Can any Black Hole be studied fully through the simulation as Big Bang
lying idle now?. KR IRS 7423
"A synthetic analog of a black hole
<https://www.sciencealert.com/black-holes> could tell us a thing or two
about an elusive radiation theoretically emitted by the real thing.

Using a chain of atoms in single-file to simulate the event horizon of a
black hole, a team of physicists observed the equivalent of what we
call Hawking
radiation <https://www.sciencealert.com/hawking-radiation> – particles born
from disturbances in the quantum fluctuations caused by the black hole's
break in spacetime.
This, they say, could help resolve the tension between two currently
irreconcilable frameworks for describing the Universe: the general theory
of relativity <https://www.sciencealert.com/general-relativity>, which
describes the behavior of gravity as a continuous field known as spacetime;
and quantum mechanics, which describes the behavior of discrete particles
using the mathematics of probability.

For a unified theory of quantum gravity that can be applied universally,
these two immiscible theories need to find a way to somehow get along.

This is where black holes <https://www.sciencealert.com/black-holes> come
into the picture – possibly the weirdest, most extreme objects in the
Universe. These massive objects are so incredibly dense that, within a
certain distance of the black hole's center of mass, no velocity in the
Universe is sufficient for escape. Not even light speed.

That distance, varying
<https://www.omnicalculator.com/physics/schwarzschild-radius> depending on
the mass of the black hole, is called the event horizon. Once an object
crosses its boundary we can only imagine what happens, since nothing
returns with vital information on its fate.
But in 1974, Stephen Hawking
<https://www.sciencealert.com/stephen-hawking> proposed
that interruptions to quantum fluctuations caused by the event horizon
result in a type of radiation very similar to thermal radiation.If this
Hawking radiation exists, it's way too faint for us to detect yet. It's
possible we'll never sift it out of the hissing static of the Universe. But
we can probe its properties
<https://www.sciencealert.com/scientists-have-stimulated-hawking-radiation-in-a-lab-analogue-of-a-black-hole>
 by creating black hole analogs
<https://www.sciencealert.com/a-black-hole-in-a-lab-has-provided-new-evidence-that-hawking-radiation-is-real>
 in laboratory settings.

This has been done before, but in a study published last year, led by Lotte
Mertens of the University of Amsterdam in the Netherlands, researchers did
something new.

A one-dimensional chain of atoms served as a path for electrons to 'hop'
from one position to another. By tuning the ease with which this hopping
can occur, the physicists could cause certain properties to vanish,
effectively creating a kind of event horizon that interfered with the
wave-like nature of the electrons.

The effect of this fake event horizon produced a rise in temperature that
matched theoretical expectations of an equivalent black hole system, the
team said, but only when part of the chain extended beyond the event
horizon.

This could mean the entanglement <https://www.sciencealert.com/entanglement> of
particles that straddle the event horizon is instrumental in generating
Hawking radiation.

The simulated Hawking radiation was only thermal for a certain range of hop
amplitudes, and under simulations that began by mimicking a kind of
spacetime considered to be 'flat'.

This suggests that Hawking radiation may only be thermal within a range of
situations, and when there is a change in the warp of space-time due to
gravity.

It's unclear what this means for quantum gravity, but the model offers a
way to study the emergence of Hawking radiation in an environment that
isn't influenced by the wild dynamics of the formation of a black hole.
And, because it's so simple, it can be put to work in a wide range of
experimental set-ups, the researchers said.

This, can open a venue for exploring fundamental quantum-mechanical aspects
alongside gravity and curved spacetimes in various condensed matter
settings," the researchers explained in their paper
<https://journals.aps.org/prresearch/abstract/10.1103/PhysRevResearch.4.043084>
.

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