These are eight transparent paintings of particle tracks from the ALICE experiment at @cern.bsky.social and visualizations of two colliding black holes
These are eight transparent paintings of particle tracks from the ALICE experiment at @cern.bsky.social and visualizations of two colliding black holes
Catering & movie organized by Absolute Delicious
absolute-delicious.nl
Catering & movie organized by Absolute Delicious
absolute-delicious.nl
The platform is kept quiet by Active Noise Cancellation which can break through the wall of noise in which gravitational wave signals are buried @vuamsterdam.bsky.social
The platform is kept quiet by Active Noise Cancellation which can break through the wall of noise in which gravitational wave signals are buried @vuamsterdam.bsky.social
ATLAS (@cern.bsky.social) detector with an 'Observation of VVZ production' event display. Einstein Telescope detector and the Pierre Auger Observatory. @km3net.bsky.social neutrino detector
ATLAS (@cern.bsky.social) detector with an 'Observation of VVZ production' event display. Einstein Telescope detector and the Pierre Auger Observatory. @km3net.bsky.social neutrino detector
www.youtube.com/playlist?lis...
www.youtube.com/playlist?lis...
Since 2016 Nikhef has been working on the @cern.bsky.social ATLAS Upgrade Inner Tracker (ITk) Strip End-cap. Two super rigid CF structures are assembled with a precise gluing jig in the Nikhef clean-room.
Since 2016 Nikhef has been working on the @cern.bsky.social ATLAS Upgrade Inner Tracker (ITk) Strip End-cap. Two super rigid CF structures are assembled with a precise gluing jig in the Nikhef clean-room.
Since 2015, Nikhef worked on the Upgrade of the @cern.bsky.social ALICE Outer Barrel (OB) Inner Tracking System (ITS). The ITS Module has 14 pixel chips which measures each 30x15mm with a thickness of only about 0.25mm
Since 2015, Nikhef worked on the Upgrade of the @cern.bsky.social ALICE Outer Barrel (OB) Inner Tracking System (ITS). The ITS Module has 14 pixel chips which measures each 30x15mm with a thickness of only about 0.25mm
Since 2015 NIKHEF has been building the @km3net.bsky.social detector. Each Digital Optical Module (DOM) contains 31 PhotoMultiplier Tubes (PMTs). Deployment in the Mediterranean Sea is at a depth of 2.5 - 3.5 km.
Since 2015 NIKHEF has been building the @km3net.bsky.social detector. Each Digital Optical Module (DOM) contains 31 PhotoMultiplier Tubes (PMTs). Deployment in the Mediterranean Sea is at a depth of 2.5 - 3.5 km.
Since 2015 NIKHEF has been building the @km3net.bsky.social detector. Each Digital Optical Module is 17 inches in diameter and contains 31 PhotoMultiplier Tubes. Deployment is in the Mediterranean Sea at a depth of 2.5-3.5 km.
Since 2015 NIKHEF has been building the @km3net.bsky.social detector. Each Digital Optical Module is 17 inches in diameter and contains 31 PhotoMultiplier Tubes. Deployment is in the Mediterranean Sea at a depth of 2.5-3.5 km.
NIKHEF was since 2010 in charge of the design and production of 5 MultiSAS systems, for Advanced Virgo, an upgrade of the Virgo interferometer with three kilometer long arms located near Pisa in Italy.
NIKHEF was since 2010 in charge of the design and production of 5 MultiSAS systems, for Advanced Virgo, an upgrade of the Virgo interferometer with three kilometer long arms located near Pisa in Italy.
Nikhef was in charge of the design and production of crucial hardware components for the vacuum, injection, and detection subsystems of Advanced Virgo, an upgrade of the Virgo interferometer located near Pisa (Italy).
Nikhef was in charge of the design and production of crucial hardware components for the vacuum, injection, and detection subsystems of Advanced Virgo, an upgrade of the Virgo interferometer located near Pisa (Italy).
Since 1999, Nikhef is involved in the VErtex LOcator (VELO) of @lhcb.bsky.social.
As a spin-off of the successful VELO CO2 cooling Nikhef built the CO2 cooling system of the Alpha Magnetic Spectrometer for at the ISS.
Since 1999, Nikhef is involved in the VErtex LOcator (VELO) of @lhcb.bsky.social.
As a spin-off of the successful VELO CO2 cooling Nikhef built the CO2 cooling system of the Alpha Magnetic Spectrometer for at the ISS.
Part 8:
Since @cern.bsky.social built the Large Hadron Collider (LHC) NIKHEF is involved in the ALICE, @atlasexperiment.bsky.social and @lhcb.bsky.social experiments.
Part 8:
Since @cern.bsky.social built the Large Hadron Collider (LHC) NIKHEF is involved in the ALICE, @atlasexperiment.bsky.social and @lhcb.bsky.social experiments.
In 2008 @cern.bsky.social converts LEP into the LHC, an accelerator with superconducting magnets.
NIKHEF is involved in 3 major experiments: @lhcb.bsky.social, @atlasexperiment.bsky.social and ALICE:
In 2008 @cern.bsky.social converts LEP into the LHC, an accelerator with superconducting magnets.
NIKHEF is involved in 3 major experiments: @lhcb.bsky.social, @atlasexperiment.bsky.social and ALICE:
In 1999, NIKHEF starts research in Astroparticle physics at the neutrino telescope ANTARES in the Mediterranean Sea.
In 1999, NIKHEF starts research in Astroparticle physics at the neutrino telescope ANTARES in the Mediterranean Sea.
In 1998 when the accelerator MEA-AmPS stopped the sections K&H were integrated. The institute name changed to: National Institute for Subatomic Physics.
NIKHEF will built at DESY detectors for the ZEUS & HERMES experiments.
In 1998 when the accelerator MEA-AmPS stopped the sections K&H were integrated. The institute name changed to: National Institute for Subatomic Physics.
NIKHEF will built at DESY detectors for the ZEUS & HERMES experiments.