Correspondences between scalar field and fluid fluctuations in curved spacetime
arXiv:2210.02130 · doi:10.1142/S0218271823500244
Abstract
A correspondence between scalar field fluctuations and generalized fluctuations in a hydrodynamic approximation of fields is obtained. The results presented here are of interest to field-fluid correspondences and form part of theoretical foundations in this area. The intention for such developments is to explore sub-hydro range mesoscopic physics for the relativistic fluids in curved spacetime. The fluid correspondences fall in the classical domain and can replace the quantum fields and fluctuations for scales around the hydrodynamic limits.The present article extends our earlier results with a more elaborate physical insight towards the quantum fluids and retention of partial quantum nature in a stochastic description in bulk of the fluids. This also accounts for non-thermal effects along with thermal and quantum fluctuations for the fields in the hydro limit. Hence the expressions presented here are very general in nature for various applications. The further scope of research that such developments give is discussed in the concluding section.
References in corpus (16)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
- A New Cosmological Model of Quintessence and Dark Matter
- Lectures on hydrodynamic fluctuations in relativistic theories
- Gravity & Hydrodynamics: Lectures on the fluid-gravity correspondence
- Quantum correlations between the light and kilogram-mass mirrors of LIGO
- Relativistic fluid dynamics: physics for many different scales
- Noise Kernel in Stochastic Gravity and Stress Energy Bi-Tensor of Quantum Fields in Curved Spacetimes
- The correspondence between a scalar field and an effective perfect fluid
- A covariant approach to relativistic large-eddy simulations: The fibration picture
- Scalar field-perfect fluid correspondence and nonlinear perturbation equations
- Strongly magnetized pulsars: explosive events and evolution
- Classical Einstein-Langevin Equation and Proposed Applications
- Correspondences of matter fluctuations in semiclassical and classical gravity for cosmological spacetime
- Correspondences of matter fluctuations in semiclassical and classical gravity for cosmological spacetime-II
- Stochastic metric perturbations (radial) in gravitationally collapsing spherically symmetric relativistic star