Refining Bounds for Snyder and GUP Models through Seismic Wave Analysis
arXiv:2310.00913 · doi:10.1016/j.aop.2025.170136
Abstract
This study investigates possibility of placing bounds on the parameters, arising from the non-commutative Snyder space-time model and Generalized Uncertainty Principle (GUP) approach, by utilizing seismic data. We investigate the dependence of constraints on the type of realization used for the quantum phase space. Results indicate improved bounds compared to prior studies, with the model parameter constrained to be less than for certain choice of realizations. This approach demonstrates the potential for using Earth's empirical data to refine constraints on GUP parameters.
10 pages, 3 figures, extended introduction and conclusions; published version
References in corpus (27)
- Mass-Radius Relationships for Solid Exoplanets
- Gravitational Wave asteroseismology revisited
- Exoplanets as Sub-GeV Dark Matter Detectors
- Scalar Field Theory on Non-commutative Snyder Space-Time
- Physics at the surface of a star in Eddington-inspired Born-Infeld gravity
- New class of quasinormal modes of neutron stars in scalar-tensor gravity
- Neutrino tomography of the Earth
- Earth as a transducer for dark-photon dark-matter detection
- First asteroseismic limits on the nature of dark matter
- Obtaining Precision Constraints on Modified Gravity with Helioseismology
- Asteroseismic constraints on the cosmic-time variation of the gravitational constant from an ancient main-sequence star
- White dwarfs as Physics laboratories: lights and shadows
- Cooling process of brown dwarfs in Palatini f(R) gravity
- Fermi gas and modified gravity
- Metric-affine effects in crystallization processes of white dwarfs
- Searching for dark energy with the Sun
- Metric-affine gravity effects on terrestrial (exo-)planets profiles
- Detectable seismic consequences of the interaction of a primordial black hole with Earth
- Constraints on Dark Matter from the Moon
- Jupiter and jovian (exo)-planets in Palatini gravity
- Heisenberg doubles for Snyder type models
- Cosmological constraints of Palatini gravity
- Planetary seismology as a test of modified gravity proposals
- Constraining Snyder and GUP models with low-mass stars
- Early evolution of fully convective stars in scalar-tensor gravity
- Non-homogeneous exoplanets in metric-affine gravity
- Effect of Non-commutativity of space-time on Thermodynamics of Photon gas