FYI by Pamela Zerbinos
If you’ve ever tried to speak with a member of the military, you know that
comprehension is nearly impossible unless you’re familiar with its language.
You probably also know that its language of acronyms sometimes seems...well,
pointless. They don’t have cars, they have POVs—Privately Owned Vehicles.
While it’s true that acronyms in the HEP—er, High Energy Physics—community
have a different purpose, it’s also true that the simple statement, “STAR is a QGP
experiment at BNL’S RHIC,” will not draw even a flicker of understanding from the
uninitiated. As the list of labs, agencies, accelerators, detectors and experiments
grows ever longer, FERMINEWS decided it was time for an AHEP update.
Please note that although space in FERMINEWS is limited,
an expanded acronym directory is available online at:
www.fnal.gov/pub/inquiring/more/acronyms.html
If we missed anything (and we did), please be sure to let us know.
LABS, FACILITIES & RESEARCH INSTITUTIONS
ANL: The Department of Energy’s Argonne
National Laboratory in Argonne, Ill.
Bates: Not an acronym. The Massachusetts
Institute of Technology Bates Linear Accelerator
Center.
BNL: The Department of Energy’s
Brookhaven National Laboratory in
Upton, Long Island, New York.
CERN: Originally “Conseil Européenne pour
Recherches Nucléaires,” now the European
Laboratory for Particle Physics, in Geneva,
Switzerland.
CNRS: Centre National de la Recherche
Scientifique, France’s equivalent to the NSF.
DESY: Deutsches Elektronen-SYnchrotron
laboratory in Hamburg, Germany.
ESRF: The European Synchrotron Radiation
Facility in Grenoble, France.
FNAL: The Department of Energy’s Fermi
National Accelerator Laboratory in Batavia, Ill.
FZK: Forschungszentrum Karlsruhe,
a nonprofit basic science research center
in Karlsruhe, Germany.
GSI: Gesellschaft für Schwerionen-forschung,
a heavy-ion research center in Darmstadt,
Germany.
HASYLAB: HAmburger
SYnchrotronstrahlungsLABor, part of DESY.
IN2P3: Institut National de Physique
Nucleaire et de Physique des Particules, the
division of CNRS that oversees nuclear and
particle physics.
JINR: The Joint Institute for Nuclear
Research in Dubna, Russia.
JLAB: The Department of Energy’s Thomas
Jefferson Newport National Accelerator Facility,
or Jefferson Lab, in Newport News, Va.
Formerly CEBAF (Continuous Electron Beam
Accelerator Facility).
KEK: Koo Energy Ken. The High Energy
Research Accelerator Organization in Tsukuba,
Japan. w
LAL: The Laboratoire de L’Accelerateur
Lineaire at the University of Paris-Sud in Orsay,
France.
LANL: The Department of Energy’s
Los Alamos National Laboratory in
Los Alamos, N.M.
LBL: The Department of Energy’s Lawrence
Berkeley Laboratory in Berkeley, Calif.
LEPP: Laboratory for Elementary-Particle
Physics at Cornell University in Ithaca,
New York. Formerly the Laboratory for
Nuclear Studies (LNS).
LLNL: The Department of Energy’s
Lawrence Livermore National Laboratory
in Livermore, Calif.
LNF: Laboratori Nazionali di Frascati, near
Rome, Italy.
LNGS: Laboratori Nazionali del Gran Sasso,
in L’Aquila, Italy. Usually referred to as
“Gran Sasso.”
NUSL: The National Underground Science
Laboratory in the Homestake Mine, S.D.
ORNL: The Department of Energy’s Oak
Ridge National Laboratory in Oak Ridge, Tenn.
PSI: Paul Scherrer Institut, a research facility
in northern Switzerland.
SLAC: The Department of Energy’s Stanford
Linear Accelerator Center in Menlo Park, Calif.
SSRL: SLAC Synchrotron Radiation
Laboratory.
TRIUMF: TRI-University Meson Facility.
(Although now there are eight universities
involved, TRIUMF started with three.) Located
at the University of British Columbia in
Vancouver, Canada.
WIPP: The Department of Energy’s Waste
Isolation Pilot Plant, a nuclear waste center
in New Mexico also being used as an
underground laboratory.
AD: Antimatter Decelerator.
New facility at CERN to study antimatter.
AGS: The Alternating Gradient Synchrotron
at Brookhaven.
ATLAS: The Argonne Tandem Linear
Accelerator, a heavy-ion accelerator at Argonne.
AWA: The Argonne Wakefield Accelerator,
working on accelerator R&D.
B Factory: SLAC’s new electron-positron
collider, built to produce B mesons, beginning
in 1999.
CLIC: CERN’s proposed Compact LInear
Collider.
CESR: The Cornell Electron Storage Ring.
Ahigh-luminosity electron-positron collider at
the Wilson Synchrotron Laboratory, Cornell
University.
DAFNE: (Sometimes DAPHNE) Double
Annular Factory for Nice Experiments.
1.0 GeV high luminosity phi factory at LNF in
Italy.
EPA: CERN’s Electron Positron Accumulator.
FMI: The Fermilab Main Injector, which began
operating in 1999 as an injector to the Tevatron.
HERA: Hadron-Electron Ring Accelerator at
DESY.
ISAC: TRIUMF’s Isotope Separator and
ACcelerator for astrophysics study.
KEKB: An electron-positron collider to study
CP violation in the B meson, at KEK.
LANSCE: Los Alamos Neutron
Science CEnter (formerly LAMPF, the
Los Alamos Meson Physics Facility).
LEIR: Low Energy Ion Ring. Used to
be LEAR, an antiproton ring. LEAR is being
converted into LEIR, a machine
to store ions for the LHC at CERN.
LEP: The Large Electron Positron Collider
at CERN.
LHC: The Large Hadron Collider,
a new international 14 TeV proton-proton
accelerator now being built at CERN,
to begin operating sometime after 2005.
LIL: The Linear Injector for LEP at CERN.
NLC: Next Linear Collider, now under study.
Apossible future electron-positron accelerator,
proposed by SLAC to be built with international
participation.
NLCTA: The Next Linear Collider
Test Accelerator at SLAC.
PEP: SLAC’s Positron Electron
Project, now the site of the B Factory.
PEP-II: The official name for the
SLAC B Factory.
PS: CERN’s Proton Synchrotron.
RHIC: Brookhaven’s Relativistic Heavy Ion
Collider began operation in 2000. RHIC collides
beams of gold ions to study what the universe
looked like in the first few moments after its
creation.
SLC: SLAC Linear electron-positron Collider.
SPEAR3: Proposed upgrade for the
Stanford Positron Electron Accelerating Ring,
completed in 1965. Now being used as
a synchrotron light source for SSRL.
SPS: CERN’s Super Proton Synchrotron.
TESLA: TeV-Energy Superconducting Linear
Accelerator, a possible future linear collider,
proposed by DESY to be built with international
participation.
Tevatron: Fermilab’s 2-TeV protonantiproton
accelerator, the world’s
highest-energy accelerator.
TTF: TESLAT est Facility at DESY.
VLHC: Very Large Hadron Collider, possible
new accelerator now under study as an
international follow-on to the LHC.
ALEPH: Apparatus for LEP PHysics,
a detector at CERN.
ALICE: ALarge Ion Collider Experiment,
destined for the LHC at CERN.
AMS: Alpha Magnetic Spectrometer.
Adetector on the international space station
to search for dark matter and antimatter.
Scheduled to launch in 2003.
ANTARES: Astronomy with a Neutrino
Telescope and Abyss environmental RESearch.
APEX: AntiProton Experiment. Fermilab
experiment to search for antiproton decay.
ATLAS: AToroidal LHC ApparatuS.
Detector for the LHC under construction at
CERN. U.S. HEP community plays a major role.
BaBar: B-Bbar (anti-B) detector at SLAC’s
B Factory. Named for the elephant in Laurent
DeBrunhoff’s children’s books.
BELLE: B detector at KEK in Japan.
BOREXINO: (sometimes Borex): An
underground solar neutrino experiment at
Gran Sasso in Italy.
BTeV: Proposed dedicated B physics
experiment at Fermilab’s Tevatron.
CAT: Cherenkov Array at Themis, an imaging
telescope in France to detect very high-energy
gamma rays.
CDF: Collider Detector at Fermilab, studies
proton-antiproton collisions at the Tevatron.
CDMS: Cryogenic Dark Matter Search.
AFermilab/university experiment to search for
the interaction of dark matter particles with the
nuclei of silicon and germanium detectors, now
at Stanford. Will place a detector in Soudan
Mine, Minnesota.
CHAOS: Canadian High Acceptance Orbit
Spectrometer.
CHOOZ: An international long-baseline
reactor neutrino experiment located at the
CHOOZ Anuclear power station, les Ardennes,
France.
CHORUS: CERN Hybrid Oscillation
Research apparatUS.
CKM: Charged Kaons at the Main Injector,
a proposed Fermilab experiment to measure
charged kaon decay.
CLEO: Not an acronym. Goes with CESR.
Get it? Upgrade of detector at Cornell’s CESR
accelerator.
CMS: Compact Muon Solenoid. Detector now
being built for CERN’s LHC by international
collaboration including many U.S. physicists.
CNGS: CERN Neutrinos to Gran Sasso,
a long-baseline neutrino oscillation experiment.
COBE: COsmic Background Explorer,
a satellite launched by NASA in 1989 to search
for evidence of the Big Bang. Currently in data
analysis. aether.
COSMOS: Cosmologically Significant Mass
Oscillation Search at Fermilab to detect muon
neutrino to tau neutrino oscillations.
CRESST: Cryogenic Rare Event Search with
Superconducting Thermometers. An experiment
in the Gran Sasso Underground Laboratory to
search for Weakly Interacting Massive Particle
(yes, WIMP) dark matter using cryogenic
detectors.
DAMA: Particle DArk MAtter search with
highly radiopure scintillators at Gran Sasso,
searching for WIMPs.
DELPHI: Detector with Lepton Photon
and Hadron Identification at CERN’s LEP
accelerator.
DONUT: Direct Observation of the Nu Tau.
AFermilab fixed-target experiment to detect
direct interactions of the tau neutrino.
DZero: (named for location on the Tevatron
Ring) Collider detector studies proton-antiproton
collisions at Fermilab’s Tevatron.
EXO: Enriched Xenon Observatory, searching
for neutrinoless double beta-decay at WIPP.
FOCUS: FOtoproduction of Charm:
Upgraded Spectrometer. AFermilab fixed
target experiment to study charm physics.
GALLEX: The Gallium EXperiment at Gran
Sasso, which has now been replaced by GNO.
GNO: Gallium Neutrino Observatory,
the successor to GALLEX.
H1: Collider experiment at DESY.
HDMS: Heidelberg Dark Matter Search.
Double beta decay and dark matter searches
taking place at the University of Heidelberg in
Germany.
HERA-B: Fixed-target experiment at DESY,
to investigate CP violation in the B meson.
HERMES: DESY fixed-target experiment
to explore spin.
Hi Res Fly’s Eye: High-energy cosmic
ray experiment in Dugway, Utah.
HOMESTAKE: Asolar neutrino
experiment in the Homestake Gold Mine
in South Dakota.
HYPER-CP (e871): Asearch for direct
CP Violation in Hyperon decays. Fermilab fixedtarget
experiment.
ICARUS: Imaging Cosmic and Rare
Underground Signal. Neutrino experiment
proposed at CERN/Gran Sasso.
ISOLDE: Isotype On-Line separator
at CERN.
K2K: KEK to Kamioka. Long-baseline
neutrino experiment using a beam from KEK
accelerator to Super-Kamiokande detector in
Japan.
KAMIOKANDE: Asolar neutrino
experiment at the Kamioka Observatory in
Japan.
KAMLAND: KAmioka Liquid Scintillator
Anti-Neutrino Detector, under construction in
Japan.
KARMEN: Karlsruhe-Rutherford Medium-
Energy Neutrino Experiment. Aneutrino
interaction experiment using a detector at the
ISIS spallation neutron source at Rutherford-
Appleton Laboratory in England.
KATRIN: KArlsruhe TRItium Neutrino
experiment at FZK to measure neutrino mass.
KLOE: AKlong experiment studying
CP violation at LNF.
KOPIO: AKlong decay experiment at
Brookhaven.
KTeV: Kaons at the Tevatron,
a Fermilab fixed-target experiment to
study CP violation in kaon decay.
L3: Detector named for its location on CERN’s
LEP accelerator.
LHCb: Large Hadron Collider
B Experiment, being built at the LHC at CERN.
LVD: Gran Sasso’s Large Volume Detector,
looking for neutrino bursts from stellar collapses.
Majorana: Not an acronym. Adouble
beta decay experiment taking place at the
DOE’s Pacific Northwest Laboratory.
MECO: Muon to Electron COnversion,
an RSVP experiment at Brookhaven’s AGS.
MiniBooNE: Booster Neutrino Experiment,
petite size. Planned experiment to study
neutrino oscillations using Fermilab’s Booster
accelerator.
MINIMAX / T-864: Asearch for
disoriented chiral condensates at Fermilab.
MINOS: Main Injector Neutrino Oscillation
Search. An experiment to study neutrino
oscillations using the NuMI beam from
Fermilab’s Main Injector accelerator.
MIPP: Main Injector Particle Production,
a proposed experiment at Fermilab.
MONOLITH: Massive Observatory
for Neutrino Oscillations or LImits on THeir
existence. Atmospheric neutrino detector
at Gran Sasso.
MPS: The Microdrop Particle Search at
SLAC, searching for extremely massive charged
particles.
MUCOOL: MUon COOLing experiment,
which hopes to develop a muon ionization
cooling channel for a high-luminosity muon
chamber.
NOE: Neutrino Oscillation Experiment,
at Gran Sasso.
NOMAD: Neutrino Oscillation MAgnetic
Detector, at CERN.
NuMI: Neutrinos at the Main Injector,
a project to send a beam of high-energy
neutrinos from Fermilab to a detector in
northern Minnesota, beginning in 2005.
NuSEA: Nucleonic Sea, Los Alamos-led
collaboration at Fermilab to measure the
proton’s excess of anti-down quarks relative
to anti-up quarks.
NuTeV: Neutrinos at the Tevatron,
a Fermilab fixed-target experiment using
a neutrino beam for precision measurement
of the mass of the W boson.
OMNIS: Observatory for Multiflavor
Neutrinos from Supernovae, an underground
experiment at WIPP.
OPERA: Oscillation Project with EmulsiontRacking
Apparatus, the neutrino detector at
Gran Sasso for the long-baseline experiment
CNGS.
ORLaND: Oak Ridge Large Neutrino
Detector, searching for neutrino oscillations at
Oak Ridge.
PHENIX: Pioneering High-Energy Nuclear
Interaction eXperiment, at Brookhaven.
PHOBOS: Not an acronym. Phobos is
a moon of Mars, which was the name of the
original proposed detector. Studies heavy-ion
collisions at Brookhaven.
Pierre Auger Project: (No acronym,
sometimes just “Auger”) International experiment
to track down the origin of ultra-high-energy
cosmic rays.
pp2pp: proton-proton to proton-proton
elastic scattering experiment at Brookhaven.
SDSS: Sloan Digital Sky Survey. Astrophysics
project to create largest-ever three-dimensional
map of the sky.
SELEX: SEgmented Large X baryon
spectrometer EXperiment. Afixed target
experiment at Fermilab to study charm baryons.
SLD: SLAC Large Detector, optimized for
physics at the SLC interaction point.
SNO: Sudbury Neutrino Observatory.
Asolar -neutrino detector near Sudbury, Ontario,
Canada.
SOUDAN II: Detector in an underground
laboratory in the Tower-Soudan Iron Mine in
Soudan, Minnesota, to search for nucleon
decay and study atmospheric neutrino physics.
STAR: Solenoidal Tracker At RHIC, looking
for quark-gluon plasma at Brookhaven.
Super-K: Super-Kamiokande experiment to
detect neutrino oscillations from atmospheric
neutrino flux, in Japan.
TAPS: Two-Arm Photon Spectrometer,
German experiment to measure hard photons
and neutral mesons.
UNO: Underground Nucleon decay and
neutrino Observatory, located at WIPP.
ZEUS: (Not an acronym, but goes with
HERA) Collider experiment at DESY’s HERA.
AIP: American Institute of Physics. Publishes
Physics Today.
APS: American Physical Society. Publishes
physics journals, organizes meetings and
conferences, communicates to policymakers
and the public.
DOE: The U.S. Department of Energy. Funds
the lion’s share of U.S. HEP.
ER: DOE’s Office of Energy Research.
Funds basic science research, including HEP.
HENP: DOE’s Office of High Energy and
Nuclear Physics; part of ER.
HEPAP: High Energy Physics Advisory
Panel. Advisory to DOE and NSF.
HEPIC: High Energy Physics Information
Center, a clearinghouse of HEP info.
NSF: National Science Foundation. Funds
university physics research, physics experiments
and projects, and the HEP lab at Cornell
University.
OSTP: Office of Science and Technology
Policy. Advises the President.
PRL: Physical Review Letters, the main
journal of the APS.
SPIRES: Stanford Public Information
REtreival System. Online gold mine of physics
information.
URA: Universities Research Association.
Contracts with DOE to run Fermilab.
An expanded version is available online:
www.fnal.gov/pub/inquiring/more/acronyms.html
|
last modified 9/17/2002 email Fermilab |
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