Nicola Tamanini

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Gravitational wave research at L2IT

The Laboratoire des 2 infinis - Toulouse (L2IT) is a research institute of IN2P3/CNRS established in 2019 with the objective to pursue fundamental research with innovative numerical and theoretical approaches. The research of the institute is focused on particle physics, gravitational waves and the nuclear equation of state, and it is supported by a complementary development of numerical computing, data analysis and data science methodologies.

The gravitational wave group at L2IT conducts research on both theoretical and experimental aspects of gravitational wave science, with a distinct focus at exploiting new ideas connecting theory with observations through data analysis and numerical simulations. The group is part of both the LISA Consortium, the Virgo Collaboration and the Einstein Telescope Consortium, and conducts cutting-edge research on gravitational waves collaborating with external groups and institutes at local, national and international levels.

Current members

The following lists the current members of the gravitational waves group at L2IT. Further information can be found on the L2IT website.

Permanent members

Permanent members contributing from other L2IT groups

Postdocs

PhD students

Interns and students

Past members

Here are the people that were part of the L2IT GW group in the past:

Recent work

Some of the most recent publications and pre-prints authored by members of the group:

  1. C. Liu, D. Laghi and N. Tamanini, Probing modified gravitational-wave propagation with extreme mass-ratio inspirals, Phys. Rev. D 109 (2024) no.6, 063521 [doi:10.1103/PhysRevD.109.063521] [arXiv:2310.12813]

  2. M. Toscani, O. Burke, C. Liu, N. B. Zamel, N. Tamanini and F. Pozzoli, Strongly-Lensed Extreme Mass-ratio Inspirals, Phys. Rev. D 109 (2024) no.6, 063505 [doi:10.1103/PhysRevD.109.063505] [arXiv:2307.06722]

  3. N. Muttoni, D. Laghi, N. Tamanini, S. Marsat and D. Izquierdo-Villalba, Dark siren cosmology with binary black holes in the era of third-generation gravitational wave detectors, Phys. Rev. D 108 (2023) no.4, 043543 [doi:10.1103/PhysRevD.108.043543] [arXiv:2303.10693]