Current status of the 2POL experiment will be summarized. The 2POL polarimeter, built in Warsaw to study quantum spin correlations of electrons originating from relativistic Moller scattering, has been recently tested on beam at Mainzer Mikrotron. Results and conclusions from the first measurements will be discussed. Our activities in the field of electron Mott polarimetry, related to experiment optimization techniques based on Monte Carlo simulation, will also be presented. Results obtained using Geant4 package with interaction models developed by our group for simulation of polarized electron beams will we shown.
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
dr Katarzyna Frankiewicz (NCBJ)
CosmicWatch is a simple, low-cost, physics-motivated project for everyone.The detector is a self-contained apparatus that employs plastic scintillator as a detection medium and a silicon photomultiplier (SiPM) for light collection. The signal from the SiPM is sent through a custom designed printed circuit board (PCB) which shapes the signal such that a micro-controller can measure the time and amplitude of the SiPM signal. We use an Arduino Nano to measure the pulse amplitude and record the count number, time of the event, pulse amplitude, and detector dead time.CosmicWatch detector can be powered through mini USB and, in conjunction with the available open-source software, can be used to make interesting physics measurements, e.g. detect cosmic ray muons. It is easy to assemble, so one may gain experience in electronics and hardware related skills like soldering, mounting electronic components, designing PCBs, using oscilloscopes, waveform generators, and multimeters. The data gathered from the detector may serve as an input for anyone who wants to learn about basic techniques in data analysis, statistics, programming, and data visualization. The detector can be used for scientific purposes and educational outreach.The project has already gained attention on websites such as Physics Today, Symmetry Magazine, Endgadget, MIT news, MSN, Reddit, and many more. We've produced over two hundred detectors and have distributed internationally, mainly to high-school and undergraduate students. These include students from the United States, Poland, Germany, Canada, Peru, Germany, United Kingdom, and India.
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
(IFD UW)
The NICA accelerator complex is the new Mega-Science project co-financed by the Joint Institute of Nuclear Research in Dubna and the Russian Federation. The complex will deliver collisions of two beams of ions, from p to Au, and center-of-mass energies of 4-11 AGeV. The collider is currently under construction at JINR, with participation from Polish contributors. The capabilities of the complex as well as the status of the construction of the machine will be shortly presented. The NICA-PL consortium of polish scientific institutions interested in the participation in NICA will also be introduced.The major scientific experiment at the NICA Complex is the Multi-Purpose Detector. Its physics program and status of the construction of the detector will be described. Recently an international collaboration of MPD has been formed, which is now in the process of formalizing its structure and governing bodies. The opportunities for polish institutions for participation in MPD will be advertised.
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
Dr Davide Franco (APC, Paryż)
The field of direct dark matter search is experiencing a significant expansion in this decade, with many new experiments coming on board and exploring new avenues to increase sensitivity to Weakly Interacting Massive Particles (WIMPs), the leading dark matter candidate. Liquid argon detectors play a major role in the search of WIMPs, especially if they take advantage of ultra-low background argon extracted from deep underground, depleted in cosmogenic contamination. Very recently, DarkSide-50 and DEAP-3600 have completed major milestones of their programs by publishing results from ~20 and ~10 tonne-days exposure campaigns, respectively. The outcomes of the dark matter searches are null results. The discrimination between events induced by natural radioactivity and nuclear recoils – the potential candidate dark matter events – is outstanding, confirming once more that a future generation of liquid argon detectors will also be able to operate completely free of background and in a real discovery mode.We will discuss the achieved results and the potential of dark matter search with next generation liquid argon detectors. In addition, we will discuss the possibility to exploit technology, specifically developed for liquid argon, for neutrino physics and medical applications.
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
prof. dr hab. Barbara Badełek (IFD UW)
European particle physics community is frantically completing documents summarising its research perspectives for 1-2 decades and its results and detailed plans for the next 6 years. These materials will be submitted to the `European Particle Physics Strategy' group by end of 2018. After consultations and consensus building within the community, a Physics Briefing Book with high energy physics programme recommendations will be created by the EPPS and submitted to the CERN Council for approval expected in March 2020.I shall tell about an initiative `Physics Beyond Colliders', set up in 2016 by CERN Management in the context of EPPS. Working groups of PBC are supposed to contribute with a particular input to the upcoming European Particle Physics Strategy Update.
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
dr hab. Artur Kalinowski (IFD UW)
Machine learning is a dynamically developing field of computer science, with many applications in the IT industry (such as the automatic PL->ENG translation of this summary), which then diffuse into the natural sciences. In the seminar I will discuss selected algorithms and their application in the field of high energy physics. I will also discuss current activity Warsaw group of the CMS experiment in the field of machine learning
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
dr hab. inz. Tomasz Szumlak (AGH)
LHCb (Large Hadron Collider beauty) is a high precision experiment dedicated to searching for New Physics beyond the Standard Model in heavy flavour sector. With the Run 2 (2015 – 2018) data taking period coming to its end it seems less and less likely that the New Physics will be observed directly (energy frontier). Since LHCb is optimised to perform indirect studies and is sensitive to mass scales up to 50 TeV (intensity frontier) it may play a key role in a potential discovery of New Physics phenomena. This expectation is supported by many intriguing anomalies, especially related to rare decays and lepton flavour universality, observed and reported by LHCb. Thus, it is essential for LHCb to enter the high luminosity phase and continue data taking beyond LHC Long Shutdown 2 (LS2). For this the LHCb experimental setup needs a major upgrade that is being planned for years 2019 and 2020.
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
Andrzej K. Drukier (Stockholm University)
The different experiments attempting direct detection of Dark Matter candidates (DM) provides divergent results. DAMA-LIBRA observed the annual modulation in count rate which suggest existence of DM with MDM = O(10 GeV/c2). However, other (mostly l. Xenon detectors) put impressive limits on DM in mass range of 15 GeV/c2 < MDM < 500 GeV/c2. There is still possibility that DM are WIMPs, they are either low mass, MDM < 15 GeV/c2 or very heavy. We propose new DM detectors based on coherent scattering of neutrinos or DM in ancient crystals. Such crystals are available from deepest holes drilled for diverse purposes (depth > 8 km or > 20 km water equivalent). Thus the background due to CR is negligible (with exception of neutrinos). In this new detectors, the target is multi-elemental (up to 10 elements) which provides the signature and improve S/B. We elucidate the principles of paleo-detectors and describe a few promising methods of the signal detection. We also provide the first estimates of sensitivities, which for low mass DM (LM-DM) extends below the current definition of the “neutrino floor”. For example, for MDM = 10 GeV our sensitivity is about thousand fold better than for Ge-based or l. Xenon detectors. The problems of backgrounds will be discussed, including the trade-offs when one try use ice from Antarctica as paleo-detector.
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
prof. dr hab. Tomasz Matulewicz (IFD UW)
Facility for Antiproton and Ion Research (FAIR) is realized as an extension of the existing nuclear research center GSI Darmstadt. FAIR is organized as a company (GmbH) with Poland (Jagiellonian University) as one of shareholders. The civil construction is now progressing. Full operation is planned for 2025. SIS-100 synchrotron (100 Tm) will be the workhorse of the facility. Research areas are: hot and dense nuclear matter, charmonium spectroscopy, neutron-rich radioactive nuclei and strong e-m fields. The beam intensity will be 3 to 4 orders of magnitude above actually available elsewhere, so study of rare processes might be feasible.
Zapraszamy do sali B2.38, ul. Pasteura 5 o godzinie 10:15
dr hab. Justyna Łagoda (NCBJ)
The XXVIII International Conference on Neutrino Physics and Astrophysics has been held in Heidelberg from 4th to Saturday 9th June 2018. The conference program covered a wide range of topics, including the neutrino mass measurements, oscillations and detection of ultrahigh energy neutrinos from space. The overview of the most interesting (in speaker's opinion) results will be presented.