Baryon number transfer could delay Quark-Hadron transition in cosmology
Silvio A. Bonometto, Roberto Mainini

TL;DR
This paper explores how baryon number transfer during the cosmological Quark-Hadron transition, potentially influenced by diquark states, could leave observable imprints on cosmological phenomena despite the transition being a crossover.
Contribution
It introduces the idea that baryon transfer and diquark states could affect cosmological evolution even during a crossover transition, a novel perspective in early Universe studies.
Findings
Baryon transfer could cause detectable deviations in cosmological models.
Diquark states' abundance influences baryon formation at the transition.
Residual effects might impact primordial nucleosynthesis.
Abstract
In the early Universe, strongly interacting matter was a quark-gluon plasma. Both lattice computations and heavy ion collision experiments however tell us that, in the absence of chemical potentials, no plasma survives at MeV. The cosmological Quark-Hadron transition, however, seems to have been a crossover; cosmological consequences envisaged when it was believed to be a phase transition no longer hold. In this paper we discuss whether even a crossover transition can leave an imprint that cosmological observations can seek or, viceversa, there are questions cosmology should address to QCD specialists. In particular, we argue that it is still unclear how baryons (not hadrons) could form at the cosmological transition. A critical role should be played by diquark states, whose abundance in the early plasma needs to be accurately evaluated. We estimate that, if the number of…
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Taxonomy
TopicsCosmology and Gravitation Theories · High-Energy Particle Collisions Research · Particle physics theoretical and experimental studies
