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Fractional Scalar Field Cosmology
Considering the Friedmann–Lemaître–Robertson–Walker (FLRW) metric and the Einstein scalar field system as an underlying gravitational model to construct fractional cosmological models has interesting implications in both classical and quantum regimes ...
Paulo Moniz +2 more
exaly +3 more sources
Some of the next articles are maybe not open access.
Second-order scalar-tensor field equations in a four-dimensional space
International Journal of Theoretical Physics, 1974exaly
Renormalization for a Scalar Field in an External Scalar Potential [PDF]
The Pauli–Villars regularization procedure confirms and sharpens the conclusions reached previously by covariant point splitting. The divergences in the stress tensor of a quantized scalar field interacting with a static scalar potential are isolated into a three-parameter local, covariant functional of the background potential.
Kimball A Milton +2 more
exaly +4 more sources
Differences between scalar field and scalar density field solutions [PDF]
Differences between scalar field and scalar density solutions are explored using a Robertson–Walker (RW) metric, and a nonrelativistic Hamiltonian is derived for a scalar density field in the post-newtonian approximation. The results are compared with those of a scalar field.
Pirinççiog˜lu N., Sert I.
openaire +3 more sources

