NOvA Experiment
|
|
NOvA is a second generation, accelerator based, long-baseline neutrino oscillation
experiment, and a flagship experiment for Fermilab's Intensity Frontier program.
NOvA is specifically designed to resolve the outstanding questions in neutrino mixing and
the structure of the neutrino sector, and features a unique "totally active" detector
design that singles it out as one of the most sensitivity and versatile neutrinos experiments
in the world.
Over the last decade, since the discovery of finite, non-zero neutrino mass through their
oscillations over the solar and atmospheric distance and energy scales— the first
evidence of physics beyond the standard model — much has been learned
about elusive world of neutrinos. Yet much remains to be learned. NOvA is poised to make
seminal measurements of neutrino properties that will answer questions of whether
neutrinos are a source for the Matter/Anti-matter asymmetry of the universe.
The NOvA experiments consists of two independent detectors separated by 810 km.
At Fermilab is the Near Detector, which counts the number of neutrinos produced
by the Fermilab accelerator. The Far Detector is sited in northern Minnesota
near the US/Canadian border, and is 14 mrad away from the primary beam axis, in
what is referred to as the "off-axis" configuration. This choice of site location
and baseline is what allows NOvA to perform precisions measurements of &theta13
and &theta23. The Far Detector, at a massive 15,000 tons, will be the
largest liquid scintillator calorimeter ever build, indeed the largest plastic
structure ever built, and has been designed to search for electron neutrino appearance
in the Fermilab muon neutrino beam.
Construction of the NOvA experiment started in May of 2009 and the first set of physics data is
expected from the Near Detector in earl 2011. The construction of the Far Detector will continue
in parallel with the Near Detector operation and will become fully operational in 2013 at its full
mass of 15,000 tons.
Virginia's role on NOvA
The University of Virginia has taken on a leading in the design and implementation of the NOvA experiment.
The Virginia group working on NOvA is Headed by Professor Craig Dukes, and is the primary focus of
a dedicated team of full time physicists, graduate students, and undergraduate students.
The Virginia group also has talented electrical engineering and technical resources which
work closely with the researchers to solve many of the engineering challenges that the
experiment presents. The Virginia group also played an important role in the
Data Acquisition Group, with Dr. Andrew Norman (who has taken a position at Fermilab)
the project manager for the Data Acquisition (DAQ) System Integration project.
The Virginia group is responsible for all aspects of two critical components of the NOvA detectors:
the Power Distribution System that provides power to all of the detector electronics, and
the Detector Controls and Monitoring Systems that runs and monitors the detectors. Two of
each system need to be fabricated: one for the Near Detector and one for the Far Detector.
The Near Detector systems have been installed and commissioned and are running smoothly.
We are receiving about $2.5M from the U.S. Department of Energy to carry out this work.
Virginia's lead role in PDS
The NOvA Power Distribution System (PDS) provide all of the power to the 357,120 channels
of electronics in the Far Detector, including 11,160 front-end boards, thermoelectric
coolers, and avalanche photo-diodes, and 180 Data Concentrator Modules. Included in the
system are 180 Power Distribution Boxes designed by the Virginia group, 60 low-voltage,
high-current power supplies, 2 multi-channel high-voltage power supplies, 16 relay racks,
23.5 km of cables, and 3.5 km of cable trays. The physical size and unique topology of the NOvA detector,
when combined with the power demands and cooling requirements of the front end electronics,
make the PDS and electronics infrastructure design a formidable challenge which requires
significant electrical and mechanical design and engineering.
Virginia's lead role in DCS
The Virginia group is responsible for the Detector Controls and Monitoring (DCS) systems.
Our group's expertise with data acquisition systems, combined with our experience
in modern computing have allowed us to develop a robust platform capable of handing
the continuous readout, buffering, and real time data processing that is required by
the NOvA physics program. The DCS systems that Virginia is responsible for provide
the full hardware/software interfaces and data readout for the experiment and are the
fundamental window to for the physicist to control monitor the NOvA detectors.
|
|
|
Experiment Web Site
The physics of NOvA |
| Selected NOvA Talks |
Accelerator Based Neutrino Physics at Fermilab:
.pptx
Dukes, BCVSPIN 2011, Hue, Vietnam, July 2011
|
Accelerator Based Neutrino Physics at Fermilab:
.ppt
Dukes, University of Illinois Seminar, December 2009
|
Accessing Particle/Astrophysics Measurements with the NOvA Detector
.pptx
.pdf
Norman, Seminar Argonne National Lab, Aug. 2009
|
NOvA: The NuMI Offaxis &nue Appearance Experiment
.ppt
.pdf
Norman, DPF2009, July 2009
|
Power Distribution and Readout Infrastructure
.ppt
.pdf
Dukes, Dept. of Energy CD-3 Review, July 2009
|
NOvA Detector Controls and DAQ Integration
.pptx
.pdf
Norman, Dept. of Energy CD-3 Review, July 2009
|
DCM Embedded Software Systems
.pptx
Norman, NOvA Collaboration Meeting, July 2009
|
Accelerator Based Neutrino Physics at Fermilab:
.ppt
Dukes, SESAPS Meeting, October 2008
|
NOvA: the NuMI Offaxis νe Appearance Experiment:
.ppt
.pptx
Norman, Nufact07, August 2007
|
The NOvA Far Detector Site at Ash River MN
|
The NOvA Power Distribution Box
|
|