LISA Pathfinder tracera la voie vers la mission eLISA en testant, dans l’espace, le concept (les principes ?) de la détection d’ondes gravitationnelles.

L'endroit le plus silencieux du système solaire

LISA Pathfinder (LPF) placera deux masses d’épreuve en "chute libre" quasi parfaite, contrôlera et mesurera leur mouvement relatif avec une précision inégalée. Ceci sera effectué grâce à des thechnologies innovantes telles que des senseurs inertiels, un système de métrologie laser, un système à compensation de trainée et des micro-propulseurs délivrant des micro-Newton. L’ensemble de ces masses d’épreuve et leur environnement constitueront probablement un des endroits les plus "calmes" du système solaire.

Toutes ces technologies sont non seulement essentielles pour la mission eLISA, elles seront également à la base de toutes les missions qui voudront tester la théorie de la relativitié générale d’Einstein.

LPF sera lancé en novembre 2015.

The LISA Consortium

The LISA Consortium is committed to supporting the LISA mission. It includes all the main investigators involved in the highly successful LISA Pathfinder mission, a number of scientists who worked on the ground-based LIGO, Virgo, and GEO projects, and a number who worked on the Laser Ranging Interferometer on the GRACE Follow-On mission, thus making full use of the expertise accumulated so far. The LISA Consortium proposed and submitted the white paper The Gravitational Universe which was accepted for the ESA L3 slot.

If you are a scientist and wish to contribute to the LISA mission, use this scientist registration form.

Latest news and consortium activities

Date Title Summary
May 23, 2013
ESA’s next large mission: LISA white paper submitted We have come remarkably far using light of different spectrums as our tool for observing...
May 20, 2013
LPF scheduled for launch in 2015 The LISA consortium strongly supports ESA's LISA Pathfinder (LPF) mission, whose launch...
Apr 07, 2013
Ready for launch: Heart of LISA Pathfinder space mission tested successfully The optical bench of the LISA Pathfinder (LPF) mission is currently being extensively...
Jun 25, 2013
Latest LISA Pathfinder hardware delivery is 'Jewel in the Crown' A team of scientists from the University of Glasgow has successfully delivered a...
Aug 29, 2013
LISA Pathfinder: from CAD models to ready-to-fly hardware Optical bench integrated into the core assembly LISA Pathfinder space mission reached...

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Conferences, publications and positions

Date News topicsort descending Image Title
Jun 19, 2020
Positions PhD position in experimental Gravitational Wave research at University of Twente/Nikhef, The Netherlands
Sep 13, 2019
Positions PhD or Masters by Research positions – University of Western Australia, Perth, Australia
Jul 08, 2020
Positions PhD student position on instrument research for a third generation gravitational wave detector at University of Hamburg, Germany
Jul 08, 2020
Positions PhD student position "LISA interferometry - experiment for ground-support equipment and noise limitations" at University of Hamburg, Germany
Jul 08, 2020
Positions Postdoc position "LISA phase readout" at University of Hamburg, Germany
Jul 08, 2020
Positions 3-year PhD position at University of the Balearic Islands, Spain
Aug 07, 2020
Positions Postdoctoral fellowship in Astronomy, Cosmology and Particle Physics at University of Stavanger
Oct 11, 2016
Papers Distinguishing between formation channels for binary black holes with LISA
Papers Perturbation method in the assessment of radiation reaction in the capture of stars by black holes
Apr 30, 2009
Papers Assembly of Supermassive Black Holes at High Redshifts
Mar 21, 2017
Papers Reconstructing the dark sector interaction with LISA
Dec 11, 2004
Papers Brans-Dicke gravity and the capture of stars by black holes: some asymptotic results
Sep 30, 2012
Papers X-ray emission from high-redshift miniquasars: self-regulating the population of massive black holes through global warming
Feb 02, 2012
Papers Low-frequency gravitational wave science with LISA
Mar 28, 2017
Papers Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals

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