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arXiv:2303.02425 · Quantum Information Processing

Quantum computation of phase transition in interacting scalar quantum field theory

Shane Thompson, George Siopsis

Published Oct 30, 2023• 5 citations
arXivHTMLPDF
DOI
10.1007/s11128-023-04149-0

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I review the Bose-Einstein condensation phase transition of dilute gases of cold atoms, for particle theorists acquainted with methods of field theory at finite temperature. I then discuss how the dependence of the phase transition temperature on the interaction strength can be computed in the large N approximation. 1 Phase Transitions in Hot Scalar Theories The standard example from particle physics of a scalar theory is the Higgs sector of electroweak theory, which has a phase transition (or a crossover) at a temperature of order the weak scale: say, a few hundred GeV or so. Let’s focus on pure scalar theory by imagining setting the gauge coupling constant gw to zero. At finite temperature, the Higgs picks up a thermal contribution #λT 2 to its effective mass, and the effective potential becomes roughly of the form V (φ) ∼ m 2 eff (T)φ2 + λφ 4 with m 2 eff (T) = −M2 + #λT 2. At sufficiently high temperature, the #λT 2 turns the potential from being concave down at the origin to concave up, and so restores the symmetry that is spontaneously broken at zero temperature.

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We analyze the onset of classical behaviour after a second-order phase transition in quantum field theory. We consider a scalar theory in which the system-field interacts with its environment, represented both by further scalar fields and by its own short-wavelength modes. We compute the decoherence time for the system-field modes and compare it with the other time scales of the model. Within our approximations we see that the long-wavelength modes have decohered by the time that the transition has been first implemented (the spinodal time)
We work perturbatively with an interacting quantum field theory comprised of two distinct scalar fields. In this theory, we introduce a sudden quench of the mass of one of the scalars at time t0{t}_{0}t0​. Also, the quartic interaction between the two scalars is turned on at time tin{t}_{\mathrm{in}}tin​. These break time-translation invariance. In this setup we examine the effects of the relative ordering of t0{t}_{0}t0​ and tin{t}_{\mathrm{in}}tin​ on composite operator mixing. We study how such operator mixing affects features of the scalar potential. We find that the late time effective potential can be sensitive enough to the quenches to trigger phase transitions.
I review the Bose-Einstein condensation phase transition of dilute gases of cold atoms, for particle theorists acquainted with methods of field theory at finite temperature. I then discuss how the dependence of the phase transition temperature on the interaction strength can be computed in the large N approximation. 1 Phase Transitions in Hot Scalar Theories The standard example from particle physics of a scalar theory is the Higgs sector of electroweak theory, which has a phase transition (or a crossover) at a temperature of order the weak scale: say, a few hundred GeV or so. Let’s focus on pure scalar theory by imagining setting the gauge coupling constant gw to zero. At finite temperature, the Higgs picks up a thermal contribution #λT 2 to its effective mass, and the effective potential becomes roughly of the form V (φ) ∼ m 2 eff (T)φ2 + λφ 4 with m 2 eff (T) = −M2 + #λT 2. At sufficiently high temperature, the #λT 2 turns the potential from being concave down at the origin to concave up, and so restores the symmetry that is spontaneously broken at zero temperature.