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IIHE - Interuniversity Institute for High Energies (ULB-VUB)

The IIHE was created in 1972 at the initiative of the academic authorities of both the Université Libre de Bruxelles and Vrije Universiteit Brussel.
Its main topic of research is the physics of elementary particles.
The present research programme is based on the extensive use of the high energy particle accelerators and experimental facilities at CERN (Switzerland) and DESY (Germany) as well as on non-accelerator experiments at the South Pole.
The main goal of this experiments is the study of the strong, electromagnetic and weak interactions of the most elementary building blocks of matter. All these experiments are performed in the framework of large international collaborations and have led to important R&D activities and/or applications concerning particle detectors and computing and networking systems.
Research at the IIHE is mainly funded by Belgian national and regional agencies, in particular the Fonds National de la Recherche Scientifique (FNRS) en het Fonds voor Wetenschappelijk Onderzoek (FWO) and by both universities through their Research Councils.
The IIHE includes 19 members of the permanent scientific staff, 20 postdocs and guests, 31 doctoral students, 8 masters students, and 15 engineering, computing and administrative professionals.

IceCube

IIHE IceCube joining in celebration 100 years of Humans on the South Pole

IIHE IceCube joining in celebration 100 years of Humans on the South Pole At the Inter-university Institute for High Energies (IIHE) in Brussels we are involved in a world wide effort to search for high-energy neutrinos originating from cosmic phenomena. For this we use the IceCube neutrino observatory at the South Pole, the world's largest neutrino telescope which is now completed and taking data. Hundred years ago, on the 14th of December 1911, the first human being arrived on the South Pole. Roald Amundsen led the original Norwegian team that arrived, so to celebrate this Norwegian triumph, the Prime Minister of Norway came to the South Pole for 4 days to engage in the festivities.

IceCube

IIHE students at the South Pole

Falling off the earth is a serious risk at the South Pole. Down there, at the very end of the world, everything is different.. At the Inter-university Institute for High Energies (IIHE) in Brussels we are involved in a world wide effort to search for high-energy neutrinos originating from cosmic phenomena. For this we use the IceCube neutrino observatory at the South Pole, the world's largest neutrino telescope which is now completed and taking data.

CMS

Observation of a New Particle with a Mass of 125 GeV

In a joint seminarar at CERN and the “ICHEP 2012” conference in Melbourne, researchers of the Compact Muon Solenoid (CMS) experiment at the Large Hadron Collider (LHC) presented their preliminary results on the search for the standard model (SM) Brout-Englert-Higgs boson in their data recorded up to June 2012. CMS observes an excess of events at a mass of approximately 125 GeV with a statistical significance of five standard deviations (5 sigma) above background expectations. The probability of the background alone fluctuating up by this amount or more is about one in three million. The evidence is strongest in the two final states with the best mass resolution: first the two-photon final state and second the final state with two pairs of charged leptons (electrons or muons). We interpret this to be due to the production of a previously unobserved particle with a mass of around 125 GeV.

IceCube

IceCube observes first hint of astrophysical high-energy neutrinos

Two neutrino candidate events detected at the IceCube Neutrino Observatory, dubbed "Bert and Ernie", are the two highest energy neutrinos ever observed so far, with an estimated deposited energy of about 1 PeV. The IceCube event displays of these two events are shown in the figures below, where for comparison one should realize that a single event covers an area comparable with the Maracana football stadium in Rio de Janeiro! The probability that these two events are not background, i.e. anything else in the detector besides astrophysical neutrinos, is at the 2.8 sigma level and does not allow claiming a first observation of astrophysical neutrinos. Further details may be found in Physical Review Letters 111 (2013) 081801. To improve the detection sensitivity, a follow-up search on the same data period has been conducted. The new analysis selects high-energy neutrino events with vertices well contained in the detector volume and exploits veto algorithms by using the outer layers of IceCube sensors. By means of this new analysis method 26 new events have been detected. The entire sample of 28 events has properties consistent in flavour, arrival direction and energy with generic expectations for neutrinos of extraterrestrial origin.

IceCube

South Pole tuning in on "Skyradio"

The Askaryan Radio Array (ARA) is one of the future South Pole neutrino observatories focusing on the detection of neutrinos with energies beyond 10^17 eV. It utilizes radio waves, emitted from neutrino induced cascades in the South Pole ice sheet, to detect neutrino interactions. The detector is currently in the construction phase as is shown in the picture below. A grid of 37 antenna clusters, spaced by 2 km, is planned to be deployed in the South Pole ice at a depth of 200 m. By this, the full ARA detector will cover an instrumented area of about 100 km^2 and represent a state of the art detector for cosmic neutrinos in the energy range between 10^17 eV and 10^19 eV.

CMS

Shown here is a result of the 2012 LHC run at the Compact Muon Solenoid,

studying the invariant mass of electron pairs produced at the Large Hadron Collider. Shown is the data, as black dots, and the simulation predicting what we should expect according to the particle physics Standard Model (coloured bands). The IIHE is actively involved in the study of this kind of collisions, in collaboration with other groups of the CMS experiment. The data points agree very well with the predictions from the Standard Model, which means that up to now no new physics beyond the Standard Model could be observed that produces electron pairs. This could change when the LHC runs at a higher collision energy in 2015 and the high mass region to the right of the spectrum can be explored. New physics could show up as a peak in the high mass region of the spectrum, and could look like a small version of the peak of the Z boson that can be seen at a mass of about 90 GeV.

IceCube

IIHE at the ICRC!

The 34th International Cosmic-Ray Conference took place in The Hague, The Netherlands from July 30 to August 6, 2015. More than 800 physicists attended the conference to discuss the latest progress in cosmic-ray and solar physics. Furthermore, recent developments in gamma-ray and neutrino astronomy as well as the hunt for dark matter were covered. The IIHE was clearly represented with 8 posters and 3 talks. Our members presented their results on the Earth WIMP (Weakly Interactive Massive Particles) searches, a possible dark matter candidate, and on multiple analyses that aim to find the sources of neutrinos emission with the IceCube Neutrino Observatory. We focus our attention on: sources with spatial extension in the sky (from 1° to 5°), Gamma-Ray Bursts - extremely energetic explosion possibly associated with the death of a star, Dust Obscured Blazars - a special type of galaxies - and solar flares. The Askaryan Radio Array (ARA) as well as a totally new way to observe high energy neutrinos using radar detection were the subject of two talks! Also, two of our new members presented their previous work on the Cherenkov Telescope Array (CTA) and the Very Energetic Radiation Imaging Telescope Array System (VERITAS). The 35th ICRC will take place in Busan, South Korea, where we hope the IIHE will be even better represented!

IceCube

First results from a realistic modeling of radio emission by particle cascades in ice

In the previous decade several new experiments (ANITA, NuMoon, ARA, ARIANNA) were proposed to detect high energy (>EeV) neutrino induced particle cascades in dense media such as ice, salt, and moon rock. At the highest energies, these neutrino's are extremely rare and a large detector volume is needed to detect them. Due to the long attenuation length, the detection of the produced radio signals is the most promising tool to search for these rare events. In light of these new experimental efforts, the EVA-code, originally constructed to model radio emission from cosmic-ray-induced air showers, is under development to model radio emission from particle cascades in the South-Pole ice. The ice geometry is included into the code, as well as a parameterized model for the particle cascade. Furthermore, the original EVA-code already incorporated Cherenkov effects in the emission for radio signals moving on curved paths due to a density gradient in the medium. The figure below shows a preliminary result for the electric field as seen by an observer positioned at the ice-air interface. The particle cascade starts at 330 meters depth traveling approximately 10 meters straight upward in the ice until it dies out. The pulses as seen by observers at different lateral distances ranging from 10 m to 300 m are shown. It is seen that the pulse becomes sharper moving outward toward the Cherenkov cone at a lateral distance of approximately 330 meters."

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