Gravity waves theory


Observations by gravitational-wave observatories will provide very valuable information regarding different astrophysical and cosmological sources. 


We focus on five large areas of research:

- LISA PATHFINDER Scientific Operations: The LISA Pathfinder mission of the European
Space Agency is demonstrating the technology to set up two test masses in space in a state of free-fall motion without precedents and compatible with the needs of a future space-based gravitational-wave observatory.  The institute has been working in the design of experiments for LISA Pathfinder, the development of data analysis tools and pipelines, and in the scientific exploitation of the mission.

- Astrophysics and Cosmology of gravitational wave sources:  The study of physical mechanisms both at astrophysical and cosmological scales that can lead to the formation of sources of gravitational waves in any of the bands of interest (high, low and very low).  The idea is to understand the rate at which different types of sources form in the Universe and to understand the distribution of physical parameters (masses, spins, orbital parameters, distance, etc.).

- Simulations of sources of gravitational waves: One the main topics in Gravitational Wave Astronomy is to produce a template bank of gravitational wave signals (waveforms) to be used in the data analysis. This is a crucial point and requires the use and development of techniques in Numerical Relativity (the solution of Einstein's field equations by means of supercomputers) and in Perturbative Relativity (the solution of Einstein's field equations using different types of approximation schemes).

- Fundamental physics with gravitational waves: One of the Holy Grails in Gravitational Wave Astronomy is to use gravitational wave detections of the coalescence of (supermassive) black holes and of extreme-mass-ratio inspirals to study different questions with impact in Fundamental Physics.  Those questions include: Tests of the Einstein Equivalence Principle; tests of the geometry of black holes, in particular of the no-hair conjecture that states that astrophysical black holes should be described by the Kerr solution of General Relativity (and hence described by two numbers: mass and spin); tests of the General Relativity theory and other alternative theories of gravity.

- Algorithms for gravitational waves data analysis: In constrast with other areas of Astronomy, the storage of the data of Gravitational Wave detectors does not present a challenge to the current available resources.  However, the processing of this data in order to detect and characterize gravitational-wave sources by means of data analysis techniques that use match filtering techniques constitutes a big challenge.  The computational cost for the most complex sources (in terms of the dimensionality of their parameter space) is so big that make necessary the development of smart algorithms for the search of sources and the estimation of their physical parameters.

Senior Institute members involved

C. Sopuerta, P. Amaro
Institute of Space Sciences (IEEC-CSIC)

Campus UAB, Carrer de Can Magrans, s/n
08193 Barcelona.
Phone: +34 93 737 9788
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An institute of the Consejo Superior de Investigaciones Científicas

An institute of the Consejo Superior de Investigaciones Científicas
Affiliated with the Institut d'Estudis Espacials de Catalunya

Affiliated with the Institut d'Estudis Espacials de Catalunya