phenomenon

exotic phase transitions

Unusual or theoretical phase transitions in diverse systems like biology and black holes.
22 related articles · 1 formulas

Description

Exotic phase transitions refer to unusual transitions that do not fit the standard paradigm of symmetry breaking, often occurring in systems far from equilibrium or with topological order. Examples include transitions in black hole accretion states, time crystals (which break time-translation symmetry), and transitions in biological systems like cell fate determination. These transitions challenge our understanding of phases and can involve non-local order parameters or emergent phenomena.

History

The concept of exotic phase transitions gained traction in the late 20th century with the discovery of topological phases (e.g., quantum Hall effect) and time crystals proposed by Frank Wilczek in 2012. Black hole state transitions have been studied since the 1980s with the advent of X-ray astronomy.

How it works

In standard phase transitions, an order parameter (like magnetization) changes continuously or discontinuously. Exotic transitions may involve topological invariants (e.g., in topological insulators) or discrete time-translation symmetry breaking (time crystals). In black holes, transitions between accretion states (e.g., from a thin disk to a radiatively inefficient flow) are driven by changes in mass accretion rate and magnetic fields, analogous to phase transitions in thermodynamics. In biology, transitions can be driven by stochastic gene expression, leading to cell fate decisions.

In practice

Exotic phase transitions are explored for quantum computing (time crystals as memory), and understanding black hole accretion helps interpret astronomical observations like tidal disruption events.

Fun fact

Time crystals, a type of exotic phase, have been realized in ion traps, where five ions show a hierarchy of rhythms, as reported in recent experiments.

Concept graph →

Formulas

$$\eta = -\frac{\nabla_n v_{\rm pec}}{aH}$$
Rate of change of radial peculiar velocity component.
What is in the formula
ηvariablepeculiar velocity gradient — dimensionless
v_pecvariableradial peculiar velocity — velocity metre per second
nvariableradial direction coordinate — length metre
avariablescale factor of the universe — dimensionless
HvariableHubble parameter — frequency per second
∇_noperatorgradient along the radial direction — nabla operator
\eta=-\frac{({n}*\nabla)({n}*{v})}{ah}=-\frac{\nabla_nv_{\rmpec}}{ah} · 2607.19938v1

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