Gravitational waves astronomy: the ultimate test for Einstein's General Relativity
Christian Corda

TL;DR
This review discusses how advanced gravitational wave detection could test Einstein's General Relativity's validity and explore alternative theories of gravity through improved interferometer response analysis.
Contribution
It highlights the potential of future gravitational wave astronomy to critically evaluate Einstein's GR against extended gravity theories using detailed interferometer response functions.
Findings
Enhanced GW detection sensitivity can test GR's predictions.
Interferometer response functions vary with different gravity theories.
Future observations may confirm or challenge Einstein's theory.
Abstract
It is well known that Einstein's General Relativity (GR) achieved a great success and overcame lots of experimental tests. On the other hand, GR also showed some shortcomings and flaws which today advise theorists to ask if it is the definitive theory of gravity. In this review we show that, if advanced projects on the detection of Gravitational Waves (GWs) will improve their sensitivity, allowing to perform a GWs astronomy, understanding if Einstein's GR is the correct and definitive theory of gravity will be possible. For this goal, accurate angular and frequency dependent response functions of interferometers for GWs arising from various Theories of Gravity, i.e. GR and Extended Theories of Gravity will have to be used. This review is founded on the Essay which won an Honorable Mention at the the 2009 Gravity Research Foundation Awards.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Advanced Differential Geometry Research
