134 papers
General Physics explores the fundamental laws that govern everything from the tiniest subatomic particles to the vastness of the cosmos. This field serves as the bedrock for understanding how the universe operates, covering mechanics, thermodynamics, and electromagnetism without getting bogged down in overly specialized sub-disciplines. It is where the big questions about matter, energy, and force come together to explain the physical world around us.
At Gist.Science, we process every new preprint in this General Physics category as it arrives from arXiv, ensuring you never miss a breakthrough. For each paper, we provide both a detailed technical summary for experts and a plain-language explanation that makes complex ideas accessible to everyone. Below are the latest papers in General Physics, freshly summarized and ready for you to explore.
This paper argues that the apparent discrepancies between early-universe galaxy properties and standard CDM predictions are resolved by the CCC+TL cosmology, which posits covarying coupling constants and a tired light effect to explain observed redshifts, thereby reconciling galaxy size, mass, and density evolution with observational data without requiring unrealistic formation rates.
This paper proposes a covariant Gross-Pitaevskii-like equation derived from a specific Lagrangian to study interacting relativistic fermions, demonstrating its applicability in explaining phenomena such as the Migdal step in Fermi liquids, superconductivity spectra, and quark confinement in (3+1) spacetime.
This paper demonstrates that applying the same entire-function regulator used to ensure ultraviolet finiteness in nonlocal quantum field theories to the energy-momentum tensor of a point mass resolves the curvature singularity by replacing it with a regular de Sitter core in the resulting static, spherically symmetric spacetime solution.
This paper demonstrates that the coefficient in the Bekenstein--Hawking black hole entropy formula arises purely from the causal geometry of null boundaries in four-dimensional spacetime, derived via symplectic structures and causal splitting without invoking gravitational field equations.
This paper investigates dynamical dark energy models within an anisotropic Bianchi Type-V universe using a covariant thermodynamics approach and confronts them with the latest DESI DR2, SNIa, and RSD datasets, finding that the combined anisotropy and dynamical dark energy framework effectively accommodates late-time observations and mitigates the and tensions, despite Bayesian criteria still favoring the standard CDM model.
This paper introduces a phenomenological model with a constant parameter describing an early-time interaction between a scalar field and radiation that modifies photon scaling, and preliminary constraints using Pantheon+SH0ES supernova and BAO data suggest this extension is favored over the standard model by the AIC criterion.
This paper proposes that the observed identity of a Damour-Solodukhin wormhole as either a black hole or a wormhole depends on the observer's location, utilizing Tangherlini's concept of gravitational indeterminacy to show that Fresnel reflection and transmission coefficients for probing photons are determined solely by the wormhole's free parameter rather than its mass.
This study employs Gaussian processes to model-independently reconstruct the dark energy equation of state and potential from Hubble and DESI data, yielding a model-independent Hubble constant estimate of km s Mpc and evaluating the viability of four specific scalar field potentials through chi-square and MCMC analyses.
This paper proposes a geometric quantization approach that extends General Relativity from a four-dimensional Riemannian manifold to an eight-dimensional phase-space framework, deriving a quantized metric tensor without relying on previous approximations to reconcile quantum mechanics with relativistic gravitational fields.
This paper proposes a teleparallel gravity framework utilizing geometric drift vectors to replace the central singularity of black holes with a smooth de Sitter-like core, where gravitational effects arise from torsion rather than curvature, allowing for analytic extensions of trajectories across event horizons.