A5046326779- Pulsars and Gravitational Waves Research
- Gamma-ray bursts and supernovae
- Cosmology and Gravitation Theories
- High-pressure geophysics and materials
- Astrophysical Phenomena and Observations
- Atomic and Subatomic Physics Research
- Geophysics and Gravity Measurements
- Magnetic confinement fusion research
- Seismic Waves and Analysis
- Radio Astronomy Observations and Technology
- Astrophysics and Cosmic Phenomena
- Superconducting Materials and Applications
- Seismology and Earthquake Studies
- Meteorological Phenomena and Simulations
- Experimental and Theoretical Physics Studies
- Radiology practices and education
- Dark Matter and Cosmic Phenomena
- Statistical Mechanics and Entropy
- Black Holes and Theoretical Physics
- earthquake and tectonic studies
- Geophysics and Sensor Technology
UCLouvain
2021-2024
Université Paris Cité
2023
Laboratoire AstroParticule et Cosmologie
2023
Centre National de la Recherche Scientifique
2023
We adapt a method, originally developed for searches quasimonochromatic, quasi-infinite duration gravitational-wave signals, to directly detect new light gauge bosons with laser interferometers, which could be candidates dark matter. To search these particles, we optimally choose the analysis coherence time as function of boson mass, such that all signal power will confined one frequency bin. focus on photon, couple baryon or baryon-lepton number, and explain its interactions interferometers...
A stochastic gravitational-wave background (SGWB) is expected to be produced by the superposition of individually undetectable, unresolved (GW) signals from cosmological and astrophysical sources. Such a signal can searched with dedicated techniques using data acquired network ground-based GW detectors. In this work, we consider SGWB resulting pulsar glitches, which are sudden increases in rotational frequency, within our Galaxy. More specifically, assume glitches associated quantized,...
A stochastic gravitational-wave background (SGWB) is expected to be produced by the superposition of individually undetectable, unresolved (GW) signals from cosmological and astrophysical sources. Such a signal can searched with dedicated techniques using data acquired network ground-based GW detectors. In this work, we consider SGWB resulting pulsar glitches, which are sudden increases in rotational frequency, within our Galaxy. More specifically, assume glitches associated quantized,...