Could this river of stars be the Bifrost Bridge between Midgard and Asgard? Now that would make an interesting story.
I just saw an article about some proposed use for miniature blackholes created in a lab. I didn't read the article, but the idea has some intriguing possibilities.Some have theorized the proposed Planet 9 is a small black hole.
I hope so…that might be used.
Some sort of 3D topographic map to figure out the effects of curvature on space/time?
Having been born "way back" in 1963, I'm not sure how I should feel about the way that date was referenced.
- Way back in 1963, Roy Kerr became the first person to write down the exact solution, in general relativity, for a realistic, rotating black hole. 60 years later, it's still used everywhere.
- Although Roger Penrose won the Nobel Prize in physics just a few years ago for demonstrating how black holes come to exist in our Universe, singularities and all, the subject isn't closed.
- We've never peered beneath the event horizon, and have no way of detecting what's inside. Using a powerful mathematical argument, Kerr argues that singularities shouldn't physically exist. He may be right.
Yes, we just don't know. If we knew for certain that unitarity is conserved, we might have more of a clue. If the white hole is actually a big bang, perhaps the energy ends up creating a new universe imprinted with information from the one containing the black hole; perhaps the information is lost and the new universe has a completely different particle zoo, fundamental constants and set of physical laws. I don't know if branchial space theory offers any insights as we don't know if or how the properties of the ruliad can vary between instantiations of universes.Sounds like the particles of the object that entered could get pushed out a white hole, just not intact (protons, neutrons, electrons, or perhaps as subatomic particles)
And, because this is just a really cool picture from the article, that could have come right out of 1963:
![]()
I thought a singularity and a black hole were one and the same.
-Will
A Postquantum Theory of Classical Gravity? (aps.org)The effort to discover a quantum theory of gravity is motivated by the need to reconcile the
incompatibility between quantum theory and general relativity. Here, we present an alternative approach
by constructing a consistent theory of classical gravity coupled to quantum field theory. The dynamics is
linear in the density matrix, completely positive, and trace preserving, and reduces to Einstein’s theory of
general relativity in the classical limit. Consequently, the dynamics does not suffer from the pathologies of
the semiclassical theory based on expectation values. The assumption that general relativity is classical
necessarily modifies the dynamical laws of quantum mechanics; the theory must be fundamentally
stochastic in both the metric degrees of freedom and in the quantum matter fields. This breakdown in
predictability allows it to evade several no-go theorems purporting to forbid classical quantum interactions.
The measurement postulate of quantum mechanics is not needed; the interaction of the quantum degrees of
freedom with classical space-time necessarily causes decoherence in the quantum system. We first derive
the general form of classical quantum dynamics and consider realizations which have as its limit
deterministic classical Hamiltonian evolution. The formalism is then applied to quantum field theory
interacting with the classical space-time metric. One can view the classical quantum theory as fundamental
or as an effective theory useful for computing the backreaction of quantum fields on geometry. We discuss a
number of open questions from the perspective of both viewpoints.
Gravitationally induced decoherence vs space-time diffusion: testing the quantum nature of gravity | Nature CommunicationsWe consider two interacting systems when one is treated classically while the other system remains quantum. Consistent dynamics of this coupling has been shown to exist, and explored in the context of treating space-time classically. Here, we prove that any such hybrid dynamics necessarily results in decoherence of the quantum system, and a breakdown in predictability in the classical phase space. We further prove that a trade-off between the rate of this decoherence and the degree of diffusion induced in the classical system is a general feature of all classical quantum dynamics; long coherence times require strong diffusion in phase-space relative to the strength of the coupling. Applying the trade-off relation to gravity, we find a relationship between the strength of gravitationally-induced decoherence versus diffusion of the metric and its conjugate momenta. This provides an experimental signature of theories in which gravity is fundamentally classical. Bounds on decoherence rates arising from current interferometry experiments, combined with precision measurements of mass, place significant restrictions on theories where Einstein’s classical theory of gravity interacts with quantum matter. We find that part of the parameter space of such theories are already squeezed out, and provide figures of merit which can be used in future mass measurements and interference experiments.
strong diffusion in phase-space
long coherence times require strong diffusion
conjugate momenta
...diffeomorphism invariant
I've heard this too. I suspect, were you to try this experiment in your freezer: time the freezing of luke warm water in your freezer, then time the freezing of hot water in your freezer, you might corroborate that suggestion. But if you put both trays in your freezer together, they would freeze at nearly the same time, unless you separate the trays.I seem to remember how heated water might freeze first before lukewarm water.
We use essential cookies to make this site work, and optional cookies to enhance your experience.