scholarly journals A longitudinal component in massive gravitational waves arising from a bimetric theory of gravity

2007 ◽  
Vol 28 (2) ◽  
pp. 247-250 ◽  
Author(s):  
Christian Corda
Keyword(s):  
Gravitational Waves ◽  
Longitudinal Component ◽  
Bimetric Theory ◽  
Theory Of Gravity

scholarly journals What are the wild waves saying? Yet another meditation on the predictions, searches for, and detections of gravitational waves

2018 ◽  
Vol 27 (14) ◽  
pp. 1830009
Author(s):  
Virginia Trimble
Keyword(s):  
General Relativity ◽  
Gravitational Waves ◽  
Point Of View ◽  
Large Majority ◽  
Laboratory Apparatus ◽  
New Information ◽  
Theory Of Gravity ◽  
To Come ◽  
The Universe

A large majority of the physics and astronomy communities are now sure that gravitational waves exist, can be looked for, and can be studied via their effects on laboratory apparatus as well as on astronomical objects. So far, everything found out has agreed with the predictions of general relativity, but hopes are high for new information about the universe and its contents and perhaps for hints of a better theory of gravity than general relativity (which even Einstein expected to come eventually). This is one version of the story, from 1905 to the present, told from an unusual point of view, because the author was, for 28.5 years, married to Joseph Weber, who built the first detectors starting in the early 1960s and operated one or more until his death on 30 September 2000.

scholarly journals The YARK Theory of Gravity Can Reproduce Neither the LIGO “GW150914 Signal”, nor the Other LIGO Detections of Gravitational Waves

Symmetry ◽  
2018 ◽  
Vol 10 (11) ◽  
pp. 558 ◽  
Author(s):  
Christian Corda
Keyword(s):  
Gravitational Waves ◽  
The Other ◽  
Theory Of Gravity ◽  
Recent Claim

We show that, based on important reasons, differently from some recent claim in the literature, the YARK theory of gravity can reproduce neither the LIGO “GW150914 signal”, nor the other LIGO detections of gravitational waves (GWs).

Detection of massive Gravitational Waves using spherical antenna

2014 ◽  
Vol 23 (05) ◽  
pp. 1450037 ◽  
Author(s):  
P. Prasia ◽  
V. C. Kuriakose
Keyword(s):  
Gravitational Wave ◽  
Gravitational Waves ◽  
Mechanical Resonators ◽  
Spherical Antenna ◽  
Wave Antenna ◽  
Gravitational Wave Antenna ◽  
Theory Of Gravity

The generation of massive Gravitational Waves (GW) from metric f(R) theory of gravity is studied and the sensitivity of a spherical antenna detector towards such a wave is looked into. The energy sensitivity is maximum for the monopole mode of the sphere. Of the five quadrupole modes of a sphere, only three are triggered by a massive wave. Also, the sensitivity of a spherical antenna with mechanical resonators attached to it is studied. The Truncated Icosahedral Gravitational wave Antenna (TIGA), originally proposed for detecting the effect of massless GW on the quadrupole modes of a sphere, has been modified in this paper to get a Modified TIGA, in order to detect the sensitivity of monopole modes towards a massive wave.

scholarly journals Gravitational waves in the relativistic theory of gravity

2009 ◽  
Vol 160 (2) ◽  
pp. 1096-1100 ◽  
Author(s):  
S. S. Gershtein ◽  
A. A. Logunov ◽  
M. A. Mestvirishvili
Keyword(s):  
Gravitational Waves ◽  
Relativistic Theory ◽  
Relativistic Theory Of Gravity ◽  
Theory Of Gravity

scholarly journals Gravitational waves in the spinor theory of gravity

2020 ◽  
pp. 2150003
Author(s):  
M. Novello ◽  
A. E. S. Hartmann
Keyword(s):  
General Relativity ◽  
Gravitational Wave ◽  
Gravitational Waves ◽  
Spinor Theory ◽  
Ricci Flat ◽  
Theory Of Gravity

We analyze the gravitational waves within the Spinor Theory of Gravity (STG) and compare it with the General Relativity proposal. In the case of STG, a gravitational wave may occur if the effective gravitational metric induced by the spinorial field is Ricci flat.

scholarly journals Probing the theory of gravity with gravitational lensing of gravitational waves and galaxy surveys

2020 ◽  
Vol 494 (2) ◽  
pp. 1956-1970 ◽  
Author(s):  
Suvodip Mukherjee ◽  
Benjamin D Wandelt ◽  
Joseph Silk
Keyword(s):  
Gravitational Wave ◽  
Gravitational Waves ◽  
Gravitational Lensing ◽  
Cross Correlation ◽  
Laser Interferometer ◽  
Galaxy Surveys ◽  
Einstein Telescope ◽  
Laser Interferometer Space Antenna ◽  
Theories Of Gravity ◽  
Theory Of Gravity

ABSTRACT The cross-correlation of gravitational wave strain with upcoming galaxy surveys probes theories of gravity in a new way. This method enables testing the theory of gravity by combining the effects from both gravitational lensing of gravitational waves and the propagation of gravitational waves in space–time. We find that within 10 yr the combination of the Advanced LIGO (Laser Interferometer Gravitational-Wave Observatory) and VIRGO (Virgo interferometer) detector networks with planned galaxy surveys should detect weak gravitational lensing of gravitational waves in the low-redshift Universe (z < 0.5). With the next-generation gravitational wave experiments such as Voyager, LISA (Laser Interferometer Space Antenna), Cosmic Explorer, and the Einstein Telescope, we can extend this test of the theory of gravity to larger redshifts by exploiting the synergies between electromagnetic wave and gravitational wave probes.

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