Particle Production by Time-Varying Dark Energy and the End of Cosmic Expansion
Nicolas Patino, Paul J. Steinhardt

TL;DR
This paper explores how time-varying dark energy, through particle production and thermal friction, influences cosmic acceleration and the universe's potential transition from expansion to contraction.
Contribution
It introduces the impact of particle production on dark energy dynamics, especially how thermal friction affects cosmic acceleration and the universe's fate.
Findings
Thermal friction can increase the universe's accelerated expansion.
Particle production may generate detectable thermal dark radiation.
Thermal friction delays the end of cosmic expansion, complicating detection of contraction onset.
Abstract
We consider various possible consequences of time-varying dark energy due to a quintessence scalar field whose energy density is partially converted to particles as the field evolves down its potential. This particle production acts as a source of thermal friction on the field that can make it difficult to distinguish whether dark energy is due to a radiating field rolling down a steep potential, a purely self-interacting field moving down a flatter potential, or a cosmological constant. By reducing the acceleration of the scalar field, thermal friction increases the amount of accelerated expansion and can cause a sizable bump in the quintessence equation of state. We take special interest in the case where a steep potential rapidly changes from positive to negative as the field evolves, resulting in the end of cosmic expansion and the beginning of contraction. Even in this case, we…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Pulsars and Gravitational Waves Research
