27-30 October 2026
Sevastopol Hotel
Europe/Moscow timezone
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Inflation from Fermion Condensation: Dynamics and Observational Signatures

27 Oct 2026, 17:00
30m
Conference Hall 2 (Sevastopol hotel)

Conference Hall 2

Sevastopol hotel

Oral talk Astroparticle physics Plenary talks

Speaker

Prof. Antonino Marciano (Fudan University)

Description

Inflation is conventionally described in terms of fundamental scalar fields whose microscopic origin remains unknown. We propose [1,2] a fundamentally different mechanism in which inflation emerges from fermion condensates generated by torsion-induced four-fermion interactions in Einstein–Cartan–Holst gravity. Starting from a purely fermionic theory, we derive a two-condensate effective description whose inflationary dynamics resembles hybrid inflation but exhibits a qualitatively new exit mechanism.
The central result is the emergence of a density-driven waterfall transition. During inflation, axial charge production continuously increases the fermion density and the associated chiral chemical potential. Solving the finite-density gap equation, we show that above a critical axial density the condensate no longer admits a symmetry-broken solution. Inflation therefore terminates through the evaporation of the condensate itself rather than through the inflaton crossing a critical field value. This mechanism naturally triggers rapid energy transfer to fermionic degrees of freedom and provides a microscopic realization of instant preheating.
The post-transition condensate is unstable to fragmentation into charged non-topological solitons. These objects can subsequently collapse into primordial black holes, generating a calculable relic population whose properties are determined by the same condensate dynamics that drives inflation [3]. Because the underlying theory is intrinsically chiral and connected to dynamical Chern–Simons gravity, the scenario simultaneously predicts parity-violating signatures [4].
The framework unifies inflation, reheating, soliton formation, primordial-black-hole production, and parity-violating phenomenology within a single gravitationally induced fermion-condensation mechanism. It provides a composite alternative to scalar-field inflation and identifies correlated observational signatures that can test the role of spacetime torsion in the early Universe.

References
[1] S. Alexander, P. Chen, J. Liu, A. Marciano, M. Sasaki and X. L. Su, Hybrid inflation from fermion condensation, Phys. Lett. B 873 (2026), 140193 doi:10.1016/j.physletb.2026.140193 arXiv:2509.25290 [gr-qc]]
[2] S. Alexander, P. Chen, J. Liu, A. Marciano, M. Sasaki and X. L. Su, Fermion Condensate Inflation, Dynamical Waterfall Mechanism and Primordial Black Holes, arXiv:2604.21535 [hep-th].
[[3] E. Cotner, A. Kusenko, M. Sasaki and V. Takhistov, Analytic Description of Primordial Black Hole Formation from Scalar Field Fragmentation, JCAP 10 (2019), 077 doi:10.1088/1475-7516/2019/10/077 arXiv:1907.10613 [astro-ph.CO].
[4] J. Liu, S. Alexander and A. Marciano, Birefringence in fermion-attenuated gravitational wave power spectrum, Phys. Lett. B 866 (2025), 139499 doi:10.1016/j.physletb.2025.139499 arXiv:2501.08240 [gr-qc].

Primary author

Prof. Antonino Marciano (Fudan University)

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