Contact
Name
Position
Email
Address
Office
UCL member card
Per Arne Sevle Myhr
Position
PhD student
Address
Centre for Cosmology, Particle Physics and Phenomenology - CP3
Université catholique de Louvain
2, Chemin du Cyclotron - Box L7.01.05
B-1348 Louvain-la-Neuve
Belgium
Université catholique de Louvain
2, Chemin du Cyclotron - Box L7.01.05
B-1348 Louvain-la-Neuve
Belgium
Office
UCL member card
Projects
Research directions:
Experiments and collaborations:
Active projects
Experiments and collaborations:
Active projects
Multi-messenger studies of astrophysical sources
Giacomo Bruno, Eliot Genton, Karlijn Kruiswijk, Mathieu Lamoureux, Jeff Lazar, Jonathan Mauro, Emile Moyaux, Christoph Raab, Leonardo Ricca, Marco Scarnera, Per Arne Sevle Myhr, Jishnu Suresh, Matthias Vereecken, Gwenhaël Wilberts Dewasseige
This project aims at studying astrophysical phenomena combining different messengers, mainly neutrinos, electromagnetic and gravitational waves.
This project aims at studying astrophysical phenomena combining different messengers, mainly neutrinos, electromagnetic and gravitational waves.
Neutrino physics and astrophysics
Eliot Genton, Karlijn Kruiswijk, Mathieu Lamoureux, Jeff Lazar, Vincent Lemaitre, Emile Moyaux, Christoph Raab, Leonardo Ricca, Marco Scarnera, Per Arne Sevle Myhr, Matthias Vereecken, Gwenhaël Wilberts Dewasseige
This project gathers researchers studying neutrino physics and astrophysics.
This project gathers researchers studying neutrino physics and astrophysics.
Neutrinos from astrophysical transient sources
Eliot Genton, Karlijn Kruiswijk, Mathieu Lamoureux, Jeff Lazar, Jonathan Mauro, Emile Moyaux, Christoph Raab, Leonardo Ricca, Marco Scarnera, Per Arne Sevle Myhr, Matthias Vereecken, Gwenhaël Wilberts Dewasseige
This project aims at optimising neutrino telescopes, especially the IceCube Neutrino Observatory and KM3NeT, to detect GeV and sub-GeV astrophysical neutrinos. The instruments are then used to search for low-energy neutrinos from transient sources, such as solar flares, compact binary mergers, or gamma-ray bursts.
This project aims at optimising neutrino telescopes, especially the IceCube Neutrino Observatory and KM3NeT, to detect GeV and sub-GeV astrophysical neutrinos. The instruments are then used to search for low-energy neutrinos from transient sources, such as solar flares, compact binary mergers, or gamma-ray bursts.
Publications in IRMP
All my publications on Inspire