A quantum quench changes a quantum system's control parameters rapidly and studies the subsequent unitary time evolution. In the ideal sudden limit, write an initial energy eigenstate using a complete final orthonormal eigenbasis:The Born rule probabilities for a nondegenerate final energy measurement are , with . For a degenerate energy eigenvalue, sum the probabilities over its orthonormal energy eigenstates. Subsequent relative quantum phases can alter other measurement probabilities even though these final energy populations stay fixed. A quench need not begin in an energy eigenstate; the same expansion applies to any initial pure state.
Take an isolated two-level system, or a spin one-half qubit, with Pauli matrices . Let and . The initial and final Hamiltonian operators areThe energy gaps are . Prepare the initial ground state , with energy eigenvalue . A final orthonormal eigenbasis isDirect matrix multiplication gives and . The unchanged initial quantum state is . Its new probability amplitudes are the inner products ; the Born rule gives . The angle between the real amplitude vectors is , whereas the Hamiltonian axis on the Bloch sphere rotates through .
At , and , so the final energy measurement gives with probability and with probability . At the initial ground state remains the final ground state; at it is the final excited energy eigenstate. These statements are about the new energy labels, not an instantaneous physical rotation of the quantum state.
The drive can supply or extract work while the quantum state stays approximately fixed. For a differentiable bounded Hamiltonian operator, the Schrödinger equation givesThe state-evolution terms cancel, leaving the external drive's power. For a finite ideal step the change in mean energy is . Thus conservation of energy for a closed system with a time-independent Hamiltonian operator does not assert conservation of the driven subsystem's energy during switching.
Specify work operationally by two energy measurements: one before the switch and one after. For the prepared initial ground state, the first outcome is definite; the second samples the new Born rule probabilities. This protocol gives a distribution of measured energy differences, rather than generally the measurement distribution of the single operator .[ref]
Fluctuation theorems: Work is not an observable by Peter Talkner and others. Talkner, Lutz and Hänggi, p. 2, equations (8)–(10): initial energy outcome, conditional transition probability and two-measurement work distribution
and henceFor and , the work is or , with probabilities and ; its expectation is and its variance is . The initial mean energy becomes . Using different initial and final scalar offsets would also shift the measured work; the displayed Hamiltonian operators fix that convention explicitly.After the quantum quench, hold fixed and evolve without an intervening energy measurement. The unitary time evolution isProjection onto the original gives probability amplitude . Squaring its modulus yields the two-level quantum return probabilityTheir sum is one. For , the first minimum of is at , and the return is complete at . At or there is no oscillation, because the initial quantum state is already a final energy eigenstate.
Changing measurement basis reveals the evolving relative quantum phase. Measuring the final energy first instead destroys this quantum coherence between final energy eigenstates in the unconditioned ensemble: its later original-basis return probability is , equal to for this example. That constant differs from the oscillation of the unmeasured pure state. The work protocol and the oscillation protocol therefore use separate preparations.
A concrete quantum quench experiment loaded a Bose-Einstein condensate of chemical atoms from a magnetic field trap into an optical lattice: three orthogonal laser standing waves, with approximately beam waists. An loading ramp preceded a increase in lattice depth. This suppressed quantum tunnelling while retaining each well's vibrational ground state. The switch preserved atom-number populations rather than freezing every motional degree of freedom.[ref]
Collapse and revival of the matter wave field of a Bose-Einstein condensate by Markus Greiner and others. Greiner and others, manuscript pp. 3–4: preparation and switching; p. 7, Methods: wavelength, beam waists and lattice geometry
After variable hold times, releasing the traps and taking photon absorption images after of flight revealed disappearance and return of interference peaks. Background-subtracted peak counts supplied a coherent fraction. Varying final depth tested the predicted revival period ; varying initial depth tested the collapse's sensitivity to atom-number statistics. Peak broadening outside counting windows and spatial variation of limited later signals.[ref]
Collapse and revival of the matter wave field of a Bose-Einstein condensate by Markus Greiner and others. Manuscript p. 4 and figure 2 caption on p. 11: flight and image extraction; figure 3 caption on p. 12: readout limitations; figures 4–5 captions on pp. 13–14: final-depth and initial-depth comparisons
Here is the on-site interaction energy. The approximate isolated-well Hamiltonian operator , with number operator , gives different quantum phases to its number states, which later rephase. This is a many-level realization of the distinction between fixed populations and changing quantum phases.[ref]
Collapse and revival of the matter wave field of a Bose-Einstein condensate by Markus Greiner and others. Manuscript pp. 2–3, equations (1)–(2): isolated-well Hamiltonian and number-state phase evolution
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