The time of flight difference between the speed of light and theĪrriving neutrino LAr-TPC events has been analysed. The ICARUS T600 detector has collected 7 beam-associatedĮvents, consistent with the CNGS delivered neutrino flux of 2.2 10^16 p.o.t.Īnd in agreement with the well known characteristics of neutrino events in the Respect to the ordinary operation of the CNGS beam, since it allows a veryĪccurate time-of-flight measurement of neutrinos from CERN to LNGS on anĮvent-to-event basis. This very tightly bunched beam structure represents a substantial progress with LHC-like extractions, each with a narrow width of 3 ns, separated by 524 ns. pulse and with a beam structure made of four
The CERN-SPS accelerator has been briefly operated in a new, lower intensity
They can be searched for either through modifications to the data analysis protocol or relatively straightforward adjustments to the operating conditions of these experiments. These searches leverage the fact that the transit of the dark matter occurs at a speed ∼220 km/s, well separated from relativistic and terrestrial sources of noise.
This includes the detection of scintillation in MACRO, XENON and LUX heat in calorimeters such as CDMS acceleration and strain in gravitational wave detectors such as LIGO and AGIS and spin precession in CASPEr. The enhanced interaction between large composite states and the standard model allows searches for such composite blobs using existing experimental techniques. We study cosmological, astrophysical and direct detection bounds on this scenario and identify experimentally accessible parameter space. The low number density of these blobs necessitates new detector strategies. This picture is dramatically altered if there are significant self-interactions within the dark sector, potentially resulting in the coalescence of dark matter particles into large composite blobs. An optional PTP/IEEE-1588 Grandmaster provides specialized PTP hardware timestamping (8-nanosecond resolution).Current dark matter detection strategies are based on the assumption that the dark matter is a gas of noninteracting particles with a reasonably large number density. A built-in stratum 1, Network Time Protocol (NTP) server is enabled with a high-performance packet timing engine (7500 NTP packets per second). The network-centric Meridian II provides dual-gigabit Ethernet ports that are security hardened to meet the highest Information Assurance (IA) requirements. An optional PTP/IEEE-1588 Grandmaster provides specialized PTP hardware timestamping (8-nanosecond resolution). This results in the lowest total cost of ownership in the industry and is backed by our Satisfaction Guarantee!
#Endview gps software
High-Reliabilityĭesigned for mission-critical applications, Meridian II is based on a high-reliability, fanless platform with a conservative MTBF of up to 30 years. The product is made in America, supported with free software upgrades, and free technical support (if needed). EndRun's GPS ReceiverĪt the core of the Meridian II is our proprietary, time-and-frequency-optimized, GPS receiver that provides industry-leading time accuracy (< 10 nanoseconds RMS) and frequency accuracy (< 6x10-14 at 100,000 seconds) to UTC. For ultimate performance, the innovative Real-Time Ionospheric Corrections (RTIC) option compensates for ionospheric delay in real-time that meets the performance of L1/L2 solutions. Meridian II can be configured with our individually-characterized ovenized oscillator options and provide spectrally pure 5 MHz or 10 MHz outputs with state-of-the-art phase noise performance (< -113 dBc 1 Hz offset at 10 MHz). We fully specify the performance of our products and we back it up with measured data and a test report from the National Institute of Standards & Technology (NIST). None of our competitors fully specify their product or publish third-party data from a national standards lab.
#Endview gps code
TDC3303e Time Code Distribution Chassis.FDC3302e Frequency Distribution Chassis.FDC3300e Frequency Distribution Chassis.
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