Gravitational waves in the Spinor Theory of Gravity
Mario Novello, Angelo E. S. Hartmann
TL;DR
This paper investigates gravitational waves predicted by the Spinor Theory of Gravity and compares their properties with those in General Relativity, focusing on conditions for wave occurrence related to Ricci-flat metrics.
Contribution
It provides a comparison of gravitational wave predictions between the Spinor Theory of Gravity and General Relativity, highlighting specific conditions for wave generation.
Findings
Gravitational waves in STG occur if the effective metric is Ricci flat.
Comparison shows similarities and differences with GR predictions.
Conditions for wave existence are explicitly characterized.
Abstract
We analyze the gravitational waves within the Spinor Theory of Gravity 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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.