KM3NeT M. de Jong Staff overleg 12 Mei 2005.  M. de Jong, P. Kooijman, G. v.d. Steenhoven, E. de Wolf (R. v. Dantzig, J. Engelen, P. de Witt Huberts,

Slides:



Advertisements
Similar presentations
Apostolos Tsirigotis KM3NeT Design Study: Detector Architecture, Event Filtering and Reconstruction Algorithms XXV Workshop on recent developments in High.
Advertisements

R.Shanidze, B. Herold, Th. Seitz ECAP, University of Erlangen (for the KM3NeT consortium) 15 October 2009 Athens, Greece Study of data filtering algorithms.
Trigger issues for KM3NeT the large scale underwater neutrino telescope the project objectives design aspects from the KM3NeT TDR trigger issues outlook.
Using HOURS to evaluate KM3NeT designs A.Leisos, A. G. Tsirigotis, S.E.Tzamarias In the framework of the KM3NeT Design Study VLVnT Athens, 15 October.
Jan 2009 U. Katz: Astroparticle Physics 1 What is KM3NeT – the Vision  Future cubic-kilometre sized neutrino telescope in the Mediterranean Sea  Exceeds.
A. BELIAS, NESTOR Institute, Pylos, Greece TeVPA 2009, July 13-17, SLAC1 KM3NeT, a deep sea neutrino telescope in the Mediterranean Sea KM3NeT objectives.
P. Sapienza, NOW 2010 The KM3NeT project  Introduction & Main objectives  The KM3NeT Technical Design Report  Telescope physics performance  New developments.
Neutrino Astronomy with KM3NeT was: Mediterranean Neutrino Telescopes - Status and Future Uli Katz ECAP / Univ. Erlangen International School.
The ANTARES Neutrino Telescope Mieke Bouwhuis 27/03/2006.
Antares/KM3NeT M. de Jong. neutrinos  p Scientific motivation: – origin cosmic rays – birth & composition relativistic jets – mechanism of cosmic particle.
Deep-sea neutrino telescopes Prof. dr. Maarten de Jong Nikhef / Leiden University.
KM3NeT IDM/TeVPA conference 23  28 June 2014, Amsterdam, the Netherlands Maarten de Jong on behalf of the KM3NeT collaboration The next generation neutrino.
The ANTARES experiment is currently the largest underwater neutrino telescope and is taking high quality data since Sea water is used as the detection.
The Transverse detector is made of an array of 256 scintillating fibers coupled to Avalanche PhotoDiodes (APD). The small size of the fibers (5X5mm) results.
Paolo Piattelli - KM3NeTIAPS - Golden, 6-8 may 2008 KM3NeT: a deep-sea neutrino telescope in the Mediterranean Sea Paolo Piattelli - INFN/LNS Catania (Italy)
Exploring the Cosmos with Neutrinos Aart Heijboer …all of them. nm
Apostolos Tsirigotis Simulation Studies of km3 Architectures KM3NeT Collaboration Meeting April 2007, Pylos, Greece The project is co-funded by the.
Report of the HOU contribution to KM3NeT TDR (WP2) A. G. Tsirigotis In the framework of the KM3NeT Design Study WP2 Meeting - Marseilles, 29June-3 July.
Status of KM3NeT (Detector Design Optimisations) Christopher Naumann, CEA Saclay – IRFU / SPP for the KM3NeT consortium 44 th Reconcontres de Moriond,
KM3NET 24 September 2004 Gerard van der Steenhoven (NIKHEF)
CEA DSM Irfu The ANTARES Neutrino Telescope A status report Niccolò Cottini on behalf of the ANTARES Collaboration 44 th Rencontres de Moriond February.
Piera Sapienza – VLVNT Workshop, 5-8 october 2003, Amsterdam Introduction and framework Simulation of atmospheric  (HEMAS and MUSIC) Response of a km.
WP2 meeting, Oct 2006, CPPM Claudine Colnard - NIKHEF Claudine Colnard, Ronald Bruijn, Eleonora Presani, Siemen Meester, Paul Kooijman (presented by Maarten.
V.Bertin CPPM / ANTARES Coll. - Moriond ANTARES : A deep-sea 0.1 km² neutrino telescope Vincent Bertin - CPPM-Marseille on behalf of the Antares.
A sensor architecture for neutrino telescopes on behalf of the KM3NeT consortium Els de Wolf Thank you, Claudio!
ANTARES  Physics motivation  Recent results  Outlook 4 senior physicists, ~5 PhD students, ~5 technicians M. de Jong RECFA 23 September 2005.
KM3NeT International Solvay Institutes 27  29 May 2015, Brussels, Belgium. Maarten de Jong Astro-particle and Oscillations Research with Cosmics in the.
Disk WP-4 “Information Technology” J. Hogenbirk/M. de Jong  Introduction (‘Antares biased’)  Design considerations  Recent developments  Summary.
CEA DSM Irfu Reconstruction and analysis of ANTARES 5 line data Niccolò Cottini on behalf of the ANTARES Collaboration XX th Rencontres de Blois 21 / 05.
Antares Slow Control Status 2007 International Conference on Accelerator and Large Experimental Physics Control Systems - Knoxville, Tennessee - October.
Time over Threshold electronics for an underwater neutrino telescope G. Bourlis, A.G.Tsirigotis, S.E.Tzamarias Physics Laboratory, School of Science and.
R. Coniglione, VLVnT08, Toulon April ‘08 KM3NeT: optimization studies for a cubic kilometer neutrino detector R. Coniglione P. Sapienza Istituto.
Disk Towards a conceptual design M. de Jong  Introduction  Design considerations  Design concepts  Summary.
Astroparticle physics with large neutrino detectors  Existing detectors  Physics motivation  Antares project  KM3NeT proposal M. de Jong.
Sebastian Kuch, Rezo Shanidze Preliminary Studies of the KM3NeT Physics Sensitivity KM3NeT Collaboration Meeting Pylos, Greece, April 2007.
Neutrinos and the sea Els de Wolf NIKHEF Ilias Meeting, Prague, February 8 th 2005.
KM 3 Neutrino Telescope European deep-sea research infrastructure DANS – symposium Maarten de Jong.
Status of Sirene Maarten de Jong. What?  Sirene is yet another program that simulates the detector response to muons and showers  It uses a general.
NEMO-O DE NEMO First results from the NEMO Test Site G. Riccobene, for the NEMO Collaboration The NEMO Collaboration is performing the Phase 1 of the project,
Calibration of Under Water Neutrino Telescope ANTARES Garabed HALLADJIAN October 15 th, 2008 GDR Neutrino, CPPM, Marseille.
Infrastructure for Neutrino astroparticle physics and Marine science KM3NeT.
Antares status and plans  Reminder  Project status  Plans M. de Jong.
Isabella Amore VLV T08, Toulon, France April 2008 International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean Sea Results.
Neutrino telescopes: ANTARES and KM3NeT Maarten de Jong Programme: Group composition (current): 6+2 staff, 4 post-doc, 4 PhD. Vidi 1, Veni 1+1.
R. Kluit Nikhef Amsterdam ET Nikhef Electronics Technology TGL Ruud Kluit 118-Apr-16.
KM3NeT – Stautus and Future Uli Katz ECAP / Univ. Erlangen th International Workshop on Next Generation Nucleon Decay and Neutrino Detectors.
Antares/KM3NeT M. de Jong. Antares  2000NL joined collaboration (3.3 M€)  2006 ‒ 2008construction  2006 ‒ todaydata taking 24h/day  2012MoU signed.
The Neutrino Telescope of the KM3NeT Deep-Sea Research Infrastructure Robert Lahmann for the KM3NeT Consortium Erlangen Centre for Astroparticle Physics.
Status report Els de Wolf Annual Meeting 2011, Nikhef.
KM3NeT Neutrino conference 2-7 June 2014, Boston, U.S.A. Maarten de Jong on behalf of the KM3NeT collaboration The next generation neutrino telescope in.
CEA Saclay – Institute of research into the fundamental laws of the Universe PPM DU Pre Production Model Detection Unit Status and plans Th. Stolarczyk.
Status of ECAP Simulations for the KM3NeT TDR KM3NeT WP2 meeting Rezo Shanidze Paris, December 2008.
Status Antares & KM3NeT SAC 2010 Maarten de Jong.
NIKHEF jaarvergadering 18 Dec. ‘06 Gerard van der Steenhoven (NIKHEF) Programmaleider ‘Astrodeeltjesfysica’ Astroparticle physics Introduction.
KM3NeT P.Kooijman Universities of Amsterdam & Utrecht for the consortium.
Deep-sea neutrino telescopes
P.Kooijman, UVA-GRAPPA, UU, Nikhef
Sebastian Kuch University Erlangen-Nürnberg
Pasquale Migliozzi INFN Napoli
Els de Wolf, Nikhef/UvA KM3NeT WP345-meeting 23 February 2009
T. Eberl for Robert Lahmann and the Erlangen acoustic group
White Rabbit in KM3NeT Mieke Bouwhuis NIKHEF 9th White Rabbit Workshop
Els de Wolf 20 February 2012, Catania
Phototube response for a multi-element Optical Module
Point-to-point connection between each DOM and the shore station
Mieke Bouwhuis on behalf of the ANTARES collaboration
Sea Operations for “km3” neutrino telescope
on behalf of the NEMO Collaboration
Robert Lahmann for the ANTARES Collaboration
Acoustic Measurements in ANTARES: Status and Aims
Presentation transcript:

KM3NeT M. de Jong Staff overleg 12 Mei 2005

 M. de Jong, P. Kooijman, G. v.d. Steenhoven, E. de Wolf (R. v. Dantzig, J. Engelen, P. de Witt Huberts, J. Oberski)  M. Bouwhuis, R. Bruijn, C. Colnard, G. Lim, B. v. Rens, G. de Vries (A. Heijboer)  E. Heine, J. Hogenbirk, L. Kruijer, H. Peek (E. Kok, P. Rewiersma)  R. v. Wijk, G. Venekamp  E. Berbee, …  B. Verlaat  KVI: N. Kalantar, H. Loehner Who?

What?  Very large neutrino telescope(~20 x Antares)  Cost: ~200 M € (~10 x Antares)  Somewhere in the Mediterranean sea  Antares + Nemo + Nestor + associated scientists Design Study

NIKHEF contributions to Antares  “All-data-to-shore” concept –DWDM –PC farm (‘tier 0’) –Online software (Run control, Trigger, monitoring)  Electrical power system  Passive cooling design  Reconstruction  Physics analyses

Focus  Explore DWDM technology(75%)  Optical module design(5-25%)  Software trigger(75%)  Production of detector units(1/5)

DWDM technology  Optical multiplexing  Modulation of light  Fiber optics NIKHEF High bandwidth (~Tb/s) signal transmission

Optical module design  Small PMTs –Segmentation of photo-cathode (2 hit resolution!) –Solid angle versus photo-cathode area  Time-over-Threshold discriminator –Analogue multiplicity counter Optimise Signal / Noise at PMT level

DWDM + T-o-T + Modulation ~No offshore electronics

Software Trigger  Fast algorithms  Flexible design  Extendable PC farm More Physics

Production (1) Optical module assembly bar ~5 / day Pressure test

Production (2) Line assembly ~500 m ~1 / week ~25 optical modules / line E/O cable

Production (3) Calibration

Production (4) Pylos Sicily Pylos

Summary  Excellent opportunity for NIKHEF to play a leading role in an important experiment  Technology –Collaboration with industry –High-tech fiber optics –State-of-the-art software –‘Tier 0’ design PC farms  Excellent prospects for exciting physics –Great discovery potential –Attractive outreach program