official News/2105551?ln=en

New safety rules:

Slide13

AOB

AOB

Next meeting