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Equation 61 · No Particle Without a Cosigner

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aa

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the acceleration. Read the equation part by part below; each part has a contextual explanation and a link to its mathematical background.

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aa

Symbol a

the acceleration.

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A second limit worth naming, because it is where the eternal-acceleration answer above starts to strain, is slow time dependence. Barbado and Visser worked out the response of a detector whose acceleration a(τ\tau) varies with proper time, expanding in powers of a˙\dot a , a¨\ddot a , and higher proper-time derivatives of the acceleration [ 8 ] . At leading order, wherever the acceleration changes slowly compared to the local orthogonalization timescale it sets for itself, the detector reports the instantaneous Unruh temperature TU(a(τ)T_U(a(\tau)) at each moment, as though briefly and locally eternal. This adiabatic recovery is the second known limit this construction inherits rather than derives: it…
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A second limit worth naming, because it is where the eternal-acceleration answer above starts to strain, is slow time dependence. Barbado and Visser worked out the response of a detector whose acceleration a(τ\tau) varies with proper time, expanding in powers of a˙\dot a , a¨\ddot a , and higher proper-time derivatives of the acceleration [ 8 ] . At leading order, wherever the acceleration changes slowly compared to the local orthogonalization timescale it sets for itself, the detector reports the instantaneous Unruh temperature TU(a(τ)T_U(a(\tau)) at each moment, as though briefly and locally eternal. This adiabatic recovery is the second known limit this construction inherits rather than derives: it says DdetD_{\rm det} between a strictly eternal trajectory at acceleration a and a slowly varying trajectory that happens to pass through a at some instant should vanish to leading order in the rate of change, with corrections controlled by exactly the jerk and snap terms Barbado and Visser compute.

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