Cosmological tests of general relativity

Nature ◽  
1977 ◽  
Vol 267 (5607) ◽  
pp. 128-130 ◽  
Author(s):  
P. HUT
2010 ◽  
Author(s):  
Alessandra Silvestri ◽  
Jean-Michel Alimi ◽  
André Fuözfa ◽  
◽  
◽  
...  

2012 ◽  
Vol 85 (4) ◽  
Author(s):  
Alireza Hojjati ◽  
Gong-Bo Zhao ◽  
Levon Pogosian ◽  
Alessandra Silvestri ◽  
Robert Crittenden ◽  
...  

2009 ◽  
Vol 103 (24) ◽  
Author(s):  
Gong-Bo Zhao ◽  
Levon Pogosian ◽  
Alessandra Silvestri ◽  
Joel Zylberberg

2009 ◽  
Vol 5 (S261) ◽  
pp. 198-199
Author(s):  
Clifford M. Will

AbstractWe review the experimental evidence for Einstein's general relativity. A variety of high precision null experiments confirm the Einstein Equivalence Principle, which underlies the concept that gravitation is synonymous with spacetime geometry, and must be described by a metric theory. Solar system experiments that test the weak-field, post-Newtonian limit of metric theories strongly favor general relativity. Binary pulsars test gravitational-wave damping and aspects of strong-field general relativity. During the coming decades, tests of general relativity in new regimes may be possible. Laser interferometric gravitational-wave observatories on Earth and in space may provide new tests via precise measurements of the properties of gravitational waves. Future efforts using X-ray, infrared, gamma-ray and gravitational-wave astronomy may one day test general relativity in the strong-field regime near black holes and neutron stars.


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