Parameter estimation in an anisotropic expanding spacetime
arXiv:2109.08252
Abstract
In this work, we investigate how the anisotropy affects the cosmological parameters estimation. Here the anisotropy is incorporated as a small gravitational disturbance. We calculate the Fisher information for both cosmological parameters (expansion volume) and (expansion rate), and we show that the anisotropy introduces oscillations in the Fisher information spectrum. This implies that the estimation of the cosmological parameters is sensible to the direction of the momentum of particles. In addition, we observe that for small values of the momentum there is a substantial difference between the Fisher information spectrum for the minimum and conformal couplings.
arXiv comment20 pages, 4 figures
References in corpus (15)
- Enhancing the sensitivity of the LIGO gravitational wave detector by using squeezed states of light
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Optimal quantum estimation of the Unruh-Hawking effect
- Entanglement in an expanding spacetime
- Phonon creation by gravitational waves
- Quantum fisher information in noninertial frames
- Quantum estimation of the Schwarzschild space-time parameters of the Earth
- Optimal estimation of entanglement
- Relativistic Quantum Metrology in Open System Dynamics
- Quantum metrology and estimation of Unruh effect
- Parameter estimation using NOON states over a relativistic quantum channel
- Parameter estimation for an expanding universe
- Optimal estimation of entanglement in optical qubit systems
- Quantum estimation in an expanding spacetime
- Spacetime anisotropy affects cosmological entanglement