Using a nonrelativistic closed quantum system without time, it is shown how evolution arises when singling out a degree of freedom that acts as a clock and placing it in a suitable semiclassical state. The path integral formalism gives an intuitive explanation: when the clock becomes classical, the Schrödinger equation emerges from the timeless dynamics. The analysis extends to generally covariant systems (including gravity) with action S: transition amplitudes often take the form exp(iS/ħ)+exp(-iS/ħ) — this is the 'cosine problem', arising from time-reversal symmetry and time-neutral boundary states. Introducing a semiclassical clock singles out the arrow of time, leaving only the forward propagator exp(iS/ħ), without modifying the fundamental dynamics. The result clarifies the mechanism of time emergence and emphasizes that in the canonical formulation, quantum gravity is fundamentally timeless.
The deepest equations of physics, like the Wheeler–DeWitt equation, contain no time. Past and future are scrambled within them, like frames on a film reel with no arrow indicating which way to play it. This symmetry is not a flaw but a feature.
Thus, in quantum gravity (for instance, in the work of Rovelli), the flow of time is born spontaneously. No tweaking of the laws: an internal metronome turns chaos into the arrow of time. This also explains how time could have started after the Big Bang. And most astonishingly, any sufficiently large object—even a spinning galaxy—can act as such a clock, selecting a future from a fan of possibilities.
🎯 Paradox: time doesn’t flow on its own—it requires an ‘observer’ in the form of a physical clock. Without one, all moments exist at once, like frames on a frozen film reel.
🎬 Just like in ‘Tenet’, where reversed entropy turns time backward, the new work shows that at a fundamental level, motion in either direction is equally valid—until a clock intervenes.