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NBIA Summer School on Neutrinos: Here, There & Everywhere

17–21 Jul 2023
Niels Bohr Institute
Europe/Copenhagen timezone
Zoom room: https://ucph-ku.zoom.us/j/66810127842?pwd=ZDVPVWV2anVtMFVkVklhcVlLUm92QT09 (password is in your e-mail)

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Contribution List

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  1. 28. Welcome
    17/07/2023, 09:15
    Oral
  2. 60. Lecture I
    Gabriela Barenboim (University of Valencia & IFIC (UV-CSIC))
    17/07/2023, 09:30
  3. 57. Lecture I
    Walter Winter (Deutsches Elektronen-Synchrotron (DESY))
    17/07/2023, 11:00
  4. 95. Exploring the dark Universe with gravitational waves
    Jose Maria Ezquiaga (Niels Bohr Institute)
    17/07/2023, 13:30
  5. 101. Hunt for Intermediate Black Holes with Gravitational Waves and Neutrinos
    Alberto Gálvez Ureña (Ceico at the Institute of Physics of the Czech Academy of Sciences), Pavel Kůs (CEICO, Institute of Physics of the Czech Academy of Sciences)
    17/07/2023, 14:00

    Intermediate mass black holes (IMBHs) have been theorized as an intermediate state between stellar and supermassive black holes (SMBHs), but not observations have confirmed their existence yet. We propose a method to search for them using Tidal Distruption Events (TDEs). In particular we focus on the disruption of white dwarfs (WDs) by IMBHs, as they are expected to produce both gravitational...

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  6. 98. Towards xenon-doped liquid argon for LEGEND
    Christoph Vogl (TU-Munich)
    17/07/2023, 14:15

    The LEGEND collaboration is searching for neutrinoless double beta decay of Ge-76. To this end, high-purity Ge detectors are operated in an instrumented liquid argon volume, shielding them from external background radiation passively and actively via the emission of scintillation light upon interaction with ionizing radiation. While liquid argon scintillation detectors are an established and...

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  7. 102. Intrinsic Resolution Limits in Low-Energy Neutrino Event Reconstruction with IceCube
    Kaustav Dutta (Universität Mainz)
    17/07/2023, 14:30

    The IceCube Observatory is a cubic-kilometer neutrino telescope built into the deep glacial ice at the South Pole. Low energy extensions to the detector include the existing DeepCore subarray and the upcoming IceCube Upgrade. These focus on neutrino oscillation physics using atmospheric neutrinos and are characterized by a denser instrumentation. These elusive particles are indirectly detected...

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  8. 105. Neutrino Decay scenarios on the Cosmic Neutrino Background
    Leonardo Ferreira Leite (State University of Campinas (Unicamp) / CERN)
    17/07/2023, 14:45

    In this work, we explore the consequences of neutrino decay facilitated by a neutral scalar on possible cosmic neutrino background (CνB) detection in the future, especially in the PTOLEMY experiment. We analyze the distortion of the expected event spectrum as a function of the singlet mass and Yukawa couplings, and we consider both a three-neutrino scenario and a scenario with an extra sterile...

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  9. 58. Lecture II
    Walter Winter (Deutsches Elektronen-Synchrotron (DESY))
    18/07/2023, 09:30
  10. 61. Lecture II
    Gabriela Barenboim (University of Valencia & IFIC (UV-CSIC))
    18/07/2023, 11:00
  11. 106. Diffusive shock acceleration and multi-messenger radiation from wind bubbles
    Enrico Peretti (Niels Bohr Institute, University of Copenhagen)
    18/07/2023, 13:30
  12. 103. Modeling neutrino emission from Active Galactic Nuclei
    Ms Arifa Khatee Zathul (University of Wisconsin-Madison)
    18/07/2023, 14:00

    The IceCube Neutrino Observatory is a cubic kilometer detector located at the South Pole that detects high-energy neutrinos by the Cherenkov radiation produced by secondary particles when they interact in the ice. With a decade of data, the IceCube Collaboration has started to identify active galactic nuclei (AGN) as neutrino sources. These had been theorized to be potential sites to...

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  13. 99. Studying the physical properties of the engines of neutrino-emitter blazars.
    Alessandra Azzollini (Julius-Maximilians Universität Würzburg)
    18/07/2023, 14:15

    High-energy neutrinos detected by the IceCube Observatory provide an exclusive opportunity to study the origin of cosmic rays and the nature of the sources producing them. Blazars are among the proposed birthplaces for the astrophysical high-energy neutrinos. We focus on a small set of blazars that are likely counterparts to IceCube neutrinos.

    In this contribution, we aim to inspect this...

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  14. 94. Investigating high-energy neutrinos from blazars with an analysis of the IceCube observatory data
    Eleonora Barbano (Julius-Maximilians-Universität Würzburg, Fakultät für Physik und Astronomie, Emil-Fischer-Str. 31, D-97074 Würzburg, Germany)
    18/07/2023, 14:30

    In the past decade, the IceCube observatory has established the presence of a diffuse flux of high-energy neutrinos (≥100 TeV to 10 PeV) that is consistent with an astrophysical origin. However, the population of sources responsible for this flux remains largely unknown.
    Among the candidate sources of neutrinos, blazars have been suggested as promising emitters of the high-energy events...

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  15. 100. Jet contribution to the 𝛾-ray Flux in NGC 1068
    Silvia Salvatore
    18/07/2023, 14:45

    NGC1068 is a Seyfert II starburst galaxy emitting in a very broad range of frequencies, from radio up until
    gamma-ray energies. Since the observed high-energy neutrinos and gamma-rays fluxes are different by at
    least 2 orders of magnitude, it becomes necessary to account for a multi-component model to describe the
    multimessenger emission by NGC1068. The neutrinos signal can be explained...

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  16. 62. Lecture III
    Gabriela Barenboim (University of Valencia & IFIC (UV-CSIC))
    19/07/2023, 09:30
  17. 63. Lecture I
    Steen Hannestad (Aarhus University)
    19/07/2023, 11:00
  18. 87. Neutrino constraints from gamma-ray bursts
    Annika Rudolph (Niels Bohr Institute, University of Copenhagen)
    19/07/2023, 13:30
  19. 97. Multi-messenger observations with the KM3NeT telescope: search for high energy neutrinos coinciding with fast radio bursts
    Mr Felix Bretaudeau (on behalf of the KM3NeT Collaboration)
    19/07/2023, 14:00

    The KM3NeT experiment is a next-generation neutrino telescope, consisting of two separate detection structures, organised as arrays of light sensors, and immersed in the depths of the Mediterranean Sea. The two detectors are the Oscillation Research with Cosmics in the Abyss (ORCA detector), located off the coast of France and the Astrophysics Research with Cosmics in the Abyss (ARCA...

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  20. 104. Light dark matter around 100 GeV from the inert doublet model
    Leila Kalhor (Shahid Beheshti University)
    19/07/2023, 14:15

    We made global fits of the inert Higgs doublet model (IDM) in the light of collider
    and dark matter search limits and the requirement for a strongly first-order elec-
    troweak phase transition (EWPT). These show that there are still IDM parameter
    spaces compatible with the observational constraints considered. In particular, the
    data and theoretical requirements imposed favour the...

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  21. 90. Improving CP Measurement with THEIA and Muon Decay at Rest
    Chui-Fan Kong (Tsung-Dao Lee Institute)
    19/07/2023, 14:30

    We explore the possibility of using the recently proposed THEIA detector to measure the $\bar \nu_\mu \rightarrow \bar \nu_e$ oscillation with neutrinos from a muon decay at rest ($\mu$DAR) source to improve the leptonic CP phase measurement. Due to its intrinsic low-energy beam, this $\mu$THEIA configuration ($\mu$DAR neutrinos at THEIA) is only sensitive to the genuine leptonic CP phase...

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  22. 65. Lecture II
    Steen Hannestad (Aarhus University)
    20/07/2023, 09:30
  23. 59. Lecture III
    Walter Winter (Deutsches Elektronen-Synchrotron (DESY))
    20/07/2023, 11:00
  24. 89. Near-future discovery of point sources of ultra-high-energy neutrinos
    Damiano Fiorillo (Niels Bohr Institute, University of Copenhagen)
    20/07/2023, 13:30
  25. 96. A First Look at Sky Anisotropies of High-Energy Neutrino Flavours
    Bernanda Telalovic (Niels Bohr Institute, University of Copenhagen)
    20/07/2023, 14:00

    High-energy astrophysical neutrinos, with TeV–PeV energies and cosmological-scale baselines, provide us with a unique opportunity to study fundemental physics. By looking for the differences in the distribution of arrival directions of neutrinos of different flavours, we can probe physics beyond the Standard Model that predicts directionally-varying flavour ratios under the reasonable...

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  26. 91. Anomalies in the Radio Neutrino Observatory Greenland
    Zachary Meyers (DESY Zeuthen)
    20/07/2023, 14:15

    After two seasons of deployment, 7 stations built and many lessons learned, the Radio Neutrino Observatory Greenland (RNO-G) is now operational. In the coming years, the construction of another 28+ stations will bring the array to full capacity as an instrument with an eye towards the ultra-high energy neutrino (>10 PeV) regime, creating another link in the fast paced and rapidly changing...

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  27. 92. The Role of Electromagnetic Cascades in High-Energy Neutrino Astrophysics
    Antonio Capanema (Pontifícia Universidade Católica do Rio de Janeiro)
    20/07/2023, 14:30

    High-energy gamma-rays do not travel freely across our Universe. Above the pair production threshold, they interact with background photon fields, giving rise to eletromagnetic cascades that take place over cosmological distances, and producing sub-TeV gamma-ray fluxes at the Earth. In this talk, we will demonstrate how one can use such cascades in a multimessenger context to infer properties...

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  28. 93. Stochastic modelling of cosmic ray sources for diffuse high-energy gamma-rays and neutrinos
    Anton Stall (Institute for Theoretical Particle Physics and Cosmology (TTK), RWTH Aachen University)
    20/07/2023, 14:45

    Cosmic rays of energies up to a few PeV are believed to be of Galactic origin, yet individual sources have still not been firmly identified. Due to inelastic collisions with the interstellar gas, cosmic-ray nuclei produce a diffuse flux of high-energy gamma-rays and neutrinos. Fermi-LAT has provided maps of galactic gamma-rays at GeV energies which can be produced by both hadronic and leptonic...

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  29. 66. Lecture III
    Steen Hannestad (Aarhus University)
    21/07/2023, 09:30
  30. 88. Coherent forward scattering of neutrinos
    Shashank Shalgar (NBIA)
    21/07/2023, 11:00

    TBA

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  31. 4. Farewell & Intro of Niels Bohr Archive
    21/07/2023, 11:30
  32. 29. Farewell