International audienceThe study of the gravitational waves opens a new window for the observation of the universe. Completing the observations obtained from electro-magnetic waves, neutrinos and cosmic rays, the gravitational waves will provide informations on the most violent phenomena in the universe, as supernova explosions, collisions of binary systems or mergers of black holes. Their study will thus increase our knowledge in astrophysics, but also in cosmology and fundamental physics. This paper will make a short presentation of the future space interferometer LISA, aiming at detecting gravitational waves, and presents an overview of the R&D developments for LISA at the APC laboratory
LISA (Laser Interferometer Space Antenna) is designed to observe gravitational waves from violent ev...
Gravitational Waves will open an entirely new window to the Universe, different from all other astro...
Abstract. The gravitational wave spectrum covers many decades in frequency. Sources in the audio-fre...
International audienceThe study of the gravitational waves opens a new window for the observation of...
Abstract. The study of the gravitational waves opens a new window for the observation of the uni-ver...
The existence of gravitational waves is the most prominent of Einstein's predictions that has not ye...
This viewgraph presentation reviews the Laser Interferometer Space Antenna (LISA). LISA os a joint E...
The Laser Interferometer Space Antenna (LISA) has been selected as the third large class mission lau...
The Laser Interferometer Space Antenna (LISA) is one of the most ambitious space science missions in...
More than 80 years ago, Einstein has predicted that accelerated masses will emit gravitational waves...
LISA is a joint NASA/ESA space mission for detection and study of low-frequency gravitational waves ...
The European Space Agency has selected LISA, a gravitational wave observatory, as a cornerstone miss...
The parallel session C5 on Space-Based Detectors gave a broad overview over the planned space missio...
In this article, which will appear as a chapter in the Handbook of Gravitational Wave Astronomy, we ...
The gravitational wave spectrum covers many decades in frequency. Sources in the audio-frequency reg...
LISA (Laser Interferometer Space Antenna) is designed to observe gravitational waves from violent ev...
Gravitational Waves will open an entirely new window to the Universe, different from all other astro...
Abstract. The gravitational wave spectrum covers many decades in frequency. Sources in the audio-fre...
International audienceThe study of the gravitational waves opens a new window for the observation of...
Abstract. The study of the gravitational waves opens a new window for the observation of the uni-ver...
The existence of gravitational waves is the most prominent of Einstein's predictions that has not ye...
This viewgraph presentation reviews the Laser Interferometer Space Antenna (LISA). LISA os a joint E...
The Laser Interferometer Space Antenna (LISA) has been selected as the third large class mission lau...
The Laser Interferometer Space Antenna (LISA) is one of the most ambitious space science missions in...
More than 80 years ago, Einstein has predicted that accelerated masses will emit gravitational waves...
LISA is a joint NASA/ESA space mission for detection and study of low-frequency gravitational waves ...
The European Space Agency has selected LISA, a gravitational wave observatory, as a cornerstone miss...
The parallel session C5 on Space-Based Detectors gave a broad overview over the planned space missio...
In this article, which will appear as a chapter in the Handbook of Gravitational Wave Astronomy, we ...
The gravitational wave spectrum covers many decades in frequency. Sources in the audio-frequency reg...
LISA (Laser Interferometer Space Antenna) is designed to observe gravitational waves from violent ev...
Gravitational Waves will open an entirely new window to the Universe, different from all other astro...
Abstract. The gravitational wave spectrum covers many decades in frequency. Sources in the audio-fre...