Cosmo: Wednesday, 14/01/2026, 11:30, Lecture Hall
Herman Sletmoen (University of Oslo, Oslo, Norway)
SymBoltz.jl: A symbolic-numeric, approximation-free and differentiable Einstein-Boltzmann code
SymBoltz (available at
https://github.com/hersle/SymBoltz.jl) is a new Julia package that solves the linear Einstein-Boltzmann equations. It features a symbolic-numeric interface for specifying equations, is free of approximation switching schemes and is compatible with automatic differentiation. Cosmological models are built from replaceable physical components in a way that scales well in model space, or alternatively written as one compact system of equations. The modeler should simply write down their equations, and SymBoltz solves them and eliminates friction in the modeling process. Symbolic knowledge enables powerful automation of tasks, such as separating computational stages like the background and perturbations, generating the analytical Jacobian matrix and its sparsity pattern, and interpolating arbitrary variables from the solution. Implicit solvers integrate the full stiff equations at all times without approximations, which greatly simplifies the code. Performance remains as good as in existing approximation-based codes due to high-order implicit methods that take long time steps, fast generated code, optimal handling of the Jacobian and efficient sparse matrix methods. Automatic differentiation gives exact derivatives of any output with respect to any input, which is important for gradient-based Markov chain Monte Carlo methods in large parameter spaces, training of emulators, Fisher forecasting and sensitivity analysis. I will present the design of the code, show some example use and highlight its current state and possible future work.
String: Friday, 16/01/2026, 14:00, seminar room 226
Petr HoĊava (University of California Berkeley, USA)
Topological Untwist in Quantum Gravity of the Ricci Flow
In recent years, a topological quantum gravity associated with nonrelativistic Ricci flow has been formulated. The path integral of this theory is localized to the flow equations formulated by Perelman to prove the Poincare conjecture. As a theory of the cohomological BRST type, this theory has no propagating gravitons. However, we show that the BRST symmetry can be ''untwisted'', much like in the similar case of the relativistic Yang-Mills gauge theories. After this untwist, the theory becomes a physical nonrelativistic quantum supergravity with propagating degrees of freedom and with positive-definite energy. The relation between the topological theory and its physical counterpart is much closer than in the Yang-Mills case, but several intriguing subtleties still separate the topological and physical phase of this system.
Cosmo: Wednesday, 21/01/2026, 11:30, Lecture Hall
Josu Aurrekoetxea (MIT, Cambridge, USA)
Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
Light scalar particles arise naturally in many extensions of the Standard Model and are compelling dark matter candidates. Gravitational interactions near black holes can trigger the growth of dense scalar configurations that, if sustained during inspiral, alter binary dynamics and imprint signatures on gravitational-wave signals. In this talk I will describe the use of numerical relativity simulations to develop a semi-analytic waveform model for black hole binaries in scalar environments, which we apply it in a Bayesian analysis of the LIGO–Virgo–KAGRA catalog. For GW190728 and GW190814, vacuum lies outside the 95% credible region. When including superradiance priors, GW190728 shows tentative evidence for a scalar environment with a Bayes factor of ln B \approx 3.5, consistent with a light scalar of mass 1e-12 eV.
Cosmo: Wednesday, 28/01/2026, 11:30, Lecture Hall
Nicolas Loayza Romero (CEICO, Prague, Czech Republic)
TBA
Cosmo: Wednesday, 04/02/2026, 11:30, Lecture Hall
Pietro Ghedini (IFIC, Valencia, Spain)
TBA
Cosmo: Wednesday, 11/02/2026, 11:30, Lecture Hall
Jorge Baeza-Ballesteros (DESY, Zeuthen, Germany)
TBA
Cosmo: Wednesday, 18/02/2026, 11:30, Lecture Hall
Manuel Del Piano (University of Southern Denmark, Odense, Denmark)
TBA
Cosmo: Wednesday, 25/02/2026, 11:30, Lecture Hall
Vitor da Fonseca (University of Lisbona, Lisbona, Portugal)
TBA
Cosmo: Wednesday, 04/03/2026, 11:30, Lecture Hall
Alexandros Papageorgiou (IFT, Madrid, Spain)
TBA
Cosmo: Wednesday, 11/03/2026, 11:30, Lecture Hall
Tays Miranda (Espirito Santo University, Brazil)
TBA
Cosmo: Wednesday, 18/03/2026, 11:30, Lecture Hall
Alberto Mangiagli (MPI, Potsdam, Germany)
TBA
Cosmo: Wednesday, 25/03/2026, 11:30, Lecture Hall
Carlos Herdeiro (Aveiro University, Aveiro, Portugal)
TBA
Cosmo: Wednesday, 01/04/2026, 11:30, Lecture Hall
Alessandra Silvestri (Leiden University, Leiden, Netherlands)
TBA
Cosmo: Wednesday, 08/04/2026, 11:30, Lecture Hall
Théo Simon (LUPM, Montpellier, France)
TBA
Cosmo: Wednesday, 15/04/2026, 11:30, Lecture Hall
Gabriella De Lucia (Trieste Observatory, Trieste, Italy)
TBA
Cosmo: Wednesday, 22/04/2026, 11:30, Lecture Hall
Clare Burrage (Nottingham University, Nottingham, UK)
TBA
Cosmo: Wednesday, 29/04/2026, 11:30, Lecture Hall
Gerasimos Rigopoulos (Newcastle University, Newcastle upon Tyne, UK)
TBA
Cosmo: Wednesday, 06/05/2026, 11:30, Lecture Hall
Laur Jarv (Tartu University, Tartu, Estonia)
TBA
Cosmo: Wednesday, 13/05/2026, 11:30, Lecture Hall
Jerôme Martin (IAP, Paris, France)
TBA