NBIA Summer School on Neutrinos: Here, There & Everywhere

Europe/Copenhagen
Auditorium A (Niels Bohr Institute)

Auditorium A

Niels Bohr Institute

Blegdamsvej 17 DK-2100 Copenhagen
Markus Ahlers (NBI), Mauricio Bustamante (Niels Bohr Institute, University of Copenhagen)
Description

Online participation (22/05/2022): In-person registration is closed, but online participation is possible. If you would like to participate of the school online, please complete the Registration form


The Niels Bohr International Academy (NBIA) invites PhD students and advanced Master students to the International PhD Summer School on Neutrinos: Here, There & Everywhere. This one-week school aims to bring the participants up to date with the latest developments in neutrino physics, from theoretical issues to experimental results, including astrophysical and cosmological aspects.

The deadline for in-person registration is April 30, 2023.  There is no participation fee.

Students will be given topical introductions, along with an overview of the current state of the field and the open questions that confront it. The invited lecturers are internationally renowned experts in their fields. The school participants will gain a broad understanding of current theoretical problems in neutrino physics, state-of-the-art neutrino experiments, and applications of neutrinos in cosmology and astrophysics.

Guest Lectures & Lecturers

Neutrino Theory & Phenomenology
Gabriela Barenboim
Instituto de Física Corpuscular (IFIC), Universidad de Valencia

Neutrino Cosmology
Steen Hannestad
Institut for Fysik og Astronomi, Aarhus Universitet

Neutrino Astrophysics & Astronomy
Walter Winter
Deutsches Elektronen-Synchrotron (DESY), Zeuthen

Local Organizers

Mauricio Bustamante
Markus Ahlers

General instructions

To participate:

  • Register as a participant
  • Registering is solely an expression of interest; you will later be informed about your admittance to the School by the organizers
  • The participation is free of charge and includes catering during coffee and lunch breaks. Students are expected to cover their travel and local expenses.

Participation mode:

  • The main form of participation of the School will be in person
  • In-person participation is limited to 50 students
  • Depending on resources available, we might provide options to participate remotely; you may indicate your preference in the registration form, but please be aware that, at this stage, remote participation is not guaranteed
  • Priority will be given to in-person participants

COVID-19 and health:

  • Please be aware of the health rules regarding COVID-19 to enter Denmark
  • These rules may change over time, so please be sure to revisit them close to your travel dates
  • The School will be carried out following the health guidelines of the Danish Health Authority
  • We ask our participants to follow best health practices at all times

Visa:

  • See here for the list of countries with a visa requirement and visa-free countries to enter Denmark
  • If you require an invitation letter to apply for a visa, please contact our administrator Gosia Dekempe.

Credit:

  • Students who wish to receive credit (2.5 ECTS) for the course are required to give a short presentation on their current research project, to attend lectures and discussion sessions, as well as to participate actively in problem classes
  • Only in-person participants may receive ECTS (unless there are exceptional circumstances)

Questions: 

      Please contact the local organizers, Markus Ahlers and Mauricio Bustamante

Sponsors

Registration
General Registration
Participants
  • Aashik Safar
  • Abhijeet Singh
  • Abhirami Suresh
  • Abhishek Dubey
  • Akash Kumar Saha
  • Akhila Kumar Pradhan
  • Alberto Gálvez Ureña
  • Alessandra Azzollini
  • Alka Singh
  • Alok Ranjan Dash
  • Aman Gupta
  • Aman Verma
  • Amit Singh
  • Ana Maria Garcia Trzeciak
  • Ananya Patankar
  • Anastasiia Mikhno
  • Andrea Heinz
  • Animesh Baral
  • Anirudh Bhatnagar
  • Anna Bjerregaard
  • Annika Rudolph
  • Anton Stall
  • Antonio Capanema
  • Anubhav Mahapatra
  • Arifa Khatee Zathul
  • Arsène Ferrière
  • Arthur Ferreira Vieira
  • Arunkumar Kotagi
  • Ashish Narayan
  • Ashok Kumar Aryal
  • Athul Sajjay
  • Attia Mohamed
  • Ayşe Bat
  • Bernanda Telalovic
  • Bharti Meena
  • Bhavna Yadav
  • Bhavya Soni
  • Bibek Karn
  • Chao Zhang
  • Christoph Vogl
  • Chui-Fan Kong
  • Damiano Fiorillo
  • Debashree Priyadarsini Das
  • Deep Das
  • Deeshani Mitra
  • Devesh Pratap Singh
  • Diwash Ghimire
  • Edis Tireli
  • Eleonora Barbano
  • Enrico Peretti
  • Eobard Ding
  • Erick Urquilla
  • Felix Bretaudeau
  • Finn Mayhew
  • Gabriela Barenboim
  • Gabriela Rodrigues Araujo
  • Gaurav Shukla
  • Gopal Garg
  • Hemant Kumar Prajapati
  • Ibrahim Mirza
  • Ilham El Atmani
  • Imtiaz Khan
  • Ishika Palit
  • Ismael Espinoza
  • Jesus Alberto Cazares Montes
  • Johanna Jallberg
  • Jose Maria Ezquiaga
  • Jothika Ramasamy
  • Julie Kiel Holm
  • János Takátsy
  • Katia Kamura Mamani Burgos
  • Kaustav Dutta
  • Kewen Zhang
  • Krittika Adhikari
  • Krittika Sarkar
  • Kusum Seervi
  • Labh Singh
  • Leander Fischer
  • Leila Kalhor
  • Lekhashri Konwar
  • Lena Saurenhaus
  • Leonardo Ferreira Leite
  • Leonardo Palombini
  • Lihang Zhou
  • Lukas Gülzow
  • Madeeha Nazish
  • Madhumita Patel
  • Marcelo Ismerio Oliveira
  • Markus Ahlers
  • Mauricio Bustamante
  • Mohamed Krab
  • Mohd Faizee
  • Mohit Singh
  • Monal Kashav
  • Muhammad Fauzi Mustamin
  • Muhammad Usman
  • Narmin Nasibova
  • Pablo Martínez-Miravé
  • Paige Kunkle
  • Patrick Adolf
  • Patrícia Duarte de Almeida
  • Pavel Kůs
  • Percy Caceres
  • Peyman Zakeri
  • Prashant Kumar
  • Prasoon Chakraborty
  • Pravi Mishra
  • Prince Kumar
  • Rasmus Ørsøe
  • Raza Ur Rehman Mir
  • Richa Gupta
  • Ricky Crisomeno Ticse Reyes
  • Rithik Rai
  • Rupali Hatte
  • Saeed Ullah Khan
  • Sagar J C
  • Sania Lewis
  • Saurabh Kumar Shukla
  • Sejal Jain
  • Sharda Pandey
  • Shashank Shalgar
  • Siddhant Dutta
  • Silvia Salvatore
  • Simony Santos da Costa
  • Sk Jeesun
  • Sofia Athanasiadou
  • Steen Hannestad
  • Subhadip Bouri
  • Subhodip Daripa
  • SURYA VAMSHI ALLADA
  • Swapnil Singh
  • Ting Wing Choi
  • Tobias Heibges
  • Tri Utari
  • Trisha Sarkar
  • Utpal Mondal
  • Vigneshwaran Palaniappan
  • Vincent Gousy-Leblanc
  • Vivek Banerjee
  • Waleed Hussain
  • Walter Winter
  • Yifan Chen
  • Yogesh Bari
  • Yuliia Borysenkova
  • Zachary Meyers
  • Zahra Bagheri
  • Zakaria El-ansary
  • +1
    • 1
      Welcome Auditorium A (NBI)

      Auditorium A

      NBI

    • Neutrino Theory & Phenomenology Auditorium A (NBI)

      Auditorium A

      NBI

    • 10:30
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • Neutrino Astrophysics & Astronomy Auditorium A (NBI)

      Auditorium A

      NBI

    • 12:00
      Lunch Auditorium C (NBI)

      Auditorium C

      NBI

    • Topical Seminar Auditorium A (NBI)

      Auditorium A

      NBI

    • Student Talks Auditorium A (NBI)

      Auditorium A

      NBI

      • 5
        Hunt for Intermediate Black Holes with Gravitational Waves and Neutrinos

        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 waves (GWs) and high energy neutrinos. This is particularly, interesting because WDs cannot be disrupted by a SMBH. We present an introductory study on this method and future prospects.

        Speakers: 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)
      • 6
        Towards xenon-doped liquid argon for LEGEND

        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 well-performing technology, they suffer from short emission wavelengths, long scintillation times, and only moderate attenuation lengths. Adding small amounts of xenon can enormously improve the scintillation properties.
        Xenon-doped liquid argon features a higher photo-electron yield, a faster scintillation time profile, and a longer attenuation length than pure liquid argon. In this talk, I will present the current knowledge on xenon-doped liquid argon scintillation, its advantages and disadvantages, and its potential future impact on LEGEND.

        Speaker: Christoph Vogl (TU-Munich)
      • 7
        Intrinsic Resolution Limits in Low-Energy Neutrino Event Reconstruction with IceCube

        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 by collecting Cherenkov photons emitted by secondary charged particles produced as a result of neutrino-nucleon interactions inside the detector. The reconstruction of event information, in particular direction and energy of an incoming neutrino, is a crucial ingredient to the oscillation analyses. The accuracy of reconstruction is therefore affected by statistical fluctuations in the particle shower development as well as by photon propagation and detection efficiencies of sensors. My current research is focussed towards identifying the theoretically achievable resolution in the absence of modeling inaccuracies and computational limitations. The study aims to analyze the factors that limit reconstruction performance, which include algorithmic deficiencies such as minimizer performance and the available information contained in the events.

        Speaker: Kaustav Dutta (Universität Mainz)
      • 8
        Neutrino Decay scenarios on the Cosmic Neutrino Background

        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 neutrino.

        Speaker: Leonardo Ferreira Leite (State University of Campinas (Unicamp) / CERN)
    • 15:00
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • Exercises Auditorium A, B & C (NBI)

      Auditorium A, B & C

      NBI

    • Discussion Auditorium A (NBI)

      Auditorium A

      NBI

    • Reception NBI

      NBI

    • Neutrino Astrophysics & Astronomy Auditorium A (NBI)

      Auditorium A

      NBI

    • 10:30
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • Neutrino Theory & Phenomenology Auditorium A (NBI)

      Auditorium A

      NBI

    • 12:00
      Lunch Auditorium C (NBI)

      Auditorium C

      NBI

    • Topical Seminar Auditorium A (NBI)

      Auditorium A

      NBI

    • Student Talks Auditorium A (NBI)

      Auditorium A

      NBI

      • 12
        Modeling neutrino emission from Active Galactic Nuclei

        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 accelerate cosmic rays and produce neutrinos. The sources are gamma-ray obscured sources, confirming evidence that they should be based on the diffuse extragalactic neutrino flux. In this talk, we present simple dimensional arguments that cosmic neutrinos are produced in AGN within less than 100 Schwarzschild radii from their central black hole.

        Speaker: Ms Arifa Khatee Zathul (University of Wisconsin-Madison)
      • 13
        Studying the physical properties of the engines of neutrino-emitter blazars.

        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 sub-population of neutrino-emitter blazars to study the observational and physical properties that govern the physics of these objects and likely make them capable of accelerating cosmic rays. We will discuss our analysis approach and the general context of the properties displayed by the overall blazar population.

        Speaker: Alessandra Azzollini (Julius-Maximilians Universität Würzburg)
      • 14
        Investigating high-energy neutrinos from blazars with an analysis of the IceCube observatory data

        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 detected by IceCube. A recent study has provided evidence of a statistically significant spatial correlation between blazars from the 5th Roma-BZCat catalog (5BZCat) and the IceCube data. In this contribution, we explore the findings from a complementary approach.

        Speaker: Eleonora Barbano (Julius-Maximilians-Universität Würzburg, Fakultät für Physik und Astronomie, Emil-Fischer-Str. 31, D-97074 Würzburg, Germany)
      • 15
        Jet contribution to the 𝛾-ray Flux in NGC 1068

        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 through hadronic processes in
        the corona of the AGN and the gamma-rays observed by Fermi-LAT can originate from the circumnuclear
        starburst ring.
        In this presentation, the pc-to-kpc scale radio jet of NGC1068 is investigated in terms of its potential gamma-
        ray contribution via hadronic or leptonic processes. Moreover, the radio data provided by VLBA and ALMA
        observations at different distances from the central engine is taken into account. So, it can be clearly shown
        that it is very unlikely that these gamma-rays can be explained by this radio jet.

        Speaker: Silvia Salvatore
    • 15:00
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • Exercises Auditorium A, B & C (NBI)

      Auditorium A, B & C

      NBI

    • Discussion Auditorium A (NBI)

      Auditorium A

      NBI

    • Neutrino Theory & Phenomenology Auditorium A (NBI)

      Auditorium A

      NBI

    • 10:30
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • Neutrino Cosmology Auditorium A (NBI)

      Auditorium A

      NBI

    • 12:00
      Lunch Auditorium C (NBI)

      Auditorium C

      NBI

    • Topical Seminar Auditorium A (NBI)

      Auditorium A

      NBI

    • Student Talks Auditorium A (NBI)

      Auditorium A

      NBI

      • 19
        Multi-messenger observations with the KM3NeT telescope: search for high energy neutrinos coinciding with fast radio bursts

        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 detector), off the coast of Sicily. Identical in the design but differing by scale, these two detectors observe neutrino interactions in the sea water through Cherenkov light produced by the interaction products at different energy ranges. Specifically, ORCA aims at detecting atmospheric neutrinos to study their oscillation parameters, while ARCA will focus at higher energies on astrophysical neutrinos and the characterisation of their sources. Among the latter topic, Fast Radio Bursts (FRB) are good candidates for multi-messenger emissions due to the huge energy involved in their burst. I will present the method and criteria of a multi-messenger analysis intended to search for spatial and temporal coincidences of astrophysical neutrino signals from KM3NeT with a FRB catalogue of around 800 sources among which 14 have been observed in this period, ranging from January 2020 to March 2021, and were visible from the KM3NeT site.

        Speaker: Mr Felix Bretaudeau (on behalf of the KM3NeT Collaboration)
      • 20
        Light dark matter around 100 GeV from the inert doublet model

        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 hypothesis for the existence
        of a scalar dark matter candidate around 100 GeV. This is mostly due to the pull
        towards lower masses by the EWPT constraint. The impact of electroweak precision
        measurements, the dark matter direct detection limits, and the condition for obtain-
        ing a strongly enough first-order EWPT, all have strong dependence, sometimes in
        opposing directions, on the mass splittings between the IDM scalars.

        Speaker: Leila Kalhor (Shahid Beheshti University)
      • 21
        Improving CP Measurement with THEIA and Muon Decay at Rest

        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 $\delta_D$ and not contaminated by the matter effect. With detailed study of neutrino energy reconstruction and backgrounds at the THEIA detector, we find that the combination with the high-energy DUNE can significantly reduce the CP uncertainty, especially around the maximal CP violation cases $\delta_D = \pm 90^\circ$. Both the $\mu$THEIA-25 with 17 kt and $\mu$THEIA-100 with 70 kt fiducial volumes are considered. For DUNE + $\mu$THEIA-100, the CP uncertainty can be better than $8^\circ$.

        Speaker: Chui-Fan Kong (Tsung-Dao Lee Institute)
    • 15:00
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • 15:30
      Free Afternoon
    • 19:00
      School Dinner Food Club / MadKlubben

      Food Club / MadKlubben

      Sortedam Dossering 7C, 2200 Copenhagen
    • Neutrino Cosmology Auditorium A (NBI)

      Auditorium A

      NBI

    • 10:30
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • Neutrino Astrophysics & Astronomy Auditorium A (NBI)

      Auditorium A

      NBI

    • 12:00
      Lunch Auditorium C (NBI)

      Auditorium C

      NBI

    • Topical Seminar Auditorium A (NBI)

      Auditorium A

      NBI

      • 24
        Near-future discovery of point sources of ultra-high-energy neutrinos
        Speaker: Damiano Fiorillo (Niels Bohr Institute, University of Copenhagen)
    • Student Talks Auditorium A (NBI)

      Auditorium A

      NBI

      • 25
        A First Look at Sky Anisotropies of High-Energy Neutrino Flavours

        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 assumption of directionally isotropic flavour ratios in astrophysical neutrino production. Using 7.5 years of IceCube High Energy Starting Events, we model a flavour-dependent spherical harmonic expansion of the neutrino flux and ground our predictions in realistic detector simulations. Further, we forecast the near-future reach of current and upcoming neutrino telescopes to constrain and detect these flavour anisotropies. We discuss the application of these predictions to constrain anisotropy-generating parameters, including those arising from Lorentz invarience violation, as well as flavour-dependant couplings of neutrinos to dark matter.

        Speaker: Bernanda Telalovic (Niels Bohr Institute, University of Copenhagen)
      • 26
        Anomalies in the Radio Neutrino Observatory Greenland

        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 landscape of multi-messenger astronomy. Until now, the data volume of our two initial seasons has remained manageable. However, as the array continues to grow, we need to develop more and more clever processes regarding how to filter our data; we must throw away the noise and identify the most promising events. Data reduction tools become crucial for anthropogenic, environmental and local noise identification/removal in order to test and monitor our instrument as we scale up. We present a convolutional encoder-decoder network that assigns an anomaly ranking to events, helping to classify different categories of background and signal.

        Speaker: Zachary Meyers (DESY Zeuthen)
      • 27
        The Role of Electromagnetic Cascades in High-Energy Neutrino Astrophysics

        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 of the IceCube astrophysical neutrino sources. We also explore the role of muon pair production in producing neutrinos along the development of ultra-high energy cascades, opening a potential window to probe cosmic accelerators at large redshifts.

        Speaker: Antonio Capanema (Pontifícia Universidade Católica do Rio de Janeiro)
      • 28
        Stochastic modelling of cosmic ray sources for diffuse high-energy gamma-rays and neutrinos

        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 processes. Neutrinos, on the other hand, are exclusively produced by the sought-after hadronic processes, yet they can be detected above backgrounds only at hundreds of TeV. Oftentimes, diffuse emission maps are extrapolated from GeV to PeV energies, but the sources contributing at either energies likely differ. We have modelled the production of diffuse emission from GeV through PeV energies in a Monte Carlo approach, taking into consideration the discrete nature of sources. We can generate realisations of the diffuse sky in a matter of seconds, thus allowing for characterising correlations in direction and energy. At hundreds of TeV, relevant for observations with LHAASO, Tibet AS-gamma, IceCube and the upcoming SWGO, variations between different realisations are sizeable. Specifically, we show that extrapolations of diffuse emission from GeV to PeV energies must fail and apply our results on the recent experimental findings.

        Speaker: Anton Stall (Institute for Theoretical Particle Physics and Cosmology (TTK), RWTH Aachen University)
    • 15:00
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • Exercises Auditorium A, B & C (NBI)

      Auditorium A, B & C

      NBI

    • Discussion Auditorium A (NBI)

      Auditorium A

      NBI

    • Neutrino Cosmology Auditorium A (NBI)

      Auditorium A

      NBI

    • 10:30
      Coffee Auditorium C (NBI)

      Auditorium C

      NBI

    • Topical Seminar Auditorium A (NBI)

      Auditorium A

      NBI

      • 30
        Coherent forward scattering of neutrinos

        TBA

        Speaker: Shashank Shalgar (NBIA)
    • 31
      Farewell & Intro of Niels Bohr Archive Auditorium A

      Auditorium A

      Niels Bohr Institute

      Blegdamsvej 17 DK-2100 Copenhagen
    • Guided Tour by Niels Bohr Archive Auditorium A

      Auditorium A

      Niels Bohr Institute

      Blegdamsvej 17 DK-2100 Copenhagen
    • 12:00
      Lunch Auditorium C (NBI)

      Auditorium C

      NBI