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Gwenhaël de Wasseige

Publications and source records attributed to Gwenhaël de Wasseige.

21 records · Page 2Linked to original sources

A better communicator is always a better scientist, or the reason why every PhD student should engage in science outreach

The ability to communicate with all audiences is a skill that is rapidly becoming a must-have for any future scientist. As more physicists engage in communicating science to non-expert audiences, research shows that this experience helps them to get a better understanding of their own research and the impact on society, improves the perception of science by lay audiences and can also become an area of personal growth as a citizen. A recent deployment of a PhD student to the Amundsen Scott South Pole Station, as part of the IceCube Collaboration, provided a ready opportunity to spark interest. We present results of the efforts made by the Université libre de Bruxelles (ULB), the Vrije Universiteit Brussel (VUB) and the Interuniversity Institute for High Energies, IIHE (ULB-VUB), to introduce Belgian students and citizens to science and the life of a scientist. The essential parts of this program will be identified to show why the contributions of a PhD student to the organization of these activities are beneficial to the development of new skills as a scientist, but also to broaden the audiences and the impact of the local university and/or the specific research outreach program.

physics.ed-ph↗

Implications of GW related searches for IceCube

At the beginning of 2016, LIGO reported the first-ever direct detection of gravitational waves. The measured signal was compatible with the merger of two black holes of about 30 solar masses, releasing about 3 solar masses of energy in gravitational waves. We consider the possible neutrino emission from a binary black hole merger relative to the energy released in gravitational waves and investigate the constraints coming from the non-detection of counterpart neutrinos, focusing on IceCube and its energy range. The information from searches for counterpart neutrinos is combined with the diffuse astrophysical neutrino flux in order to put bounds on neutrino emission from binary black hole mergers. Prospects for future LIGO observation runs are shown and compared with model predictions.

astro-ph.HE↗

Constraints and prospects on GW and neutrino emissions using GW150914

Recently, the LIGO observatory reported the first direct observation of gravitational waves, with a signal consistent with a binary black hole merger. This detection triggered several follow-up searches for coincident emission in electromagnetic waves as well as neutrinos, but no such emission was found. In this article, the implications of the non-detection of counterpart neutrinos are investigated using general arguments. The results are interpreted with a parameter denoting the energy emitted in neutrinos relative to the energy emitted in gravitational waves. The bound on this parameter from the diffuse astrophysical neutrino flux detected by the IceCube Neutrino Observatory is discussed. It is found that, currently, the non-detection of counterpart neutrinos puts a bound comparable to the one from the diffuse astrophysical neutrino flux. This bound is then used to constrain the amount of matter in the black hole binary environment. Finally, the sensitivity to this parameter in future gravitational wave observation runs is investigated. It is shown how the detection of one or more neutrinos from a single merger would strongly constrain the source population and evolution.

astro-ph.HE↗