# Search results

Astronomische Nachrichten > 342 > 1-2 > 364 - 368

Astronomische Nachrichten > 342 > 1-2 > 305 - 309

Astronomische Nachrichten > 342 > 1-2 > 135 - 141

*pseudo‐complex General Relativity*(pc‐GR) and comparing it with the standard

*General Relativity*(GR). The path, on how to determine the axial modes, serve as a starting point for more general extensions of GR, involving additions of

*r*‐dependent functions to

*g*

_{00}.

Astronomische Nachrichten > 342 > 1-2 > 49 - 53

Journal of Mechanical and Energy Engineering > 2020 > Vol. 4, No 2 > 189--196

Annalen der Physik > 532 > 7 > n/a - n/a

Rendiconti Lincei. Scienze Fisiche e Naturali > 2019 > 30 > 1 > 231-240

Frontiers of Physics > 2020 > 15 > 2 > 1-7

Rendiconti Lincei. Scienze Fisiche e Naturali > 2019 > 30 > 1 > 71-77

General Relativity and Gravitation > 2019 > 51 > 11 > 1-3

Moscow University Physics Bulletin > 2019 > 74 > 4 > 413-418

Earth, Moon, and Planets > 2019 > 123 > 1-2 > 9-13

Annalen der Physik > 531 > 8 > n/a - n/a

Experimental Astronomy > 2019 > 48 > 1 > 77-95

Advances in Applied Clifford Algebras > 2019 > 29 > 4 > 1-41

General Relativity and Gravitation > 2019 > 51 > 7 > 1-12

*a*(

*t*) and the scalar field $$\phi (t)$$ ϕ(t) in unperturbed JBD theory are dependent on the $$\omega $$ ω parameter which determines how the scalar field is coupled to geometry of space–time....

Frontiers of Physics > 2019 > 14 > 6 > 1-11

*t*, of GW-GRB associations within the context of compact binary coalescence (CBC) — short GRB (sGRB) associations and GW burst...

Living Reviews in Relativity > 2019 > 22 > 1 > 1-104

The Astronomy and Astrophysics Review > 2019 > 27 > 1 > 1-78

General Relativity and Gravitation > 2019 > 51 > 6 > 1-14

*f*(

*R*,

*T*) gravity ($$\lambda $$ λ being the model parameter). The spatially flat universe model is perturbed via Regge–Wheeler perturbations inducing polar gravitational waves and the field equations are formulated...