Descripción del proyecto
Las predicciones teóricas de alta precisión son fundamentales para la investigación de las ondas gravitatorias
La observación de las ondas gravitatorias por parte de LIGO/VIRGO puso en marcha una nueva era para la astronomía. La posibilidad de realizar descubrimientos en este incipiente campo depende de la capacidad de llevar a cabo predicciones teóricas precisas que estén basadas en el análisis de datos y la interpretación de señales. El objetivo del proyecto LHCtoLISA, financiado con fondos europeos, es ensanchar los límites del conocimiento analítico en la dinámica gravitatoria mediante el marco de la «teoría de campo efectivo». El nuevo formalismo recientemente desarrollado por el proyecto ha sido esencial para la construcción del banco modelo de última generación. Los cálculos de alta precisión que llevará a cabo el proyecto podrían tener grandes implicaciones, desde demostrar la materia que interactúa fuertemente hasta permitir el descubrimiento de objetos compactos exóticos y partículas ultraligeras putativas en la naturaleza.
Objetivo
The nascent field of gravitational wave (GW) science will be an interdisciplinary subject, enriching different branches of physics, yet the associated computational challenges are enormous. Faithful theoretical templates are a compulsory ingredient for successful data analysis and reliable physical interpretation of the signals. This is critical, for instance, to study the equation of state of neutron stars, the nature of black holes, and binary formation channels. However, while current templates for compact binary sources may be sufficient for detection and crude parameter estimation, they are too coarse for precision physics with GW data. We then find ourselves in a situation in which, for key processes within empirical reach, theoretical uncertainties may dominate. To move forward, profiting the most from GW observations, more accurate waveforms will be needed.
I have played a pioneering role in the development and implementation of a new formalism, known as the ‘effective field theory approach’, which has been instrumental for the construction of the state-of-the-art GW template bank. The goal of my proposal is thus to redefine the frontiers of analytic understanding in gravity through the effective field theory framework. Even more ambitiously, to go beyond the current computational paradigm with powerful tools which have been crucial for `new-physics' searches at the Large Hadron Collider.
The impact of the high-accuracy calculations I propose to undertake will be immense: from probes of dynamical spacetime and strongly interacting matter, to the potential to discover exotic compact objects and ultra-light particles in nature. Furthermore, GW observations scan gravity in a regime which is otherwise unexplored. Consequently, the coming decade will tell whether Einstein's theory withstands precision scrutiny. In summary, my program will provide novel techniques and key results that will enable foundational investigations in physics through GW precision data.
Ámbito científico
- natural sciencescomputer and information sciencesdata science
- natural sciencesphysical sciencestheoretical physicsparticle physicsparticle accelerator
- natural sciencesphysical sciencesastronomyobservational astronomygravitational waves
- natural sciencesphysical sciencesastronomystellar astronomyneutron stars
- natural sciencesphysical sciencesastronomyastrophysicsblack holes
Palabras clave
Programa(s)
Régimen de financiación
ERC-COG - Consolidator GrantInstitución de acogida
22607 Hamburg
Alemania