Frank Linde (Nikhef) VDL, 15 february 2011 hele kleine deeltjes & hele grote experimenten.

Slides:



Advertisements
Similar presentations
Proposal for the Establishment and Funding of the Cluster of Excellence Origin and Structure of the Universe The Cluster of Excellence for Fundamental.
Advertisements

An intruder in the neutrino school and to finish...THE AXION CAST: The CERN Axion Solar Telescope Iñaki Ortega ISAPP 2013 LSC, Canfranc.
Frank Linde (Nikhef) VDL, 15 february 2011 hele kleine deeltjes & hele grote experimenten.
NikhefFrank Linde LHC/ATLASIvo van Vulpen APP/ANTARESAart Heijboer OIO/TheorieSander Mooij Engineering/CO 2 Bart Verlaat IndustrieJan Visser RondleidingJan.
Elementaire deeltjesfysica anti-materie anti elektron anti quarks u d e anti up anti down materie elektron quarks u d e up down positron.
Laboratoire d’Annecy-le-Vieux de Physique des particules CNRS/IN2P3 laboratory (since 1976) and part of the Université de Savoie (since 1995) Most slides.
Trigger issues for KM3NeT the large scale underwater neutrino telescope the project objectives design aspects from the KM3NeT TDR trigger issues outlook.
Laser Interferometer Gravitational-wave Detectors: Advancing toward a Global Network Stan Whitcomb LIGO/Caltech ICGC, Goa, 18 December 2011 LIGO-G v1.
The Large Hadron Collider By Kathleen McKay. What is the LHC? The most powerful particle accelerator in the world. A synchrotron (ring-shaped particle.
FJPPL, May 17 th, Researchers Engineers, Technicians, Administrative in 1300 lab IN2P3INSUSPMSTICSPISCSDVSHS Nuclear Particle.
Cosmic rays and how a Bristol Physicist won the Nobel Prize Dr Helen Heath.
Components of the Milky Way. Examples of Rotation Curves.
Jean Zinn-Justin, Dapnia ECFA 12/05/06 1 France with two institutions : CEA/DSM/Dapnia, CNRS/IN2P3.
LIGO Hanford Observatory
Large Magellanic Cloud, 1987 (51.4 kparsec) SN 1987a after before 2006 Hubble.
Survey of the Universe Greg Snow U Nebraska Lincoln CROP.
1 Observing the Most Violent Events in the Universe Virgo Barry Barish Director, LIGO Virgo Inauguration 23-July-03 Cascina 2003.
The LIGO Project ( Laser Interferometer Gravitational-Wave Observatory) Rick Savage – Scientist LIGO Hanford Observatory.
The CERN Scientific Program Le programme scientifique du CERN A tour around the accelerator facilities Un voyage à travers les accélérateurs CERN is the.
Astroparticle Physics (APP) research in the Netherlands Restricted-ECFA meeting NIKHEF, Amsterdam, 23 Sept. 2005, Gerard van der Steenhoven* ? LOFAR Gravitation.
2/27/2012Katsushi Arisaka, UCLA 1 Katsushi Arisaka University of California, Los Angeles Department of Physics and Astronomy Why.
Current European programs (prelim) Data PRC census (66 projects) Total cost 365 M€
Symmetry and Its Violation -unifying concept of universe- Tatsuya Nakada Lausanne, 8 February 2000.
Exploring the Cosmos with Neutrinos Aart Heijboer …all of them. nm
ASPERA Status Astronet GB 20 September 2006 S.Katsanevas CNRS/IN2P3.
Richard E. Hughes lastClass p.1 “The most incomprehensible thing about the universe is that it is comprehensible” - Albert Einstein.
Science astronomyparticle physics astroparticle physics particle astrophysics IHEF Stan Bentvelsen IAP Ralph Wijers ITFA Erik Verlinde theoretical physics.
October 2011 David Toback, Texas A&M University Research Topics Seminar 1 David Toback Texas A&M University Mitchell Institute for Fundamental Physics.
National Institute for Subatomic Physics Frank Linde, Nikhef director.
ANTARES  Physics motivation  Recent results  Outlook 4 senior physicists, ~5 PhD students, ~5 technicians M. de Jong RECFA 23 September 2005.
Astronomy particle physics astroparticle physics.
Astroparticle Physics in the Netherlands Gerard van der Steenhoven Amsterdam, November 15 th, 2004 NIKHEF Scientific Advisory Committee ? LOFAR Gravitation.
1 Gravitational Wave Astronomy using 0.1Hz space laser interferometer Takashi Nakamura GWDAW-8 Milwaukee 2003/12/17.
Frank Linde, 18 December 2007 FOM mission budget +450 k€/year (2008)
European Organization for Nuclear Research. Topics Founding Organization The accelerator Experiments Practical applications Video?
Alexander Kappes Erlangen Centre for Astroparticle Physics for the ANTARES collaboration IAU GA, SpS 10, Rio de Janeiro, Aug Status of Neutrino.
DARK MATTER & GALACTIC ROTATION 2012 ASTRO SUMMER SCHOOL.
Gravitational Waves.
DARK MATTER IN THE UNIVERSE? PRESENTED BY L. KULL AT THE R.H.FLEET SCIENCE CENTER December 14,2005.
Richard Wade PSD 2007 PPARC Science Challenges. Position sensitive detectors and PPARC Technology Challenges. Big Questions, Big Projects. Developing technology,
The Astroparticle Road Ahead Uli Katz ECAP / Univ. Erlangen Splinter Meeting on Multi-Messenger Astroparticle Physics Hamburg, 27 – 28 September.
Astroparticle physics with large neutrino detectors  Existing detectors  Physics motivation  Antares project  KM3NeT proposal M. de Jong.
High Energy Accelerators Dennis Silverman Physics and Astronomy U. C. Irvine.
KM 3 Neutrino Telescope European deep-sea research infrastructure DANS – symposium Maarten de Jong.
Fermilab: Present and Future Young-Kee Kim Data Preservation Workshop May 16, 2011.
Anne Green The Large Hadron Collider and the search for dark matter The Large Hadron Collider and the search for dark matter.
Particle Physics: building blocks of the universe Dr. James Catmore, Lancaster University Physics Dept.
1/16 NIKHEF National Institute for Nuclear - & High Energy Physics Frank Linde, RECFA Amsterdam 23 September 2005 NetherlandsNIKHEF & CERNResearchLEP &
Measurement devices Cloud chamber Geiger counter Bubble chamber Nuclear emulsion 2.
CERN Richard Jacobsson 1 Welcome to CERN!. CERN Richard Jacobsson 2 What is CERN? l European Organization for Nuclear Research, founded in 1954 l Currently.
Gravitational waves Gideon Koekoek January 9 th 2008 Research done at Nikhef.
05 Novembre years of research in physics European Organization for Nuclear Research.
Neutrino. Game Board FERMILABHAPPENINGSFIRSTSNEUTRINOSDETECTION.
Nov 2003 CERN - Particles, Fields and the Big Bang SPEAKERS Rolf Landua CERN Physicist, Research on Antimatter (Antihydrogen) Chairman Education and Communication.
LAPP Introduction Catherine ADLOFF for Yannis KARYOTAKIS.
Key figures ,86 M€ Details ● 40 PhDs (8,64 M€) ● 13 Postdocs (2,73 M€) ● 1,77 M€ travel ● 0,99 M€ ‘per diem’ ● 2,74 M€ fees ATLAS:LHCb:ALICE=5:3:2.
LISA October 3, 2005 LISA Laser Interferometer Space Antenna Using Gravitational Waves To Probe Black Hole Physics and.
Astroparticle Physics research in the Netherlands Scientific Advisory Committee NIKHEF, Amsterdam, 21 May 2005, Gerard van der Steenhoven ? LOFAR Gravitation.
Wilkinson Microwave Anisotropy Probe (WMAP) By Susan Creager April 20, 2006.
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.
What is the Astroparticle Physics European Consortium ? (ApPEC) S. Katsanevas ApPEC chairman.
The Quest for Gravitational Waves: a global strategy
The search for those elusive gravitational waves
Stanford Linear Accelerator
ATF2 meeting in Annecy October 9 to 11, 2006
UCLA High Energy & Astro-Particle (HEAP) Seminar
Welcome to Annecy and LAPP
Stanford Linear Accelerator
Frank Linde, Philips meets particle physics, 31 January 2012
Gideon Koekoek January 10th 2007
Presentation transcript:

Frank Linde (Nikhef) VDL, 15 february 2011 hele kleine deeltjes & hele grote experimenten

astronomy particle physics astroparticle physics

now abundance of chemical elements Big Bang’s afterglow Big Bang

Origin of particle masses? Newton didn’t know – neither do we … How did the Universe look directly after the Big Bang? Observe it! What is the Universe made of? We barely know 4%! Where is all the antimatter? Universe ought to be symmetric!

Astroparticle physics Accelerator-based particle physics VIRGO gravitational-wave detector Nikhef research: experiment XENON-1t deep-underground dark matter detector ANTARES deep-sea neutrino telescope AUGER cosmic ray observatory CERN: ALICE ATLAS LHCb

Nikhef = collaboration RuG NIOZ UT LEI TUe ASTRON TUD SRON +

natural particle sources astroparticle physics

natural source: cosmic rays,

AUGER cosmic ray observatory Argentina (pampa amarilla) Challenges: - huge area - wireless - solar power - ns timing - noise

ANTARES neutrino telescope Mediterranean Sea (2.5 km deep) Challenges: - size - deep sea - low power - noise - motions - ns timing

ANTARES neutrino telescope Mediterranean Sea (2.5 km deep)

ANTARES neutrino telescope Mediterranean Sea (2.5 km deep)

VIRGO laser interferometer Italy (Cascina near Pisa) Challenges: - signal size - noise

VIRGO laser interferometer Italy (Cascina near Pisa)

LISA laser interferometer Far away! (launch: 2018)

XENON-1t dark matter detector Italy (Gran Sasso near Aquila) Challenges: - background!

man-made particle sources accelerators: CERN!

PS ISR SPS SppS LEP LHC  CLIC ? CERN Netherlands: ~4.5% 1.9 € per person per year

man-made source: accelerator

ATLAS detector

Future projects LHC upgrades KM3NeT CLIC

LHC  2030 Versneller: -onderhoud -magneten -cryogenie Experimenten: -trackers -elektronica

ILC/CLIC Versneller: -structuren -supports -uitlijning Experimenten: -nog ver weg

ZFEL

questions?