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Emploi
Postdoctoral position: "Gravitational waves and compact objects" - IP2I (UMR 5822)
CDD - 2 ansVilleurbanne, France
Date limite de réponse : 15 février 2021
Missions :
Research project
Since the discovery of gravitational waves (GWs) in 2015, LIGO and Virgo have observed numerous gravitational wave signals originating from the mergers of compact objects such as black holes or neutron stars. In addition to this wonderful discovery, which confirms a 100-year old prediction of general relativity, the observations of gravitational waves offer new ways to observe the Universe in absence of, or in a complementary way to, electromagnetic counterparts, together with the possibility to test general relativity. In particular the LIGO/Virgo experimental program is an ambitious way to better understand our Universe by detecting the extremely faint GW emitted by compact objects.
At IP2I, two groups have recently emerged in the context of gravitational waves: a theory group, which simulates mergers of binary black holes and neutron stars in order to find constraints on black hole and neutron star models; an experimental Virgo group, which contributes to the analysis of the LIGO/Virgo data in particular for the search and characterization of signals emitted by the coalescences and mergers of black holes and neutron stars. Both groups interact in order to interpret the experimental data, and they currently work on the possibility to clearly disentangle gravitational waves emitted by light primordial black hole mergers from the ones emitted by neutron star mergers.
The combination of experimental and theoretical expertise is a strong IP2I asset which will allow the postdoc to make an original contribution to the determination of the properties of astrophysical objects, strengthening the Lyon (and in general French) commitment to the GW community. A better determination of the parameters will have a significant impact on the results of the LIGO/Virgo publications on the data available and for those collected in the next data-taking period, scheduled for the end of 2021. For such an ambitious project, the recruited postdoctoral researcher is expected to have an expertise on gravitational waves, on numerical simulations of compact object mergers and on high performance computing.
Since the discovery of gravitational waves (GWs) in 2015, LIGO and Virgo have observed numerous gravitational wave signals originating from the mergers of compact objects such as black holes or neutron stars. In addition to this wonderful discovery, which confirms a 100-year old prediction of general relativity, the observations of gravitational waves offer new ways to observe the Universe in absence of, or in a complementary way to, electromagnetic counterparts, together with the possibility to test general relativity. In particular the LIGO/Virgo experimental program is an ambitious way to better understand our Universe by detecting the extremely faint GW emitted by compact objects.
At IP2I, two groups have recently emerged in the context of gravitational waves: a theory group, which simulates mergers of binary black holes and neutron stars in order to find constraints on black hole and neutron star models; an experimental Virgo group, which contributes to the analysis of the LIGO/Virgo data in particular for the search and characterization of signals emitted by the coalescences and mergers of black holes and neutron stars. Both groups interact in order to interpret the experimental data, and they currently work on the possibility to clearly disentangle gravitational waves emitted by light primordial black hole mergers from the ones emitted by neutron star mergers.
The combination of experimental and theoretical expertise is a strong IP2I asset which will allow the postdoc to make an original contribution to the determination of the properties of astrophysical objects, strengthening the Lyon (and in general French) commitment to the GW community. A better determination of the parameters will have a significant impact on the results of the LIGO/Virgo publications on the data available and for those collected in the next data-taking period, scheduled for the end of 2021. For such an ambitious project, the recruited postdoctoral researcher is expected to have an expertise on gravitational waves, on numerical simulations of compact object mergers and on high performance computing.
Starting date of the contract: September the 1st, 2021
PROFIL RECHERCHÉ
Formations requises :
PhD in physics or astrophysics
Compétences requises :
The ideal candidate must hold a PhD in physics or astrophysics (to be defended before December 1st, 2021).
She/He is expected to have knowledge on common programming languages such as Python or C++, and skills on Bayesian inference and HPC environments, and optionally knowledge about the “Einstein Toolkit” general relativity code.
The candidate should have experience in numerical general relativity and in analysis of data from gravitational wave interferometers.
She/He is expected to have knowledge on common programming languages such as Python or C++, and skills on Bayesian inference and HPC environments, and optionally knowledge about the “Einstein Toolkit” general relativity code.
The candidate should have experience in numerical general relativity and in analysis of data from gravitational wave interferometers.
Renseignements pratiques
Informations sur l'organisme
IP2I (UMR 5822)
Adresse : IP2I, 4 rue Enrico Fermi
Villeurbanne, France
Villeurbanne, France
Job location and description
The recruited postdoctoral researcher will work at IP2I, Lyon, France.
She/he will join the theory group, and perform in HPC environments numerical simulations of compact object mergers, in particular of binary black holes, of binary neutron stars and of binaries composed of one black hole and one neutron star. For neutron star physics, she/he will be helped by the local expertise in the theory group, which will provide nuclear equations of state in a format readable by the numerical simulations.
She/he will also join the Virgo Collaboration, where she/he will participate to the analysis of merger signals and to the generation of catalogs of templates to interpret the results. Within the LIGO/Virgo collaboration, a handful of independent analyses (among which, the one developed at IP2I) are used in order to probe the interferometers' data collected during the O3 run (April 2019 - March 2020). The aim of these analyses is to detect gravitational wave signals from the coalescences of compact objects. The results of such detections are then studied by a dedicated working group (called Parameter Estimation), to obtain the best possible determination of the properties of the astrophysical objects which have generated the signals. Dozens of new events have been recorded by LIGO/Virgo interferometers. These data are currently under study and will be the subject of several publications in 2021. The project that the postdoctoral researcher will have to pursue will imply an involvement in the Parameter Estimation working group and will help the IP2I Virgo group to gain visibility on new research subjects in the collaboration.
The recruited postdoctoral researcher will work at IP2I, Lyon, France.
She/he will join the theory group, and perform in HPC environments numerical simulations of compact object mergers, in particular of binary black holes, of binary neutron stars and of binaries composed of one black hole and one neutron star. For neutron star physics, she/he will be helped by the local expertise in the theory group, which will provide nuclear equations of state in a format readable by the numerical simulations.
She/he will also join the Virgo Collaboration, where she/he will participate to the analysis of merger signals and to the generation of catalogs of templates to interpret the results. Within the LIGO/Virgo collaboration, a handful of independent analyses (among which, the one developed at IP2I) are used in order to probe the interferometers' data collected during the O3 run (April 2019 - March 2020). The aim of these analyses is to detect gravitational wave signals from the coalescences of compact objects. The results of such detections are then studied by a dedicated working group (called Parameter Estimation), to obtain the best possible determination of the properties of the astrophysical objects which have generated the signals. Dozens of new events have been recorded by LIGO/Virgo interferometers. These data are currently under study and will be the subject of several publications in 2021. The project that the postdoctoral researcher will have to pursue will imply an involvement in the Parameter Estimation working group and will help the IP2I Virgo group to gain visibility on new research subjects in the collaboration.