Physics of Gravitational Interaction: Geometry of Space or Quantum Field in Space?
Yurij Baryshev
Abstract
Gravity theory is the basis of modern cosmological models. Thirring-Feynman's tensor field approach to gravitation is an alternative to General Relativity (GR). Though Field Gravity (FG) approach is still developing subject, it opens new understanding of gravitational interaction, stimulates novel experiments on the nature of gravity and gives possibility to construct new cosmological models in Minkowski space. According to FG, the universal gravity force is caused by exchange of gravitons - the quanta of gravity field. Energy of this field is well-defined and excludes the singularity. All classical relativistic effects are the same as in GR, though there are new effects, such as free fall of rotating bodies, scalar gravitational radiation, surface of relativistic compact bodies, which may be tested experimentally. The intrinsic scalar (spin 0) part of gravity field corresponds to "antigravity" and only together with the pure tensor (spin 2) part gives the usual Newtonian force. Laboratory and astrophysical experiments for testing new predictions of FG, will be performed in near future. In particular observations with bar and interferometric detectors, like Explorer, Nautilus, LIGO and VIRGO, will check the predicted scalar gravitational waves from supernova explosions.
Create a lesson
Related papers
Testing compact binary nature in eccentric orbits with third-generation detectors
Syed U. Naqvi, Kaushik Paul, Chandra Kant Mishra
Turning Selection Bias into a New Statistic: Asymmetry and Fringes of Lensed Gravitational Waves
Juno C. L. Chan, Elwin K. Y. Li
Exact two-loop gravitational tail integrals and their ultraviolet-infrared structure
Gabriel Luz Almeida
Noncommutative BTZ Gravastar in Gauss-Bonnet Gravity
M. A. Anacleto, A. T. N. Silva, L. Casarini et al.
Mini-Superspace Hamiltonian Dynamics and Canonical Quantization of Bumblebee Cosmology
Pranjal Sarmah
Dynamical stability and observational constraints on a late-time dark-matter particle-creation model
Anirban Chatterjee