News
The compact morphology, low entropy, a Predicts fossil galaxies at z > 15 using non-singular relativity; simulates 180 Gyr; self-refutes if data contradicts its metric evolution. We’re not discarding ...
DUT Quantum Simulator interface: a decentralized scientific tool for testing cosmological hypotheses based on non-singular ...
In a recently published paper in Physical Review Letters, scientists propose a comprehensive theoretical framework indicating ...
TheFirstHammer on MSN17dOpinion
General Relativity Simplified: Discover How Mass Distorts Space-Time and Alters Time ItselfEver wondered what gravity really is? Is it a force, or is there more to it than we know? In this video, we break down the ...
"In general relativity, the interior of a black hole is like a contracting universe, where the singularity represents the moment when space itself collapses," Molina-Niñirola said.
The study introduces a new entropic action, which quantifies the difference between the metric of spacetime and the metric induced by matter fields. This approach leads to modified Einstein equations ...
This approach leads to modified Einstein equations that, in the low coupling regime, i.e., low energies and small curvature, reduce to the classical equations of general relativity.
By modifying Einstein's theory of general relativity, the center of a black hole with infinite curvature could be replaced by a highly curved but regular region of space-time, the researchers ...
Curvature is the core concept of general relativity. Matter and energy tell spacetime how to bend, curve and warp. In turn, that bending of spacetime tells matter how to move.
Albert Einstein’s theory of gravity, general relativity, is famously incomplete. As proven by physics Nobel laureate Roger Penrose, when matter collapses under its own gravitational pull, the result ...
Some results have been hidden because they may be inaccessible to you
Show inaccessible results