Name: N-pact meeting 2025
Start: 2025-06-19T01:30:00+02:00
End: 2025-06-20T13:00:00+02:00
Location: No location set

N-pact meeting 2025

from Thursday 19 June 2025 (01:30) to Friday 20 June 2025 (13:00)

Monday 16 June 2025
Tuesday 17 June 2025
Wednesday 18 June 2025
Thursday 19 June 2025
08:50
08:50 - 09:00
Contributions

08:50 Welcome - Jens Oluf Andersen
09:00
09:00 - 10:30
Contributions

09:00 Compact Stars with the Quark-Meson Model - Carl Fredrik Andresen (University of Oslo)

09:30 Color superconductivity and non-strange hybrid stars - Mathias Pavely Nødtvedt (Norwegian University of Science and Technology (NTNU))

10:00 Dark pions at next-to-leading order - Daniil Krichevskiy (University of Stavanger)
10:30 Coffee break
Coffee break
10:30 - 11:00
11:00
11:00 - 12:30
Contributions

11:00 Curious case of the maximum energy distribution of cosmic-ray accelerators - Domenik Ehlert (Norwegian University of Science and Technology)

11:30 Effective field theory dualities from the classical equations of motion - Tomas Brauner (University of Stavanger)

12:00 PT2GWFinder: a Handy Tool for Cosmological Phase Transitions and Gravitational Waves - Marco Finetti (Aveiro University)
12:30 Lunch
Lunch
12:30 - 13:30
13:30
13:30 - 14:30
Contributions

13:30 Modeling Gravitational Waves via Post-Newtonian Expansion and Geometric Optics - Kristine de Boer

14:00 Update of gravitational waves - Alex Nielsen (University of Stavanger)
14:30 Coffee break
Coffee break
14:30 - 15:00

15:00 Future of N-pact
Future of N-pact
15:00 - 16:30
Friday 20 June 2025
09:00
09:00 - 10:30
Contributions

09:00 Blazars as a potential source of very-high-energy astrophysical neutrinos - Egor Podlesnyi (Norwegian University of Science and Technology (NTNU))

09:30 The SIMP and the vector meson - Halvor Melkild (University of Oslo)

10:00 CFTs at large Charge Sector and Heavy Ion collisions - Narcis Mestre (Bergen)
10:30 Coffee break
Coffee break
10:30 - 11:00
11:00
11:00 - 12:00
Contributions

11:00 Higgs mediated Neutralino pair production in the Next-to-Minimal Supersymmetric Standard model - Sofiya Sianiuta (Norwegian University of Science and Technology)

11:30 Interactions of accelerated dark matter with nuclei and implications for DUNE - Helena Kolešová (University of Stavanger)
12:00 Farewell
Farewell
12:00 - 12:10

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