The Gravitational Universe
The eLISA Consortium: P. Amaro Seoane, S. Aoudia, H. Audley, G. Auger,, S. Babak, J. Baker, E. Barausse, S. Barke, M. Bassan, V. Beckmann, M., Benacquista, P. L. Bender, E. Berti, P. Bin\'etruy, J. Bogenstahl, C. Bonvin,, D. Bortoluzzi, N. C. Brause, J. Brossard, S. Buchman

TL;DR
The paper discusses the potential of gravitational wave astronomy, enabled by the eLISA mission, to revolutionize our understanding of the Universe by observing phenomena inaccessible to electromagnetic observations.
Contribution
It introduces the eLISA mission as the first to study the Universe through gravitational waves, highlighting its capabilities to explore black holes, early universe, and fundamental physics.
Findings
eLISA will detect gravitational waves from black hole mergers.
It will observe the early Universe at redshifts up to z ~ 20.
The mission will test deviations from General Relativity.
Abstract
The last century has seen enormous progress in our understanding of the Universe. We know the life cycles of stars, the structure of galaxies, the remnants of the big bang, and have a general understanding of how the Universe evolved. We have come remarkably far using electromagnetic radiation as our tool for observing the Universe. However, gravity is the engine behind many of the processes in the Universe, and much of its action is dark. Opening a gravitational window on the Universe will let us go further than any alternative. Gravity has its own messenger: Gravitational waves, ripples in the fabric of spacetime. They travel essentially undisturbed and let us peer deep into the formation of the first seed black holes, exploring redshifts as large as z ~ 20, prior to the epoch of cosmic re-ionisation. Exquisite and unprecedented measurements of black hole masses and spins will make it…
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Taxonomy
TopicsComputational Physics and Python Applications
