A communication resource from the world's particle physics laboratories.
ICFA was encouraged by the reports from Mr. H. Masuko, Deputy-Director General, MEXT Research Promotion Bureau and Hon. T. Kawamura, Chairperson of the Federation of Diet Members for the ILC, at the ICFA meeting held at the SLAC National Accelerator Laboratory, Stanford, USA, on the 20th February 2020.
The ALPHA experiment in the Antiproton Decelerator hall at CERN. (Image: CERN)
“Finding any difference between these two forms of matter would shake the foundations of the Standard Model of particle physics, and these new measurements probe aspects of antimatter interaction – such as the Lamb shift – that we have long looked forward to addressing,” says Jeffrey Hangst, spokesperson for the ALPHA experiment.
The project consists of the Hyper-K detector, which has an 8.4 times larger fiducial mass than its predecessor, Super-Kamiokande, equipped with newly developed high-sensitivity photosensors and a high-intensity neutrino beam produced by an upgraded J-PARC accelerator facility.
For the first time scientists have observed muon ionization cooling – a major step in being able to create the world’s most powerful particle accelerator. This new muon accelerator will give us a better understanding of the fundamental constituents of matter.
Fig 1: Inflation stretched the initial microscopic Universe to a macroscopic size and turned the cosmic energy into matter. However, it likely created an equal amount of matter and anti-matter predicting complete annihilation of our universe. The authors discuss the possibility that a phase transition after inflation led to a tiny imbalance between the amount of matter and anti-matter, so that some matter could survive a near-complete annihilation. Such a phase transition is likely to lead to a network of "rubber-band"-like objects called cosmic strings, that would produce ripples of space-time known as gravitational waves. These propagating waves can get through the hot and dense Universe and reach us today, 13.8 billion years after the phase transition. Such gravitational waves can most likely be discovered by current and future experiments. (Original credit: R. Hurt/Caltech-JPL, NASA, and ESA Credit: Kavli IPMU - Kavli IPMU modified this figure based on the image credited by R.Hurt/Caltech-JPL, NASA, and ESA)
According to the Big Bang theory of modern cosmology, matter was created with an equal amount of anti-matter. If it had stayed that way, matter and anti-matter should have eventually met and annihilated one to one, leading up to a complete annihilation.
But our existence contradicts this theory.
Georg Hoffstaetter (left) and Dejan Trbojevic at the CBETA facility at Cornell University.
“Reusing a particle beam’s energy in this new kind of accelerator makes brighter beams available, which would have required too much energy until now,” said Georg Hoffstaetter, physics professor and principle investigator for Cornell. In addition to the above-mentioned applications, Hoffstaetter points out that “such innovative technology and these brighter beams will likely lead to additional uses yet to be imagined.”
Electrons will collide with protons or larger atomic nuclei at the Electron-Ion Collider to produce dynamic 3-D snapshots of the building blocks of all visible matter.
"The EIC promises to keep America in the forefront of nuclear physics research and particle accelerator technology, critical components of overall U.S. leadership in science,” said U.S. Secretary of Energy Dan Brouillette. “This facility will deepen our understanding of nature and is expected to be the source of insights ultimately leading to new technology and innovation.”
Researchers work on the assembly of the CUORE experiment before it begins taking data. (Credit: CUORE Collaboration)
In an underground laboratory deep beneath a mountain in Central Italy, an array of crystals, chilled to within a hair of absolute zero – the coldest possible temperature in the universe – has been steadily compiling one of the most precise measurements to date in pursuit of a rare particle process. If it is proven to exist, this process may well be the “smoking gun” of how matter was created in the universe.
Part of the DESY staff in Hamburg holds the DESY-60 logo (photo: DESY/H. Müller-Elsner).
Building upon six decades of experience, DESY is excellently placed to tackle the global challenges of the future: “We bring together strong national and international research partners, and create the necessary conditions for innovation in important areas such as energy supply, medicine and new technologies,” says Helmut Dosch.
The STAR detector at the Relativistic Heavy Ion Collider (RHIC).
“This will be the second in a three-year campaign to scan the phase diagram of hot matter governed by quantum chromodynamics (QCD), the theory that describes the interactions of quarks and gluons,” said Jamie Dunlop, Associate Chair for Nuclear Physics in Brookhaven Lab’s Physics Department. The range of collision energies over the three years will allow nuclear physicists to search for telltale signs of what’s called a critical point—a change in the way the transition from quarks and gluons to ordinary matter takes place.
SNOLAB Board Appoints Dr. Nigel Smith as New ED
"It is a great honour to be asked to continue to lead the SNOLAB team and facility over the next three years, which I am delighted to accept. SNOLAB has a fantastic team, dedicated to bringing the best scientific research in the world to Sudbury, helping it succeed, and illuminating some of the greatest challenges in contemporary science. With our research partners in Canada and around the world, SNOLAB has a bright future programme in deep underground science, and I am privileged to play a part in its continued successes."
Among the Fermilab Quantum Institute’s suite of programs is a project to look for direct evidence of dark matter. Photo: Reidar Hahn
Laboratory to use particle physics expertise to kickstart quantum technology for computing, sensors, simulations and communication
“With today’s ceremony, the Long-Baseline Neutrino Facility steps into a new phase, and the Department of Energy is excited to see work on the Fermilab site moving forward. The LBNF/DUNE project is ambitious, and the scientific rewards will be tremendous.”
Jim Siegrist, DOE Associate Director of Science for High-Energy Physics
President of the CERN Council, Ursula Bassler and Director-General of CERN, Fabiola Gianotti (Image: CERN)
"I congratulate Fabiola Gianotti very warmly for her reappointment as Director-General for another five-year term of office. With her at the helm, CERN will continue to benefit from her strong leadership and experience, especially for important upcoming projects such as the High-Luminosity LHC, implementation of the European Strategy for Particle Physics, and the construction of the Science Gateway,” said President of the CERN Council, Ursula Bassler. “During her first term, she excelled in leading our diverse and international scientific organisation, becoming a role model, especially for women in science”.
Scientists gathering in Sendai, Japan, for a scientific conference about a possible future particle physics projects to lead next generation of research following the Large Hadron Collider (LHC) at CERN in Geneva, Switzerland, reaffirmed their commitment to engage in the construction and scientific exploitation of the International Linear Collider (ILC) as a global project.
Crews at the Sanford Underground Research Laboratory in Lead, South Dakota, begin to lower the LUX-ZEPLIN central detector. Its nearly mile-long descent down an elevator shaft, and its delivery to a research cavern where it will hunt for dark matter, were successfully carried out last week. (Credit: Nick Hubbard/Sanford Underground Research Facility)
Q: How do you get a 5,000-pound, 9-foot-tall particle detector, designed to hunt for dark matter, nearly a mile underground?
A: Very carefully.
DESI’s 5000 spectroscopic “eyes” can cover an area of sky about 38 times larger than that of the full moon, as seen in this overlay of DESI’s focal plane on the night sky (top). Each one of these robotically controlled eyes can fix a fiber-optic cable on a single object to gather its light. The gathered light collected from a small region in the Triangulum galaxy (bottom) by a single fiber-optic cable (red dot) is split into a spectrum (bottom) that reveals the fingerprints of the elements present in the galaxy and aid in gauging the distance to the galaxy. The test spectrum shown here was collected by DESI on Oct. 22. (Credit: DESI Collaboration; Legacy Surveys; NASA/JPL-Caltech/UCLA)
“Most of the universe’s matter and energy are dark and unknown, and next-generation experiments like DESI are our best bet for unraveling these mysteries."
What keeps galaxies from flying apart? What is the invisible mass that bends light in space? For now, we’re calling it dark matter and this October 31st, laboratories around the world are shining a light on the search for it.
KEK published a document on the recommendations for the International Linear Collider (ILC), a next-generation particle physics project, based on the report by the International Working Group on the ILC. The purpose of this document is to present some important aspects on implementation of the ILC project.
Brookhaven physicist Shaochun Tang is shown with the new ATLAS trigger board he designed and engineered for the U.S. ATLAS Phase I Upgrade project.
“This milestone will enable us to push the boundaries of our understanding, following the discovery of the Higgs boson at CERN, which resulted in the 2013 Nobel Prize in Physics,” said Project Director Jonathan Kotcher, a senior scientist at DOE’s Brookhaven National Laboratory. “The completion of this project is a major step in the physics campaign being mounted at the energy frontier, which integrates state-of-the-art accelerator and detector technology to probe the fundamental forces and particles of nature. We are very excited to turn to the physics and data analysis that all this hard work has enabled.”
SLAC National Accelerator Laboratory installs the first of Brookhaven's 21 rafts that make up LSST's digital sensor array. Photo courtesy SLAC National Accelerator Laboratory.
“This is the biggest charge-coupled device (CCD) array that has ever been built,” said Paul O’Connor, senior scientist at Brookhaven Lab’s instrumentation division. “It’s three billion pixels. No telescope has ever put this many sensors into one camera.”
The recently assembled LUX-ZEPLIN xenon detector in the Surface Assembly Lab cleanroom at Sanford Underground Research Facility on July 26, 2019.
Photo by Matthew Kapust Sanford Underground Research Facility.
“The TPC is a complex system and it's a major achievement to have it fully assembled,” Shutt said. “It takes us one important step closer to being able to look for dark matter. It is also gratifying because it involved assembling a large number of sub-systems designed and built by groups across the US and the UK over a number of years. So, it’s a coming together of sorts for the collaboration.”
Lower (left) and upper photomultiplier tube arrays are prepared for LZ at the Sanford Underground Research Facility in Lead, South Dakota. (Credit: Matt Kapust/SURF)
Most of the remaining components needed to fully assemble an underground dark matter-search experiment called LUX-ZEPLIN (LZ) arrived at the project’s South Dakota home during a rush of deliveries in June.
Candidates for a Higgs produced with a Z. ATLAS (l): both decay ultimately to leptons, leaving two electrons (green) and four muons (red). CMS (r): the Higgs decays to two charm quarks forming jets (cones); the Z decays to electrons (green) (Image: ATLAS/CMS/CERN)
Among the highlights are the latest precision measurements involving the Higgs boson. In only seven years since its discovery, scientists have carefully studied several of the properties of this unique particle, which is increasingly becoming a powerful tool in the search for new physics.
The two-stage miniature accelerator is operated with terahertz radiation (shown here in red). In a first step (left) the electron bunches (shown in blue) are compressed, in a second step (right) they are accelerated. The two individual elements are each about two centimetres wide. Credit: DESY, Gesine Born
“The wavelength of terahertz radiation is about a hundred times shorter than the radio waves currently used to accelerate particles,” explained Kärtner. “This means that the components of the accelerator can also be built to be around a hundred times smaller.”
A multicolor mosaic image of the massive galaxy cluster, Abell 370, located in the constellation Cetus – named for a sea monster in Greek mythology. Galaxy clusters are the largest structures in the universe bound by gravity, and consist of thousands of galaxies and large amounts of dark matter. Abell 370 formed when two less massive galaxy clusters merged together billions of years ago. It is more than 6.5 billion light-years away from Earth. The mosaic is approximately 4.5 million light-years across and has been constructed from deep optical imaging in the Legacy Surveys’ eighth data release. (Credit: John Moustakas/Siena College; Legacy Surveys team)
“We are building a detailed map of the universe and measuring its expansion history over the last 10 to 12 billion years,” Dey said. “The DESI experiment represents the most detailed – and definitely the coolest – cosmic cartography experiment undertaken to date. Although the imaging was carried out for the DESI project, the data are publicly available so everyone can enjoy the sky and explore the cosmos.”
The 2019 CERN Beamline for Schools winners: (from left) Team from the West High School in Salt Lake City, USA (Image: Kara Budge) and team from the Praedinius Gymnasium in Groningen, Netherlands (Image: Martin Mug).
“We are all very excited to welcome this year’s winners to DESY. This is a new chapter in the history of this competition because, for the first time, we are taking the finals of the competition to another research laboratory. As always, the more then 60 voluntary experts from CERN and DESY evaluated all the proposals for their creativity, motivation, proposed methodology, feasibility and their overall ability to explore some of the concepts of modern particle physics” said Sarah Aretz, BL4S project manager.
From the colour difference of two slightly delayed laser flashes (left) a non-linear crystal generates an energetic terahertz pulse (right). Credit: DESY, Lucid Berlin
“The wavelength of terahertz radiation is about a thousand times shorter than the radio waves that are currently used to accelerate particles,” says Kärtner, who is a lead scientist at DESY. “This means that the components of the accelerator can also be built to be around a thousand times smaller.”
“The Granada symposium is an important step in the process of updating the European Strategy for Particle Physics and aims to prioritise our scientific goals and prepare for the upcoming generation of facilities and experiments,” said the President of the CERN Council, Ursula Bassler. “The discussions will focus on the scientific reach of potential new projects, the associated technological challenges and the resources required.”
The BESIII collaboration observed baryon polarization in baryon-antibaryon (matter-antimatter particle) events from J/ψ particles produced at the BEPCII collider.
Artistic view of the Science Gateway. (Image: RPBW)
“The Science Gateway will enable CERN to expand significantly its education and outreach offering for the general public, in particular the younger generations. We will be able to share with everybody the fascination of exploring and learning how matter and the universe work, the advanced technologies we need to develop in order to build our ambitious instruments and their impact on society, and how science can influence our daily life,” says CERN Director-General Fabiola Gianotti. “I am deeply grateful to the donors for their crucial support in the fulfilment of this beautiful project.”
DESI "first light" image of the Whirlpool Galaxy, also known as Messier 51. This image was obtained the first night of observing with the DESI Commissioning Instrument on the Mayall Telescope at the Kitt Peak National Observatory in Tucson, Arizona; an r-band filter was used to capture the red light from the galaxy. (Credit: DESI Collaboration)
”It was an incredible moment to see those first images on the control room monitors,” said Connie Rockosi, who is leading this early commissioning of the DESI lenses. “A whole lot of people have worked really hard on this, and it’s really exciting to show how much has come together already.”
This year, results from the main experiments at the Large Hadron Collider (ALICE, ATLAS, CMS and LHCb) included new pentaquarks, new charmed beauty particles, a more precise measurement of matter–antimatter asymmetry in strange beauty particles, and new results from heavy-ion collisions.
The first hadronic event in the Belle II Phase3 physics run
On March 25 19:44 (JST), 2019, electron-positron collisions have restarted at the SuperKEKB collider, and the Belle II experiment has now kicked off its physics data taking. Belle II is now fully instrumented with a state-of-the-art vertex detector, just in time for the start of the cherry blossom season in Japan.
(From left) Mladen Šarčević, Serbian Minister of Education, Science and Technological Development, Ana Brnabić, Prime Minister of the Republic of Serbia, Fabiola Gianotti, CERN Director-General, and Charlotte Warakaulle, CERN Director for International Relations.
(Image: CERN)
“Serbia has a longstanding relationship with CERN, with the continuous involvement of Serbian scientists in CERN’s major experiments. I’m very happy to see that Serbia’s initiative to seek membership status of CERN has now converged and that we can welcome Serbia as a Member State,”said Ursula Bassler, President of the CERN Council.
“The result is a milestone in the history of particle physics. Ever since the discovery of the D meson more than 40 years ago, particle physicists have suspected that CP violation also occurs in this system, but it was only now, using essentially the full data sample collected by the experiment, that the LHCb collaboration has finally been able to observe the effect,” said CERN Director for Research and Computing, Eckhard Elsen.
The interior vacuum "tank" of TRIUMF's main cyclotron, the largest in the world. (Courtesy of TRIUMF)
“This investment from the federal government will allow TRIUMF to realize its full potential,” said Dr. Digvir Jayas, Chair of the TRIUMF Board of Management. “By leveraging ARIEL, IAMI, and TRIUMF Innovations, TRIUMF will continue to be a global leader in translating science and technology into innovation and commercialization. Today’s announcement represents a major milestone for the lab’s community of university members, researchers, students, users, industry partners and collaborators, and for all the people the lab serves.”
This new complex of buildings, located near Fermilab’s Wilson Hall, will host the 215-meter-long (700-foot-long) PIP-II particle accelerator, the new heart of the Fermilab accelerator complex. Credit: Fermilab
“The PIP-II accelerator project will fuel discovery at Fermilab for decades to come, facilitating new innovations and new insights into our universe. I’m excited for the further cooperation between America’s premier particle physics and accelerator laboratory and its international partners, and the resulting better understanding of the universe.”
Under Secretary for Science Paul Dabbar
The proton spin puzzle: Scientists want to know how different constituents of the proton contribute to its spin, a fundamental property that plays a role in how these building blocks give rise to nearly all visible matter in the universe. Pieces of the puzzle include the orbital angular momentum of quarks and gluons (top left), gluon spin (top right) and quark and antiquark spin (bottom). The latest data from RHIC reveal that the antiquarks' contribution is more complex than previously thought.
“This measurement shows that the quark piece of the proton spin puzzle is made of several pieces,” said James Drachenberg, a deputy spokesperson for STAR from Abilene Christian University. “It’s not a boring puzzle; it’s not evenly divided. There’s a more complicated picture and this result is giving us the first glimpse of what that picture looks like.”
Belle II and SuperKEKB are poised to become the world’s first Super B factory facility. Belle II aims to accumulate 50 times more data than its predecessor, Belle, and to seek out new physics hidden in subatomic particles that could shed light on mysteries of the early universe.
A 3D picture of the planned FASER detector as seen in the TI12 tunnel. The detector is precisely aligned with the collision axis in ATLAS, 480 m away from the collision point (Image: FASER/CERN)
“FASER is a neat physics proposal that addresses a particular aspect in the search for physics beyond the Standard Model and I am pleased to see it being implemented so efficiently,” adds Eckhard Elsen, CERN’s Director for Research and Computing.
While working at CERN, Sir Tim Berners-Lee invented the World Wide Web.
“It is a great honour and a source of pride for CERN to host an event to mark the 30th anniversary of Tim Berners-Lee’s proposal for what would become the World Wide Web, and I am delighted that Sir Tim will be with us on the day,” said CERN Director-General, Fabiola Gianotti. "The Web's invention has transformed our world, and continues to show how fundamental research fuels innovation. CERN's culture of openness was a key factor in the Laboratory’s decision in 1993 to make the web available free to everybody, a key step in its development and subsequent spread.”
Figure 2: Schematic view of the detector system of the KOTO experiment. The neutral kaon beam enters from the left. The electromagnetic calorimeter in purple measures two gamma-rays from a neutral pion.
The KOTO collaboration set the upper limit of once in three hundred million on the rate of the neutral K-meson (kaon) decay into a neutral pi meson and a pair of neutrinos from the analysis of the data set collected in 2015, and improved the world’s best sensitivity by an order of magnitude.
Fabiola Gianotti, CERN Director-General, and Blaženka Divjak, Minister of Science and Education of the Republic of Croatia, signed an Agreement admitting Croatia as an Associate Member of CERN.
“It is a great pleasure to welcome Croatia into the CERN family as an Associate Member. Croatian scientists have made important contributions to a large variety of experiments at CERN for almost four decades and as an Associate Member, new opportunities open up for Croatia in scientific collaboration, technological development, education and training,” said Fabiola Gianotti.
A snapshot of a plasma channel’s electron density profile (blue) formed inside a sapphire tube (gray) with the combination of an electrical discharge and an 8-nanosecond laser pulse (red, orange, and yellow). This plasma channel was used to guide femtoseconds-long “driver” laser pulses from the BELLA petawatt laser system, which generated plasma waves and accelerated electrons to 8 billion electron volts in just 20 centimeters. (Credit: Gennadiy Bagdasarov/Keldysh Institute of Applied Mathematics; Anthony Gonsalves and Jean-Luc Vay/Berkeley Lab)
“In the future, multiple high-energy stages of electron acceleration could be coupled together to realize an electron-positron collider to explore fundamental physics with new precision,” said Eric Esarey, BELLA Center Director.
The BESIII detector finished accumulating a sample of 10 billion J/ψ events together with a continuum data sample on Feb. 11. The 10 billion J/ψ-event sample accumulated at BESIII is the world’s largest data sample produced directly from electron-positron annihilations.
The proposed layout of the future circular collider (Image: CERN)
“The FCC’s ultimate goal is to provide a 100-km superconducting proton accelerator ring, with an energy of up to 100 TeV, meaning an order of magnitude more powerful than the LHC”, said CERN Director for Accelerators and Technology, Frédérick Bordry. “The FCC timeline foresees starting with an electron-positron machine, just as LEP preceded the LHC. This would enable a rich programme to benefit the particle physics community throughout the twenty-first century.”
The National Science Foundation’s Cerro Tololo Inter-American Observatory in Chile houses the Dark Energy Camera. Photo: Fermilab
"Although the data-taking for DES is coming to an end, DECam will continue its exploration of the universe from the Blanco telescope and is expected remain a front-line engine of discovery for many years,” Heathcote said.
RHIC's STAR detector tracks the thousands of particles produced by each ion collision. It weighs 1,200 tons and is as large as a house.
Berndt Mueller, Brookhaven’s Associate Laboratory Director for Nuclear and Particle Physics, noted, “This 19th year of operations demonstrates once again how the RHIC team — both accelerator physicists and experimentalists — is continuing to explore innovative technologies and ways to stretch the physics capabilities of the most versatile particle accelerator in the world.”
-- Symmetry Magazine, Kathryn Jepsen
This year, October 31 was more than just Halloween. It was also the first global celebration of Dark Matter Day. In 25 countries, 11 US states and online, people interacted with scientists, watched demonstrations, viewed films, took in art exhibits and toured laboratories to learn about the ongoing search for dark matter.
Symmetry has collected a series of photos from participants around the world. Check out how people celebrated Dark Matter Day and download a commemorative dark matter poster (to be printed using visible matter).
This report distills the findings of a series of international peer reviews of the communications and outreach functions of large-scale multidisciplinary science laboratories around the world.