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IceCube Gen2

The world's largest particle detector IceCube uses the glacial ice at the South Pole as a gigantic detector medium to hunt for cosmic neutrinos. It is already the world's most advanced neutrino telescope, but the upgrade to IceCube-Gen2 will enlarge the detector by a factor of ten IceCube-Gen2 strings in the optical high-energy array, with 120 new strings (shown as orange points) spaced 240 m apart and instrumented with optical modules over a vertical length of 1.25 km. The total instrumented volume in this design is 7.9 times larger than the current IceCube detector array (blue points) Die Hauptaufgabe ist die Erforschung des hochenergetischen Universums. Die Niederenergiekomponente von IceCube-Gen2, PINGU, besteht aus etwa 40 zusätzlichen Strings (graues Volumen innerhalb des grünen Bereichs der Grafik), die in kurzen horizontalen Abständen installiert werden und ein Volumen von mehreren Megatonnen Eis instrumentieren The high-energy component of IceCube-Gen2 (blue volume in the graphics) will enclose the current detector (red) with about 140 additional strings, each equipped with up to 80 optical sensors, thereby instrumenting 5-10 km 3 of ice. Its main mission is the exploration of the high-energy universe with neutrinos IceCube-Gen2 will increase the annual rate of observed cosmic neutrinos by a factor of ten compared to IceCube, and will be able to detect sources five times fainter than its predecessor. Furthermore, through the addition of a radio array, IceCube-Gen2 will extend the energy range by several orders of magnitude compared to IceCube

IceCube-Gen2 will open a new window on the univers

IceCube-Gen2, a ten-cubic-kilometer detector The incredible clarity of the Antarctic glacier, revealed by the construction and operation of IceCube, will allow the spacing between light sensors to exceed 250 meters, instead of the current 125 meters in IceCube This document presents a vision for an substantial expansion of the current IceCube detector, IceCube-Gen2, including the aim of instrumenting a volume of clear glacial ice at the South Pole to deliver substantial increases in the astrophysical neutrino sample for all flavors •The high energy extensionof IceCube, Gen2 is under design •New sensor R&D are on-going and maturing •Gen2will provide a new and uniqueview of the high- energy Universe •Sources, sourceproperties and connections with UHECRare to be discovered 18 1

AG Kappes_ IceCube-Gen2 - uni-muenster

Left: POCAM as a 48 multi-port integrating sphere with a

[2008.04323] IceCube-Gen2: The Window to the Extreme Univers

Als nächster Schritt in Richtung eines Instrumentes der nächsten Generation (IceCube-Gen2), wird zurzeit eine Erweiterung des aktuellen Teleskops mit mindestens 7 Strings aus neuartigen Sensoren vorbereitet (IceCube-Upgrade). Diese Strings werden die Messgenauigkeit des gesamten Teleskops deutlich verbessern. Die Installation ist für den. IceCube-Gen2 . Universität Karlsruhe (TH) / University of Karlsruhe. Twitter account. Dieses Profil melden Aktivitäten Thanks to the students, the KIT / AIFB team and Messe Karlsruhe for making a historic moment possible! Today's #KIT exam on foundations of computer Beliebt bei Andreas Haungs. This was shared by my colleague and friend Toshikazu Ebisuzaki, with the comment that this is a. icecube-gen2.com is 1 year 11 months old. It is a domain having com extension. This website is estimated worth of $ 8.95 and have a daily income of around $ 0.15. As no active threats were reported recently by users, icecube-gen2.com is SAFE to browse. icecube-gen2.co IceCube-Gen2 high-energy array to measure properties of the observed quasi-diffuse neutrino flux and discover steady point sources of neutrinos. 2.1 Event rate calculation We have parameterized the performance of each of our proposed detector geometries to detect and reconstruct tracks and cascades. We then calculate event rates by folding these quantities with the probabilities for neutrinos. Inspired by the discovery of a comogenic high-energy neutrino flux in IceCube, plans are under way for the construction of new neutrino observatory at the South pole. This next-generation neutrino telescope, IceCube-Gen2, will expand the sensitivity range to lower as well as towards higher neutrino energies with respect to the currently operating IceCube detector

IceCube-Gen2 Collaboration Surface Veto 17.10.2015 MANTS Meeting 2015 - Amsterdam 9 Generic surface array simulations just released at IceCube Gen2 meeting actually predict substantive gains in several FoM for CRA in the 10's of millions price. We have just adopted a 75 km2 CRA as baseline. Technology still unspecified: scintillator, frozen pool Dieser dient dazu, die Lichtsensoren fur IceCube-Gen2 zu kalibrieren, Hierbei wurde ein Photodiodensystem mit der Photodiode S2281 von Hamamatsu und ein Vor-verst arkersystem, welches im Rahmen einer anderen Arbeit [ 12] entworfen wurde, auf die Linearit at und Stabilit at gepr uft. Da die S2281 Diode f ur ihre Stabilit at in einem weiten Bereich bekannt ist, ist eine Pr azisions-Illumination. IceCube-Gen2 Simulaion of an idealized precision optical calibration module for IceCube-Gen2 Nicola Söker 26. Oktober 2015. Erstgutachter(Themensteller):Prof.Dr.E.Resconi Zweitgutachter:Prof.Dr.W.Petry. Abstract A new calibration device called presition optical calibration module or shortened POCAM is currently under development. POCAM will be used for IceCube-Gen2. Here we present design studies for IceCube-Gen2,the next-generation neutrino observatory for the South Pole.IceCube-Gen2 will have an instrumented volume nearly 10 times greater than IceCubealone, substantially increasing sensitivity to high-energy neutrinos.On the surface, a large air shower detectorwill veto high-energy atmospheric muons and neutrinos from the southernhemisphere, enhancing. Danach soll bis Ende des Jahrzehnts im Rahmen des IceCube-Gen2 Projektes das Volumen von IceCube fast verzehnfacht werden, wodurch sich dann die Zahl gemessener Neutrinoreaktionen entsprechend vergrößert. Mit IceCube ist uns erstmalig der Nachweis der Glashow-Resonanz gelungen und mit IceCube-Gen2 werden wir die Reaktion nutzen können, den Fluss von kosmischen Anti-Elektron-Neutrinos.

Beyond IceCube - IceCub

IceCube-Gen2 Collaboration Conceptual Design A conceptual drawing of the IceCube Gen2 Facility is shown at right. Specific points of design are likely to evolve quite a bit. However salient points are the multiple sub-detectors: • PINGU -low energy, mass hierarchy • High Energy Array (HEA) -PeV scale neutrino detector using optica IceCube-Gen2 Facility 3 Gen2 High-Energy Array Gen2 Surface Veto IceCube DeepCore PINGU Multi-component observatory: • Surface air shower detector • Gen2 High-Energy Array • Sub-surface radio detector • PINGU A wide band neutrino observatory (MeV - EeV) using several detection technologies - optical, radio, and surface veto - to maximize the science . Open questions for neutrino.

Cosmic Neutrinos Lab - Wissel Lab

[1412.5106] IceCube-Gen2: A Vision for the Future of ..

  1. IceCube-Gen2 Detector upgrade. Artists rendition of IceCube (red) with a possible Gen2 detector update (Credit: IceCube collaboration) After the discovery of a cosmic high-energy neutrino flux in 2013, a next-generation neutrino telescope at the South Pole, IceCube-Gen2, is now in the planning stage that will provide extended physics potential both at the highest and lower energies. The.
  2. IceCube-Gen2 Calibration Workshop - April 8 What to do in Gen2 - Upgrading the logger design Intensity monitoring of the output beam No absolute calibration of present dust log. Laser driver power was manually adjusted to avoid saturating the optical detector. This is fine for tilt map; where only vertical peak positions needed. Absolute calibration is possible if we monitor the light with a.
  3. g tracks. This can be done by the installation of surface veto 10.
  4. Dank der zusätzlichen Sensoren könnte IceCube-Gen2 dann die Detektionsrate vor allem der energiereichen Neutrinos um das Zehnfache erhöhen. (Nature, 2021; doi: 10.1038/s41586-021-03256-1
  5. toriums, IceCube-Gen2, in Entwicklung. An IceCu-be-Gen2 ist die Arbeitsgruppe an der Erforschung und Entwicklung neuer Detektor Prototypen und Datenerfassungssystemen beteiligt. Eine am KIT neu entwickelter Prototyp einer Ober-flächendetektor-Station besteht aus acht Szintil-lationsdetektoren und drei Radio Antennen. Eine Vielzahl dieser Stationen, großflächig am Südpol verteilt, werden.
  6. Forschende der JGU an IceCube Upgrade und künftigem IceCube-Gen2 beteiligt Mit den zusätzlichen Lichtsensoren wird die Sensitivität vor allem bei niedrigen Energien im Bereich von 5 bis 10 Gigaelektronenvolt deutlich gesteigert. Dies ist der Energiebereich, in dem die Wissenschaftlerinnen und Wissenschaftler bei IceCube Neutrinooszillationen von atmosphärischen Neutrinos beobachten können.

IceCube Gen2: concept-stage future (2026+) facility enhancement - 10x bigger IceCube for neutrino astrophysics. IceCube Collaboration: scientific collaboration of 350+ researchers world-wide that provide resources (cash, computing, labor) to M&O and receive computing and storage, processed data, simulated data The recent observation by the IceCube neutrino observatory of an astrophysical flux of neutrinos represents the first light in the nascent field of neutrino astronomy. The observed diffuse neutrino flux seems to suggest a much larger level of hadronic activity in the non-thermal universe than previously thought and suggests a rich discovery potential for a larger neutrino observatory. IceCube Gen2 - scope IceCube and Gen2 on different scales reflecting different energies 10 PeV 10 TeV 1 TeV few GeV. Sensor design R&D for improved performance 27 IceCube DOM 33 cm FOM Smaller diameter MDOM and Degg are primary sensors for Upgrade. R&D for Gen2 for multi DOM and including other sensor concept. Upgrade primary sensors. Gen2 - R&D Optical sensors (previous slide) Power and.

IceCube-Gen2 covers particle physics from MeV to EeV with real discovery potential. Teppei Katori, Queen Mary University of London 2017/07/21 4 Physics of IceCube-Gen2 Astrophysical neutrino flavour - very sensitive to new physics such as neutrino decay, non-standard interaction, quantum gravity, etc Unlimited list of science! - low mass dark matter - neutrino mass ordering - multi-messenger. Mit dem IceCube-Upgrade und dem späteren Ausbau zu IceCube-Gen2 erweitert dieses weltweit einzigartige Neutrino-Observatorium unseren Blick ins All an entscheidender Stelle und trägt dadurch bei, die Rätsel um die Physik der höchstenergetischsten Prozesse in unserem Universum zu lösen, sagt der Leiter der KIT-IceCube-Gruppe, Andreas Haungs. Durch die Erweiterung steigt jedoch nicht.

Zugehörige Institution(en) am KIT: Institut für Kernphysik (IKP) Publikationstyp: Poster: Publikationsjahr: 2017: Sprache: Englisch : Identifikator: KITopen-ID. Mit IceCube ist uns erstmalig der Nachweis der Glashow-Resonanz gelungen und mit IceCube-Gen2 werden wir die Reaktion nutzen können, den Fluss von kosmischen Anti-Elektron-Neutrinos genau zu vermessen, sagt Professor Dr. Marek Kowalski vom DESY, der die Vorbereitungen von IceCube-Gen2 koordiniert. Das wird uns einen ganz neuen Zugang liefern, die wenig bekannten. Mit dem IceCube-Upgrade und dem späteren Ausbau zu IceCube-Gen2 erweitert dieses weltweit einzig­artige Neutrino-Obser­vatorium unseren Blick ins All an entscheidender Stelle und trägt dadurch bei, die Rätsel um die Physik der höchst­energetischsten Prozesse in unserem Universum zu lösen, sagt der Leiter der KIT-IceCube-Gruppe, Andreas Haungs. Durch die Erweiterung steigt jedoch.

IceCube‐Gen2. Schematische Darstellung des geplanten IceCube‐Gen2‐Observatoriums. IceCube (mittlere Kontur) wird in einer ersten Phase durch neue Sensoren im Zentrum (innere Kontur) erweitert und danach das Volumen auf acht Kubikkilometer vergrößert (äußere Kontur). An der Oberfläche sieht man Teile der Radiodetektoren, die sich bis zum Horizont erstrecken (Grafik: DESY/SciComLab. Eine Erweiterung des IceCube-Detektors, genannt IceCube-Gen2, würde es den Physikern ermöglichen, solche Messungen mit statistischer Signifikanz durchzuführen. In den nächsten Jahren wird als erster Schritt in diese Richtung ein Upgrade in den Detektor implementiert. Auch Glashow, jetzt emeritierter Professor für Physik an der Boston University, betont die Notwendigkeit, mehr Glashow. IceCube plans to extend the IceCube observatory (IceCube-Gen2) by increasing the detection volume substantially to study cosmic neutrinos in detail, by lowering the energy threshold to a few GeV in order to determine the neutrino mass hierarchy and precise measure neutrino oscillation parameters and by covering the surface with a large detector to veto cosmic ray muons and to study cosmic rays. IceCube-Gen2 Preliminary Gen2 will have sensitivity to neutrinos produced in Galactic sources, constraining CR acceleration processes. Shown are TeVHAWC sources near the galactic plane, color coded to indicate possible detections (if !-ray emission arises solely from hadronic processes) and where Gen2 can constrain the level of hadronic emission. IceCube-Gen2 Preliminary We are grateful to the. IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica . IsoDAR (Isotope Decay-at-Rest) is an experiment to search for electron antineutrino disappearance using an extremely high intensity source of neutrinos from the decay of 8 Li isotopes. The large number of 8 Li isotopes are produced using a 10 ma, 60 MeV proton cyclotron that is being developed in collaboration with.

IceCube - Größter Neutrinodetektor der Welt am Südpo

Darüber hinaus verfügt IceCube über einen Oberflächendetektor IceTop für kosmische Strahlung. Unsere Gruppe am KIT arbeitet hauptsächlich am Upgrade von IceTop sowie an der nächsten Generation des IceCube Experiments, IceCube-Gen2. Beim ERC-Projekt PeV-Radio geht es um eine Erweiterung von IceTop mit Radioantennen IceCube-Gen2: The next generation neutrino observatory in Antarctica (UHECR2016) dual-PMT optical module (D-Egg) for IceCube-Gen2 (ICRC2015) Photon search at the Pierre Auger Observatory (SciNeGHE2014 IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica. Abstract: The recent observation by the IceCube neutrino observatory of an astrophysical flux of neutrinos represents the first light in the nascent field of neutrino astronomy. The observed diffuse neutrino flux seems to suggest a much larger level of hadronic activity in the non-thermal universe than previously. Gleichzeitig misst IceCube eine beispiellose Anzahl von Neutrinos, die in unserer Atmosphäre erzeugt werden, und bestimmt deren fundamentale Eigenschaften. Der im Bau befindliche IceCube Upgrade Detektor und das Zukunftsprojekt IceCube-Gen2 werden die Empfindlichkeit von IceCube weiter erhöhen

Multi-PMT optical modules for IceCube-Gen

icecube-gen2.net was registered on May 8, 2019 and is associated with b1013e77d2cd4b5fa9be16baef1946c9.protect@whoisguard.com. It is registered at Namecheap. No. Der geplante IceCube-Upgrade-Detektor wird aus zwei verschiedenen Typen von optischen Modulen bestehen, um die beiden Technologien für die zukünftige etwa zehnfach größere Erweiterung von IceCube - IceCube-Gen2 - zu testen. Einer der neuen optischen Sensoren, das multi-Pixel Digital Optical Module (mDOM), wurde in Deutschland von Forschungsgruppen an den Universitäten Erlangen. IceCube-Gen2 by Joost Pieter Veenkamp 6132812 January 31, 2016 60 EC November 2015 - November 2016 Supervisor: Prof. E. Resconi Prof. P. Decowski Assessor: Dr. D. Samtleben. Master of Science A Precision Optical Calibration Module for IceCube-Gen2 Abstract by Joost Pieter VEENKAMP IceCube is a cubic kilometer neutrino detector in the Antarctic ice. With the detection of high energy neutrinos.

IceCube-Gen2: The Window to the Extreme Universe - NASA/AD

IceCube Gen2 Phase 1: an IceCube Extension for Precision Neutrino Physics and Astrophysics. NSF Org: PHY Division Of Physics: Awardee: UNIVERSITY OF WISCONSIN SYSTEM: Initial Amendment Date: September 18, 2018: Latest Amendment Date: December 30, 2020: Award Number: 1719277: Award Instrument: Cooperative Agreement : Program Manager: Jonathan Whitmore jwhitmor@nsf.gov (703)292-8908 PHY Division. Wir arbeiten daran, den Ursprung höchstenergetischer kosmischer Strahlung mit Cherenkov-Teleskopen (MAGIC, FACT, CTA/LST), mit Neutrino-Teleskopen (AMANDA, IceCube/GEN2) und mit Radioteleskopen (MeerKAT, GLOW) zu ver­ste­hen.Dazu wer­den kosmische Botenteilchen nach­ge­wie­sen und im Rah­men der Multimessenger-Astronomie korreliert. In theoretischen astro- und teilchenphysikalischen. rung von IceCube - IceCube-Gen2 - zu testen. Einer der neuen op-tischen Sensoren, das multi-Pixel Digital Optical Module (mDOM), wurde in Deutschland von Forschungsgruppen an den Universitäten Erlangen-Nürnberg und Münster sowie vom Deutschen Elektronen-Synchrotron DESY federführend entwickelt. Das DESY und das KIT sind als Forschungszentren der Helmholtz-Gemeinschaft mit insge-samt 5.

IceCube-Gen2 - INSPIR

IceCube-Gen2 The IceCube-Gen2 Collaboration Mike DuVernois (Univ. Wisconsin-Madison) Neutrino Drilling IDP Virtual Drill Workshop 2 April 2020. The energy frontier in astronomy 2 Universe opaque to photons for ¼ of the spectrum. 10 yrs of IceCube - a first view on the PeV Universe 3 Some highlights: 2013: Discovery of cosmic PeV neutrino flux 2018: Evidence for Blazars as neutrino sources. Papers submitted to the 34th International Cosmic Ray Conference (ICRC 2015, The Hague) by the IceCube-Gen2 Collaboration IceCube-Gen2 is designed to: 1) resolve the high-energy neutrino sky from TeV to EeV energies, 2) investigate cosmic particle acceleration through multi-messenger observations, 3) reveal the sources and propagation of the high-est energy particles in the universe, 4) probe fundamental physics with high-energy neutrinos. With IceCube-Gen2 we propose a detector of sufficient volume to increase. We gratefully acknowledge support from the Simons Foundation and member institutions the planned upgrade to neutrino detector{IceCube-Gen2 , which is well-positioned to make dramatic improvements in both avor and spectral measurements. We show that various models in neutrino physics beyond the Standard Model, such as neutrino decay, pseudo-Dirac states, and neutrino self-scattering, may be found or strongly constrained at IceCube-Gen2 and KM3NeT. We nd that the additional avor.

IceCube - RWTH AACHEN UNIVERSITY III

Develop improved Optical Module for IceCube-Gen2 based on the proven technology with IceCube DOMs Y. Makino 24th ICEPP symposium 19/Feb./2018. 6 D-Egg D E G G 9 Φ = 300 mm Narrower than IceCube DOM. Reduce drilling costc 8 inch PMT x 2 high QE UV transparent glass Thickness of glass varies along longitude, for mechanical tolerance and UV efficiency 10 inch PMT DOM Φ = 330 mm D-Egg for. Um aber einzelne Quellen auflösen zu können, muss IceCube erweitert werden mit dem finalen Ziel, IceCube-Gen2 zu installieren - ein Detektor, der nochmal um einen Faktor 10 größer ist als IceCube. Ein erster Schritt hierbei ist der Ausbau von IceCube, das IceCube Upgrade. Die Ruhr-Universität Bochum ist konkret an der Erweiterung von IceCube durch das Oberflächenarray IceAct beteiligt. The meeting will be held in the Schuster Building on Brunswick Street within the main campus of the University of Manchester. For full travel information please see. The IceCube-Gen2 project is to provide a substantial expansion of the current 1 km3 IceCube detector with the aim of instrumenting a 10 km3 volume of clear glacial ice at the South Pole and delivering substantial increases in astrophysical neutrino samples of all flavors. A detector of this size would have a rich physics program and would aim to resolve the sources of these astrophysical.

IceCube-Gen2 - The Next Generation Neutrino Observatory at. IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica M. G. Aartsen,2 M. Ackermann,54 J. Adams,16 J. A. Aguilar,12 M. Ahlers,31 M. Ahrens,44 D.

IceCube-Gen2 collaboration is the next generation collaboration to focus on extending low and high energy physics of the IceCube Neutrino Observatory, Antarctica. Especially, PINGU (Precision IceCube Next Generation Upgrade) is the low energy extension of IceCube to detect the atmospheric neutrino oscillation below 10 GeV. The IceCube detector is a large array of DOMs (digital optical modules. Forschende der JGU an IceCube Upgrade und künftigem IceCube-Gen2 beteiligt Mit den zusätzlichen Lichtsensoren wird die Sensitivität vor allem bei niedrigen Energien im Bereich von 5 bis 10 Gigaelektronenvolt deutlich gesteigert. Dies ist der Energiebereich, in dem die Wissenschaftlerinnen und Wissenschaftler bei IceCube Neutrinooszillationen von atmosphärischen Neutrinos beobachten können.

Abstract. Papers submitted to the 34th International Cosmic Ray Conference (ICRC 2015, The Hague) by the IceCube-Gen2 Collaboration. IceTop is the 1 km2 surface array of the IceC IceCube-Gen2. $23M NSF Grant Funds to Upgrade Antarctic IceCube Neutrino Observatory Tuesday, July 16, 2019. The IceCube Neutrino Observatory, the Antarctic detector that identified the first likely source of high-energy neutrinos and cosmic rays, is getting an upgrade. The National Science Foundation Read More. Can't find what you're looking for? Contact research@msu.edu. Helpful Links. IceCube-Gen2 Collaboration; Instructions for updating the author list. If you are not a PI: Ask your PI to make the changes. If you are a PI: Email help@icecube.wisc.edu with any change request. Note that we also handle legacy authors and acknowledgements, with approval from ExecComm.. IceCube-Gen2 Radio Pathfinders. The Wissel group works towards developing the next-generation of in-ice radio instruments through the Askaryan Radio Array (ARA) experiment at the South Pole and the Radio Neutrino Observatory in Greenland . Radio experiments are required for neutrino searches at the highest energies, where the flux is low. at those enregies, sources might show signs of cutoffs.

Unsere Gruppe am KIT arbeitet hauptsächlich an der nächsten Generation des IceCube Experiments, IceCube-Gen2. KSETA PI Ansprechpartner sind Andreas Haungs, Ralph Engel, Tim Huege und Frank Schröder. Dunkle Materie. Wir betreiben intensive Forschung und Entwicklung (F & E) für die aktuelle Suche nach dunkler Materie sowie für die nächste Generation von Experimenten. Die Gruppe Dunkle. For the IceCube-Gen2 high-energy array the definition of the veto has to be optimized and new techniques will be introduced, as the geometry will be different and the distances between the optical modules will be larger than in IceCube. In this contribution we present the results of a data-driven analysis that uses real IceCube data to estimate the expected veto energy threshold. In addition.

Andreas Haungs - Researcher - IceCube-Gen2 LinkedI

IceCube-Gen2 will consist of an approximately ten times larger array that will allow to see smaller neutrino fluxes and study feeble neutrino interactions.In support of his experimental work, Argüelles-Delgado also develops neutrino phenomenology. His recent work includes calculating signatures of heavy neutrinos and neutrino-dark matter interactions. He is collaborating on a project to. Website of the German partners for IceCube-Gen2 The planned expansion of the IceCube observatory at the South Pole marks a new era in neutrino astronomy. External Support. Emmy Noether Programme; ERC Grants; Helmholtz Funding Programs For Leading Female Scientists; Helmholtz-Russia Joint Research Groups ; Humboldt Research Fellowship; Young Investigators Groups; Home / About us / Group Members. It is involved in the construction of the IceCube Upgrade and the preparations for the next-generation neutrino observatory IceCube-Gen2. This next-gen observatory will also feature a novel technique to detect neutrinos by the radio emission produced in their interactions. DESY researchers develop and field test this new technology in Greenland as part of an international team IceCube Gen2: The Next Generation of Neutrino Astronomy ERIK BLAUFUSS, Univ of Maryland-College Park, ICECUBE COLLABORATION | The observations of an astrophysical ux of neutrinos by the IceCube neutrino observatory signaled the start of the era of neutrino astronomy. While the source of these astrophysical neutrinos remains unclear, many strong constraints have al- ready been made.

AG Kappes_Sensorentwicklung

Our group at KIT is mainly working in the frame of the next generation of the IceCube experiment, IceCube-Gen2. KSETA PIs working in this field are Andreas Haungs, Ralph Engel, Tim Huege, Frank Schröder. Dark Matter. We are conducting intensive research and development (R&D) for the current search for dark matter as well as for the next generation of experiments. The Dark Matter Group at KIT. Compact style; Indico style; Indico style - inline minutes; Indico Weeks Vie IceCube-Gen2 will take neutrino astronomy to the next level, moving from a discovery instrument like IceCube to an observational facility which will operate simultaneously with next generation of electromagnetic and gravitational wave detectors, allowing for multi-messenger observations. 5. Conclusions . IceCube has opened a new horizon in astroparticle physics, proving the existence of extra. This is an important benefit for neutrino studies, but it becomes even more relevant for planning the larger IceCube-Gen2. The $37 million extension, to be deployed during the 2022-23 polar field season, has now secured $23 million in NSF funding. Last fall, the upgrade office was set up, thanks to initial funding from NSF and additional support from international partners in Japan and Germany. FIG. 3. Deposited energies of events observed in 3 years of data with predictions. The hashed region shows uncertainties on the sum of all backgrounds. Muons (red) are computed from simulation to overcome statistical limitations in our background measurement and scaled to match the total measured background rate. Atmospheric neutrinos and uncertainties thereon are derived from previous.

icecube-gen2.com : icecube-gen2.com - Registered at ..

1 IceCube-Gen2: the next-generation neutrino observatory for the South Pole. 2 IceAct: Imaging Air Cherenkov Telescopes with SiPMs at the South Pole for IceCube-Gen2. 3 Overview and performance of the D-Egg optical sensor for IceCube-Gen2. 4 Muon track reconstruction and veto performance with D-Egg sensor for IceCube-Gen2 . 5 In-ice self-veto techniques for IceCube-Gen2. 6 A camera system for. RNO-G and IceCube-Gen2. We are involved in the design and development of RNO-G, an in-ice radio detector that we will deploy to Summit Station in Greenland beginning in Summer 2021. RNO-G builds on the succcess of ARA, and incorporates new interferometric phased array trigger technology. RNO-G will have the sensitivity required to discover ultra-high energy neutrinos, while also serving as a. Visitors. In keeping with our vision, we encourage and support visits from researchers who have interests, or who wish to develop interests, in several of our research areas Here we present design studiesfor IceCube-Gen2, the next-generation neutrino observatory for the South Pole. IceCube-Gen2will have an instrumented volume nearly 10 times greater than IceCube alone, substantially in-creasing sensitivity to high-energy neutrinos. On the surface, a large air shower detector willveto high-energy atmospheric muons and neutrinos from the southern hemisphere.

DESY News: Neutrino observatory IceCube receivesThe Vieregg Lab(PDF) Timing the neutrino signal of a Galactic supernova
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