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X-WR-CALNAME:Erlangen Centre for Astroparticle Physics
X-ORIGINAL-URL:https://ecap.nat.fau.de
X-WR-CALDESC:Events for Erlangen Centre for Astroparticle Physics
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DTSTART:20250330T010000
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DTSTART:20251026T010000
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DTSTART:20260329T010000
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BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20250508T130000
DTEND;TZID=Europe/Berlin:20250508T140000
DTSTAMP:20260417T212726
CREATED:20250502T122359Z
LAST-MODIFIED:20250516T160657Z
UID:5719-1746709200-1746712800@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Oliver Friedrich\, LMU Sternwarte
DESCRIPTION:Forcing neutrinos to obey the holographic principle\nGravity does not like the vast amounts of states present in QFT\, and\nquantum gravitational effects are expected to drastically reduce the\ndimension of the QFT Hilbert space. This is e.g. achieved by “operator\ndressing”\, which changes the commutation relations of quantum fields.\nIn https://arxiv.org/abs/2402.11016 we build a model for neutrinos\,\nthat incorporates this dressing and fixes it such that neutrinos obey\na cosmic entropy bound. A key consequence of this construction is that\nparticles scatter in the vacuum. This e.g. implies a finite mean free\npath of cosmic neutrinos. We confront this result with observed\nneutrino emissions and find that the holographic principle is\npotentially in tension with current neutrino data.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2025-05-08-oliver-friedrich/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20250522T130000
DTEND;TZID=Europe/Berlin:20250522T140000
DTSTAMP:20260417T212726
CREATED:20250507T133938Z
LAST-MODIFIED:20250519T122758Z
UID:5728-1747918800-1747922400@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Philipp Windischhofer\, U Chicago
DESCRIPTION:Exploring the Universe at the Highest Energies: when Particle Physics and Astronomy meet\nHigh-energy neutrinos propagating over cosmological distances are the ideal messenger particles for astrophysical phenomena\, but the neutrino landscape above 10 PeV is still mostly unexplored. At these extreme energies\, neutrinos can image the most extreme objects in remote corners of our cosmos and help access fundamental physics at extremely short distances.In this talk\, I will show how we are presently constructing the Radio Neutrino Observatory in Greenland\, the largest-ever terrestrial neutrino detector\, and how the century-old physics of electrodynamics plays a central role in its operation. Combining ideas from particle collider instrumentation with high-performance computing\, we will see what it takes to fully exploit the science potential of this unique instrument and thereby extend neutrino astronomy into the regime of the exaelectronvolt.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2025-05-22-philipp-windischhofer/
LOCATION:Physikum\, Hörsaal HF\, Staudtstr. 5\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20250605T130000
DTEND;TZID=Europe/Berlin:20250605T140000
DTSTAMP:20260417T212726
CREATED:20250528T080141Z
LAST-MODIFIED:20250528T080141Z
UID:5756-1749128400-1749132000@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Benedikt Bergmann\, IEAP/CTU\, Prague
DESCRIPTION:Particle tracking and identification with Timepix-series detector setups in nuclear\, particle and astrophysics\nIn high energy physics experiments\, hybrid pixel detectors are an integral part of the tracking systems closest to the interaction points\, where their good spatial resolution and high radiation resilience allow for particle tracking by connection of “dots” registered in different layers of an onion-like detector. Another approach to particle detection and tracking relies on a complex analysis of the imprints seen in the pixel matrices (tracks)\, which provide a rich set of features. These allow for identification of impinging particles\, particle trajectory or reaction kinematics reconstruction. The latter is particularly valuable for applications with limited resources\, for example in space experiments\, but it also enables fundamental-science-reach measurements with simple table-top experiments. In this contribution\, I will present the latest results from Timepix-type detectors used within LHC experiments\, as space radiation monitors in low Earth orbit\, their possible application for measurement for galactic-cosmic-ray properties or as an X-ray polarimeter.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2025-06-05-benedikt-bergmann/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20250612T130000
DTEND;TZID=Europe/Berlin:20250612T140000
DTSTAMP:20260417T212726
CREATED:20250602T103424Z
LAST-MODIFIED:20250602T103424Z
UID:5761-1749733200-1749736800@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Branden Allen\, University of Hawaii
DESCRIPTION:Introduction to the Space Science and Engineering Initiative\, and Opportunities and Applications for the Next Generation of X and gamma-ray Detector Systems and Technologies\nThe Space Science and Engineering Initiative (SSEI) was created as a joint effort between the UHM College of Engineering (CoE) and the Institute for Astronomy (IfA) for the establishment of an interisland advanced technology research and development center based in Hilo\, which aims to significantly expand technical capabilities to support the space sciences\, particularly targeting application for the observatories on Maunakea and Haleakalā. Here\, I will discuss the current status of the SSEI and give a brief overview of our current portfolio of activities. \nAfterward\, I will discuss my own research program which focuses primarily on the development of high-energy detectors\, associated technologies\, telescopes and missions for spaceflight. This will be followed by a discussion of plans and potential for their future deployment for use in astrophysics and planetary science.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2025-06-05-branden-allen/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20250626T130000
DTEND;TZID=Europe/Berlin:20250626T140000
DTSTAMP:20260417T212726
CREATED:20250624T151715Z
LAST-MODIFIED:20250625T043109Z
UID:5779-1750942800-1750946400@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Mauricio Bustamante
DESCRIPTION:Fundamental physics with high-energy and ultra-high-energy cosmic neutrinos\nHigh-energy cosmic neutrinos probe fundamental physics at scales of energy and distance otherwise unreachable\, where new physics may manifest. Since the discovery of TeV-PeV astrophysical neutrinos in 2013\, we have explored this progressively more broadly and with increasing precision\, thanks to a growing number of detected neutrinos and to improvements in reconstruction and analysis techniques. By means of illustration\, I will survey the rich landscape of high-energy physics with cosmic neutrinos\, from the perspectives of theory and experiment. I will also touch upon new opportunities made possible by the recent discovery of an ultra-high-energy neutrino\, with about 200 PeV\, by KM3NeT—with a warning.  Looking ahead\, I will show two prospects for transformative change in the next decade\, driven by new\, upcoming neutrino telescopes: a boost in the detection rate of TeV-PeV neutrinos and the possible detection of more ultra-high-energy neutrinos.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2025-06-26-mauricio-bustamante/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20251013T130000
DTEND;TZID=Europe/Berlin:20251013T140000
DTSTAMP:20260417T212726
CREATED:20251013T053811Z
LAST-MODIFIED:20251013T053811Z
UID:5993-1760360400-1760364000@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Kendall Mahn\, Michigan State University
DESCRIPTION:You’re sending particles across a country? The Tokai to Kamioka experiment\nNeutrinos are a tiny subatomic particle with surprising properties under active study. In particular\, neutrinos oscillate\, that is\, they convert from one type of neutrino to another\, is a surprising phenomenon under active study. The origin of neutrino mass is important for astrophysics\, cosmology and particle physics\, and many open questions surrounding neutrino oscillation exist. The Tokai-to-Kamioka (T2K) neutrino oscillation experiment sends a beam of muon flavor neutrinos or antineutrinos 295km across Japan. This seminar will talk about the wonderful world of neutrinos\, the surprising landscape of neutrino oscillation\, through the lens of recent activities on T2K\, and toward the future\, global neutrino exploration of neutrinos.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2025-10-13-kendall-mahn/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20251023T130000
DTEND;TZID=Europe/Berlin:20251023T140000
DTSTAMP:20260417T212726
CREATED:20251013T100356Z
LAST-MODIFIED:20251013T100356Z
UID:5996-1761224400-1761228000@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Milena Crnogorcevic\, Stockholm University
DESCRIPTION:Gamma Rays from the Littlest Galaxies: Tracing Accretion and Dark Matter in the Low-Mass Universe\nNow in its 17th year of operation\, the Fermi Large Area Telescope (LAT) continues to transform our understanding of the smallest galaxies in the Universe. Dwarf galaxies host some of the most extreme environments known—from ultra-faint systems dominated by dark matter to those harboring actively accreting intermediate-mass black holes (IMBHs). In the first part of this talk\, I will present results from the first systematic Fermi-LAT search for gamma-ray emission from active galactic nuclei in dwarf galaxies\, revealing hints of a soft-spectrum excess that may trace the onset of high-energy activity in low-mass black holes. In the second part\, I will discuss our complementary search for dark matter annihilation in dwarf galaxies\, including limits from ultra-faint systems. Together\, these studies illustrate how the littlest galaxies provide powerful and complementary laboratories in gamma rays—probing both the physics of black hole growth and the nature of dark matter. Looking ahead\, I will address the (exciting) uncertainties and challenges facing space-based gamma-ray astronomy\, as well as highlight the promising prospects offered by next-generation ground-based gamma-ray observatories.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2025-10-23-milena-crnogorcevic/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20251120T130000
DTEND;TZID=Europe/Berlin:20251120T140000
DTSTAMP:20260417T212726
CREATED:20251105T101708Z
LAST-MODIFIED:20251105T101708Z
UID:6027-1763643600-1763647200@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Lucas de Sa\, Heidelberg University
DESCRIPTION:Prospects for pulsars and pulsar associations in multi-messenger astrophysics with population synthesis\nPopulation synthesis seeks to integrate the full framework of stellar evolution with predictions for observations of different products of said evolution\, potentially allowing constraints to be placed on multiple evolutionary steps at the same time. It has become a central tool in gravitational-wave astronomy when simulating populations of compact object mergers and predicting merger rates over redshift\, where it nevertheless faces the challenge of dealing with the high level of uncertainty surrounding massive stellar evolution\, and the degeneracy between multiple physical assumptions when making predictions for a single kind of event. This degeneracy\, however\, could be lifted in part by accounting for a broader range of stages a star goes through during its life\, as well as alternative outcomes. In this talk\, I will explore the prospects of using these same tools to study observed populations of pulsars and pulsar associations – pulsar wind nebulae and halos. In particular\, I will highlight current advances in supernova theory and stellar angular momentum evolution\, and the potential for a more detailed picture of pulsar formation. I will also present ongoing work on the generation of synthetic pulsar association populations for the study of observations of current gamma-ray observatories\, in particular HAWC\, and for the prediction of observations by the future SWGO.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2025-11-20-lucas-de-sa/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260315T140000
DTEND;TZID=Europe/Berlin:20260320T130000
DTSTAMP:20260417T212726
CREATED:20260210T144400Z
LAST-MODIFIED:20260210T144400Z
UID:6159-1773583200-1774011600@ecap.nat.fau.de
SUMMARY:DPG Spring Meeting at FAU
DESCRIPTION:ECAP is happy to organise the  \n89 Annual Conference of the DPG and DPG Spring Meeting of the Matter and Cosmos Section (SMuK)\n15 – 20 March 2026 \nWe expect around 2000 physicists to join this conference downtown Erlangen. \nMore information at https://erlangen26.dpg-tagungen.de
URL:https://ecap.nat.fau.de/index.php/event/dpg-spring-meeting-at-fau/
LOCATION:Philosophie\, Kollegienhaus and Alte Mathemathik\, Erlangen\, Universitätsstr. 15\, Erlangen\, 91054\, Germany
ATTACH;FMTTYPE=image/jpeg:https://ecap.nat.fau.de/wp-content/uploads/2026/02/0a685858-0dd0-477b-ac54-d8a84e725e4d.jpeg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260416T130000
DTEND;TZID=Europe/Berlin:20260416T140000
DTSTAMP:20260417T212726
CREATED:20260216T122502Z
LAST-MODIFIED:20260410T071822Z
UID:6220-1776344400-1776348000@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Matthias Danninger\, Simon Fraser University
DESCRIPTION:The Pacific Ocean Neutrino Experiment\n\n\n\n\n\n\n\n\n\n\n\n\nEvery time researchers have pushed the energy boundary in particle physics we have found something new about our Universe. Recently\, IceCube has demonstrated that Neutrino Telescopes can use neutrinos from the cosmos as excellent tools to continue this exploration. To unlock the true potential of this field\, advanced detectors are needed that will push the forefront of the cosmic frontier\, revealing new knowledge of extreme astrophysical phenomena\, including through multi-messenger follow-up programs\, and testing fundamental physics at scales well beyond those reachable by Earth-bound accelerators. We aim to construct one of the largest neutrino telescopes deep in the northern Pacific Ocean off the coast of British Columbia\, the Pacific Ocean Neutrino Experiment (P-ONE). The first detector line is planned to be deployed this year – marking the start of an exciting phase for this new project. In this talk I will cover results from early pathfinder missions and discuss a detailed status of the P-ONE detector concept.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-04-16-matthias-danninger/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260430T130000
DTEND;TZID=Europe/Berlin:20260430T140000
DTSTAMP:20260417T212726
CREATED:20260302T153000Z
LAST-MODIFIED:20260413T065531Z
UID:6357-1777554000-1777557600@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Tanguy Pierog\, KIT
DESCRIPTION:EPOS LHC-R : a global approach to solve the muon puzzle\nThe hadron production in the simulation of extensive air showers is a long standing problem and the origin of large uncertainties in the reconstruction of the mass of the high energy primary cosmic rays. Hadronic interaction models re-tuned after early LHC data give more consistent results among each other compared to the first generation of models\, but still can’t reproduce extended air shower data (EAS) consistently resulting in the so-called “muon puzzle”. Using more recent LHC data like in the QGSJET-III model improve further the description of EAS by such a model but is not enough to resolve the discrepancy. On the other hand\, the EPOS project is a theoretical global approach aiming at describing data from very fundamental electron-positron interactions to central heavy ions collisions. We will demonstrate that this approach can provide new constraints\, changing the correlation between the measured data at mid-rapidity and the predicted particle production at large rapidities\, which drive the EAS development. Thus\, using the same accelerator data\, different predictions are obtained in air shower simulations in much better agreement with the current air shower data (for both the maximum shower development depth Xmax and the energy spectrum of the muons at ground). Using the EPOS LHC-R model\, the detailed changes will be addressed and their consequences on EAS observable at various energies.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-04-30-tanguy-pierog/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260528T130000
DTEND;TZID=Europe/Berlin:20260528T140000
DTSTAMP:20260417T212726
CREATED:20260226T114612Z
LAST-MODIFIED:20260227T115613Z
UID:6334-1779973200-1779976800@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Ernst-Jan Buis\, Nikhef
DESCRIPTION:Acoustic neutrino detection\nAbstract
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-05-28-ernst-jan-buis/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260602T150000
DTEND;TZID=Europe/Berlin:20260602T160000
DTSTAMP:20260417T212726
CREATED:20260226T173939Z
LAST-MODIFIED:20260226T173939Z
UID:6338-1780412400-1780416000@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Kavitha Arur\, University of Maryland / NASA
DESCRIPTION:Introduction to and Science highlights from the Imaging X-ray Polarimetry Explorer\nThe Imaging X-ray Polarimetry Explorer (IXPE) is a NASA Small Explorer Mission resulting from the collaboration of NASA Marshall Space Flight Center\, the Italian Space Agency and other partners. IXPE has been successfully performing science operations since January 2022. IXPE provides unique and powerful X-ray polarization capabilities and has been providing crucial insights into our understanding of X-ray production and the geometry of several objects such as neutron stars and pulsar wind nebulae\, as well as stellar and supermassive black holes\, among others. In this talk\, I will give an overview of the mission\, science highlights from IXPE\, and upcoming opportunities to get involved.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-06-02-kavitha-arur/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260625T130000
DTEND;TZID=Europe/Berlin:20260625T140000
DTSTAMP:20260417T212726
CREATED:20260216T122819Z
LAST-MODIFIED:20260226T114642Z
UID:6228-1782392400-1782396000@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Philipp Eller\, Technical University Munich
DESCRIPTION:TBA\nTBA
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-06-25-philipp-eller/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260709T130000
DTEND;TZID=Europe/Berlin:20260709T140000
DTSTAMP:20260417T212726
CREATED:20260304T100844Z
LAST-MODIFIED:20260304T100844Z
UID:6375-1783602000-1783605600@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Tim Huege\, KIT
DESCRIPTION:TBA\nTBA
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-07-09-tim-huege/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260723T130000
DTEND;TZID=Europe/Berlin:20260723T140000
DTSTAMP:20260417T212726
CREATED:20260302T154406Z
LAST-MODIFIED:20260302T154406Z
UID:6364-1784811600-1784815200@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Julia Herzen\, TUM
DESCRIPTION:TBA\nTBA
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-07-23-julia-herzen/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20260917T130000
DTEND;TZID=Europe/Berlin:20260917T140000
DTSTAMP:20260417T212726
CREATED:20260216T123059Z
LAST-MODIFIED:20260226T114608Z
UID:6231-1789650000-1789653600@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Thijs van Eden\, DESY
DESCRIPTION:Neutrino flavors with the IceCube Neutrino Observatory\nAbstract
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-09-17-thijs-van-eden/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20261001T130000
DTEND;TZID=Europe/Berlin:20261001T140000
DTSTAMP:20260417T212726
CREATED:20260318T101532Z
LAST-MODIFIED:20260318T101714Z
UID:6397-1790859600-1790863200@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Laura Olivera-Nieto\, University of Amsterdam
DESCRIPTION:TBA\nTBA
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-2026-10-01-laura-olivera-nieto/
LOCATION:ECAP Laboratory\, 00.061\, Nikolaus-Fiebiger-Str. 2\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
END:VCALENDAR