Investigation of Electronic Recombination in Helium and Argon Afterglow Plasmas by Means of Laser Interferometric Measurements

1966 ◽  
Vol 149 (1) ◽  
pp. 91-96 ◽  
Author(s):  
M. A. Gusinow ◽  
J. B. Gerardo ◽  
J. T. Verdeyen
2003 ◽  
Author(s):  
Shibin Wang ◽  
Jingwei Tong ◽  
Mario Cottron ◽  
Linan Li ◽  
Zhiyong Wang

2008 ◽  
Vol 17 (2) ◽  
pp. 024019 ◽  
Author(s):  
L Ottaviano ◽  
F Bussolotti ◽  
S Piperno ◽  
M Rinaldi ◽  
S Santucci ◽  
...  

2009 ◽  
Author(s):  
D. Margarone ◽  
M. Kozlova ◽  
J. Nejdl ◽  
B. Rus ◽  
T. Mocek ◽  
...  

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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