method

quantum gravity analogues

Systems that simulate aspects of quantum gravity or spacetime emergence in laboratory settings.
13 related articles · 2 formulas

Description

Quantum gravity analogues are laboratory systems that mimic specific aspects of quantum gravity or the emergence of spacetime, even though they do not involve actual gravitational fields. These analogues are typically built from condensed matter systems, such as ultracold atomic gases, fluids of light, or even water waves, where the mathematical equations governing excitations resemble those of fields in curved spacetime. By studying these systems, physicists can probe phenomena that would otherwise be inaccessible, such as Hawking radiation from artificial event horizons or the thermodynamics of spacetime.

History

The concept was pioneered by William Unruh in 1981, who proposed that sound waves in a moving fluid could mimic black hole physics. Experimental realizations followed decades later, with the first sonic black hole analogue demonstrated in 2009 by Jeff Steinhauer and colleagues using a Bose-Einstein condensate.

How it works

The key mechanism is the analogy between the propagation of waves in a moving medium and the propagation of light in a curved spacetime. For example, in a fluid with a sufficiently fast flow, sound waves can be trapped behind a 'sonic horizon'—a point where the flow speed exceeds the local speed of sound—mirroring the event horizon of a black hole. Quantum fluctuations near this horizon can produce phonon pairs, analogous to Hawking radiation. In other setups, carefully engineered interactions in ultracold atoms or photonic crystals create effective metrics that simulate spacetime curvature, allowing researchers to study phenomena like particle creation or the emergence of spacetime from entanglement.

In practice

These analogues are used to test theoretical predictions of quantum gravity, such as Hawking radiation, in controlled laboratory settings, and to explore analog models of cosmological phenomena like inflation or the early universe.

Fun fact

In 2016, Jeff Steinhauer's lab at the Technion reported the first observation of spontaneous Hawking radiation from a sonic black hole analogue, using a Bose-Einstein condensate of rubidium atoms.

Concept graph →

Formulas

$$K = C_{ab} + C_{a'b} + C_{ab'} - C_{a'b'} \leq 2$$
Tests macrorealism against quantum mechanics.
What is in the formula
KvariableLeggett-Garg combination of correlation functions
C_{ab}variableCorrelation function between measurements at times a and b — correlation function
C_{a'b}variableCorrelation function between measurements at times a' and b — correlation function
C_{ab'}variableCorrelation function between measurements at times a and b' — correlation function
C_{a'b'}variableCorrelation function between measurements at times a' and b' — correlation function
b_{\max}=\max\{0,\frac{c_{ab}+c_{a'b}+c_{ab'}-c_{a'b'}-2}{2\sqrt{2}-2}\} · 2505.01379v1
$$k_{qJ} = \left( \frac{16\pi G m^2 \rho}{\hbar^2} \right)^{1/4}$$
Scale where quantum pressure balances gravity.
What is in the formula
k_{qJ}variableQuantum Jeans wavenumber — wavenumber reciprocal metre
mvariableParticle mass — mass kilogram
\rhovariableMass density — mass density kilogram per cubic metre
GconstantUniversal constant of gravitation — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared
\hbarconstantPlanck constant divided by 2π — reduced planck constant = 1.054571817e-34 joule second
k_{qj}=(\frac{16πgm^2ρ_0}{ħ^2})^{1/4} · 2607.04893
k_{qj}=(\frac{16πgm^2ρ_0}{ħ^2})^{1/4} · 2607.04893v1

Related articles · 13

Cosmology2026-07-203 minarXiv:2607.18107
General Relativity2026-07-011 minarXiv:2607.01118express
How Black Holes Actually Glow: A Simple Discovery
A black hole is not just a vacuum cleaner. It glows faintly, emitting particles — this idea was proposed by Jacob Bekenstein, who connected the hole's temperature to its degree of disorder. Detecting such radiation in space is incredibly difficult.
Quantum Gases2026-06-172 minarXiv:2606.19444express
How to See Invisible Fermions with Chameleon Atoms
The quantum world is full of transformations. Sometimes a system made of one type of particle starts behaving as if it harbors completely different ones. For example, in a chain of bosons, sociable particles that like to crowd into the same state, fermions from the Standard Model may unexpectedly appear, even though they usually keep to themselves.
General Relativity2026-06-132 minarXiv:2606.15295express
Gravitational Waves to Put New Theory to the Test
In 2015, detectors caught a gravitational wave for the first time — a ripple in space that traveled from merging black holes. Since then, such signals have become a new window into the universe for astrophysics. But gravitational waves can do more: they carry the imprint of the very theory of gravity.
Quantum Tremor of Parallel Worlds: Gravity on a Laboratory Table
Two parallel streams of atoms, released from Bose condensates, begin their journey in free fall. In the classical picture, their separation remains unchanged — like two skiers gliding down a perfectly smooth slope. But if spacetime is not frozen snow, but a living, rippling membrane, then every tremble of it is transmitted to matter.
HEP Theory2026-05-111 minarXiv:2605.11046express
Laboratory Black Holes: Playing with Temperature
An ordinary kettle: you heat it up — temperature rises, molecular chaos grows, and steam shoots out. But in the lab, they've created a peculiar "kettle"—an analog black hole made from superconducting circuits cooled to the extreme.
General Relativity2026-05-111 minarXiv:2605.11280express
General Relativity2026-04-272 minarXiv:2604.24861express
Black Holes in a Sink of Water
Water flowing through a pipe can become a trap for sound. If the flow speed exceeds the speed of sound in water, then sound waves trying to go against the current can no longer escape: they are swept away, like light beyond a black hole's horizon.
HEP Phenomenology2026-03-031 minarXiv:2603.02493express
Gravitational Waves Will Unveil Quantum Gravity
Primordial black holes behave like boiling kettles: as they evaporate, they whistle gravitational waves. The character of the whistle, its spectrum, depends on how the hole's temperature relates to its mass.
Mesoscale2026-03-022 minarXiv:2603.01664express
Black Holes from Light and Vortices
Black holes are among the most mysterious objects in the universe. Their gravity is so strong that even light cannot escape their vicinity. But studying them directly is extremely difficult: the nearest black hole is thousands of light-years away, and mergers of two black holes take millions of years.
Statistical Mech2026-02-042 minarXiv:2602.04593express
Hawking Radiation on a Tabletop
A black hole is a place from which even light cannot escape. But quantum theory says it still glows faintly. This glow is called Hawking radiation. In space, it's impossible to spot: it's too faint. So physicists build models of black holes from ordinary materials.
General Relativity2026-01-051 minarXiv:2601.02197express
A Black Hole Like a Bell: How a Light Pulse Gives Rise to Echoes
If you briefly flash light near a black hole, it will respond with a long echo, like a bell that keeps ringing after being struck. The light gets trapped near the hole, bouncing repeatedly off an invisible boundary: the photon sphere, where rays circle around like sound in a metal.
HEP Theory2025-10-291 minarXiv:2510.25852express
A Black Hole Cooks Up Radiation Like a Pot of Soup
The 'double copy' method in physics is a culinary trick: a chef takes a cold soup recipe, doubles the ingredients, and gets a recipe for a hot roast. Likewise, particle interactions via electric forces (the basis of the Standard Model) morph into gravity, which describes spacetime curvature.