Login

4th Annual Niels Bohr Institute MSc. Student Symposium

14 March 2025
H.C. Ørsted Institute
Europe/Copenhagen timezone
Abstract submission and Registration is now CLOSED! But you can always sneakpeek...

Session

Presentations

14 Mar 2025, 13:00
Auditorium 3 & Hall (H.C. Ørsted Institute)

Auditorium 3 & Hall

H.C. Ørsted Institute

Universitetsparken 5 2100 København Ø

Conveners

Presentations

  • Thea Guntofte

Presentations

  • Jens Milan Nielsen

Presentation materials

There are no materials yet.

  1. 28. Gravitational waves lensing by the strong field of a black hole
    Matilde Garcia (Center of Gravity - Niels Bohr Institute)
    14/03/2025, 13:00
    Presentation
  2. 29. Effects of non-linear excitation on the propagation of light
    Deniz Adigüzel
    14/03/2025, 13:20
    Presentation
  3. 30. Exploring nematic behaviour in systems with polar symmetry
    Niels de Graaf Sousa
    14/03/2025, 13:40
  4. 31. Quantifying the Reduction in Carbon Footprint of Physics-Informed Machine Learning in the Pursuit of Greener Artificial Intelligence Practices
    Sophia Wilson (Niels Bohr Institute)
    14/03/2025, 14:00
  5. 32. Construction of Fault Tolerant Interfaces for Topological Quantum Error Correcting Codes
    Max Emil K.S. Sondergaard (University of Copenhagen)
    14/03/2025, 14:45
    Presentation
  6. 33. Neutron Star properties through Collider experiments
    Andreas Vitsos (University of Copenhagen)
    14/03/2025, 15:05
    Presentation
  7. 34. Diatoms - A novel sea-ice proxy
    Johanna-Sophia Köberl
    14/03/2025, 15:25
    Presentation
  8. 35. Modelling bursty star formation in high redshift galaxies
    Elie Cueto (University of Copenhagen, Niels Bohr Institute)
    14/03/2025, 15:45
  9. 8. Effects of non-linear excitation on the propagation of light
    Presentation

    With the increasing number of nuclear-resonant photons per pulse at x-ray free electron lasers (XFELs), achieving higher excitation levels experimentally becomes feasible. This development makes it particularly compelling to investigate light propagation and dynamics beyond the low-excitation regime (LER) and around population inversion. Thus, in my thesis, we examined the time response of...

    Go to contribution page
  10. 3. Exploring nematic behaviour in systems with polar symmetry.
    Presentation

    Active matter encompasses a wide range of systems, from bird-flocks to bacterial colonies. Two main formalisms describe these systems based on individual particle symmetries: polar and nematic. Each formalism leads to unique behaviours, the most significant being the appearance of half and full integer topological defects for nematic and polar respectively. However, recent advances in the...

    Go to contribution page
  11. 9. Gravitational waves lensing by the strong field of a black hole
    Presentation

    The first detection of gravitational waves (GWs) in 2015 opened the door to GW physics, which has allowed us to test Gravity with unprecedented precision.

    When emitted by a source, usually a merging binary of compact objects such as black holes (BHs), gravitational waves propagate moslty unaltered through the cosmos. However, if they encounter objects in their path that are massive/compact...

    Go to contribution page
  12. 1. Quantifying the Reduction in Carbon Footprint of Physics-Informed Machine Learning in the Pursuit of Greener Artificial Intelligence Practices
    Presentation

    This thesis explores the potential reduction in the carbon footprint of machine learning (ML) models by integrating physical constraints into their design. Traditional ML models rely on large datasets and extensive parameter optimization, leading to significant computational costs and associated carbon dioxide (CO₂) emissions. However, by adopting a physics-informed approach, it may be...

    Go to contribution page
Building timetable...