Cosmology: Conformally Invariant Theory of Gravity

Nature ◽  
1972 ◽  
Vol 236 (5342) ◽  
pp. 100-100
Author(s):  
2011 ◽  
Vol 28 (4) ◽  
pp. 045005 ◽  
Author(s):  
Henrique Gomes ◽  
Sean Gryb ◽  
Tim Koslowski

Author(s):  
PATRICIO SALGADO ◽  
FERNANDO IZAURIETA ◽  
EDUARDO RODRÍGUEZ

2021 ◽  
Vol 2021 (12) ◽  
Author(s):  
Gustavo P. de Brito ◽  
Oleg Melichev ◽  
Roberto Percacci ◽  
Antonio D. Pereira

Abstract We formally prove the existence of a quantization procedure that makes the path integral of a general diffeomorphism-invariant theory of gravity, with fixed total spacetime volume, equivalent to that of its unimodular version. This is achieved by means of a partial gauge fixing of diffeomorphisms together with a careful definition of the unimodular measure. The statement holds also in the presence of matter. As an explicit example, we consider scalar-tensor theories and compute the corresponding logarithmic divergences in both settings. In spite of significant differences in the coupling of the scalar field to gravity, the results are equivalent for all couplings, including non-minimal ones.


Author(s):  
S.N. Pandey ◽  
Sacheendra Shukla

Over the last few years, among various alternatives to the Einstein theory of gravity, especially f(R) theories of gravity have received more importance due to number of interesting results in cosmology and astrophysics. Pandey [10] gave an f(R) theory of gravity to obtain conformally invariant gravitational waves in which field equations have the form given by (3). In this paper we have investigated Lyttleton Bondi Cosmological model in view of field equations of f(R) theory of gravity for Generalized Peres spacetime and finally a wave like solution is obtained.


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