2017/04/30 by Sumanta Chakraborty · 1 citation
Physics and Astronomy · #Advanced Differential Geometry Research #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Curvature #Field equation #Gravitation #Gravitational field #Homogeneous space #Null (SQL) #Riemann curvature tensor #Riemann hypothesis #Tensor (intrinsic definition) #gr-qc #hep-th
paper · pdf · doi:10.1155/2018/6509045
published as Adv. High Energy Phys. 6509045 (2018) · Invited Article; 11 pages, no figures
openalex publication_date 2018/01/01 · arxiv created 2018/04/20 · arxiv updated 2018/04/23 · openalex created_date 2018/05/07 · openalex updated_date 2026/08/05
We present an alternative derivation of the gravitational field equations for Lovelock gravity starting from Newton’s law, which is closer in spirit to the thermodynamic description of gravity. As a warm up exercise, we have explicitly demonstrated that, projecting the Riemann curvature tensor appropriately and taking a cue from Poisson’s equation, Einstein’s equations immediately follow. The above derivation naturally generalizes to Lovelock gravity theories where an appropriate curvature tensor satisfying the symmetries as well as the Bianchi derivative properties of the Riemann tensor has to be used. Interestingly, in the above derivation, the thermodynamic route to gravitational field equations, suited for null hypersurfaces, emerges quiet naturally.