1. GLINT
- Author
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Aria, Shafa, Azevedo, Rui, Burow, Rick, Cahill, Fiachra, Ducheckova, Lada, Holroyd, Alexa, Huarcaya, Victor, Järvelä, Emilia, Koßagk, Martin, Moeckel, Chris, Rodriguez-Aramendia, Ana, Royer, Fabien, Sypniewski, Richard, Vittori, Edoardo, Yttergren, Madeleine, University of Oslo, University of Porto, University of Bremen, Maynooth University, Czech Technical University in Prague, University of Bristol, National University of Singapore, Metsähovi Radio Observatory, Technische Universität Dresden, Delft University of Technology, University of Vienna, Institut supérieur de l'aéronautique et de l'espace, FOTEC Forschungs- und Technologietransfer GmbH, Imperial College London, Chalmers University of Technology, Aalto-yliopisto, and Aalto University
- Subjects
General Relativity and Quantum Cosmology ,Supermassive black holes ,Laser interferometry ,Gravitational waves - Abstract
When the universe was roughly one billion years old, supermassive black holes (103-106 solar masses) already existed. The occurrence of supermassive black holes on such short time scales are poorly understood in terms of their physical or evolutionary processes. Our current understanding is limited by the lack of observational data due the limits of electromagnetic radiation. Gravitational waves as predicted by the theory of general relativity have provided us with the means to probe deeper into the history of the universe. During the ESA Alpach Summer School of 2015, a group of science and engineering students devised GLINT (Gravitational-wave Laser INterferometry Triangle), a space mission concept capable of measuring gravitational waves emitted by black holes that have formed at the early periods after the big bang. Morespecifically at redshifts of 15 < z < 30(∼ 0.1 − 0.3× 109 years after the big bang) in the frequency range 0.01 − 1 Hz. GLINT design strain sensitivity of (Formula presented.) will theoretically allow the study of early black holes formations as well as merging events and collapses. The laser interferometry, the technology used for measuring gravitational waves, monitors the separation of test masses in free-fall, where a change of separation indicates the passage of a gravitational wave. The test masses will be shielded from disturbing forces in a constellation of three geocentric orbiting satellites.
- Published
- 2017