The Large Observatory for X-ray Timing (LOFT)
M. Feroci, and the LOFT Consortium

TL;DR
LOFT is a proposed ESA mission with a large-area X-ray detector designed to study extreme matter and gravity near black holes and neutron stars, promising groundbreaking insights into fundamental physics.
Contribution
LOFT introduces an innovative large-area Silicon Drift Detector instrument, enabling unprecedented X-ray observations of compact objects in space.
Findings
Effective area of ~12 m^2 in 2-30 keV range
Spectral resolution of <260 eV
Potential to test general relativity near black holes
Abstract
High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultra-dense matter and to black hole masses and spins. A 10 m^2-class instrument in combination with good spectral resolution is required to exploit the relevant diagnostics and answer two of the fundamental questions of the European Space Agency (ESA) Cosmic Vision Theme "Matter under extreme conditions", namely: does matter orbiting close to the event horizon follow the predictions of general relativity? What is the equation of state of matter in neutron stars? The Large Observatory For X-ray Timing (LOFT), selected by ESA as one of the four Cosmic Vision M3 candidate missions to undergo an assessment phase, will revolutionise the study of collapsed objects in our galaxy and of the brightest supermassive black holes in active galactic nuclei. Thanks to…
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